1803:
orbits around
Jupiter. The northern pole has eight cyclones moving around a central cyclone (NPC) while the southern pole only has five cyclones around a central cyclone (SPC), with a gap between the first and second cyclones. The cyclones look like the hurricanes on Earth with trailing spiral arms and a denser center, although there are differences between the centers depending on the individual cyclone. Northern CPCs generally maintain their shape and position compared to the southern CPCs and this could be due to the faster wind speeds that are experienced in the south, where the maximum wind velocities are around 80 m/s to 90 m/s. Although there is more movement among the southern CPCs they tend to retain the pentagonal structure relative to the pole. It has also been observed that the angular wind velocity increases as the center is approached and radius becomes smaller, except for one cyclone in the north, which may have rotation in the opposite direction. The difference in the number of cyclones in the north compared to the south is probably due to the size of the cyclones. The southern CPCs tend to be bigger with radii ranging from 5,600 km to 7,000 km while northern CPCs range from 4,000 km to 4,600 km.
1603:
or even white. The higher temperature of the reddest central region is the first evidence that the Spot's color is affected by environmental factors. The spot occasionally disappears from the visible spectrum, becoming evident only through the Red Spot Hollow, which is its niche in the South
Equatorial Belt (SEB). The visibility of GRS is apparently coupled to the appearance of the SEB; when the belt is bright white, the spot tends to be dark, and when it is dark, the spot is usually light. The periods when the spot is dark or light occur at irregular intervals; in the 50 years from 1947 to 1997, the spot was darkest in the periods 1961–1966, 1968–1975, 1989–1990, and 1992–1993. In November 2014, an analysis of data from NASA's Cassini mission revealed that the red color is likely a product of simple chemicals being broken apart by solar ultraviolet irradiation in the planet's upper atmosphere.
1839:
each perijove (53 days), but JIRAM is able to collect enough data to understand the northern CPCs. The limited illumination makes it difficult to see the northern central cyclone, but by making four orbits, the NPC can be partially seen and the octagonal structure of the cyclones can be identified. Limited illumination also makes it difficult to view the motion of the cyclones, but early observations show that the NPC is offset from the pole by about 0.5˚ and the CPCs generally maintained their position around the center. Despite data being harder to obtain, it has been observed that the northern CPCs have a drift rate of about 1˚ to 2.5˚ per perijove to the west. The seventh cyclone in the north (n7) drifts a little more than the others and this is due to an anticyclonic white oval (AWO) that pulls it farther from the NPC, which causes the octagonal shape to be slightly distorted.
1474:, but stay at approximately the same latitude as they are unable to escape from the confining zone. The wind speeds at their periphery are about 100 m/s. Different anticyclones located in one zone tend to merge when they approach each other. However Jupiter has two anticyclones that are somewhat different from all others. They are the Great Red Spot (GRS) and the Oval BA; the latter formed only in 2000. In contrast to white ovals, these structures are red, arguably due to dredging up of red material from the planet's depths. On Jupiter the anticyclones usually form through merges of smaller structures including convective storms (see below), although large ovals can result from the instability of jets. The latter was observed in 1938–1940, when a few white ovals appeared as a result of instability of the southern temperate zone; they later merged to form Oval BA.
1242:
1230:
1283:, which is in turn maintained by moist convection in the outer layer of the atmosphere (above the water clouds). The moist convection is a phenomenon related to the condensation and evaporation of water and is one of the major drivers of terrestrial weather. The production of the jets in this model is related to a well-known property of two dimensional turbulence—the so-called inverse cascade, in which small turbulent structures (vortices) merge to form larger ones. The finite size of the planet means that the cascade can not produce structures larger than some characteristic scale, which for Jupiter is called the Rhines scale. Its existence is connected to production of
1591:, however, is subject to constant variation. Because Jupiter's visible features do not rotate uniformly at all latitudes, astronomers have defined three different systems for defining the longitude. System II is used for latitudes of more than 10°, and was originally based on the average rotation rate of the Great Red Spot of 9h 55m 42s. Despite this, the spot has "lapped" the planet in System II at least 10 times since the early 19th century. Its drift rate has changed dramatically over the years and has been linked to the brightness of the South Equatorial Belt, and the presence or absence of a South Tropical Disturbance.
1714:. The Baby Red Spot encountered the GRS in late June to early July 2008, and in the course of a collision, the smaller red spot was shredded into pieces. The remnants of the Baby Red Spot first orbited, then were later consumed by the GRS. The last of the remnants with a reddish color to have been identified by astronomers had disappeared by mid-July, and the remaining pieces again collided with the GRS, then finally merged with the bigger storm. The remaining pieces of the Baby Red Spot had completely disappeared by August 2008. During this encounter Oval BA was present nearby, but played no apparent role in the destruction of the Baby Red Spot.
1731:
1514:
1850:. The locations over time were revealed to form an oscillatory motion of each of the 6 cyclones, with periods of approximately one (Earth) year and radii of about 400 km. These oscillations around the CPCs' mean positions were explained to be a result of imbalances between the beta-drift, pulling the CPCs toward the pole and the rejection forces that develop due to the interactions between the cyclones, similar to a 6-body spring system. In addition to this periodic motion, the south polar cyclones were observed to drift westward by 7.5±0.7˚ per year. The reason for this drift is still unknown.
1151:
1580:(prograde) to its south and a very strong westward (retrograde) one to its north. Though winds around the edge of the spot peak at about 120 m/s (432 km/h), currents inside it seem stagnant, with little inflow or outflow. The rotation period of the spot has decreased with time, perhaps as a direct result of its steady reduction in size. In 2010, astronomers imaged the GRS in the far infrared (from 8.5 to 24 μm) with a spatial resolution higher than ever before and found that its central, reddest region is warmer than its surroundings by between 3–4
2113:
1443:
31:
8638:
1663:
9163:
1435:, anticyclones predominate over cyclones on Jupiter—more than 90% of vortices larger than 2000 km in diameter are anticyclones. The lifetime of Jovian vortices varies from several days to hundreds of years, depending on their size. For instance, the average lifetime of an anticyclone between 1000 and 6000 km in diameter is 1–3 years. Vortices have never been observed in the equatorial region of Jupiter (within 10° of latitude), where they are unstable. As on any rapidly rotating planet, Jupiter's anticyclones are high
1595:
8508:
1180:
and erupts dark brownish material which is stretched into a new belt by
Jupiter's winds. The belt most recently disappeared in May 2010. Another characteristic of the SEB is a long train of cyclonic disturbances following the Great Red Spot. Like the NTropZ, the STropZ is one of the most prominent zones on the planet; not only does it contain the GRS, but it is occasionally rent by a South Tropical Disturbance (STropD), a division of the zone that can be very long-lived; the most famous one lasted from 1901 to 1939.
216:
2065:
1942:
1325:
1858:
1005:. The EZ is an exception to this rule, showing a strong eastward (prograde) jet and has a local minimum of the wind speed exactly at the equator. The jet speeds are high on Jupiter, reaching more than 100 m/s. These speeds correspond to ammonia clouds located in the pressure range 0.7–1 bar. The prograde jets are generally more powerful than the retrograde jets. The jets extend thousands of kilometers into the interior, as measured by the gravitometer instrument onboard of the
1155:
the planet. The Great Red Spot is at the southern margin of the SEB. Strings of small storms rotate around northern-hemisphere ovals. Small, very bright features, possible lightning storms, appear quickly and randomly in turbulent regions. The smallest features visible at the equator are about 600 kilometers across. This 14-frame animation spans 24 Jovian days, or about 10 Earth days. The passage of time is accelerated by a factor of 600,000. The occasional black spots in the image are
1795:
1082:
motion in the deeper atmosphere. Juno's microwave measurements probe the atmosphere down to ~240 bar. These measurements confirmed the existence of these motions as a part of mid-latitudes large circulation cells with upward motion in the belts and downward motions in the zones, extending from ~1 bar down to at least ~240 bar. So far, 8 cells have been identified at each of
Jupiter's hemispheres along latitudes 20°-60° N\S. The mid-latitude cells are driven by breaking of
1451:
1029:
8520:
1099:
9077:
1655:
1184:
1550:
1723:
1854:
the edge with a dark inner portion. There are four "filled" cyclones and four "chaotic" cyclones in the north. The southern cyclones all have an extensive fine-scale spiral structure on their outside but they all differ in size and shape. There is very little observation of the cyclones due to low sun angles and a haze that is typically over the atmosphere but what little has been observed shows the cyclones to be a reddish color.
8484:
296:. The latter is about 2.5 times stronger than on Earth, but the average molecular weight is about 15 times less.) In the stratosphere, the temperatures rise to about 200 K at the transition into the thermosphere, at an altitude and pressure of around 320 km and 1 μbar. In the thermosphere, temperatures continue to rise, eventually reaching 1000 K at about 1000 km, where pressure is about 1 nbar.
1295:, the Rhines scale in the direction parallel to the equator is larger than in the direction orthogonal to it. The ultimate result of the process described above is production of large scale elongated structures, which are parallel to the equator. The meridional extent of them appears to match the actual width of jets. Therefore, in shallow models vortices actually feed the jets and should disappear by merging into them.
934:
157:
9088:
8496:
2194:
8472:
8532:
2140:
1635:
1561:, between 1996 and 2006 the spot lost 15 percent of its diameter along its major axis. Xylar Asay-Davis, who was on the team that conducted the study, noted that the spot is not disappearing because "velocity is a more robust measurement because the clouds associated with the Red Spot are also strongly influenced by numerous other phenomena in the surrounding atmosphere."
357:. The high temperatures prevalent in the thermosphere (800–1000 K) have not been explained yet; existing models predict a temperature no higher than about 400 K. They may be caused by absorption of high-energy solar radiation (UV or X-ray), by heating from the charged particles precipitating from the Jovian magnetosphere, or by dissipation of upward-propagating
1119:, and the general diffuseness of features. However, the North-North Temperate Belt (NNTB) is the northernmost distinct belt, though it occasionally disappears. Disturbances tend to be minor and short-lived. The North-North Temperate Zone (NNTZ) is perhaps more prominent, but also generally quiet. Other minor belts and zones in the region are occasionally observed.
273:, is commonly treated as the base of the troposphere. In scientific literature, the 1 bar pressure level is usually chosen as a zero point for altitudes—a "surface" of Jupiter. As is generally the case, the top atmospheric layer, the exosphere, does not have a specific upper boundary. The density gradually decreases until it smoothly transitions into the
1399:
338:, which are generated in the upper stratosphere (1–100 μbar) from methane under the influence of the solar ultraviolet radiation (UV). The methane abundance relative to molecular hydrogen in the stratosphere is about 10, while the abundance ratio of other light hydrocarbons, like ethane and acetylene, to molecular hydrogen is about 10.
153:. Zones, which are colder than belts, correspond to upwellings, while belts mark descending gas. The zones' lighter color is believed to result from ammonia ice; what gives the belts their darker colors is uncertain. The origins of the banded structure and jets are not well understood, though a "shallow model" and a "deep model" exist.
288:, which is the boundary between the troposphere and stratosphere. On Jupiter, the tropopause is approximately 50 km above the visible clouds (or 1 bar level). The pressure and temperature at the tropopause are about 0.1 bar and 110 K. (This gives a drop of 340−110=230 °C over 90+50=140 km. The adiabatic
1750:), which bring the wet air from the depths to the upper part of the troposphere, where it condenses in clouds. A typical vertical extent of Jovian storms is about 100 km; as they extend from a pressure level of about 5–7 bar, where the base of a hypothetical water cloud layer is located, to as high as 0.2–0.5 bar.
1299:
to observations. In addition, the jets tend to be unstable and can disappear over time. Shallow models cannot explain how the observed atmospheric flows on
Jupiter violate stability criteria. More elaborated multilayer versions of weather–layer models produce more stable circulation, but many problems persist. Meanwhile, the
1919:
substances are found in today's
Jupiter atmosphere. Jupiter's atmosphere has a strong vertical air flow that carries these compounds into lower regions. But there are higher temperatures inside Jupiter, which will decompose these chemicals and hinder the formation of life similar to Earth. This was speculated by
1838:
The northern cyclones tend to maintain an octagonal structure with the NPC as a center point. Northern cyclones have less data than southern cyclones because of limited illumination in the north-polar winter, making it difficult for JunoCam to obtain accurate measurements of northern CPC positions at
1834:
where the circumpolar cyclones are positioned (~84°) fits, in calculations, the hypothesis that the poleward beta-drift force balances the equatorward rejection of the polar cyclone on the circumpolar cyclones, assuming they have an anticyclonic ring around them, consistent with model simulations and
1642:
Oval BA is a red storm in
Jupiter's southern hemisphere similar in form to, though smaller than, the Great Red Spot (it is often affectionately referred to as "Red Spot Jr.", "Red Jr." or "The Little Red Spot"). A feature in the South Temperate Belt, Oval BA was first seen in 2000 after the collision
1546:
40,000 km in diameter. At the present rate of reduction, it could potentially become circular by 2040, although this is unlikely because of the distortion effect of the neighboring jet streams. It is not known how long the spot will last, or whether the change is a result of normal fluctuations.
1490:
The deep structure of vortices is not completely clear. They are thought to be relatively thin, as any thickness greater than about 500 km will lead to instability. The large anticyclones are known to extend only a few tens of kilometers above the visible clouds. As of 2008, the early hypothesis
1266:
The theories regarding the dynamics of the Jovian atmosphere can be broadly divided into two classes: shallow and deep. The former hold that the observed circulation is largely confined to a thin outer (weather) layer of the planet, which overlays the stable interior. The latter hypothesis postulates
320:
S, between 1–2 bar) and water (3–7 bar) are thought to exist. There are no methane clouds as the temperatures are too high for it to condense. The water clouds form the densest layer of clouds and have the strongest influence on the dynamics of the atmosphere. This is a result of the higher
193:
tend to be white. Vortices are thought to be relatively shallow structures with depths not exceeding several hundred kilometers. Located in the southern hemisphere, the GRS is the largest known vortex in the Solar System. It could engulf two or three Earths and has existed for at least three hundred
1786:
longitude. They significantly disturbed the belt. The dark material that was shed by the storms mixed with clouds and changed the belt's color. The storms moved with a speed as high as 170 m/s, slightly faster than the jet itself, hinting at the existence of strong winds deep in the atmosphere.
1785:
Every 15–17 years
Jupiter is marked by especially powerful storms. They appear at 23°N latitude, where the strongest eastward jet, that can reach 150 m/s, is located. The last time such an event was observed was in March–June 2007. Two storms appeared in the northern temperate belt 55° apart in
1745:
on Earth. They reveal themselves via bright clumpy clouds about 1000 km in size, which appear from time to time in the belts' cyclonic regions, especially within the strong westward (retrograde) jets. In contrast to vortices, storms are short-lived phenomena; the strongest of them may exist for
1709:
Oval BA should not be confused with another major storm on
Jupiter, the South Tropical Little Red Spot (LRS) (nicknamed "the Baby Red Spot" by NASA), which was destroyed by the GRS. The new storm, previously a white spot in Hubble images, turned red in May 2008. The observations were led by Imke de
1602:
It is not known exactly what causes the Great Red Spot's reddish color. Theories supported by laboratory experiments suppose that the color may be caused by complex organic molecules, red phosphorus, or yet another sulfur compound. The GRS varies greatly in hue, from almost brick-red to pale salmon,
1320:
ideal liquid, the flows are organized in a series of cylinders parallel to the rotational axis. The conditions of the theorem are probably met in the fluid Jovian interior. Therefore, the planet's molecular hydrogen mantle may be divided into cylinders, each cylinder having a circulation independent
1298:
While these weather–layer models can successfully explain the existence of a dozen narrow jets, they have serious problems. A glaring failure of the model is the prograde (super-rotating) equatorial jet: with some rare exceptions shallow models produce a strong retrograde (subrotating) jet, contrary
1262:
may occur throughout the planet's outer molecular envelope. As of 2008, a comprehensive theory of the dynamics of the Jovian atmosphere has not been developed. Any such theory needs to explain the following facts: the existence of narrow stable bands and jets that are symmetric relative to
Jupiter's
1191:
The South Temperate Region, or South Temperate Belt (STB), is yet another dark, prominent belt, more so than the NTB; until March 2000, its most famous features were the long-lived white ovals BC, DE, and FA, which have since merged to form Oval BA ("Red Jr."). The ovals were part of South Temperate
961:
of approximately 7°S to 7°N. Above and below the EZ, the North and South Equatorial belts (NEB and SEB) extend to 18°N and 18°S, respectively. Farther from the equator lie the North and South Tropical zones (NtrZ and STrZ). The alternating pattern of belts and zones continues until the polar regions
2342:
atmospheric probe failed to measure the deep abundance of oxygen, because the water concentration continued to increase down to the pressure level of 22 bar, when it ceased operating. While the actually measured oxygen abundances are much lower than the solar value, the observed rapid increase
1883:
Some of the most mysterious features in the atmosphere of Jupiter are hot spots. In them, the air is relatively free of clouds and heat can escape from the depths without much absorption. The spots look like bright spots in the infrared images obtained at the wavelength of about 5 μm. They are
1853:
The circumpolar cyclones have different morphologies, especially in the north, where cyclones have a "filled" or "chaotic" structure. The inner part of the "chaotic" cyclones have small-scale cloud streaks and flecks. The "filled" cyclones have a sharply-bound, lobate area that is bright white near
1802:
Other notable features of Jupiter are its cyclones near the northern and southern poles of the planet. These are called circumpolar cyclones (CPCs) and they have been observed by the Juno Spacecraft using JunoCam and JIRAM. The cyclones have now been observed for about 5 years, as Juno completed 39
1545:
days. Its dimensions are 24,000–40,000 km east-to-west and 12,000–14,000 km north-to-south. The spot is large enough to contain two or three planets the size of Earth. At the start of 2004, the Great Red Spot had approximately half the longitudinal extent it had a century ago, when it was
1537:
in 1635, Leander Bandtius, whom Riccioli identified as the Abbot of Dunisburgh who possessed an "extraordinary telescope", observed a large spot that he described as "oval, equaling one seventh of Jupiter's diameter at its longest." According to Riccioli, "these features are seldom able to be seen,
1340:
within Jupiter. One model published in 2004 successfully reproduced the Jovian band-jet structure. It assumed that the molecular hydrogen mantle is thinner than in all other models; occupying only the outer 10% of Jupiter's radius. In standard models of the Jovian interior, the mantle comprises the
1195:
There are other features on Jupiter that are either temporary or difficult to observe from Earth. The South South Temperate Region is harder to discern even than the NNTR; its detail is subtle and can only be studied well by large telescopes or spacecraft. Many zones and belts are more transient in
1179:
jet stream. The SEB is usually the broadest, darkest belt on Jupiter; it is sometimes split by a zone (the SEBZ), and can fade entirely every 3 to 15 years before reappearing in what is known as an SEB Revival cycle. A period of weeks or months following the belt's disappearance, a white spot forms
965:
The difference in the appearance between zones and belts is caused by differences in the opacity of the clouds. Ammonia concentration is higher in zones, which leads to the appearance of denser clouds of ammonia ice at higher altitudes, which in turn leads to their lighter color. On the other hand,
1955:
Early modern astronomers, using small telescopes, recorded the changing appearance of Jupiter's atmosphere. Their descriptive terms—belts and zones, brown spots and red spots, plumes, barges, festoons, and streamers—are still used. Other terms such as vorticity, vertical motion, cloud heights have
1477:
In contrast to anticyclones, the Jovian cyclones tend to be small, dark and irregular structures. Some of the darker and more regular features are known as brown ovals (or badges). However the existence of a few long–lived large cyclones has been suggested. In addition to compact cyclones, Jupiter
1154:
Zones, belts and vortices on Jupiter. The wide equatorial zone is visible in the center surrounded by two dark equatorial belts (SEB and NEB). The large grayish-blue irregular "hot spots" at the northern edge of the white Equatorial Zone change over the course of time as they march eastward across
1056:
on Earth, and white ammonia clouds evaporate, revealing lower, darker clouds. The location and width of bands, speed and location of jets on Jupiter are remarkably stable, having changed only slightly between 1980 and 2000. One example of change is a decrease of the speed of the strongest eastward
754:
at depths of more than 10,000 km, helium separates from it forming droplets which, being denser than the metallic hydrogen, descend towards the core. This can also explain the severe depletion of neon (see Table), an element that easily dissolves in helium droplets and would be transported in
197:
Jupiter has powerful storms, often accompanied by lightning strikes. The storms are a result of moist convection in the atmosphere connected to the evaporation and condensation of water. They are sites of strong upward motion of the air, which leads to the formation of bright and dense clouds. The
1989:
Today, astronomers have access to a continuous record of Jupiter's atmospheric activity thanks to telescopes such as Hubble Space Telescope. These show that the atmosphere is occasionally wracked by massive disturbances, but that, overall, it is remarkably stable. The vertical motion of Jupiter's
1697:
Why Oval BA turned red is not well understood. According to a 2008 study by Dr. Santiago Pérez-Hoyos of the University of the Basque Country, the most likely mechanism is "an upward and inward diffusion of either a colored compound or a coating vapor that may interact later with high energy solar
2108:
The present GRS was first seen only after 1830 and well-studied only after a prominent apparition in 1879. A 118-year gap separates the observations made after 1830 from its 17th-century discovery; whether the original spot dissipated and re-formed, whether it faded, or even if the observational
1870:
The normal pattern of bands and zones is sometimes disrupted for periods of time. One particular class of disruption are long-lived darkenings of the South Tropical Zone, normally referred to as "South Tropical Disturbances" (STD). The longest lived STD in recorded history was followed from 1901
1146:
The NEB is one of the most active belts on the planet. It is characterized by anticyclonic white ovals and cyclonic "barges" (also known as "brown ovals"), with the former usually forming farther north than the latter; as in the NTropZ, most of these features are relatively short-lived. Like the
1081:
cells. On Jupiter, the visible cloud bands gave indication for upward motion in the zones and downward motion in the belts, indicative only for the upper few bars. However, higher frequency of lightning flashes in the belts, indicative of upward atmospheric motion, gave indication for a reversed
1646:
The formation of the three white oval storms that later merged into Oval BA can be traced to 1939, when the South Temperate Zone was torn by dark features that effectively split the zone into three long sections. Jovian observer Elmer J. Reese labeled the dark sections AB, CD, and EF. The rifts
1341:
outer 20–30%. The driving of deep circulation is another problem. The deep flows can be caused both by shallow forces (moist convection, for instance) or by deep planet-wide convection that transports heat out of the Jovian interior. Which of these mechanisms is more important is not clear yet.
1335:
The deep model easily explains the strong prograde jet observed at the equator of Jupiter; the jets it produces are stable and do not obey the 2D stability criterion. However it has major difficulties; it produces a very small number of broad jets, and realistic simulations of 3D flows are not
1136:
The North Tropical Region is composed of the NTropZ and the North Equatorial Belt (NEB). The NTropZ is generally stable in coloration, changing in tint only in tandem with activity on the NTB's southern jet stream. Like the NTZ, it too is sometimes divided by a narrow band, the NTropB. On rare
160:
2159:
shortly after their formation, but contracted rapidly during their first decade; their length stabilized at 10 degrees or less after 1965. Although they originated as segments of the STZ, they evolved to become completely embedded in the South Temperate Belt, suggesting that they moved north,
1918:
proved that the combination of lightning and compounds existing in the primitive Earth's atmosphere can form organic matter (including amino acids), which can be used as the cornerstone of life. The simulated atmosphere consists of water, methane, ammonia and hydrogen molecules; all of these
1376:
may be important for the dynamics of the Jovian atmosphere. While Jupiter has a small obliquity of about 3°, and its poles receive much less solar radiation than its equator, the tropospheric temperatures do not change appreciably from the equator to poles. One explanation is that Jupiter's
159:
165:
163:
158:
1267:
that the observed atmospheric flows are only a surface manifestation of deeply rooted circulation in the outer molecular envelope of Jupiter. As both theories have their own successes and failures, many planetary scientists think that the true theory will include elements of both models.
2130:
spacecraft was 9.2 million kilometers from Jupiter it transmitted the first detailed image of the Great Red Spot back to Earth. Cloud details as small as 160 km across were visible. The colorful, wavy cloud pattern seen to the west (left) of the GRS is the spot's wake region, where
1701:
Oval BA is getting stronger according to observations made with the Hubble Space Telescope in 2007. The wind speeds have reached 618 km/h; about the same as in the Great Red Spot and far stronger than any of the progenitor storms. As of July 2008, its size is about the diameter of
1698:
photons at the upper levels of Oval BA." Some believe that small storms (and their corresponding white spots) on Jupiter turn red when the winds become powerful enough to draw certain gases from deeper within the atmosphere which change color when those gases are exposed to sunlight.
164:
1769:
spacecraft revealed regular light flashes in Jovian belts and near the locations of the westward jets, particularly at 51°N, 56°S and 14°S latitudes. On Jupiter lightning strikes are on average a few times more powerful than those on Earth. However, they are less frequent; the light
2377:
reported that storms on Jupiter are similar to those on Earth, which form close to the equator, then move towards the poles. However, Jupiter's storms do not experience any friction from the land or oceans; hence, they drift until they reach the poles, which generate the so-called
1168:) features known as festoons (hot spots). Though the southern boundary of the EZ is usually quiescent, observations from the late 19th into the early 20th century show that this pattern was then reversed relative to today. The EZ varies considerably in coloration, from pale to an
1192:
Zone, but they extended into STB partially blocking it. The STB has occasionally faded, apparently due to complex interactions between the white ovals and the GRS. The appearance of the South Temperate Zone (STZ)—the zone in which the white ovals originated—is highly variable.
5255:
Tabataba-Vakili, F.; Rogers, J.H.; Eichstädt, G.; Orton, G.S.; Hansen, C.J.; Momary, T.W.; Sinclair, J.A.; Giles, R.S.; Caplinger, M.A.; Ravine, M.A.; Bolton, S.J. (January 2020). "Long-term tracking of circumpolar cyclones on Jupiter from polar observations with JunoCam".
1068:
are a large-scale atmospheric motion where gas rises at a certain latitude, travel in the north-south (meridional) direction, descends, and get back to the origin in a closed cell circulation. On Earth, the meridional circulation is composed of 3 cells in each hemisphere:
1571:
of the GRS are about 8 km above the surrounding clouds. Furthermore, careful tracking of atmospheric features revealed the spot's counterclockwise circulation as far back as 1966 – observations dramatically confirmed by the first time-lapse movies from the
1137:
occasions, the southern NTropZ plays host to "Little Red Spots". As the name suggests, these are northern equivalents of the Great Red Spot. Unlike the GRS, they tend to occur in pairs and are always short-lived, lasting a year on average; one was present during the
1369:. The latter value is approximately equal to one billionth of the total power radiated by the Sun. This excess heat is mainly the primordial heat from the early phases of Jupiter's formation, but may result in part from the precipitation of helium into the core.
1107:
The belts and zones that divide Jupiter's atmosphere each have their own names and unique characteristics. They begin below the North and South Polar Regions, which extend from the poles to roughly 40–48° N/S. These bluish-gray regions are usually featureless.
966:
in belts clouds are thinner and are located at lower altitudes. The upper troposphere is colder in zones and warmer in belts. The exact nature of chemicals that make Jovian zones and bands so colorful is not known, but they may include complicated compounds of
162:
1102:
Idealized illustration of Jupiter's cloud bands, labeled with their official abbreviations. Lighter zones are indicated to the right, darker belts to the left. The Great Red Spot and Oval BA are shown in the South Tropical Zone and South Temperate Belt,
1287:. This process works as follows: when the largest turbulent structures reach a certain size, the energy begins to flow into Rossby waves instead of larger structures, and the inverse cascade stops. Since on the spherical rapidly rotating planet the
6610:
Baines, Kevin H.; Simon-Miller, Amy A; Orton, Glenn S.; Weaver, Harold A.; Lunsford, Allen; Momary, Thomas W.; Spencer, John; Cheng, Andrew F.; Reuter, Dennis C. (12 October 2007). "Polar Lightning and Decadal-Scale Cloud Variability on Jupiter".
1057:
jet located at the boundary between the North Tropical zone and North Temperate belts at 23°N. However bands vary in coloration and intensity over time (see "specific band"). These variations were first observed in the early seventeenth century.
2663:
Smith, Bradford A.; Soderblom, Laurence A.; Johnson, Torrence V.; Ingersoll, Andrew P.; Collins, Stewart A.; Shoemaker, Eugene M.; Hunt, G. E.; Masursky, Harold; Carr, Michael H. (1979-06-01). "The Jupiter System Through the Eyes of Voyager 1".
329:
chemical element than either nitrogen or sulfur). Various tropospheric (at 200–500 mbar) and stratospheric (at 10–100 mbar) haze layers reside above the main cloud layers. The stratospheric haze layers are made from condensed heavy
2086:, who described a spot on the planet in May 1664; however, it is likely that Hooke's spot was in the wrong belt altogether (the North Equatorial Belt, versus the current location in the South Equatorial Belt). Much more convincing is
1303:
found that the winds on Jupiter extend well below the water clouds at 5–7 bar and do not show any evidence of decay down to 22 bar pressure level, which implies that circulation in the Jovian atmosphere may in fact be deep.
1377:
convective interior acts like a thermostat, releasing more heat near the poles than in the equatorial region. This leads to a uniform temperature in the troposphere. While heat is transported from the equator to the poles mainly
1163:
The Equatorial Region (EZ) is one of the most stable regions of the planet, in latitude and in activity. The northern edge of the EZ hosts spectacular plumes that trail southwest from the NEB, which are bounded by dark, warm (in
254:. Jupiter does not have a solid surface, and the lowest atmospheric layer, the troposphere, smoothly transitions into the planet's fluid interior. This is a result of having temperatures and the pressures well above those of the
202:
observations suggest Jovian lightning strikes occur above the altitude of water clouds (3-7 bars). A charge separation between falling liquid ammonia-water droplets and water ice particles may generate higher-altitude lightning.
749:
value. The reason for this low abundance is not entirely understood, but some of the helium may have condensed into the core of Jupiter. This condensation is likely to be in the form of helium rain: as hydrogen turns into the
6027:
Mura, A.; Adriani, A.; Bracco, A.; Moriconi, M. L.; Grassi, D.; Plainaki, C.; Ingersoll, A.; Bolton, S.; Sordini, R.; Altieri, F.; Ciarravano, A.; Cicchetti, A.; Dinelli, B. M.; Filacchione, G.; Migliorini, A. (2021-07-28).
2799:
Giles, Rohini S.; Greathouse, Thomas K.; Bonfond, Bertrand; Gladstone, G. Randall; Kammer, Joshua A.; Hue, Vincent; Grodent, Denis C.; Gérard, Jean-Claude; Versteeg, Maarten H.; Wong, Michael H.; Bolton, Scott J. (2020).
2328:
is the gravitational acceleration at the surface of Jupiter. As the temperature varies from 110 K in the tropopause up to 1000 K in the thermosphere, the scale height can assume values from 15 to 150 km.
5788:
Mura, A.; Scarica, P.; Grassi, D.; Adriani, A.; Bracco, A.; Piccioni, G.; Sindoni, G.; Moriconi, M. L.; Plainaki, C.; Ingersoll, A.; Altieri, F.; Cicchetti, A.; Dinelli, B. M.; Filacchione, G.; Migliorini, A. (2022).
5197:
Mura, A.; Scarica, P.; Grassi, D.; Adriani, A.; Bracco, A.; Piccioni, G.; Sindoni, G.; Moriconi, M. L.; Plainaki, C.; Ingersoll, A.; Altieri, F.; Cicchetti, A.; Dinelli, B. M.; Filacchione, G.; Migliorini, A. (2022).
2729:; Alexander, James W.; Atreya, Sushil K.; Bolton, Scott J.; Brennan, Martin J.; Brown, Shannon T.; Guillaume, Alexandre; Guillot, Tristan; Ingersoll, Andrew P.; Levin, Steven M.; Lunine, Jonathan I. (5 August 2020).
1584:. The warm airmass is located in the upper troposphere in the pressure range of 200–500 mbar. This warm central spot slowly counter-rotates and may be caused by a weak subsidence of air in the center of GRS.
1349:
As has been known since 1966, Jupiter radiates much more heat than it receives from the Sun. It is estimated that the ratio of the thermal power emitted by the planet to the thermal power absorbed from the Sun is
2056:, as it plunged into Jupiter, measured the wind, temperature, composition, clouds, and radiation levels down to 22 bar. However, below 1 bar elsewhere on Jupiter there is uncertainty in the quantities.
1674:
amateur astronomer Christopher Go discovered the color change, noting that it had reached the same shade as the GRS. As a result, NASA writer Dr. Tony Phillips suggested it be called "Red Spot Jr." or "Red Jr."
1321:
of the others. Those latitudes where the cylinders' outer and inner boundaries intersect with the visible surface of the planet correspond to the jets; the cylinders themselves are observed as zones and belts.
6452:
Atreya, Sushil K.; Mahaffy, P. R.; Niemann, H. B.; Wong, M. H.; Owen, T. C. (February 2003). "Composition and origin of the atmosphere of Jupiter—an update, and implications for the extrasolar giant planets".
1486:
region) in the southern equatorial belt. These patches are called cyclonic regions (CR). The cyclones are always located in the belts and tend to merge when they encounter each other, much like anticyclones.
299:
Jupiter's troposphere contains a complicated cloud structure. The upper clouds, located in the pressure range 0.6–0.9 bar, are made of ammonia ice. Below these ammonia ice clouds, denser clouds made of
1553:
An infrared image of GRS (top) and Oval BA (lower left) showing its cool center, taken by the ground based Very Large Telescope. An image made by the Hubble Space Telescope (bottom) is shown for comparison.
3691:
Duer, Keren; Gavriel, Nimrod; Galanti, Eli; Kaspi, Yohai; Fletcher, Leigh N.; Guillot, Tristan; Bolton, Scott J.; Levin, Steven M.; Atreya, Sushil K.; Grassi, Davide; Ingersoll, Andrew P. (2021-12-16).
2175:), and their proximity to the GRS (they accelerated when within 50 degrees of the Spot). The overall trend of the white oval drift rate was deceleration, with a decrease by half between 1940 and 1990.
1647:
expanded, shrinking the remaining segments of the STZ into the white ovals FA, BC, and DE. Ovals BC and DE merged in 1998, forming Oval BE. Then, in March 2000, BE and FA joined, forming Oval BA. (see
993:) jets mark the transition from belts to zones. Such flow velocity patterns mean that the jets' eastward momentum decreases in belts and increases in zones from the equator to the pole. Therefore,
161:
7401:
Pearl, J. C.; Conrath, B. J.; Hanel, R. A.; Pirraglia, J. A.; Coustenis, A. (March 1990). "The albedo, effective temperature, and energy balance of Uranus, as determined from Voyager IRIS data".
1133:
encounters), making the North Temperate Zone (NTZ) apparently merge into the North Tropical Zone (NTropZ). Other times, the NTZ is divided by a narrow belt into northern and southern components.
198:
storms form mainly in belt regions. The lightning strikes on Jupiter are hundreds of times more powerful than those seen on Earth, and are assumed to be associated with the water clouds. Recent
1875:
on February 28, 1901. It took the form of darkening over part of the normally bright South Tropical zone. Several similar disturbances in the South Tropical Zone have been recorded since then.
1746:
several months, while the average lifetime is only 3–4 days. They are believed to be due mainly to moist convection within Jupiter's troposphere. Storms are actually tall convective columns (
1982:. The two spacecraft were able to image details at a resolution as low as 5 km in size in various spectra, and also able to create "approach movies" of the atmosphere in motion. The
1774:
emitted from a given area is similar to that on Earth. A few flashes have been detected in polar regions, making Jupiter the second known planet after Earth to exhibit polar lightning. A
2101:. It is a part of a series of panels in which different (magnified) heavenly bodies serve as backdrops for various Italian scenes, the creation of all of them overseen by the astronomer
2343:
of water content of the atmosphere with depth makes it highly likely that the deep abundance of oxygen indeed exceeds the solar value by a factor of about 3—much like other elements.
365:
in 1983. The energetic particles coming from Jupiter's magnetosphere create bright auroral ovals, which encircle the poles. Unlike their terrestrial analogs, which appear only during
385:) was discovered. This ion emits strongly in the mid-infrared part of the spectrum, at wavelengths between 3 and 5 μm; this is the main cooling mechanism of the thermosphere.
1175:
The South Tropical Region includes the South Equatorial Belt (SEB) and the South Tropical Zone. It is by far the most active region on the planet, as it is home to its strongest
1025:
above the clouds, while below the cloud level, winds increase slightly and then remain constant down to at least 22 bar—the maximum operational depth reached by the probe.
1263:
equator, the strong prograde jet observed at the equator, the difference between zones and belts, and the origin and persistence of large vortices such as the Great Red Spot.
2182:
fly-bys, the ovals extended roughly 9000 km from east to west, 5000 km from north to south, and rotated every five days (compared to six for the GRS at the time).
2352:
Various explanations of the overabundance of carbon, oxygen, nitrogen and other elements have been proposed. The leading one is that Jupiter captured a large number of icy
3631:
Janssen, M. A.; Oswald, J. E.; Brown, S. T.; Gulkis, S.; Levin, S. M.; Bolton, S. J.; Allison, M. D.; Atreya, S. K.; Gautier, D.; Ingersoll, A. P.; Lunine, J. I. (2017).
2109:
record was simply poor are unknown. The older spots had a short observational history and slower motion than that of the modern spot, which make their identity unlikely.
1906:
heated and dried or, alternatively, they can be a manifestation of planetary scale waves. The latter hypotheses explains the periodical pattern of the equatorial spots.
3282:
Galanti, Eli; Kaspi, Yohai; Duer, Keren; Fletcher, Leigh; Ingersoll, Andrew P.; Li, Cheng; Orton, Glenn S.; Guillot, Tristan; Levin, Steven M.; Bolton, Scott J. (2021).
1129:
on the planet—a westerly current that forms the southern boundary of the North Temperate Belt (NTB). The NTB fades roughly once a decade (this was the case during the
7702:
Seiff, A.; Kirk, D.B.; Knight, T.C.D.; et al. (1998). "Thermal structure of Jupiter's atmosphere near the edge of a 5-μm hot spot in the north equatorial belt".
7356:
Noll, K.S.; McGrath, M.A.; Weaver, H.A.; Yelle, R.V.; et al. (1995). "HST Spectroscopic Observations of Jupiter Following the Impact of Comet Shoemaker-Levy 9".
5307:
Grassi, D.; Adriani, A.; Moriconi, M. L.; Mura, A.; Tabataba-Vakili, F.; Ingersoll, A.; Orton, G.; Hansen, C.; Altieri, F.; Filacchione, G.; Sindoni, G. (June 2018).
3209:
Kaspi, Y.; Galanti, E.; Hubbard, W. B.; Stevenson, D. J.; Bolton, S. J.; Iess, L.; Guillot, T.; Bloxham, J.; Connerney, J. E. P.; Cao, H.; Durante, D. (2018-03-08).
1122:
The North Temperate Region is part of a latitudinal region easily observable from Earth, and thus has a superb record of observation. It also features the strongest
687:
The composition of Jupiter's atmosphere is similar to that of the planet as a whole. Jupiter's atmosphere is the most comprehensively understood of those of all the
5439:
Adriani, A.; Mura, A.; Orton, G.; Hansen, C.; Altieri, F.; Moriconi, M. L.; Rogers, J.; Eichstädt, G.; Momary, T.; Ingersoll, A. P.; Filacchione, G. (March 2018).
4603:"Interim reports on STB (Oval BA passing GRS), STropB, GRS (internal rotation measured), EZ(S. Eq. Disturbance; dramatic darkening; NEB interactions), & NNTB"
5085:
4725:
6405:(October–November 1999). "A comparison of the atmospheres of Jupiter and Saturn: Deep atmospheric composition, cloud structure, vertical mixing, and origin".
1626:
in 1989, may have been an atmospheric hole rather than a storm. It was no longer present in 1994, although a similar spot had appeared farther to the north.
1172:, or even coppery hue; it is occasionally divided by an Equatorial Band (EB). Features in the EZ move roughly 390 km/h relative to the other latitudes.
2105:
for accuracy. Creti's painting is the first known to depict the GRS as red. No Jovian feature was officially described as red before the late 19th century.
1525:, 22° south of Jupiter's equator; observations from Earth establish a minimum storm lifetime of 350 years. A storm was described as a "permanent spot" by
7194:
5032:
4532:
9434:
1048:. When air enriched in ammonia rises in zones, it expands and cools, forming high and dense white clouds. In belts, however, the air descends, warming
6886:
Graney, C. M. (2010). "Changes in the Cloud Belts of Jupiter, 1630–1664, as reported in the 1665 Astronomia Reformata of Giovanni Battista Riccioli".
105:
lacks a clear lower boundary and gradually transitions into the liquid interior of the planet. From lowest to highest, the atmospheric layers are the
7319:
Miller, Steve; Aylward, Alan; Millward, George (January 2005). "Giant Planet Ionospheres and Thermospheres: The Importance of Ion-Neutral Coupling".
1895:
located to the west of it and reaching up to 10,000 km in size. Hot spots generally have round shapes, although they do not resemble vortices.
7984:
7605:
7575:
7545:
7298:
1690:, predicted the storms would have their closest passing on July 4, 2006. On July 20, the two storms were photographed passing each other by the
1538:
and then only by a telescope of exceptional quality and magnification". The Great Spot has been continually observed since the 1870s, however.
4398:
6308:
4366:
6865:
6863:
Go, C.Y.; de Pater, I.; Wong, M.; Lockwood, S.; Marcus, P.; Asay-Davis, X.; Shetty, S. (2006). "Evolution Of The Oval Ba During 2004–2005".
5001:
4951:
2090:'s description of a "permanent spot" in the following year. With fluctuations in visibility, Cassini's spot was observed from 1665 to 1713.
1021:
measured the vertical profile of a jet along its descent trajectory into Jupiter's atmosphere, finding the winds to decay over two to three
698:
when it entered the Jovian atmosphere on December 7, 1995. Other sources of information about Jupiter's atmospheric composition include the
7857:
1567:
data have long indicated that the Great Red Spot is colder (and thus, higher in altitude) than most of the other clouds on the planet; the
4428:
4897:
4778:
3114:
1986:, which suffered an antenna problem, saw less of Jupiter's atmosphere but at a better average resolution and a wider spectral bandwidth.
1606:
The Great Red Spot should not be confused with the Great Dark Spot, a feature observed near Jupiter's north pole (bottom) in 2000 by the
922:
2373:
recorded on 25 August 2020, a storm traveling around the planet at 350 miles per hour (560 km/h). In addition, researches from the
6988:
Hammel, H.B.; Lockwood, G.W.; Mills, J.R.; Barnet, C.D. (1995). "Hubble Space Telescope Imaging of Neptune's Cloud Structure in 1994".
1884:
preferentially located in the belts, although there is a train of prominent hot spots at the northern edge of the Equatorial Zone. The
1587:
The Great Red Spot's latitude has been stable for the duration of good observational records, typically varying by about a degree. Its
1147:
South Equatorial Belt (SEB), the NEB has sometimes dramatically faded and "revived". The timescale of these changes is about 25 years.
7626:
Sanchez-Lavega, A.; Orton, G.S.; Morales R.; et al. (2001). "The Merger of Two Giant Anticyclones in the Atmosphere of Jupiter".
4868:
1678:
In April 2006, a team of astronomers, believing that Oval BA might converge with the GRS that year, observed the storms through the
1336:
possible as of 2008, meaning that the simplified models used to justify deep circulation may fail to catch important aspects of the
945:
The visible surface of Jupiter is divided into several bands parallel to the equator. There are two types of bands: lightly colored
9162:
1810:, a known effect causing cyclones to move poleward and anti-cyclones to move equatorward due to the conservation of momentum along
1208:(SEBZ). Belts are also occasionally split by a sudden disturbance. When a disturbance divides a normally singular belt or zone, an
1086:, similar to the Ferrel cells on Earth. While on Earth, the return flow in the cells' lower branch is balanced by friction in the
219:
Vertical structure of the atmosphere of Jupiter. Note that the temperature drops together with altitude above the tropopause. The
181:), storms and lightning. The vortices reveal themselves as large red, white or brown spots (ovals). The largest two spots are the
17:
1959:
The first observations of the Jovian atmosphere at higher resolution than possible with Earth-based telescopes were taken by the
1811:
794:). Their abundances in the deep (below 10 bar) troposphere imply that the atmosphere of Jupiter is enriched in the elements
1466:
The anticyclones in Jupiter's atmosphere are always confined within zones, where the wind speed increases in direction from the
1279:, which had become well developed by that time. Those shallow models assumed that the jets on Jupiter are driven by small scale
1036:
The origin of Jupiter's colored banded structure is not completely clear, though it may resemble the cloud structure of Earth's
8782:
3110:
194:
years. Oval BA, south of GRS, is a red spot a third the size of GRS that formed in 2000 from the merging of three white ovals.
6659:
1312:
The deep model was first proposed by Busse in 1976. His model was based on another well-known feature of fluid mechanics, the
9125:
8810:
8140:
7961:
7927:
7518:
7495:
7202:
7137:
7099:
6709:
4460:
3430:
1682:. The storms pass each other about every two years, but the passings of 2002 and 2004 did not produce anything exciting. Dr.
1818:. Thus, cyclones forming in the polar regions may congregate at the pole and form a polar cyclone such as those observed on
8805:
2164:
on their northern and southern boundaries, with an eastward jet to their north and a retrograde westward one to the south.
369:, aurorae are permanent features of Jupiter's atmosphere. The thermosphere was the first place outside the Earth where the
7786:
7156:
2216:
1382:
258:
for hydrogen and helium, meaning that there is no sharp boundary between gas and liquid phases. Hydrogen is considered a
1275:
The first attempts to explain Jovian atmospheric dynamics date back to the 1960s. They were partly based on terrestrial
292:
on Earth is around 9.8 °C per km. The adiabatic lapse rate is proportional to the average molecular weight and the
2374:
1711:
1558:
326:
5107:
4742:
Loeffer, Mark J.; Hudson, Reggie L. (2018). "Coloring Jupiter's clouds: Radiolysis of ammonium hydrosulfide (NH4SH)".
8564:
7733:
Smith, B.A.; Soderblom, L.A.; Johnson, T.V.; et al. (1979). "The Jupiter system through the eyes of Voyager 1".
6340:"Modeling the stability of polygonal patterns of vortices at the poles of Jupiter as revealed by the Juno spacecraft"
5723:"Modeling the stability of polygonal patterns of vortices at the poles of Jupiter as revealed by the Juno spacecraft"
5081:
4722:
8445:
8455:
1329:
86:. Although water is thought to reside deep in the atmosphere, its directly-measured concentration is very low. The
6493:
5504:"A Series Solution for the Barotropic Vorticity Equation and its Application in the Study of Atmospheric Vortices"
1090:, the balance in Jupiter in yet unknown, but one possibility is that the friction is maintained by magnetic drag.
8637:
7704:
7091:
1241:
1229:
361:. The thermosphere and exosphere at the poles and at low latitudes emit X-rays, which were first observed by the
331:
255:
125:. The lowest layer, the troposphere, has a complicated system of clouds and hazes composed of layers of ammonia,
9266:
8252:
8216:
8100:
6828:
8354:
8288:
7819:
7808:
7781:
7177:
5028:
4528:
7296:
McKim, R.J. (1997). "P. B. Molesworth's discovery of the great South Tropical Disturbance on Jupiter, 1901".
2408:
2356:
during the later stages of its accretion. The volatiles like noble gases are thought to have been trapped as
4710:
2160:"digging" a niche into the STB. Indeed, much like the GRS, their circulations were confined by two opposing
9305:
9300:
6555:
1176:
1010:
990:
7999:
Youssef, Ashraf; Marcus, Philip S. (2003). "The dynamics of jovian white ovals from formation to merger".
7438:
Reese, E.J.; Solberg, H.G. (1966). "Recent measures of the latitude and longitude of Jupiter's red spot".
7118:
4923:
1666:
Oval BA (bottom), Great Red Spot (top) and "Baby Red Spot" (middle) during a brief encounter in June, 2008
9394:
6941:
6563:
6455:
6407:
6401:
Atreya, Sushil K.; Wong, M. H.; Owen, T. C.; Mahaffy, P. R.; Niemann, H. B.; de Pater, I.; Drossart, P.;
2167:
The longitudinal movement of the ovals seemed to be influenced by two factors: Jupiter's position in its
1775:
1687:
1313:
341:
Jupiter's thermosphere is located at pressures lower than 1 μbar and demonstrates such phenomena as
204:
9410:
Atmospheres in boldface are significant atmospheres; atmospheres in italics are unconfirmed atmospheres.
7817:
Vasavada, A.R.; Showman, A. (2005). "Jovian atmospheric dynamics: An update after Galileo and Cassini".
989:) jets are found at the transition from zones to belts (going away from the equator), whereas westward (
9360:
8983:
8828:
8462:
8452:
of Jupiter's atmospheric activity from 19 December 2014 to 31 March 2015 from amateur astronomer images
7980:
7902:
7868:
7510:
7129:
2801:
2207:
1995:
1915:
1598:
Approximate size comparison of Earth superimposed on this Dec 29, 2000 image showing the Great Red Spot
1534:
699:
142:
9246:
1891:
descended into one of those equatorial spots. Each equatorial spot is associated with a bright cloudy
842:) are present only in trace amounts. The upper atmosphere of Jupiter contains small amounts of simple
325:
of water and higher water abundance as compared to the ammonia and hydrogen sulfide (oxygen is a more
173:
The Jovian atmosphere shows a wide range of active phenomena, including band instabilities, vortices (
9118:
8843:
8838:
8833:
8787:
2243:
2238:
1991:
1216:
is added to indicate whether the component is the northern or southern one; e.g., NEB(N) and NEB(S).
8345:
6829:"Thermal structure and composition of Jupiter's Great Red Spot from high-resolution thermal imaging"
6585:
5848:
4394:
3943:
921:(3.5 × 10). The latter discovery is especially significant since the previous theories of
8820:
8612:
6316:
1990:
atmosphere was largely determined by the identification of trace gases by ground-based telescopes.
1730:
1415:—circular rotating structures that, as in the Earth's atmosphere, can be divided into two classes:
938:
8225:
1513:
962:
at approximately 50 degrees latitude, where their visible appearance becomes somewhat muted.
8627:
8622:
8401:
8363:
8317:
8297:
8261:
8189:
8151:
8109:
8073:
8029:
5005:
4976:
4947:
4424:
3530:
1385:
heat. The convection in the Jovian interior is thought to be driven mainly by the internal heat.
1378:
1255:
1065:
1014:
7872:
3356:
9285:
8857:
8340:
6580:
4420:
3568:
Ingersoll, A. P.; Gierasch, P. J.; Banfield, D.; Vasavada, A. R.; Galileo Imaging Team (2000).
2412:
2370:
1936:
1806:
The mechanism for the stability of these two symmetric structures of cyclones is an outcome of
1679:
879:
39:
6337:
4901:
4782:
1807:
1150:
909:
that gave birth to the Solar System. The ratio of nitrogen isotopes in the Jovian atmosphere,
9179:
8557:
7567:
7214:"Jupiter's Atmospheric Composition from the Cassini Thermal Infrared Spectroscopy Experiment"
6795:
6733:
6402:
4367:"Release 14-135 - NASA's Hubble Shows Jupiter's Great Red Spot is Smaller than Ever Measured"
1892:
1842:
The instantaneous locations of the south polar cyclones have been tracked for 5 years by the
1747:
1526:
1432:
918:
859:
301:
284:. The temperature of the troposphere decreases with height until it reaches a minimum at the
274:
247:
126:
7597:
6964:
6811:
6677:
6576:
6468:
6420:
4450:
269:, at an altitude of about 90 km below 1 bar with a temperature of around 340
189:, which is also red. These two and most of the other large spots are anticyclonic. Smaller
129:, and water. The upper ammonia clouds visible at Jupiter's surface are organized in a dozen
9384:
9333:
9220:
9111:
9015:
8945:
8908:
8416:
8378:
8332:
8276:
8240:
8204:
8166:
8120:
8088:
8074:"Planetary Circulations: 1. Barotropic representation of Jovian and terrestrial turbulence"
8044:
8008:
7828:
7795:
7744:
7713:
7672:
7637:
7614:
7584:
7554:
7449:
7410:
7365:
7328:
7307:
7276:
7267:
7227:
7190:
7165:
7148:
7050:
6999:
6960:
6907:
6874:
6843:
6807:
6775:
6742:
6673:
6622:
6572:
6508:
6464:
6416:
6351:
6109:
6097:
6041:
5985:
5963:
5920:
5898:
5861:
5802:
5734:
5679:
5658:"The number and location of Jupiter's circumpolar cyclones explained by vorticity dynamics"
5609:
5515:
5452:
5397:
5376:"The number and location of Jupiter's circumpolar cyclones explained by vorticity dynamics"
5320:
5265:
5211:
4872:
4751:
3788:
3715:
3693:
3644:
3581:
3542:
3477:
3368:
3305:
3283:
3222:
2823:
2742:
2673:
2248:
2014:) was recorded—the first detection of either in Jupiter, and only the second detection of S
1765:
1759:
894:
710:
704:
362:
322:
130:
122:
51:
6798:(February 2003). "ISO observations of the giant planets and Titan: what have we learnt?".
3570:"Moist convection as an energy source for the large-scale motions in Jupiter's atmosphere"
2112:
8:
9326:
9252:
9192:
9185:
9092:
9062:
9022:
8896:
8500:
7945:
7891:
3766:
3172:
2199:
2117:
2019:
1976:
spacecraft. The first truly detailed images of Jupiter's atmosphere were provided by the
1941:
1872:
1819:
1608:
1288:
1187:
This image from the HST reveals a rare wave structure just north of the planet's equator.
1111:
The North North Temperate Region rarely shows more detail than the polar regions, due to
1013:
rather than in a radial direction (toward the center of the planet), consistent with the
281:
265:
Since the lower boundary of the atmosphere is ill-defined, the pressure level of 10
259:
9295:
8420:
8382:
8336:
8280:
8244:
8208:
8170:
8124:
8092:
8048:
8012:
7981:"Researcher predicts global climate change on Jupiter as giant planet's spots disappear"
7832:
7799:
7748:
7717:
7676:
7641:
7618:
7588:
7558:
7453:
7414:
7369:
7332:
7311:
7280:
7231:
7169:
7054:
7003:
6911:
6878:
6847:
6827:
Fletcher, Leigh N.; Orton, G.S.; Mousis, O.; Yanamandra-Fisher, P.; et al. (2010).
6779:
6746:
6626:
6512:
6355:
6113:
6045:
5989:
5924:
5865:
5806:
5738:
5683:
5613:
5519:
5503:
5456:
5401:
5324:
5269:
5215:
4755:
3792:
3719:
3648:
3585:
3546:
3481:
3372:
3309:
3226:
2827:
2746:
2677:
1442:
280:
The vertical temperature gradients in the Jovian atmosphere are similar to those of the
30:
9399:
9199:
9151:
9057:
9035:
8584:
8536:
8488:
8060:
7844:
7768:
7389:
7344:
7253:
7074:
7037:"Simulation of equatorial and high-latitude jets on Jupiter in a deep convection model"
7023:
6976:
6950:
6923:
6897:
6646:
6542:
6374:
6339:
6067:
6009:
5975:
5944:
5910:
5879:
5846:
Rogers, John; Eichstädt, Gerald; Hansen, Candice; Orton, Glenn; Momary, Thomas (2021).
5828:
5765:
5722:
5721:
Li, Cheng; Ingersoll, Andrew P.; Klipfel, Alexandra P.; Brettle, Harriet (2020-09-08).
5703:
5669:
5578:
5527:
5484:
5421:
5387:
5356:
5289:
5237:
5112:
3812:
3778:
3747:
3705:
3668:
3613:
3506:
3467:
3337:
3295:
3264:
2855:
2813:
2774:
2705:
2357:
2222:
2102:
1815:
1691:
1662:
1522:
1431:
in the southern); anticyclones rotate in the reverse direction. However, unlike in the
906:
746:
718:
370:
346:
59:
9315:
8132:
8020:
6972:
6819:
6476:
6428:
925:
considered the terrestrial value for the ratio of nitrogen isotopes to be primordial.
230:
The atmosphere of Jupiter is classified into four layers, by increasing altitude: the
9277:
8878:
8442:
8136:
7967:
7957:
7933:
7923:
7840:
7760:
7735:
7690:
7537:
7524:
7514:
7491:
7461:
7426:
7422:
7381:
7348:
7245:
7218:
7198:
7133:
7105:
7095:
7066:
7015:
6990:
6927:
6787:
6715:
6705:
6701:
6664:
6638:
6613:
6598:
6534:
6480:
6440:
6432:
6379:
6133:
6125:
6071:
6059:
6013:
6001:
5948:
5936:
5883:
5832:
5820:
5770:
5752:
5707:
5695:
5657:
5635:
5570:
5531:
5476:
5468:
5425:
5413:
5375:
5360:
5348:
5293:
5281:
5241:
5229:
4456:
3804:
3751:
3739:
3672:
3660:
3632:
3605:
3597:
3511:
3493:
3436:
3426:
3380:
3341:
3329:
3256:
3248:
2859:
2847:
2778:
2766:
2758:
2697:
2689:
2232:
2212:
1924:
1496:
1479:
1458:
1049:
1006:
751:
199:
9320:
8064:
7848:
7772:
7659:"Depth of the strong Jovian jet from a planetary scale disturbance driven by storms"
7393:
7257:
7027:
6980:
6650:
6546:
5964:"The Oscillatory Motion of Jupiter's Polar Cyclones Results From Vorticity Dynamics"
5899:"The Oscillatory Motion of Jupiter's Polar Cyclones Results From Vorticity Dynamics"
5059:
4602:
3118:
2730:
2709:
1998:
gave a glimpse of the Jupiter's composition beneath the cloud tops. The presence of
1541:
The GRS rotates counter-clockwise, with a period of about six Earth days or 14
1398:
893:
Earth- and spacecraft-based measurements have led to improved knowledge of the
353:
emissions. Within it lie layers of increased electron and ion density that form the
226:
stopped transmitting at a depth of 132 km below the 1 bar "surface" of Jupiter.
35:
9429:
9367:
9290:
9080:
8646:
8617:
8550:
8476:
8424:
8386:
8350:
8284:
8248:
8212:
8174:
8128:
8096:
8052:
8016:
7836:
7803:
7752:
7721:
7680:
7663:
7645:
7628:
7465:
7457:
7440:
7418:
7373:
7336:
7284:
7235:
7173:
7078:
7058:
7041:
7007:
6968:
6915:
6888:
6851:
6815:
6783:
6766:
6750:
6681:
6630:
6590:
6524:
6516:
6472:
6424:
6369:
6359:
6117:
6049:
5993:
5928:
5869:
5810:
5760:
5742:
5687:
5625:
5617:
5582:
5562:
5523:
5488:
5460:
5405:
5338:
5328:
5309:"First Estimate of Wind Fields in the Jupiter Polar Regions From JIRAM-Juno Images"
5273:
5219:
4759:
3816:
3796:
3731:
3723:
3652:
3617:
3589:
3550:
3501:
3485:
3454:
Fletcher, Leigh N.; Kaspi, Yohai; Guillot, Tristan; Showman, Adam P. (2020-03-12).
3376:
3321:
3313:
3268:
3238:
3230:
2839:
2831:
2750:
2681:
2151:
The white ovals that were to become Oval BA formed in 1939. They covered almost 90
2087:
2031:
2007:
1827:
1530:
1424:
1156:
1053:
771:
309:
98:
abundances in Jupiter's atmosphere exceed solar values by a factor of about three.
79:
8507:
7950:
7011:
5550:
3456:"How Well Do We Understand the Belt/Zone Circulation of Giant Planet Atmospheres?"
1470:
to the poles. They are usually bright and appear as white ovals. They can move in
1009:. The direction at which the jets extend into the planet is parallel to Jupiter's
874:
and water present in the upper atmosphere are thought to originate from impacting
9389:
8951:
8923:
8902:
8740:
8730:
8709:
8704:
8671:
8666:
7756:
6855:
6554:
Atreya, Sushil K.; Wong, Ah-San; Baines, K. H.; Wong, M. H.; Owen, T. C. (2005).
6494:"Coupled Clouds and Chemistry of the Giant Planets — A Case for Multiprobes"
6121:
5566:
5277:
4763:
4729:
3554:
2726:
2685:
2144:
1999:
1978:
1961:
1771:
1671:
1617:
1594:
1337:
871:
293:
215:
9353:
9310:
8402:"Equatorial Superrotation and Barotropic Instability: Static Stability Variants"
2400:
2064:
741:
relative to molecular hydrogen by number of molecules, and its mass fraction is
8990:
8797:
8755:
8686:
8605:
8524:
8512:
7484:
5691:
5409:
4316:
3976:
2152:
2043:
1508:
1483:
1116:
1112:
867:
863:
366:
262:
when the temperature is above 33 K and the pressure is above 13 bar.
9259:
8449:
7340:
6594:
6520:
3656:
3489:
2754:
1857:
1324:
9423:
8725:
8699:
7528:
7430:
6764:
Busse, F.H. (1976). "A simple model of convection in the Jovian atmosphere".
6719:
6602:
6538:
6484:
6436:
6338:
Cheng Li; Andrew P. Ingersoll; Alexandra P. Klipfel; Harriet Brettle (2020).
6129:
6063:
6005:
5940:
5824:
5756:
5699:
5639:
5574:
5535:
5472:
5440:
5417:
5352:
5285:
5233:
3808:
3743:
3664:
3601:
3497:
3440:
3333:
3252:
3210:
2851:
2762:
2693:
2226:
2050:
1983:
1885:
1581:
1373:
1300:
1123:
1018:
986:
692:
220:
9227:
7937:
7918:(1999). Beatty, Kelly J.; Peterson, Carolyn Collins; Chaiki, Andrew (eds.).
7470:
7377:
7240:
7213:
7109:
7036:
6919:
6634:
6364:
5747:
5598:"Polar vortex formation in giant-planet atmospheres due to moist convection"
3455:
2462:
2460:
2458:
2456:
2454:
2452:
2450:
1794:
9238:
8917:
8745:
8735:
8676:
8661:
7971:
7764:
7694:
7649:
7249:
7070:
7019:
6642:
6444:
6383:
6137:
5774:
5480:
3609:
3515:
3260:
2802:"Possible Transient Luminous Events Observed in Jupiter's Upper Atmosphere"
2770:
2701:
2448:
2446:
2444:
2442:
2440:
2438:
2436:
2434:
2432:
2430:
2353:
2306:
2098:
2094:
2093:
A minor mystery concerns a Jovian spot depicted around 1700 on a canvas by
2083:
1742:
1403:
1258:. The interior of Jupiter is fluid and lacks any solid surface. Therefore,
1022:
887:
688:
358:
239:
235:
114:
110:
55:
9213:
7385:
7187:
Giant Planets of Our Solar System. Atmospheres, Composition, and Structure
5343:
5178:
3977:"Hubble's planetary portrait captures changes in Jupiter's Great Red Spot"
3800:
3735:
3569:
3325:
1423:. Cyclones rotate in the direction similar to the rotation of the planet (
8750:
7265:
Low, F.J. (1966). "Observations of Venus, Jupiter, and Saturn at λ20 μ".
6955:
6755:
6728:
6529:
6054:
6029:
5997:
5932:
5815:
5790:
5630:
5333:
5308:
5224:
5199:
3727:
3317:
3243:
2835:
1450:
1420:
1292:
1284:
1276:
1087:
1083:
1078:
1074:
1070:
1045:
1037:
1028:
1002:
914:
910:
855:
843:
601:
597:
231:
190:
178:
106:
70:; other chemical compounds are present only in small amounts and include
8391:
7685:
7658:
7062:
5874:
5464:
3234:
2972:
2970:
2968:
2427:
1726:
Lightning on Jupiter's night side, imaged by the Galileo orbiter in 1997
981:
The Jovian bands are bounded by zonal atmospheric flows (winds), called
9134:
8936:
8929:
8226:"Jovian Dynamics.Part II: The genesis and equilibration of vortex sets"
7897:. In Bagenal, Fran.; Dowling, Timothy E.; McKinnon, William B. (eds.).
6098:"A Production of Amino Acids Under Possible Primitive Earth Conditions"
3211:"Jupiter's atmospheric jet streams extend thousands of kilometres deep"
3092:
3090:
2843:
2161:
1972:
1966:
1920:
1670:
Oval BA slowly began to turn red in August 2005. On February 24, 2006,
1577:
1492:
1317:
1280:
1259:
1139:
1126:
994:
982:
971:
886:
acts like a cold trap, effectively preventing water from rising to the
883:
672:
534:
354:
289:
285:
266:
251:
8519:
8428:
8179:
7863:. In Bagenal, Fran; Dowling, Timothy E.; McKinnon, William B. (eds.).
7725:
7124:. In Bagenal, Fran; Dowling, Timothy E.; McKinnon, William B. (eds.).
5597:
4421:"The Solar System – The Planet Jupiter – The Great Red Spot"
4249:
2987:
2985:
1822:. The polar cyclone (the central cyclone in the polygons) also emit a
1549:
1183:
1098:
9344:
9028:
9008:
8964:
8957:
8694:
8262:"Jovian Dynamics, Part III: Multiple, migrating, and equatorial jets"
8056:
5621:
5596:
O'Neill, Morgan E; Emanuel, Kerry A.; Flierl, Glenn R. (2015-06-15).
3593:
2965:
2257:
2253:
2156:
2126:
2070:
1947:
1903:
1899:
1823:
1754:
1722:
1683:
1622:
1588:
1471:
1428:
1355:
1041:
1040:. The simplest interpretation is that zones are sites of atmospheric
898:
897:
in Jupiter's atmosphere. As of July 2003, the accepted value for the
851:
822:
also appear in abundance relative to solar levels (see table), while
787:
668:
584:
580:
335:
243:
137:
and are bounded by powerful zonal atmospheric flows (winds) known as
118:
95:
67:
7117:
Ingersoll, A.P.; Dowling, T.E.; Gierasch, P.J.; et al. (2004).
6936:
3531:"Dynamical implications of Jupiter's tropospheric ammonia abundance"
3087:
2906:
2904:
2902:
2900:
2898:
2896:
1254:
Circulation in Jupiter's atmosphere is markedly different from that
8190:"Jovian Dynamics. Part I: Vortex stability, structure, and genesis"
7288:
5980:
5915:
5791:"Five Years of Observations of the Circumpolar Cyclones of Jupiter"
5674:
5392:
5254:
5200:"Five Years of Observations of the Circumpolar Cyclones of Jupiter"
3710:
3472:
3300:
2982:
2818:
2731:"Small lightning flashes from shallow electrical storms on Jupiter"
2172:
1831:
1654:
1564:
1529:
after observing the feature in July 1665 with his instrument-maker
1478:
has several large irregular filamentary patches, which demonstrate
1436:
1365:
1165:
958:
799:
655:
651:
621:
617:
500:
417:
87:
6902:
3783:
8573:
7487:
5060:"The collision of the Little Red Spot and Great Red Spot: Part 2"
3567:
2893:
2379:
2131:
extraordinarily complex and variable cloud motions are observed.
2023:
1847:
1735:
1613:
1542:
1467:
1416:
998:
954:
933:
835:
815:
779:
763:
638:
634:
458:
342:
174:
134:
102:
75:
71:
7998:
7657:
Sanchez-Lavega, A.; Orton, G.S.; Hueso, S.; et al. (2008).
9171:
7212:
Kunde, V.G.; Flasar, F.M.; Jennings, D.E.; et al. (2004).
5108:"NASA's Jupiter Mission Reveals the "Brand-New and Unexpected""
3284:"Constraints on the Latitudinal Profile of Jupiter's Deep Jets"
2798:
2068:
A narrower view of Jupiter and the Great Red Spot as seen from
2039:
1412:
975:
967:
847:
827:
807:
803:
795:
734:
548:
517:
486:
413:
270:
91:
63:
9103:
7856:
West, R.A.; Baines, K.H.; Friedson, A.J.; et al. (2004).
4365:
Harrington, J.D.; Weaver, Donna; Villard, Ray (May 15, 2014).
2662:
882:. The water cannot come from the troposphere because the cold
6451:
4977:"On Jupiter, a Battle of the Red Spots, With the Baby Losing"
2466:
2168:
2139:
1843:
1703:
1643:
of three small white storms, and has intensified since then.
1568:
1169:
875:
819:
811:
759:
472:
444:
350:
83:
3208:
3173:"Helium rain on Jupiter explains lack of neon in atmosphere"
1634:
1576:
flybys. The spot is spatially confined by a modest eastward
9142:
8253:
10.1175/1520-0469(2002)059<1356:JDPITG>2.0.CO;2
8217:
10.1175/1520-0469(1996)053<2685:JDPVSS>2.0.CO;2
8119:. Advances in Geophysics. Vol. 28A. pp. 381–429.
8101:
10.1175/1520-0469(1978)035<1399:PCBROJ>2.0.CO;2
7922:(4th ed.). Massachusetts: Sky Publishing Corporation.
4371:
3633:"MWR: Microwave Radiometer for the Juno Mission to Jupiter"
3453:
2725:
941:
of Jupiter's atmosphere centered about Jupiter's south pole
858:, which form from methane under the influence of the solar
823:
430:
8542:
8355:
10.1175/1520-0469(2003)060<2136:BIAES>2.0.CO;2
8289:
10.1175/1520-0469(2003)60<1270:JDPIMM>2.0.CO;2
7917:
7809:
10.1175/1520-0469(1974)031<1471:OJROR>2.0.CO;2
7598:"The accelerating circulation of Jupiter's Great Red Spot"
7178:
10.1175/1520-0469(1969)026<0981:DOJCB>2.0.CO;2
6609:
6030:"Oscillations and Stability of the Jupiter Polar Cyclones"
5845:
5184:
5149:
5147:
5145:
5004:. Johns Hopkins Applied Physics Laboratory. Archived from
207:
has also been observed 260 km above the 1 bar level.
145:. The bands alternate in color: the dark bands are called
6553:
6026:
5720:
5306:
3425:(4th ed.). Burlington, MA: Elsevier Academic Press.
2976:
2143:
The white ovals that later formed Oval BA, imaged by the
1898:
The origin of hot spots is not clear. They can be either
1757:. The imaging of the night–side hemisphere of Jupiter by
1495:(or convective columns) is not shared by the majority of
758:
The atmosphere contains various simple compounds such as
5787:
5595:
5196:
4948:"Diffusion Caused Jupiter's Red Spot Junior To Color Up"
4924:"Gemini Captures Close Encounter of Jupiter's Red Spots"
3630:
3281:
1517:
The Great Red Spot is decreasing in size (May 15, 2014).
1482:. One of them is located to the west of the GRS (in its
917:, is 2.3 × 10, a third lower than that in the
905:, which probably represents the primordial value in the
810:
by a factor of 2–4 relative to the Sun. The noble gases
6400:
5142:
4817:
4815:
4364:
3690:
3357:"A simple model of convection in the Jovian atmosphere"
3139:
3137:
3135:
2991:
717:
The two main constituents of the Jovian atmosphere are
7088:
Galileo's Planet: Observing Jupiter Before Photography
5438:
8460:
8448:(2017-05-09) by Peter Rosén describing assembly of a
8318:"Barotropic instability and equatorial superrotation"
8152:"Planetary vortices and Jupiter's vertical structure"
7956:(Revised ed.). London: Faber and Faber Limited.
7318:
6937:"A comparison of the interiors of Jupiter and Saturn"
2910:
2518:
1196:
nature and are not always visible. These include the
8110:"Jovian and Comparative Atmospheric Modeling Gareth"
7400:
5849:"Behaviour of Jupiter's polar polygons over 4 years"
4812:
4255:
3694:"Evidence for Multiple Ferrel-Like Cells on Jupiter"
3132:
2316:
is the average molar mass in the Jovian atmosphere,
2189:
1706:—approximately half the size of the Great Red Spot.
8399:
8361:
8315:
8295:
8259:
8223:
8187:
8149:
8107:
8071:
8027:
6556:"Jupiter's ammonia clouds—localized or ubiquitous?"
4723:
Jupiter's Red Spot is Likely a Sunburn, Not a Blush
2046:were not detected, to the surprise of astronomers.
7949:
5847:
3767:"Mechanisms of Jet Formation on the Giant Planets"
745:, which is slightly lower than the Solar System's
7899:Jupiter: The Planet, Satellites and Magnetosphere
7865:Jupiter: The Planet, Satellites and Magnetosphere
7126:Jupiter: The Planet, Satellites and Magnetosphere
6726:
5441:"Clusters of cyclones encircling Jupiter's poles"
5026:
4216:
4214:
4212:
3096:
1411:The atmosphere of Jupiter is home to hundreds of
277:approximately 5,000 km above the "surface".
9421:
7568:"Jupiter in 1999/2000. II: Infrared wavelengths"
5168:
5166:
5132:
5130:
2225:(a mission that included both an orbiter and an
8305:Bulletin of the American Meteorological Society
7606:Journal of the British Astronomical Association
7576:Journal of the British Astronomical Association
7546:Journal of the British Astronomical Association
7299:Journal of the British Astronomical Association
5727:Proceedings of the National Academy of Sciences
5057:
5002:"Storm Winds Blow in Jupiter's Little Red Spot"
4621:
4619:
4299:
4297:
4295:
4293:
4291:
4278:
4276:
4152:
4150:
4113:
4111:
4109:
4107:
4105:
4103:
4056:
4054:
3889:
3887:
3885:
3883:
3881:
3528:
3420:
3021:
3019:
2646:
2644:
2642:
2640:
2627:
2625:
2623:
2621:
2608:
2606:
2604:
1060:
8371:Journal of the Meteorological Society of Japan
6727:Bhardwaj, Anil; Gladstone, G. Randall (2000).
5555:Geophysical & Astrophysical Fluid Dynamics
5053:
5051:
5049:
4866:
4209:
4071:
4069:
3941:
2591:
2589:
2587:
2585:
2572:
2570:
2568:
2120:took the GRS region at its smallest size ever.
1032:Zonal wind speeds in the atmosphere of Jupiter
9119:
8558:
6866:Bulletin of the American Astronomical Society
6197:
6195:
5854:European Planetary Science Congress Abstracts
5656:Gavriel, Nimrod; Kaspi, Yohai (August 2021).
5374:Gavriel, Nimrod; Kaspi, Yohai (August 2021).
5163:
5127:
5099:
4741:
4358:
4084:
3392:
3390:
3050:
3048:
3046:
3044:
3042:
3040:
3038:
3036:
3034:
2940:
2938:
2936:
2923:
2921:
2919:
2871:
2869:
2555:
2553:
2481:
2479:
2477:
2475:
1753:Storms on Jupiter are always associated with
826:is scarcer. Other chemical compounds such as
27:Layer of gases surrounding the planet Jupiter
6180:
6144:
5962:Gavriel, Nimrod; Kaspi, Yohai (2022-08-16).
5961:
5897:Gavriel, Nimrod; Kaspi, Yohai (2022-08-16).
5896:
5655:
5373:
5029:"Jupiter's Little Red Spot Growing Stronger"
4616:
4346:
4288:
4273:
4226:
4186:
4174:
4162:
4147:
4100:
4051:
3878:
3765:Liu, Junjun; Schneider, Tapio (2010-11-01).
3764:
3016:
2637:
2618:
2601:
2551:
2549:
2547:
2545:
2543:
2541:
2539:
2537:
2535:
2533:
8117:Jovian and comparative atmospheric modeling
7952:The Planet Jupiter: The Observer's Handbook
7035:Heimpel, M.; Aurnou, J.; Wicht, J. (2005).
6243:
6241:
6212:
6210:
5046:
4999:
4970:
4968:
4735:
4066:
3164:
3115:Harvard-Smithsonian Center for Astrophysics
2582:
2565:
2505:
2503:
2501:
2499:
2497:
2495:
2493:
2401:"Hubble takes close-up portrait of Jupiter"
1956:entered in use later, in the 20th century.
1861:False color image of an equatorial hot spot
1658:Formation of Oval BA from three white ovals
1612:spacecraft. A feature in the atmosphere of
9126:
9112:
8565:
8551:
7481:Norton's Star Atlas and Reference Handbook
6491:
6192:
5551:"Polar accumulation of cyclonic vorticity"
4942:
4940:
4694:
4692:
4261:
4135:
4123:
4029:
4014:
3844:
3842:
3840:
3838:
3387:
3192:
3190:
3031:
2933:
2916:
2866:
2524:
2472:
1909:
1826:field which can repel other cyclones (see
1557:According to a study by scientists at the
1439:centers, while cyclones are low pressure.
395:Elemental abundances relative to hydrogen
9435:Planetary atmospheres of the Solar System
8390:
8344:
8178:
7807:
7684:
7469:
7239:
6954:
6901:
6754:
6584:
6528:
6373:
6363:
6156:
6053:
5979:
5914:
5873:
5814:
5764:
5746:
5673:
5629:
5391:
5342:
5332:
5223:
4455:. Cambridge University Press. p. 6.
4418:
4198:
3782:
3709:
3529:Showman, Adam P.; de Pater, Imke (2005).
3505:
3471:
3299:
3242:
3149:
3065:
3063:
3002:
3000:
2955:
2953:
2817:
2530:
2059:
1945:Time-lapse sequence from the approach of
1712:University of California, at Berkeley, US
1521:The Great Red Spot (GRS) is a persistent
1204:(NEBZ, a white zone within the belt) and
6794:
6729:"Auroral emissions of the giant planets"
6492:Atreya, Sushil K.; Wong, Ah-San (2005).
6238:
6207:
5795:Journal of Geophysical Research: Planets
5313:Journal of Geophysical Research: Planets
5204:Journal of Geophysical Research: Planets
4974:
4965:
4895:
4891:
4889:
4776:
4497:
3143:
3108:
2806:Journal of Geophysical Research: Planets
2490:
2138:
2111:
2063:
2022:— together with other molecules such as
1940:
1930:
1856:
1793:
1729:
1721:
1661:
1653:
1633:
1593:
1548:
1512:
1449:
1441:
1397:
1323:
1182:
1149:
1097:
1027:
932:
928:
714:orbiters, and Earth-based observations.
691:because it was observed directly by the
214:
155:
29:
7892:"Jupiter's Thermosphere and Ionosphere"
4937:
4921:
4689:
4529:"Jupiter's Great Red Spot Is Shrinking"
4423:. Dept. Physics & Astronomy –
4317:"Great Cold Spot discovered on Jupiter"
3835:
3187:
3170:
1789:
1717:
388:
14:
9422:
6095:
5651:
5649:
5027:Steigerwald, Bill (October 10, 2006).
4954:from the original on 30 September 2008
4847:
4845:
4711:Is Jupiter's Great Red Spot a Sunburn?
4600:
4448:
3423:An introduction to dynamic meteorology
3075:
3060:
2997:
2950:
2881:
1871:until 1939, having been first seen by
1044:, whereas belts are manifestations of
526:0.033 ± 0.015 (12 bar)
9107:
8546:
7147:Ingersoll, A.P.; Cuzzi, J.N. (1969).
5548:
5105:
5079:
4886:
4526:
4395:"Jupiter Data Sheet – SPACE.com"
4392:
3686:
3684:
3682:
3354:
2721:
2719:
1814:in a vortex, under the change of the
1741:The storms on Jupiter are similar to
1381:on Earth, on Jupiter deep convection
1362:, whereas the total emitted power is
1328:Thermal image of Jupiter obtained by
1316:. It holds that in any fast-rotating
680:2.25 ± 0.35 × 10
663:1.66 ± 0.05 × 10
210:
7978:
7944:
5501:
5035:from the original on 1 November 2008
4950:. ScienceDaily. September 26, 2008.
1388:
511:3.2 ± 1.4 (9–12 bar)
8409:Journal of the Atmospheric Sciences
8325:Journal of the Atmospheric Sciences
8269:Journal of the Atmospheric Sciences
8233:Journal of the Atmospheric Sciences
8197:Journal of the Atmospheric Sciences
8081:Journal of the Atmospheric Sciences
8030:"Jupiter's atmospheric circulation"
7787:Journal of the Atmospheric Sciences
7157:Journal of the Atmospheric Sciences
7149:"Dynamics of Jupiter's cloud bands"
6315:. 17 September 2020. Archived from
5646:
4842:
4238:
3771:Journal of the Atmospheric Sciences
2079:
677:3.0 ± 0.17 × 10
609:2.3 ± 0.3 × 10
564:Isotopic ratios in Jupiter and Sun
182:
24:
7911:
7536:Rogers, J.H.; Metig, H.J. (2001).
7146:
7119:"Dynamics of Jupiter's Atmosphere"
5528:10.1111/j.2153-3490.1956.tb01234.x
5082:"Third red spot erupts on Jupiter"
5062:. British Astronomical Association
5058:Rogers, John H. (August 8, 2008).
4605:. British Astronomical Association
4535:from the original on 11 March 2009
4091:
3679:
3111:"Jonathan's Space Report, No. 267"
2716:
2467:Atreya Mahaffy Niemann et al. 2003
2375:California Institute of Technology
2363:
2346:
2332:
2270:
1830:) similar to the beta-effect. The
1559:University of California, Berkeley
862:and charged particles coming from
660:1.5 ± 0.3 × 10
25:
9446:
8436:
6826:
6096:Miller, Stanley L. (1953-05-15).
4975:Fountain, Henry (July 22, 2008).
4781:. Science at NASA. Archived from
4777:Phillips, Tony (March 12, 2003).
4625:
3171:Sanders, Robert (22 March 2010).
3109:McDowell, Jonathan (1995-12-08).
1502:
1270:
1093:
509:3.6 ± 0.5 (8 bar)
141:exhibiting a phenomenon known as
121:. Each layer has characteristic
9161:
9086:
9076:
9075:
8636:
8530:
8518:
8506:
8494:
8482:
8470:
7987:from the original on 9 June 2007
7890:Yelle, R.V.; Miller, S. (2004).
7656:
7625:
7595:
7034:
6393:
6331:
6309:"A New View of Jupiter's Storms"
6301:
6289:
6277:
6265:
6253:
6222:
6186:
6168:
6089:
6078:
6020:
5955:
5890:
5839:
5781:
5714:
5589:
5542:
5495:
5432:
5367:
5300:
5248:
5190:
5153:
5088:from the original on 5 July 2008
5073:
5020:
4993:
4922:Michaud, Peter (July 20, 2006).
4915:
4867:Phillips, Tony (March 3, 2006).
4860:
4830:
4821:
4796:
4770:
4716:
4704:
4677:
4665:
4654:
4527:Britt, Robert Roy (2009-03-09).
4431:from the original on 7 June 2008
4401:from the original on 11 May 2008
4075:
2192:
1648:
1620:. The latter feature, imaged by
1344:
1330:NASA Infrared Telescope Facility
1240:
1228:
890:(see Vertical structure above).
332:polycyclic aromatic hydrocarbons
34:Jupiter's swirling clouds, in a
9133:
8159:Journal of Geophysical Research
7782:"On Jupiter's Rate of Rotation"
7705:Journal of Geophysical Research
7565:
7535:
7092:Institute of Physics Publishing
7085:
6216:
5185:Baines Simon-Miller et al. 2007
5106:Chang, Kenneth (May 25, 2017).
4896:Phillips, Tony (June 5, 2006).
4642:
4631:
4594:
4582:
4570:
4558:
4546:
4520:
4509:
4481:
4469:
4442:
4412:
4386:
4334:
4309:
4040:
4035:
4020:
4002:
3990:
3969:
3957:
3935:
3923:
3911:
3899:
3866:
3854:
3823:
3758:
3624:
3561:
3522:
3447:
3414:
3402:
3348:
3275:
3202:
3102:
2792:
2656:
2124:On February 25, 1979, when the
1994:studies after the collision of
1865:
1427:in the northern hemisphere and
1407:IR view of Jupiter's atmosphere
1159:getting into the field of view.
755:them towards the core as well.
8783:Jupiter-crossing minor planets
7979:Yang, Sarah (April 21, 2004).
7820:Reports on Progress in Physics
7184:
7116:
6660:"Jupiter's Shrinking Red Spot"
6150:
4900:. Science@NASA. Archived from
4503:
4267:
4141:
4129:
3396:
3054:
2977:Atreya Wong Baines et al. 2005
2944:
2927:
2875:
2559:
2393:
2364:
2347:
2333:
2271:
2134:
1902:, where the descending air is
1307:
149:, while light ones are called
13:
1:
8133:10.1016/S0065-2687(08)60231-9
8021:10.1016/S0019-1035(02)00060-X
7816:
7355:
7012:10.1126/science.268.5218.1740
6973:10.1016/S0032-0633(99)00043-4
6820:10.1016/S0032-0633(02)00145-9
6477:10.1016/S0032-0633(02)00144-7
6429:10.1016/S0032-0633(99)00047-1
6162:
5172:
5136:
5080:Shiga, David (May 22, 2008).
5031:. NASA Goddard Space Center.
4601:Rogers, John (30 July 2006).
4419:Anonymous (August 10, 2000).
4352:
4340:
4303:
4282:
4232:
4220:
4192:
4180:
4168:
4156:
4117:
4060:
3893:
3421:James R. Holton, ed. (2004).
3097:Bhardwaj & Gladstone 2000
3025:
2650:
2631:
2612:
2595:
2576:
2387:
8400:Williams, Gareth P. (2006).
8362:Williams, Gareth P. (2003).
8316:Williams, Gareth P. (2003).
8296:Williams, Gareth P. (2003).
8260:Williams, Gareth P. (2003).
8224:Williams, Gareth P. (2002).
8188:Williams, Gareth P. (1996).
8150:Williams, Gareth P. (1997).
8108:Williams, Gareth P. (1985).
8072:Williams, Gareth P. (1978).
8028:Williams, Gareth P. (1975).
7757:10.1126/science.204.4396.951
7478:
7462:10.1016/0019-1035(66)90036-4
7423:10.1016/0019-1035(90)90155-3
6934:
6856:10.1016/j.icarus.2010.01.005
6788:10.1016/0019-1035(76)90053-1
6700:(2nd ed.). Washington:
6122:10.1126/science.117.3046.528
6034:Geophysical Research Letters
5968:Geophysical Research Letters
5903:Geophysical Research Letters
5567:10.1080/03091929.2010.509927
5502:ADEM, JULIÁN (August 1956).
5278:10.1016/j.icarus.2019.113405
5000:Buckley, M. (May 20, 2008).
4764:10.1016/j.icarus.2017.10.041
4449:Rogers, John Hubert (1995).
4046:
3999:, pp. 219–221, 223, 228–229.
3698:Geophysical Research Letters
3555:10.1016/j.icarus.2004.10.004
3381:10.1016/0019-1035(76)90053-1
3288:Geophysical Research Letters
2992:Atreya Wong Owen et al. 1999
2686:10.1126/science.204.4396.951
2485:
2097:, which is exhibited in the
1878:
1798:JIRAM image of southern CPCs
1782:detected many more in 2018.
1734:Jupiter – southern storms –
1533:. According to a report by
1066:Meridional circulation cells
1061:Meridional circulation cells
903:(2.25 ± 0.35) × 10
186:
7:
9395:Extraterrestrial atmosphere
8572:
7504:
6987:
6942:Planetary and Space Science
6885:
6800:Planetary and Space Science
6657:
6564:Planetary and Space Science
6456:Planetary and Space Science
6408:Planetary and Space Science
6283:
6271:
6259:
6247:
6201:
6174:
4836:
4802:
4732:NASA.com, November 11, 2014
4683:
4671:
4648:
4588:
4564:
4552:
4515:
4475:
4008:
3996:
3963:
3944:"Jupiter, It Is A-Changing"
3917:
3905:
3872:
3860:
3848:
3829:
3408:
3196:
2185:
2042:-bearing molecules such as
1688:Goddard Space Flight Center
1491:that the vortices are deep
1393:
1219:
205:Upper-atmospheric lightning
10:
9451:
8984:Jupiter Icy Moons Explorer
7903:Cambridge University Press
7889:
7869:Cambridge University Press
7841:10.1088/0034-4885/68/8/R06
7779:
7743:(4396): 951–957, 960–972.
7732:
7701:
7511:Cambridge University Press
7437:
7295:
7211:
7130:Cambridge University Press
6763:
6695:
6295:
6228:
6084:
5692:10.1038/s41561-021-00781-6
5549:Scott, R.K. (2010-09-15).
5410:10.1038/s41561-021-00781-6
4713:NASA.com November 28, 2014
4698:
4660:
4637:
4576:
4487:
4204:
3929:
3155:
3081:
3069:
2959:
2911:Miller Aylward et al. 2005
2887:
2509:
2078:The first sighting of the
1934:
1629:
1535:Giovanni Battista Riccioli
1506:
1446:Great Cold Spot on Jupiter
1256:in the atmosphere of Earth
1206:South Equatorial belt zone
1202:North Equatorial belt zone
737:. The helium abundance is
700:Infrared Space Observatory
592:0.0108 ± 0.0005
143:atmospheric super-rotation
9408:
9377:
9343:
9276:
9237:
9170:
9159:
9141:
9071:
9050:
9001:
8976:
8888:
8870:
8856:
8844:2016 Jupiter impact event
8839:2010 Jupiter impact event
8834:2009 Jupiter impact event
8819:
8796:
8775:
8768:
8718:
8685:
8654:
8645:
8634:
8593:
8580:
7855:
7483:(19th ed.). Harlow:
7341:10.1007/s11214-005-1960-4
7090:. Bristol, Philadelphia:
6595:10.1016/j.pss.2004.04.002
6521:10.1007/s11214-005-1951-5
4256:Pearl Conrath et al. 1990
3657:10.1007/s11214-017-0349-5
3490:10.1007/s11214-019-0631-9
3006:
2755:10.1038/s41586-020-2532-1
2244:2010 Jupiter impact event
2239:2009 Jupiter impact event
18:Jupiter's atmosphere
7858:"Jovian Clouds and Haze"
7507:The Giant Planet Jupiter
7264:
6698:Jupiter the Giant Planet
4869:"Jupiter's New Red Spot"
4452:The Giant Planet Jupiter
4244:
3175:. University of Berkeley
2263:
939:stereographic projection
528:0.19–0.58 (19 bar)
9093:Solar System portal
7378:10.1126/science.7871428
7241:10.1126/science.1100240
6965:1999P&SS...47.1183G
6920:10.1515/astro-2017-0425
6862:
6812:2003P&SS...51...89E
6678:2002S&T...103d..24B
6635:10.1126/science.1147912
6577:2005P&SS...53..498A
6469:2003P&SS...51..105A
6421:1999P&SS...47.1243A
6365:10.1073/pnas.2008440117
5748:10.1073/pnas.2008440117
4851:
4701:, pp. 38–41.
4638:Reese and Gordon (1966)
4425:University of Tennessee
4036:Rogers and Metig (2001)
3942:Nancy Atkinson (2010).
2227:atmospheric-entry probe
2171:(they became faster at
1910:The possibility of life
1314:Taylor–Proudman theorem
1291:of the Rossby waves is
1015:Taylor-Proudman theorem
1001:, while in zones it is
864:Jupiter's magnetosphere
425:0.807 ± 0.02
58:. It is mostly made of
8829:Comet Shoemaker–Levy 9
7650:10.1006/icar.2000.6548
4898:"Huge Storms Converge"
4871:. NASA. Archived from
2525:Atreya & Wong 2005
2371:Hubble Space Telescope
2268:
2208:Comet Shoemaker–Levy 9
2148:
2121:
2075:
2060:Great Red Spot studies
1996:Comet Shoemaker–Levy 9
1952:
1937:Exploration of Jupiter
1916:Miller–Urey experiment
1862:
1799:
1776:Microwave Radiometer (
1738:
1727:
1680:Hubble Space Telescope
1667:
1659:
1639:
1599:
1554:
1518:
1463:
1447:
1433:terrestrial atmosphere
1408:
1332:
1188:
1160:
1104:
1033:
942:
923:Solar System formation
643:13.81 ± 0.08
606:<2.8 × 10
439:0.10 ± 0.01
227:
170:
133:bands parallel to the
43:
40:Hubble Space Telescope
7596:Rogers, J.H. (2008).
7566:Rogers, J.H. (2003).
7505:Rogers, J.H. (1995).
7321:Space Science Reviews
6734:Reviews of Geophysics
6658:Beatty, J.K. (2002).
6501:Space Science Reviews
5139:, pp. 1982, 1985–1987
4779:"The Great Dark Spot"
3801:10.1175/2010JAS3492.1
3637:Space Science Reviews
3460:Space Science Reviews
2812:(11): e2020JE006659.
2142:
2115:
2082:is often credited to
2067:
1944:
1931:Observational history
1860:
1797:
1733:
1725:
1665:
1657:
1637:
1597:
1552:
1527:Gian Domenico Cassini
1516:
1453:
1445:
1401:
1327:
1186:
1153:
1101:
1031:
957:(EZ) extends between
936:
929:Zones, belts and jets
860:ultraviolet radiation
629:5.6 ± 0.25
626:5.77 ± 0.08
557:2.5 ± 0.15
302:ammonium hydrosulfide
275:interplanetary medium
218:
168:
127:ammonium hydrosulfide
123:temperature gradients
48:atmosphere of Jupiter
33:
9385:Prebiotic atmosphere
8628:Jupiter's South Pole
8623:Jupiter's North Pole
8298:"Super Circulations"
7983:. UC Berkeley News.
7920:The New Solar System
7780:Stone, P.H. (1974).
7712:(E10): 22857–22889.
7538:"Jupiter in 1998/99"
7479:Ridpath, I. (1998).
7268:Astronomical Journal
6949:(10–11): 1183–1200.
6935:Guillot, T. (1999).
6756:10.1029/1998RG000046
6415:(10–11): 1243–1262.
6055:10.1029/2021GL094235
5998:10.1029/2022GL098708
5933:10.1029/2022GL098708
5816:10.1029/2022JE007241
5334:10.1029/2018JE005555
5225:10.1029/2022JE007241
4926:. Gemini Observatory
4478:(2010), p. 266.
3728:10.1029/2021GL095651
3355:Busse, F.H. (1976).
3318:10.1029/2021GL092912
2836:10.1029/2020JE006659
2249:Ulysses (spacecraft)
1790:Circumpolar cyclones
1718:Storms and lightning
1694:without converging.
1616:was also called the
1497:planetary scientists
949:and relatively dark
611:(0.08–2.8 bar)
523:8.51 × 10
506:1.12 × 10
495:2.9 ± 0.5
481:2.6 ± 0.5
467:2.7 ± 0.5
453:2.5 ± 0.5
389:Chemical composition
363:Einstein Observatory
250:, Jupiter's lacks a
52:planetary atmosphere
9023:Io Volcano Observer
8421:2006JAtS...63.1548W
8392:10.2151/jmsj.81.439
8383:2003JMeSJ..81..439W
8337:2003JAtS...60.2136W
8281:2003JAtS...60.1270W
8245:2002JAtS...59.1356W
8209:1996JAtS...53.2685W
8171:1997JGR...102.9303W
8125:1985AdGeo..28..381W
8093:1978JAtS...35.1399W
8049:1975Natur.257..778W
8013:2003Icar..162...74Y
7833:2005RPPh...68.1935V
7800:1974JAtS...31.1471S
7749:1979Sci...204..951S
7718:1998JGR...10322857S
7686:10.1038/nature06533
7677:2008Natur.451..437S
7642:2001Icar..149..491S
7619:2008JBAA..118...14R
7589:2003JBAA..113..136R
7559:2001JBAA..111..321R
7454:1966Icar....5..266R
7415:1990Icar...84...12P
7370:1995Sci...267.1307N
7364:(5202): 1307–1313.
7333:2005SSRv..116..319M
7312:1997JBAA..107..239M
7281:1966AJ.....71R.391L
7232:2004Sci...305.1582K
7226:(5690): 1582–1586.
7170:1969JAtS...26..981I
7086:Hockey, T. (1999).
7063:10.1038/nature04208
7055:2005Natur.438..193H
7004:1995Sci...268.1740H
6998:(5218): 1740–1742.
6912:2010BaltA..19..265G
6879:2006DPS....38.1102G
6848:2010Icar..208..306F
6780:1976Icar...29..255B
6747:2000RvGeo..38..295B
6627:2007Sci...318..226B
6513:2005SSRv..116..121A
6356:2020PNAS..11724082L
6350:(39): 24082–24087.
6114:1953Sci...117..528M
6046:2021GeoRL..4894235M
5990:2022GeoRL..4998708G
5925:2022GeoRL..4998708G
5875:10.5194/epsc2021-57
5866:2021EPSC...15...57R
5807:2022JGRE..12707241M
5739:2020PNAS..11724082L
5733:(39): 24082–24087.
5684:2021NatGe..14..559G
5614:2015NatGe...8..523O
5520:1956Tell....8..364A
5465:10.1038/nature25491
5457:2018Natur.555..216A
5402:2021NatGe..14..559G
5325:2018JGRE..123.1511G
5270:2020Icar..33513405T
5216:2022JGRE..12707241M
4756:2018Icar..302..418L
4674:, pp. 48, 193.
4567:, pp. 194–196.
4506:, 2003, p. 171
3908:, pp. 133, 145–147.
3793:2010JAtS...67.3652L
3720:2021GeoRL..4895651D
3649:2017SSRv..213..139J
3586:2000Natur.403..630I
3547:2005Icar..174..192S
3482:2020SSRv..216...30F
3373:1976Icar...29..255B
3310:2021GeoRL..4892912G
3235:10.1038/nature25793
3227:2018Natur.555..223K
3099:, pp. 299–302.
2828:2020JGRE..12506659G
2747:2020Natur.584...55B
2678:1979Sci...204..951S
2320:is temperature and
2217:larger than Jupiter
2200:Solar System portal
2118:Wide Field Camera 3
2020:astronomical object
1873:Percy B. Molesworth
1289:dispersion relation
565:
554:1.62 × 10
540:3.73 × 10
492:3.62 × 10
478:1.68 × 10
464:1.61 × 10
450:3.62 × 10
436:1.23 × 10
398:
397:in Jupiter and Sun
294:gravitational force
282:atmosphere of Earth
260:supercritical fluid
9400:Stellar atmosphere
9278:Natural satellites
8585:Outline of Jupiter
7185:Irwin, P. (2003).
6696:Beebe, R. (1997).
5113:The New York Times
4981:The New York Times
4904:on 2 February 2007
4875:on 19 October 2008
4728:2016-07-06 at the
4258:, pp. 12, 26.
2405:spacetelescope.org
2358:clathrate hydrates
2223:Galileo Spacecraft
2149:
2122:
2103:Eustachio Manfredi
2076:
1953:
1863:
1846:instrument and by
1816:Coriolis parameter
1800:
1739:
1728:
1692:Gemini Observatory
1668:
1660:
1640:
1600:
1555:
1523:anticyclonic storm
1519:
1464:
1448:
1409:
1379:via the atmosphere
1333:
1189:
1161:
1105:
1034:
943:
919:Earth's atmosphere
719:molecular hydrogen
563:
394:
371:trihydrogen cation
248:Earth's atmosphere
228:
211:Vertical structure
171:
101:The atmosphere of
60:molecular hydrogen
44:
9415:
9414:
9101:
9100:
9046:
9045:
8852:
8851:
8764:
8763:
8443:Planetary Society
8429:10.1175/JAS3711.1
8331:(17): 2136–2152.
8275:(10): 1270–1296.
8203:(18): 2685–2734.
8180:10.1029/97JE00520
8165:(E4): 9303–9308.
8142:978-0-12-018828-4
7963:978-0-571-18026-4
7946:Peek, Bertrand M.
7929:978-0-933346-86-4
7726:10.1029/98JE01766
7671:(7177): 437–440.
7520:978-0-521-41008-3
7497:978-0-582-35655-9
7204:978-3-540-00681-7
7139:978-0-521-81808-7
7101:978-0-7503-0448-1
7049:(7065): 193–196.
6796:Encrenaz, Thérèse
6711:978-1-56098-685-0
6702:Smithsonian Books
6665:Sky and Telescope
6621:(5848): 226–229.
6108:(3046): 528–529.
5662:Nature Geoscience
5602:Nature Geoscience
5451:(7695): 216–219.
5380:Nature Geoscience
5084:. New Scientist.
5008:on March 25, 2012
4462:978-0-521-41008-3
3777:(11): 3652–3672.
3580:(6770): 630–632.
3432:978-0-08-047021-4
3221:(7695): 223–226.
3013:, pp. 9–10, 20–23
2672:(4396): 951–972.
2276:The scale height
2213:Extrasolar planet
2054:atmospheric probe
1925:Edwin E. Salpeter
1493:convective plumes
1480:cyclonic rotation
1389:Discrete features
1084:atmospheric waves
907:protosolar nebula
696:atmospheric probe
684:
683:
646:13 ± 2
561:
560:
323:condensation heat
224:atmospheric probe
166:
68:solar proportions
16:(Redirected from
9442:
9165:
9128:
9121:
9114:
9105:
9104:
9091:
9090:
9089:
9079:
9078:
8986:(2023, en route)
8868:
8867:
8773:
8772:
8652:
8651:
8640:
8567:
8560:
8553:
8544:
8543:
8535:
8534:
8533:
8523:
8522:
8511:
8510:
8499:
8498:
8497:
8487:
8486:
8485:
8475:
8474:
8473:
8466:
8432:
8415:(5): 1548–1557.
8406:
8396:
8394:
8368:
8358:
8348:
8322:
8312:
8302:
8292:
8266:
8256:
8239:(8): 1356–1370.
8230:
8220:
8194:
8184:
8182:
8156:
8146:
8114:
8104:
8087:(8): 1399–1426.
8078:
8068:
8057:10.1038/257778a0
8034:
8024:
7995:
7993:
7992:
7975:
7955:
7941:
7906:
7896:
7886:
7884:
7883:
7877:
7871:. Archived from
7862:
7852:
7827:(8): 1935–1996.
7813:
7811:
7794:(5): 1471–1472.
7776:
7729:
7698:
7688:
7653:
7622:
7602:
7592:
7572:
7562:
7542:
7532:
7501:
7475:
7473:
7471:2060/19650022425
7448:(1–6): 266–273.
7434:
7397:
7352:
7327:(1–2): 319–343.
7315:
7292:
7261:
7243:
7208:
7181:
7153:
7143:
7123:
7113:
7082:
7031:
6984:
6958:
6956:astro-ph/9907402
6931:
6905:
6889:Baltic Astronomy
6882:
6859:
6833:
6823:
6791:
6760:
6758:
6723:
6692:
6690:
6689:
6680:. Archived from
6654:
6606:
6588:
6560:
6550:
6532:
6507:(1–2): 121–136.
6498:
6488:
6448:
6388:
6387:
6377:
6367:
6335:
6329:
6328:
6326:
6324:
6319:on 29 March 2023
6305:
6299:
6293:
6287:
6281:
6275:
6269:
6263:
6257:
6251:
6245:
6236:
6226:
6220:
6214:
6205:
6199:
6190:
6184:
6178:
6172:
6166:
6160:
6154:
6151:Ingersoll (2004)
6148:
6142:
6141:
6093:
6087:
6082:
6076:
6075:
6057:
6024:
6018:
6017:
5983:
5959:
5953:
5952:
5918:
5894:
5888:
5887:
5877:
5851:
5843:
5837:
5836:
5818:
5785:
5779:
5778:
5768:
5750:
5718:
5712:
5711:
5677:
5653:
5644:
5643:
5633:
5622:10.1038/ngeo2459
5593:
5587:
5586:
5561:(4–5): 409–420.
5546:
5540:
5539:
5499:
5493:
5492:
5436:
5430:
5429:
5395:
5371:
5365:
5364:
5346:
5336:
5319:(6): 1511–1524.
5304:
5298:
5297:
5252:
5246:
5245:
5227:
5194:
5188:
5182:
5176:
5170:
5161:
5151:
5140:
5134:
5125:
5124:
5122:
5120:
5103:
5097:
5096:
5094:
5093:
5077:
5071:
5070:
5068:
5067:
5055:
5044:
5043:
5041:
5040:
5024:
5018:
5017:
5015:
5013:
4997:
4991:
4990:
4988:
4987:
4972:
4963:
4962:
4960:
4959:
4944:
4935:
4934:
4932:
4931:
4919:
4913:
4912:
4910:
4909:
4893:
4884:
4883:
4881:
4880:
4864:
4858:
4849:
4840:
4834:
4828:
4819:
4810:
4800:
4794:
4793:
4791:
4790:
4774:
4768:
4767:
4739:
4733:
4720:
4714:
4708:
4702:
4696:
4687:
4681:
4675:
4669:
4663:
4658:
4652:
4646:
4640:
4635:
4629:
4623:
4614:
4613:
4611:
4610:
4598:
4592:
4586:
4580:
4574:
4568:
4562:
4556:
4550:
4544:
4543:
4541:
4540:
4524:
4518:
4513:
4507:
4501:
4495:
4485:
4479:
4473:
4467:
4466:
4446:
4440:
4439:
4437:
4436:
4416:
4410:
4409:
4407:
4406:
4390:
4384:
4383:
4381:
4379:
4362:
4356:
4350:
4344:
4338:
4332:
4331:
4329:
4327:
4313:
4307:
4301:
4286:
4280:
4271:
4268:Ingersoll (2004)
4265:
4259:
4253:
4247:
4242:
4236:
4230:
4224:
4218:
4207:
4202:
4196:
4190:
4184:
4178:
4172:
4166:
4160:
4154:
4145:
4142:Ingersoll (2004)
4139:
4133:
4130:Ingersoll (2004)
4127:
4121:
4115:
4098:
4088:
4082:
4073:
4064:
4058:
4049:
4044:
4038:
4033:
4027:
4018:
4012:
4006:
4000:
3994:
3988:
3987:
3985:
3983:
3973:
3967:
3961:
3955:
3954:
3952:
3951:
3946:. Universe Today
3939:
3933:
3927:
3921:
3915:
3909:
3903:
3897:
3891:
3876:
3870:
3864:
3858:
3852:
3846:
3833:
3827:
3821:
3820:
3786:
3762:
3756:
3755:
3713:
3688:
3677:
3676:
3643:(1–4): 139–185.
3628:
3622:
3621:
3594:10.1038/35001021
3565:
3559:
3558:
3526:
3520:
3519:
3509:
3475:
3451:
3445:
3444:
3418:
3412:
3406:
3400:
3397:Ingersoll (2004)
3394:
3385:
3384:
3352:
3346:
3345:
3303:
3279:
3273:
3272:
3246:
3206:
3200:
3194:
3185:
3184:
3182:
3180:
3168:
3162:
3153:
3147:
3141:
3130:
3129:
3127:
3126:
3117:. Archived from
3106:
3100:
3094:
3085:
3079:
3073:
3067:
3058:
3055:Ingersoll (2004)
3052:
3029:
3023:
3014:
3004:
2995:
2989:
2980:
2974:
2963:
2957:
2948:
2945:Ingersoll (2004)
2942:
2931:
2928:Ingersoll (2004)
2925:
2914:
2908:
2891:
2885:
2879:
2876:Ingersoll (2004)
2873:
2864:
2863:
2821:
2796:
2790:
2789:
2787:
2785:
2727:Becker, Heidi N.
2723:
2714:
2713:
2660:
2654:
2648:
2635:
2629:
2616:
2610:
2599:
2593:
2580:
2574:
2563:
2560:Ingersoll (2004)
2557:
2528:
2522:
2516:
2507:
2488:
2483:
2470:
2464:
2425:
2424:
2422:
2420:
2397:
2368:
2351:
2337:
2327:
2315:
2304:
2297:
2275:
2202:
2197:
2196:
2195:
2088:Giovanni Cassini
2032:hydrogen sulfide
2008:carbon disulfide
1828:Fujiwhara effect
1686:-Miller, of the
1531:Eustachio Divini
1425:counterclockwise
1368:
1361:
1358:from Jupiter is
1353:
1244:
1232:
1157:moons of Jupiter
1054:convergence zone
1011:axis of rotation
985:. The eastward (
904:
880:Shoemaker-Levy 9
772:hydrogen sulfide
744:
740:
732:
731:
730:
566:
562:
399:
393:
384:
383:
382:
310:ammonium sulfide
169:Clouds in motion
167:
80:hydrogen sulfide
36:true-color image
21:
9450:
9449:
9445:
9444:
9443:
9441:
9440:
9439:
9420:
9419:
9416:
9411:
9404:
9373:
9339:
9272:
9233:
9166:
9157:
9137:
9132:
9102:
9097:
9087:
9085:
9067:
9042:
8997:
8972:
8952:Voyager program
8924:Pioneer program
8903:Galileo project
8897:Cassini–Huygens
8884:
8863:
8861:
8848:
8815:
8792:
8760:
8714:
8681:
8641:
8632:
8589:
8576:
8571:
8541:
8531:
8529:
8517:
8505:
8495:
8493:
8483:
8481:
8471:
8469:
8461:
8439:
8404:
8366:
8346:10.1.1.144.5975
8320:
8300:
8264:
8228:
8192:
8154:
8143:
8112:
8076:
8032:
7990:
7988:
7964:
7930:
7914:
7912:Further reading
7909:
7894:
7881:
7879:
7875:
7860:
7600:
7570:
7540:
7521:
7498:
7490:. p. 107.
7205:
7151:
7140:
7121:
7102:
6831:
6712:
6687:
6685:
6586:10.1.1.553.8220
6558:
6496:
6396:
6391:
6336:
6332:
6322:
6320:
6307:
6306:
6302:
6294:
6290:
6282:
6278:
6270:
6266:
6258:
6254:
6246:
6239:
6227:
6223:
6215:
6208:
6200:
6193:
6185:
6181:
6173:
6169:
6161:
6157:
6149:
6145:
6094:
6090:
6083:
6079:
6025:
6021:
5960:
5956:
5895:
5891:
5844:
5840:
5786:
5782:
5719:
5715:
5654:
5647:
5594:
5590:
5547:
5543:
5500:
5496:
5437:
5433:
5372:
5368:
5305:
5301:
5253:
5249:
5195:
5191:
5183:
5179:
5175:, pp. 1983–1985
5173:Vasavada (2005)
5171:
5164:
5154:Sanchez-Lavega
5152:
5143:
5137:Vasavada (2005)
5135:
5128:
5118:
5116:
5104:
5100:
5091:
5089:
5078:
5074:
5065:
5063:
5056:
5047:
5038:
5036:
5025:
5021:
5011:
5009:
4998:
4994:
4985:
4983:
4973:
4966:
4957:
4955:
4946:
4945:
4938:
4929:
4927:
4920:
4916:
4907:
4905:
4894:
4887:
4878:
4876:
4865:
4861:
4850:
4843:
4835:
4831:
4822:Sanchez-Lavega
4820:
4813:
4801:
4797:
4788:
4786:
4785:on 15 June 2007
4775:
4771:
4740:
4736:
4730:Wayback Machine
4721:
4717:
4709:
4705:
4697:
4690:
4682:
4678:
4670:
4666:
4659:
4655:
4647:
4643:
4636:
4632:
4626:Fletcher (2010)
4624:
4617:
4608:
4606:
4599:
4595:
4587:
4583:
4575:
4571:
4563:
4559:
4551:
4547:
4538:
4536:
4525:
4521:
4514:
4510:
4502:
4498:
4486:
4482:
4474:
4470:
4463:
4447:
4443:
4434:
4432:
4417:
4413:
4404:
4402:
4391:
4387:
4377:
4375:
4363:
4359:
4353:Vasavada (2005)
4351:
4347:
4341:Vasavada (2005)
4339:
4335:
4325:
4323:
4315:
4314:
4310:
4304:Vasavada (2005)
4302:
4289:
4283:Vasavada (2005)
4281:
4274:
4270:, pp. 11, 17–18
4266:
4262:
4254:
4250:
4243:
4239:
4233:Vasavada (2005)
4231:
4227:
4223:, pp. 1966–1972
4221:Vasavada (2005)
4219:
4210:
4203:
4199:
4193:Vasavada (2005)
4191:
4187:
4183:, pp. 1962–1966
4181:Vasavada (2005)
4179:
4175:
4171:, pp. 1945–1947
4169:Vasavada (2005)
4167:
4163:
4157:Vasavada (2005)
4155:
4148:
4140:
4136:
4128:
4124:
4120:, pp. 1947–1958
4118:Vasavada (2005)
4116:
4101:
4089:
4085:
4074:
4067:
4063:, pp. 1943–1945
4061:Vasavada (2005)
4059:
4052:
4045:
4041:
4034:
4030:
4019:
4015:
4007:
4003:
3995:
3991:
3981:
3979:
3975:
3974:
3970:
3962:
3958:
3949:
3947:
3940:
3936:
3928:
3924:
3916:
3912:
3904:
3900:
3896:, pp. 1987–1989
3894:Vasavada (2005)
3892:
3879:
3871:
3867:
3859:
3855:
3847:
3836:
3832:, pp. 85, 91–4.
3828:
3824:
3763:
3759:
3689:
3680:
3629:
3625:
3566:
3562:
3527:
3523:
3452:
3448:
3433:
3419:
3415:
3407:
3403:
3395:
3388:
3353:
3349:
3280:
3276:
3207:
3203:
3195:
3188:
3178:
3176:
3169:
3165:
3154:
3150:
3142:
3133:
3124:
3122:
3107:
3103:
3095:
3088:
3080:
3076:
3068:
3061:
3053:
3032:
3026:Vasavada (2005)
3024:
3017:
3005:
2998:
2990:
2983:
2975:
2966:
2958:
2951:
2943:
2934:
2926:
2917:
2909:
2894:
2886:
2882:
2874:
2867:
2797:
2793:
2783:
2781:
2741:(7819): 55–58.
2724:
2717:
2661:
2657:
2651:Vasavada (2005)
2649:
2638:
2634:, pp. 1980–1982
2632:Vasavada (2005)
2630:
2619:
2615:, pp. 1978–1980
2613:Vasavada (2005)
2611:
2602:
2596:Vasavada (2005)
2594:
2583:
2577:Vasavada (2005)
2575:
2566:
2558:
2531:
2523:
2519:
2508:
2491:
2484:
2473:
2465:
2428:
2418:
2416:
2399:
2398:
2394:
2390:
2385:
2325:
2321:
2314:≈ 0.0023 kg/mol
2310:
2299:
2294:
2281:
2266:
2198:
2193:
2191:
2188:
2145:Galileo orbiter
2137:
2062:
2037:
2029:
2017:
2013:
2005:
2000:diatomic sulfur
1939:
1933:
1912:
1881:
1868:
1792:
1720:
1632:
1618:Great Dark Spot
1609:Cassini–Huygens
1511:
1505:
1462:; October 2017)
1455:
1396:
1391:
1363:
1360:5.44 ± 0.43 W/m
1359:
1354:. The internal
1351:
1347:
1310:
1273:
1252:
1251:
1250:
1249:
1248:
1245:
1237:
1236:
1233:
1222:
1198:Equatorial band
1096:
1063:
1007:Juno spacecraft
955:Equatorial Zone
931:
902:
895:isotopic ratios
872:carbon monoxide
841:
833:
793:
785:
777:
769:
742:
738:
729:
726:
725:
724:
722:
685:
396:
391:
381:
378:
377:
376:
374:
367:magnetic storms
319:
315:
307:
256:critical points
213:
156:
50:is the largest
28:
23:
22:
15:
12:
11:
5:
9448:
9438:
9437:
9432:
9413:
9412:
9409:
9406:
9405:
9403:
9402:
9397:
9392:
9387:
9381:
9379:
9375:
9374:
9372:
9371:
9364:
9357:
9349:
9347:
9341:
9340:
9338:
9337:
9330:
9323:
9318:
9313:
9308:
9303:
9298:
9293:
9288:
9282:
9280:
9274:
9273:
9271:
9270:
9263:
9256:
9249:
9243:
9241:
9235:
9234:
9232:
9231:
9224:
9217:
9210:
9203:
9196:
9189:
9182:
9176:
9174:
9168:
9167:
9160:
9158:
9156:
9155:
9147:
9145:
9139:
9138:
9131:
9130:
9123:
9116:
9108:
9099:
9098:
9096:
9095:
9083:
9072:
9069:
9068:
9066:
9065:
9060:
9054:
9052:
9048:
9047:
9044:
9043:
9041:
9040:
9032:
9026:
9020:
9012:
9005:
9003:
8999:
8998:
8996:
8995:
8991:Europa Clipper
8987:
8980:
8978:
8974:
8973:
8971:
8970:
8969:
8968:
8961:
8949:
8942:
8941:
8940:
8933:
8921:
8914:
8913:
8912:
8900:
8892:
8890:
8886:
8885:
8883:
8882:
8874:
8872:
8865:
8854:
8853:
8850:
8849:
8847:
8846:
8841:
8836:
8831:
8825:
8823:
8817:
8816:
8814:
8813:
8808:
8802:
8800:
8794:
8793:
8791:
8790:
8788:Solar eclipses
8785:
8779:
8777:
8770:
8766:
8765:
8762:
8761:
8759:
8758:
8756:Pasiphae group
8753:
8748:
8743:
8738:
8733:
8728:
8722:
8720:
8716:
8715:
8713:
8712:
8707:
8702:
8697:
8691:
8689:
8683:
8682:
8680:
8679:
8674:
8669:
8664:
8658:
8656:
8649:
8643:
8642:
8635:
8633:
8631:
8630:
8625:
8620:
8615:
8610:
8609:
8608:
8606:Great Red Spot
8597:
8595:
8591:
8590:
8588:
8587:
8581:
8578:
8577:
8570:
8569:
8562:
8555:
8547:
8540:
8539:
8527:
8515:
8503:
8491:
8479:
8459:
8458:
8456:The Atmosphere
8453:
8438:
8437:External links
8435:
8434:
8433:
8397:
8377:(3): 439–476.
8359:
8313:
8293:
8257:
8221:
8185:
8147:
8141:
8105:
8069:
8025:
7996:
7976:
7962:
7942:
7928:
7913:
7910:
7908:
7907:
7887:
7853:
7814:
7777:
7730:
7699:
7654:
7636:(2): 491–495.
7623:
7593:
7583:(3): 136–140.
7563:
7553:(6): 321–332.
7533:
7519:
7502:
7496:
7485:Addison Wesley
7476:
7435:
7398:
7353:
7316:
7306:(5): 239–245.
7293:
7289:10.1086/110110
7262:
7209:
7203:
7182:
7164:(5): 981–985.
7144:
7138:
7114:
7100:
7083:
7032:
6985:
6932:
6883:
6860:
6842:(1): 306–328.
6824:
6792:
6774:(2): 255–260.
6761:
6741:(3): 295–353.
6724:
6710:
6693:
6655:
6607:
6571:(5): 498–507.
6551:
6489:
6463:(2): 105–112.
6449:
6397:
6395:
6392:
6390:
6389:
6330:
6300:
6288:
6276:
6264:
6252:
6237:
6235:, pp. 951–972.
6221:
6206:
6191:
6179:
6167:
6155:
6143:
6088:
6077:
6019:
5954:
5889:
5838:
5780:
5713:
5668:(8): 559–563.
5645:
5608:(7): 523–526.
5588:
5541:
5514:(3): 364–372.
5494:
5431:
5386:(8): 559–563.
5366:
5344:2027.42/145242
5299:
5247:
5189:
5187:, p. 226.
5177:
5162:
5141:
5126:
5098:
5072:
5045:
5019:
4992:
4964:
4936:
4914:
4885:
4859:
4841:
4829:
4811:
4795:
4769:
4734:
4715:
4703:
4688:
4686:, p. 193.
4676:
4664:
4653:
4641:
4630:
4615:
4593:
4591:, p. 195.
4581:
4569:
4557:
4555:, p. 191.
4545:
4519:
4508:
4496:
4494:, p. 954.
4480:
4468:
4461:
4441:
4411:
4393:Staff (2007).
4385:
4357:
4345:
4333:
4308:
4287:
4272:
4260:
4248:
4237:
4225:
4208:
4197:
4185:
4173:
4161:
4146:
4134:
4122:
4099:
4083:
4065:
4050:
4047:Ridpath (1998)
4039:
4028:
4013:
4001:
3989:
3968:
3956:
3934:
3922:
3910:
3898:
3877:
3875:, pp. 125–130.
3865:
3853:
3851:, pp. 101–105.
3834:
3822:
3757:
3736:2027.42/170953
3678:
3623:
3560:
3541:(1): 192–204.
3521:
3446:
3431:
3413:
3401:
3386:
3367:(2): 255–260.
3347:
3326:2027.42/167748
3274:
3201:
3186:
3163:
3148:
3131:
3101:
3086:
3074:
3059:
3030:
3015:
2996:
2981:
2964:
2949:
2932:
2915:
2892:
2880:
2865:
2791:
2715:
2655:
2636:
2617:
2600:
2581:
2579:, p. 1942–1974
2564:
2529:
2517:
2489:
2486:Guillot (1999)
2471:
2426:
2415:. 6 April 2017
2391:
2389:
2386:
2384:
2383:
2361:
2360:in water ice.
2344:
2330:
2323:
2303:= 8.31 J/mol/K
2292:
2280:is defined as
2267:
2265:
2262:
2261:
2260:
2251:
2246:
2241:
2236:
2230:
2220:
2210:
2204:
2203:
2187:
2184:
2136:
2133:
2061:
2058:
2044:sulfur dioxide
2035:
2027:
2015:
2011:
2003:
1935:Main article:
1932:
1929:
1911:
1908:
1880:
1877:
1867:
1864:
1835:observations.
1820:Saturn's poles
1791:
1788:
1719:
1716:
1638:Oval BA (left)
1631:
1628:
1509:Great Red Spot
1507:Main article:
1504:
1503:Great Red Spot
1501:
1454:Jupiter clouds
1395:
1392:
1390:
1387:
1346:
1343:
1338:fluid dynamics
1309:
1306:
1272:
1271:Shallow models
1269:
1246:
1239:
1238:
1234:
1227:
1226:
1225:
1224:
1223:
1221:
1218:
1117:foreshortening
1113:limb darkening
1095:
1094:Specific bands
1092:
1062:
1059:
930:
927:
868:carbon dioxide
839:
831:
791:
783:
775:
767:
752:metallic state
727:
682:
681:
678:
675:
665:
664:
661:
658:
648:
647:
644:
641:
631:
630:
627:
624:
614:
613:
607:
604:
594:
593:
590:
587:
577:
576:
573:
570:
559:
558:
555:
552:
545:
544:
541:
538:
531:
530:
524:
521:
514:
513:
507:
504:
497:
496:
493:
490:
483:
482:
479:
476:
469:
468:
465:
462:
455:
454:
451:
448:
441:
440:
437:
434:
427:
426:
423:
420:
410:
409:
406:
403:
392:
390:
387:
379:
317:
313:
305:
212:
209:
183:Great Red Spot
26:
9:
6:
4:
3:
2:
9447:
9436:
9433:
9431:
9428:
9427:
9425:
9418:
9407:
9401:
9398:
9396:
9393:
9391:
9388:
9386:
9383:
9382:
9380:
9376:
9370:
9369:
9365:
9363:
9362:
9358:
9356:
9355:
9351:
9350:
9348:
9346:
9342:
9336:
9335:
9331:
9329:
9328:
9324:
9322:
9319:
9317:
9314:
9312:
9309:
9307:
9304:
9302:
9299:
9297:
9294:
9292:
9289:
9287:
9284:
9283:
9281:
9279:
9275:
9269:
9268:
9264:
9262:
9261:
9257:
9255:
9254:
9250:
9248:
9245:
9244:
9242:
9240:
9239:Dwarf planets
9236:
9230:
9229:
9225:
9223:
9222:
9218:
9216:
9215:
9211:
9209:
9208:
9204:
9202:
9201:
9197:
9195:
9194:
9190:
9188:
9187:
9183:
9181:
9178:
9177:
9175:
9173:
9169:
9164:
9154:
9153:
9149:
9148:
9146:
9144:
9140:
9136:
9129:
9124:
9122:
9117:
9115:
9110:
9109:
9106:
9094:
9084:
9082:
9074:
9073:
9070:
9064:
9061:
9059:
9056:
9055:
9053:
9049:
9038:
9037:
9033:
9030:
9027:
9024:
9021:
9018:
9017:
9013:
9010:
9007:
9006:
9004:
9000:
8993:
8992:
8988:
8985:
8982:
8981:
8979:
8975:
8967:
8966:
8962:
8960:
8959:
8955:
8954:
8953:
8950:
8948:
8947:
8943:
8939:
8938:
8934:
8932:
8931:
8927:
8926:
8925:
8922:
8920:
8919:
8915:
8911:
8910:
8906:
8905:
8904:
8901:
8899:
8898:
8894:
8893:
8891:
8887:
8881:
8880:
8876:
8875:
8873:
8869:
8866:
8859:
8855:
8845:
8842:
8840:
8837:
8835:
8832:
8830:
8827:
8826:
8824:
8822:
8818:
8812:
8809:
8807:
8804:
8803:
8801:
8799:
8795:
8789:
8786:
8784:
8781:
8780:
8778:
8774:
8771:
8767:
8757:
8754:
8752:
8749:
8747:
8744:
8742:
8739:
8737:
8734:
8732:
8729:
8727:
8726:Himalia group
8724:
8723:
8721:
8717:
8711:
8708:
8706:
8703:
8701:
8698:
8696:
8693:
8692:
8690:
8688:
8684:
8678:
8675:
8673:
8670:
8668:
8665:
8663:
8660:
8659:
8657:
8653:
8650:
8648:
8644:
8639:
8629:
8626:
8624:
8621:
8619:
8616:
8614:
8613:Magnetosphere
8611:
8607:
8604:
8603:
8602:
8599:
8598:
8596:
8592:
8586:
8583:
8582:
8579:
8575:
8568:
8563:
8561:
8556:
8554:
8549:
8548:
8545:
8538:
8528:
8526:
8521:
8516:
8514:
8509:
8504:
8502:
8492:
8490:
8480:
8478:
8468:
8467:
8464:
8457:
8454:
8451:
8447:
8444:
8441:
8440:
8430:
8426:
8422:
8418:
8414:
8410:
8403:
8398:
8393:
8388:
8384:
8380:
8376:
8372:
8365:
8360:
8356:
8352:
8347:
8342:
8338:
8334:
8330:
8326:
8319:
8314:
8310:
8306:
8299:
8294:
8290:
8286:
8282:
8278:
8274:
8270:
8263:
8258:
8254:
8250:
8246:
8242:
8238:
8234:
8227:
8222:
8218:
8214:
8210:
8206:
8202:
8198:
8191:
8186:
8181:
8176:
8172:
8168:
8164:
8160:
8153:
8148:
8144:
8138:
8134:
8130:
8126:
8122:
8118:
8111:
8106:
8102:
8098:
8094:
8090:
8086:
8082:
8075:
8070:
8066:
8062:
8058:
8054:
8050:
8046:
8043:(5529): 778.
8042:
8038:
8031:
8026:
8022:
8018:
8014:
8010:
8006:
8002:
7997:
7986:
7982:
7977:
7973:
7969:
7965:
7959:
7954:
7953:
7947:
7943:
7939:
7935:
7931:
7925:
7921:
7916:
7915:
7904:
7901:. Cambridge:
7900:
7893:
7888:
7878:on 2014-08-23
7874:
7870:
7867:. Cambridge:
7866:
7859:
7854:
7850:
7846:
7842:
7838:
7834:
7830:
7826:
7822:
7821:
7815:
7810:
7805:
7801:
7797:
7793:
7789:
7788:
7783:
7778:
7774:
7770:
7766:
7762:
7758:
7754:
7750:
7746:
7742:
7738:
7737:
7731:
7727:
7723:
7719:
7715:
7711:
7707:
7706:
7700:
7696:
7692:
7687:
7682:
7678:
7674:
7670:
7666:
7665:
7660:
7655:
7651:
7647:
7643:
7639:
7635:
7631:
7630:
7624:
7620:
7616:
7612:
7608:
7607:
7599:
7594:
7590:
7586:
7582:
7578:
7577:
7569:
7564:
7560:
7556:
7552:
7548:
7547:
7539:
7534:
7530:
7526:
7522:
7516:
7512:
7509:. Cambridge:
7508:
7503:
7499:
7493:
7489:
7486:
7482:
7477:
7472:
7467:
7463:
7459:
7455:
7451:
7447:
7443:
7442:
7436:
7432:
7428:
7424:
7420:
7416:
7412:
7408:
7404:
7399:
7395:
7391:
7387:
7383:
7379:
7375:
7371:
7367:
7363:
7359:
7354:
7350:
7346:
7342:
7338:
7334:
7330:
7326:
7322:
7317:
7313:
7309:
7305:
7301:
7300:
7294:
7290:
7286:
7282:
7278:
7274:
7270:
7269:
7263:
7259:
7255:
7251:
7247:
7242:
7237:
7233:
7229:
7225:
7221:
7220:
7215:
7210:
7206:
7200:
7196:
7192:
7188:
7183:
7179:
7175:
7171:
7167:
7163:
7159:
7158:
7150:
7145:
7141:
7135:
7131:
7128:. Cambridge:
7127:
7120:
7115:
7111:
7107:
7103:
7097:
7093:
7089:
7084:
7080:
7076:
7072:
7068:
7064:
7060:
7056:
7052:
7048:
7044:
7043:
7038:
7033:
7029:
7025:
7021:
7017:
7013:
7009:
7005:
7001:
6997:
6993:
6992:
6986:
6982:
6978:
6974:
6970:
6966:
6962:
6957:
6952:
6948:
6944:
6943:
6938:
6933:
6929:
6925:
6921:
6917:
6913:
6909:
6904:
6899:
6895:
6891:
6890:
6884:
6880:
6876:
6872:
6868:
6867:
6861:
6857:
6853:
6849:
6845:
6841:
6837:
6830:
6825:
6821:
6817:
6813:
6809:
6806:(2): 89–103.
6805:
6801:
6797:
6793:
6789:
6785:
6781:
6777:
6773:
6769:
6768:
6762:
6757:
6752:
6748:
6744:
6740:
6736:
6735:
6730:
6725:
6721:
6717:
6713:
6707:
6703:
6699:
6694:
6684:on 2011-05-27
6683:
6679:
6675:
6671:
6667:
6666:
6661:
6656:
6652:
6648:
6644:
6640:
6636:
6632:
6628:
6624:
6620:
6616:
6615:
6608:
6604:
6600:
6596:
6592:
6587:
6582:
6578:
6574:
6570:
6566:
6565:
6557:
6552:
6548:
6544:
6540:
6536:
6531:
6530:2027.42/43766
6526:
6522:
6518:
6514:
6510:
6506:
6502:
6495:
6490:
6486:
6482:
6478:
6474:
6470:
6466:
6462:
6458:
6457:
6450:
6446:
6442:
6438:
6434:
6430:
6426:
6422:
6418:
6414:
6410:
6409:
6404:
6399:
6398:
6394:Cited sources
6385:
6381:
6376:
6371:
6366:
6361:
6357:
6353:
6349:
6345:
6341:
6334:
6318:
6314:
6310:
6304:
6297:
6292:
6285:
6284:Rogers (1995)
6280:
6273:
6272:Rogers (1995)
6268:
6262:, p. 226–227.
6261:
6260:Rogers (1995)
6256:
6249:
6248:Rogers (1995)
6244:
6242:
6234:
6232:
6225:
6218:
6213:
6211:
6203:
6202:Rogers (1995)
6198:
6196:
6188:
6187:Rogers (2008)
6183:
6176:
6175:Rogers (1995)
6171:
6164:
6159:
6152:
6147:
6139:
6135:
6131:
6127:
6123:
6119:
6115:
6111:
6107:
6103:
6099:
6092:
6086:
6081:
6073:
6069:
6065:
6061:
6056:
6051:
6047:
6043:
6039:
6035:
6031:
6023:
6015:
6011:
6007:
6003:
5999:
5995:
5991:
5987:
5982:
5977:
5973:
5969:
5965:
5958:
5950:
5946:
5942:
5938:
5934:
5930:
5926:
5922:
5917:
5912:
5908:
5904:
5900:
5893:
5885:
5881:
5876:
5871:
5867:
5863:
5859:
5855:
5850:
5842:
5834:
5830:
5826:
5822:
5817:
5812:
5808:
5804:
5800:
5796:
5792:
5784:
5776:
5772:
5767:
5762:
5758:
5754:
5749:
5744:
5740:
5736:
5732:
5728:
5724:
5717:
5709:
5705:
5701:
5697:
5693:
5689:
5685:
5681:
5676:
5671:
5667:
5663:
5659:
5652:
5650:
5641:
5637:
5632:
5631:1721.1/100773
5627:
5623:
5619:
5615:
5611:
5607:
5603:
5599:
5592:
5584:
5580:
5576:
5572:
5568:
5564:
5560:
5556:
5552:
5545:
5537:
5533:
5529:
5525:
5521:
5517:
5513:
5509:
5505:
5498:
5490:
5486:
5482:
5478:
5474:
5470:
5466:
5462:
5458:
5454:
5450:
5446:
5442:
5435:
5427:
5423:
5419:
5415:
5411:
5407:
5403:
5399:
5394:
5389:
5385:
5381:
5377:
5370:
5362:
5358:
5354:
5350:
5345:
5340:
5335:
5330:
5326:
5322:
5318:
5314:
5310:
5303:
5295:
5291:
5287:
5283:
5279:
5275:
5271:
5267:
5263:
5259:
5251:
5243:
5239:
5235:
5231:
5226:
5221:
5217:
5213:
5209:
5205:
5201:
5193:
5186:
5181:
5174:
5169:
5167:
5160:, pp. 437–438
5159:
5157:
5150:
5148:
5146:
5138:
5133:
5131:
5115:
5114:
5109:
5102:
5087:
5083:
5076:
5061:
5054:
5052:
5050:
5034:
5030:
5023:
5007:
5003:
4996:
4982:
4978:
4971:
4969:
4953:
4949:
4943:
4941:
4925:
4918:
4903:
4899:
4892:
4890:
4874:
4870:
4863:
4857:
4855:
4848:
4846:
4838:
4837:Rogers (1995)
4833:
4827:
4825:
4818:
4816:
4808:
4806:
4799:
4784:
4780:
4773:
4765:
4761:
4757:
4753:
4749:
4745:
4738:
4731:
4727:
4724:
4719:
4712:
4707:
4700:
4695:
4693:
4685:
4684:Rogers (1995)
4680:
4673:
4672:Rogers (1995)
4668:
4662:
4657:
4650:
4649:Rogers (1995)
4645:
4639:
4634:
4628:, p. 306
4627:
4622:
4620:
4604:
4597:
4590:
4589:Rogers (1995)
4585:
4579:, p. 35.
4578:
4573:
4566:
4565:Rogers (1995)
4561:
4554:
4553:Rogers (1995)
4549:
4534:
4531:. Space.com.
4530:
4523:
4517:
4516:Beatty (2002)
4512:
4505:
4500:
4493:
4491:
4484:
4477:
4472:
4464:
4458:
4454:
4453:
4445:
4430:
4426:
4422:
4415:
4400:
4397:. Imaginova.
4396:
4389:
4374:
4373:
4368:
4361:
4354:
4349:
4342:
4337:
4322:
4318:
4312:
4305:
4300:
4298:
4296:
4294:
4292:
4284:
4279:
4277:
4269:
4264:
4257:
4252:
4246:
4241:
4234:
4229:
4222:
4217:
4215:
4213:
4206:
4201:
4194:
4189:
4182:
4177:
4170:
4165:
4158:
4153:
4151:
4143:
4138:
4131:
4126:
4119:
4114:
4112:
4110:
4108:
4106:
4104:
4097:
4095:
4087:
4081:
4079:
4072:
4070:
4062:
4057:
4055:
4048:
4043:
4037:
4032:
4026:
4024:
4017:
4010:
4009:Rogers (1995)
4005:
3998:
3997:Rogers (1995)
3993:
3978:
3972:
3966:, pp. 159–160
3965:
3964:Rogers (1995)
3960:
3945:
3938:
3931:
3926:
3919:
3918:Rogers (1995)
3914:
3907:
3906:Rogers (1995)
3902:
3895:
3890:
3888:
3886:
3884:
3882:
3874:
3873:Rogers (1995)
3869:
3863:, pp.113–117.
3862:
3861:Rogers (1995)
3857:
3850:
3849:Rogers (1995)
3845:
3843:
3841:
3839:
3831:
3830:Rogers (1995)
3826:
3818:
3814:
3810:
3806:
3802:
3798:
3794:
3790:
3785:
3780:
3776:
3772:
3768:
3761:
3753:
3749:
3745:
3741:
3737:
3733:
3729:
3725:
3721:
3717:
3712:
3707:
3703:
3699:
3695:
3687:
3685:
3683:
3674:
3670:
3666:
3662:
3658:
3654:
3650:
3646:
3642:
3638:
3634:
3627:
3619:
3615:
3611:
3607:
3603:
3599:
3595:
3591:
3587:
3583:
3579:
3575:
3571:
3564:
3556:
3552:
3548:
3544:
3540:
3536:
3532:
3525:
3517:
3513:
3508:
3503:
3499:
3495:
3491:
3487:
3483:
3479:
3474:
3469:
3465:
3461:
3457:
3450:
3442:
3438:
3434:
3428:
3424:
3417:
3410:
3405:
3398:
3393:
3391:
3382:
3378:
3374:
3370:
3366:
3362:
3358:
3351:
3343:
3339:
3335:
3331:
3327:
3323:
3319:
3315:
3311:
3307:
3302:
3297:
3293:
3289:
3285:
3278:
3270:
3266:
3262:
3258:
3254:
3250:
3245:
3244:11573/1091959
3240:
3236:
3232:
3228:
3224:
3220:
3216:
3212:
3205:
3198:
3197:Rogers (1995)
3193:
3191:
3174:
3167:
3161:
3159:
3152:
3145:
3144:Encrenaz 2003
3140:
3138:
3136:
3121:on 2011-08-10
3120:
3116:
3112:
3105:
3098:
3093:
3091:
3083:
3078:
3071:
3066:
3064:
3056:
3051:
3049:
3047:
3045:
3043:
3041:
3039:
3037:
3035:
3027:
3022:
3020:
3012:
3010:
3003:
3001:
2993:
2988:
2986:
2978:
2973:
2971:
2969:
2961:
2956:
2954:
2946:
2941:
2939:
2937:
2929:
2924:
2922:
2920:
2912:
2907:
2905:
2903:
2901:
2899:
2897:
2889:
2884:
2877:
2872:
2870:
2861:
2857:
2853:
2849:
2845:
2841:
2837:
2833:
2829:
2825:
2820:
2815:
2811:
2807:
2803:
2795:
2780:
2776:
2772:
2768:
2764:
2760:
2756:
2752:
2748:
2744:
2740:
2736:
2732:
2728:
2722:
2720:
2711:
2707:
2703:
2699:
2695:
2691:
2687:
2683:
2679:
2675:
2671:
2667:
2659:
2652:
2647:
2645:
2643:
2641:
2633:
2628:
2626:
2624:
2622:
2614:
2609:
2607:
2605:
2597:
2592:
2590:
2588:
2586:
2578:
2573:
2571:
2569:
2561:
2556:
2554:
2552:
2550:
2548:
2546:
2544:
2542:
2540:
2538:
2536:
2534:
2526:
2521:
2515:
2513:
2506:
2504:
2502:
2500:
2498:
2496:
2494:
2487:
2482:
2480:
2478:
2476:
2468:
2463:
2461:
2459:
2457:
2455:
2453:
2451:
2449:
2447:
2445:
2443:
2441:
2439:
2437:
2435:
2433:
2431:
2414:
2410:
2406:
2402:
2396:
2392:
2381:
2376:
2372:
2367:
2366:
2362:
2359:
2355:
2354:planetesimals
2350:
2349:
2345:
2341:
2336:
2335:
2331:
2319:
2313:
2308:
2302:
2295:
2288:
2284:
2279:
2274:
2273:
2269:
2259:
2255:
2252:
2250:
2247:
2245:
2242:
2240:
2237:
2234:
2231:
2228:
2224:
2221:
2218:
2214:
2211:
2209:
2206:
2205:
2201:
2190:
2183:
2181:
2176:
2174:
2170:
2165:
2163:
2158:
2154:
2146:
2141:
2132:
2129:
2128:
2119:
2114:
2110:
2106:
2104:
2100:
2096:
2091:
2089:
2085:
2081:
2073:
2072:
2066:
2057:
2055:
2053:
2047:
2045:
2041:
2033:
2025:
2021:
2009:
2001:
1997:
1993:
1992:Spectroscopic
1987:
1985:
1984:Galileo Probe
1981:
1980:
1975:
1974:
1969:
1968:
1964:
1963:
1957:
1950:
1949:
1943:
1938:
1928:
1926:
1922:
1917:
1914:In 1953, the
1907:
1905:
1904:adiabatically
1901:
1896:
1894:
1890:
1888:
1876:
1874:
1859:
1855:
1851:
1849:
1845:
1840:
1836:
1833:
1829:
1825:
1821:
1817:
1813:
1809:
1804:
1796:
1787:
1783:
1781:
1779:
1773:
1768:
1767:
1762:
1761:
1756:
1751:
1749:
1744:
1743:thunderstorms
1737:
1732:
1724:
1715:
1713:
1710:Pater of the
1707:
1705:
1699:
1695:
1693:
1689:
1685:
1681:
1676:
1673:
1664:
1656:
1652:
1650:
1644:
1636:
1627:
1625:
1624:
1619:
1615:
1611:
1610:
1604:
1596:
1592:
1590:
1585:
1583:
1579:
1575:
1570:
1566:
1562:
1560:
1551:
1547:
1544:
1539:
1536:
1532:
1528:
1524:
1515:
1510:
1500:
1498:
1494:
1488:
1485:
1481:
1475:
1473:
1469:
1461:
1460:
1452:
1444:
1440:
1438:
1434:
1430:
1426:
1422:
1418:
1414:
1406:
1405:
1400:
1386:
1384:
1380:
1375:
1374:internal heat
1370:
1367:
1357:
1345:Internal heat
1342:
1339:
1331:
1326:
1322:
1319:
1315:
1305:
1302:
1301:Galileo Probe
1296:
1294:
1290:
1286:
1282:
1278:
1268:
1264:
1261:
1257:
1243:
1231:
1217:
1215:
1211:
1207:
1203:
1199:
1193:
1185:
1181:
1178:
1173:
1171:
1167:
1158:
1152:
1148:
1144:
1142:
1141:
1134:
1132:
1128:
1125:
1120:
1118:
1114:
1109:
1103:respectively.
1100:
1091:
1089:
1085:
1080:
1076:
1072:
1067:
1058:
1055:
1051:
1050:adiabatically
1047:
1043:
1039:
1030:
1026:
1024:
1023:scale heights
1020:
1019:Galileo Probe
1016:
1012:
1008:
1004:
1000:
996:
992:
988:
984:
979:
977:
973:
969:
963:
960:
956:
952:
948:
940:
935:
926:
924:
920:
916:
912:
908:
901:abundance is
900:
896:
891:
889:
885:
881:
877:
873:
869:
865:
861:
857:
853:
849:
845:
837:
829:
825:
821:
817:
813:
809:
806:and possibly
805:
801:
797:
789:
781:
773:
765:
761:
756:
753:
748:
743:0.234 ± 0.005
739:0.157 ± 0.004
736:
720:
715:
713:
712:
707:
706:
701:
697:
695:
690:
689:giant planets
679:
676:
674:
670:
667:
666:
662:
659:
657:
653:
650:
649:
645:
642:
640:
636:
633:
632:
628:
625:
623:
619:
616:
615:
612:
608:
605:
603:
599:
596:
595:
591:
588:
586:
582:
579:
578:
574:
571:
568:
567:
556:
553:
550:
547:
546:
542:
539:
536:
533:
532:
529:
525:
522:
519:
516:
515:
512:
508:
505:
502:
499:
498:
494:
491:
488:
485:
484:
480:
477:
474:
471:
470:
466:
463:
460:
457:
456:
452:
449:
446:
443:
442:
438:
435:
432:
429:
428:
424:
421:
419:
415:
412:
411:
407:
404:
401:
400:
386:
372:
368:
364:
360:
359:gravity waves
356:
352:
348:
344:
339:
337:
333:
328:
324:
311:
303:
297:
295:
291:
287:
283:
278:
276:
272:
268:
263:
261:
257:
253:
249:
246:. Unlike the
245:
241:
237:
233:
225:
223:
217:
208:
206:
201:
195:
192:
188:
184:
180:
176:
154:
152:
148:
144:
140:
136:
132:
128:
124:
120:
116:
112:
108:
104:
99:
97:
93:
89:
85:
81:
77:
73:
69:
65:
61:
57:
53:
49:
42:in April 2017
41:
38:taken by the
37:
32:
19:
9417:
9366:
9359:
9352:
9332:
9325:
9265:
9258:
9251:
9226:
9219:
9212:
9206:
9205:
9198:
9191:
9184:
9150:
9034:
9014:
8989:
8963:
8956:
8944:
8935:
8928:
8918:New Horizons
8916:
8907:
8895:
8877:
8746:Ananke group
8600:
8501:Solar System
8412:
8408:
8374:
8370:
8328:
8324:
8308:
8304:
8272:
8268:
8236:
8232:
8200:
8196:
8162:
8158:
8116:
8084:
8080:
8040:
8036:
8007:(1): 74–93.
8004:
8000:
7989:. Retrieved
7951:
7919:
7898:
7880:. Retrieved
7873:the original
7864:
7824:
7818:
7791:
7785:
7740:
7734:
7709:
7703:
7668:
7662:
7633:
7627:
7613:(1): 14–20.
7610:
7604:
7580:
7574:
7550:
7544:
7506:
7480:
7445:
7439:
7409:(1): 12–28.
7406:
7402:
7361:
7357:
7324:
7320:
7303:
7297:
7272:
7266:
7223:
7217:
7186:
7161:
7155:
7125:
7087:
7046:
7040:
6995:
6989:
6946:
6940:
6896:(3–4): 266.
6893:
6887:
6870:
6864:
6839:
6835:
6803:
6799:
6771:
6765:
6738:
6732:
6697:
6686:. Retrieved
6682:the original
6669:
6663:
6618:
6612:
6568:
6562:
6504:
6500:
6460:
6454:
6412:
6406:
6403:Encrenaz, T.
6347:
6343:
6333:
6323:25 September
6321:. Retrieved
6317:the original
6312:
6303:
6296:Beebe (1997)
6291:
6279:
6267:
6255:
6250:, pp. 224–5.
6230:
6224:
6219:, pp. 40–41.
6217:Hockey, 1999
6189:, pp.111–112
6182:
6170:
6158:
6146:
6105:
6101:
6091:
6085:McKim (1997)
6080:
6037:
6033:
6022:
5971:
5967:
5957:
5906:
5902:
5892:
5857:
5853:
5841:
5798:
5794:
5783:
5730:
5726:
5716:
5665:
5661:
5605:
5601:
5591:
5558:
5554:
5544:
5511:
5507:
5497:
5448:
5444:
5434:
5383:
5379:
5369:
5316:
5312:
5302:
5261:
5257:
5250:
5207:
5203:
5192:
5180:
5155:
5117:. Retrieved
5111:
5101:
5090:. Retrieved
5075:
5064:. Retrieved
5037:. Retrieved
5022:
5010:. Retrieved
5006:the original
4995:
4984:. Retrieved
4980:
4956:. Retrieved
4928:. Retrieved
4917:
4906:. Retrieved
4902:the original
4877:. Retrieved
4873:the original
4862:
4853:
4832:
4823:
4804:
4798:
4787:. Retrieved
4783:the original
4772:
4747:
4743:
4737:
4718:
4706:
4699:Beebe (1997)
4679:
4667:
4661:Stone (1974)
4656:
4644:
4633:
4607:. Retrieved
4596:
4584:
4577:Beebe (1997)
4572:
4560:
4548:
4537:. Retrieved
4522:
4511:
4499:
4489:
4483:
4471:
4451:
4444:
4433:. Retrieved
4414:
4403:. Retrieved
4388:
4376:. Retrieved
4370:
4360:
4348:
4336:
4324:. Retrieved
4320:
4311:
4263:
4251:
4240:
4228:
4205:Busse (1976)
4200:
4188:
4176:
4164:
4137:
4125:
4093:
4090:See, e. g.,
4086:
4077:
4042:
4031:
4022:
4016:
4004:
3992:
3980:. Retrieved
3971:
3959:
3948:. Retrieved
3937:
3930:Beebe (1997)
3925:
3913:
3901:
3868:
3856:
3825:
3774:
3770:
3760:
3701:
3697:
3640:
3636:
3626:
3577:
3573:
3563:
3538:
3534:
3524:
3463:
3459:
3449:
3422:
3416:
3404:
3364:
3360:
3350:
3291:
3287:
3277:
3218:
3214:
3204:
3177:. Retrieved
3166:
3157:
3151:
3123:. Retrieved
3119:the original
3104:
3082:Yelle (2004)
3077:
3070:Yelle (2004)
3008:
2960:Yelle (2004)
2888:Yelle (2004)
2883:
2809:
2805:
2794:
2782:. Retrieved
2738:
2734:
2669:
2665:
2658:
2520:
2511:
2417:. Retrieved
2413:Hubble Media
2404:
2395:
2365:
2348:
2339:
2334:
2317:
2311:
2307:gas constant
2300:
2290:
2286:
2282:
2277:
2272:
2179:
2177:
2166:
2150:
2125:
2123:
2107:
2095:Donato Creti
2092:
2084:Robert Hooke
2077:
2069:
2051:
2048:
1988:
1977:
1971:
1965:
1960:
1958:
1954:
1946:
1913:
1897:
1886:
1882:
1869:
1866:Disturbances
1852:
1841:
1837:
1805:
1801:
1784:
1777:
1764:
1758:
1752:
1740:
1708:
1700:
1696:
1677:
1669:
1645:
1641:
1621:
1607:
1605:
1601:
1586:
1573:
1563:
1556:
1540:
1520:
1489:
1476:
1465:
1457:
1421:anticyclones
1410:
1404:New Horizons
1402:
1383:equilibrates
1371:
1348:
1334:
1311:
1297:
1285:Rossby waves
1274:
1265:
1253:
1213:
1209:
1205:
1201:
1197:
1194:
1190:
1174:
1162:
1145:
1138:
1135:
1130:
1121:
1110:
1106:
1064:
1038:Hadley cells
1035:
1003:anticyclonic
997:in belts is
980:
964:
950:
946:
944:
892:
888:stratosphere
844:hydrocarbons
757:
716:
709:
703:
693:
686:
610:
527:
510:
408:Jupiter/Sun
340:
298:
279:
264:
240:thermosphere
236:stratosphere
229:
221:
196:
191:anticyclones
179:anticyclones
172:
150:
146:
138:
115:thermosphere
111:stratosphere
100:
56:Solar System
47:
45:
9361:HD 209458 b
9135:Atmospheres
8858:Exploration
8811:Trojan camp
8751:Carme group
8537:Outer space
8489:Spaceflight
6163:Noll (1995)
5012:October 16,
4750:: 418–425.
4321:www.eso.org
4144:, pp. 14–15
4132:, pp. 16–17
3084:, pp. 22–27
2962:, pp. 15–16
2878:, pp. 13–14
2844:2268/252816
2178:During the
2162:jet streams
2135:White ovals
1812:streamlines
1649:White ovals
1352:1.67 ± 0.09
1308:Deep models
1293:anisotropic
1277:meteorology
1143:encounter.
1088:Ekman layer
1046:downwelling
856:diacetylene
702:(ISO), the
232:troposphere
107:troposphere
66:in roughly
9424:Categories
9345:Exoplanets
8937:Pioneer 11
8930:Pioneer 10
8806:Greek camp
8601:Atmosphere
8364:"Jet sets"
8311:(9): 1190.
7991:2007-06-14
7882:2010-08-21
6688:2008-08-10
5981:2209.00309
5916:2209.00309
5675:2110.09422
5393:2110.09422
5264:: 113405.
5092:2008-05-23
5066:2008-11-29
5039:2008-10-16
4986:2010-06-18
4958:2008-10-16
4930:2007-06-15
4908:2007-01-08
4879:2008-10-16
4789:2007-06-20
4651:, 192–193.
4609:2007-06-15
4539:2009-02-04
4435:2008-06-03
4405:2008-06-03
4245:Low (1966)
4092:Ingersoll
3982:15 October
3950:2010-12-24
3711:2110.07255
3473:1907.01822
3301:2102.10595
3125:2007-05-06
3072:, pp. 1–12
2819:2010.13740
2784:17 January
2388:References
2038:S), while
1951:to Jupiter
1921:Carl Sagan
1900:downdrafts
1808:Beta-drift
1578:jet stream
1318:barotropic
1281:turbulence
1260:convection
1177:retrograde
1140:Pioneer 10
1127:jet stream
995:wind shear
991:retrograde
972:phosphorus
953:The wider
884:tropopause
878:, such as
747:primordial
355:ionosphere
290:lapse rate
286:tropopause
252:mesosphere
185:(GRS) and
9368:Kepler-7b
9354:GJ 1132 b
9311:Enceladus
9063:Mythology
9029:Tianwen-4
9009:Laplace-P
8965:Voyager 2
8958:Voyager 1
8769:Astronomy
8719:Irregular
8594:Geography
8477:Astronomy
8446:blog post
8341:CiteSeerX
7529:219591510
7431:0019-1035
7349:119906560
6928:117677021
6903:1008.0566
6720:224014042
6672:(4): 24.
6603:0032-0633
6581:CiteSeerX
6539:0032-0633
6485:0032-0633
6437:0032-0633
6286:, p. 225.
6274:, p. 226.
6165:, p. 1307
6130:0036-8075
6072:237698857
6064:0094-8276
6014:249810436
6006:0094-8276
5949:249810436
5941:0094-8276
5884:241446672
5833:252099924
5825:2169-9097
5757:0027-8424
5708:236096014
5700:1752-0908
5640:1752-0894
5575:0309-1929
5536:0040-2826
5473:0028-0836
5426:236096014
5418:1752-0894
5361:133852380
5353:2169-9097
5294:202132980
5286:0019-1035
5242:252099924
5234:2169-9097
4839:, p. 223.
4809:, p. 1740
4355:, p. 1979
4343:, p. 1975
4306:, p. 1977
4285:, p. 1978
4235:, p. 1970
4195:, p. 1966
4159:, p. 1949
4011:, p. 235.
3920:, p. 133.
3809:1520-0469
3784:0910.3682
3752:238856819
3744:0094-8276
3673:125905820
3665:0038-6308
3602:0028-0836
3498:1572-9672
3466:(2): 30.
3441:162572802
3342:231985747
3334:0094-8276
3253:0028-0836
3028:, p. 1937
2930:, pp. 5–7
2860:225075904
2852:2169-9100
2779:220980694
2763:1476-4687
2694:0036-8075
2653:, p. 1976
2598:, p. 1974
2562:, pp. 2–5
2258:Voyager 2
2254:Voyager 1
2157:longitude
2127:Voyager 1
2116:Hubble's
2071:Voyager 1
1948:Voyager 1
1879:Hot spots
1824:vorticity
1755:lightning
1684:Amy Simon
1651:, below)
1623:Voyager 2
1589:longitude
1569:cloudtops
1472:longitude
1429:clockwise
1366:petawatts
1364:335 ± 26
1356:heat flux
1042:upwelling
959:latitudes
899:deuterium
852:acetylene
788:phosphine
336:hydrazine
308:)SH) or
244:exosphere
119:exosphere
96:noble gas
9378:See also
9306:Callisto
9301:Ganymede
9260:Makemake
9081:Category
9002:Proposed
8864:missions
8741:Valetudo
8731:Themisto
8710:Callisto
8705:Ganymede
8687:Galilean
8672:Amalthea
8667:Adrastea
8065:43539227
7985:Archived
7948:(1981).
7938:39464951
7849:53596671
7773:33147728
7765:17800430
7695:18216848
7394:37686143
7258:45296656
7250:15319491
7191:Springer
7110:39733730
7071:16281029
7028:11688794
7020:17834994
6981:19024073
6651:28540751
6643:17932285
6547:31037195
6445:11543193
6384:32900956
6298:, p. 43.
6204:, p. 188
6138:13056598
5775:32900956
5481:29516997
5086:Archived
5033:Archived
4952:Archived
4726:Archived
4533:Archived
4429:Archived
4399:Archived
4326:17 April
4076:Heimpel
3932:, p. 24.
3610:10688192
3516:32214508
3261:29516995
3199:, p. 81.
2771:32760043
2710:33147728
2702:17800430
2419:10 April
2382:storms.
2326:≈ 25 m/s
2298:, where
2186:See also
2173:aphelion
1979:Voyagers
1832:latitude
1672:Filipino
1565:Infrared
1437:pressure
1417:cyclones
1413:vortices
1394:Vortices
1220:Dynamics
1166:infrared
1124:prograde
1052:as in a
999:cyclonic
987:prograde
937:A polar
846:such as
800:nitrogen
575:Jupiter
345:, polar
327:abundant
175:cyclones
88:nitrogen
9430:Jupiter
9228:Neptune
9207:Jupiter
9180:Mercury
9172:Planets
9058:Fiction
9051:Related
9016:Shensuo
8946:Ulysses
8909:Galileo
8871:Current
8862:orbital
8821:Impacts
8798:Trojans
8776:General
8574:Jupiter
8525:Science
8513:Weather
8463:Portals
8417:Bibcode
8379:Bibcode
8333:Bibcode
8277:Bibcode
8241:Bibcode
8205:Bibcode
8167:Bibcode
8121:Bibcode
8089:Bibcode
8045:Bibcode
8009:Bibcode
7972:8318939
7829:Bibcode
7796:Bibcode
7745:Bibcode
7736:Science
7714:Bibcode
7673:Bibcode
7638:Bibcode
7615:Bibcode
7585:Bibcode
7555:Bibcode
7488:Longman
7450:Bibcode
7411:Bibcode
7386:7871428
7366:Bibcode
7358:Science
7329:Bibcode
7308:Bibcode
7277:Bibcode
7275:: 391.
7228:Bibcode
7219:Science
7166:Bibcode
7079:4414668
7051:Bibcode
7000:Bibcode
6991:Science
6961:Bibcode
6908:Bibcode
6875:Bibcode
6873:: 495.
6844:Bibcode
6808:Bibcode
6776:Bibcode
6743:Bibcode
6674:Bibcode
6623:Bibcode
6614:Science
6573:Bibcode
6509:Bibcode
6465:Bibcode
6417:Bibcode
6375:7533696
6352:Bibcode
6177:, p. 6.
6110:Bibcode
6102:Science
6042:Bibcode
5986:Bibcode
5921:Bibcode
5862:Bibcode
5803:Bibcode
5766:7533696
5735:Bibcode
5680:Bibcode
5610:Bibcode
5583:2050846
5516:Bibcode
5489:4438233
5453:Bibcode
5398:Bibcode
5321:Bibcode
5266:Bibcode
5212:Bibcode
5119:May 27,
4803:Hammel
4752:Bibcode
4378:May 16,
4021:Rogers
3817:9416783
3789:Bibcode
3716:Bibcode
3645:Bibcode
3618:4381087
3582:Bibcode
3543:Bibcode
3507:7067733
3478:Bibcode
3369:Bibcode
3306:Bibcode
3269:4120368
3223:Bibcode
3179:24 July
2947:, p. 12
2824:Bibcode
2743:Bibcode
2674:Bibcode
2666:Science
2380:polygon
2369:NASA's
2340:Galileo
2305:is the
2180:Voyager
2153:degrees
2147:in 1997
2099:Vatican
2074:in 1979
2052:Galileo
2024:ammonia
2018:in any
1962:Pioneer
1887:Galileo
1848:JunoCam
1766:Cassini
1760:Galileo
1736:JunoCam
1630:Oval BA
1614:Neptune
1574:Voyager
1468:equator
1131:Voyager
836:germane
816:krypton
780:ammonia
764:methane
711:Cassini
705:Galileo
694:Galileo
402:Element
347:aurorae
343:airglow
222:Galileo
187:Oval BA
135:equator
103:Jupiter
76:ammonia
72:methane
54:in the
9334:Triton
9296:Europa
9221:Uranus
9214:Saturn
9039:(2030)
9031:(2029)
9025:(2026)
9019:(2024)
9011:(2023)
8994:(2024)
8977:Future
8700:Europa
8343:
8139:
8063:
8037:Nature
8001:Icarus
7970:
7960:
7936:
7926:
7847:
7771:
7763:
7693:
7664:Nature
7629:Icarus
7527:
7517:
7494:
7441:Icarus
7429:
7403:Icarus
7392:
7384:
7347:
7256:
7248:
7201:
7195:Praxis
7136:
7108:
7098:
7077:
7069:
7042:Nature
7026:
7018:
6979:
6926:
6836:Icarus
6767:Icarus
6718:
6708:
6649:
6641:
6601:
6583:
6545:
6537:
6483:
6443:
6435:
6382:
6372:
6233:(1979)
6231:et al.
6229:Smith
6153:, p. 2
6136:
6128:
6070:
6062:
6040:(14).
6012:
6004:
5974:(15).
5947:
5939:
5909:(15).
5882:
5831:
5823:
5773:
5763:
5755:
5706:
5698:
5638:
5581:
5573:
5534:
5508:Tellus
5487:
5479:
5471:
5445:Nature
5424:
5416:
5359:
5351:
5292:
5284:
5258:Icarus
5240:
5232:
5158:(2008)
5156:et al.
4856:(2006)
4854:et al.
4826:(2001)
4824:et al.
4807:(1995)
4805:et al.
4744:Icarus
4492:(1979)
4490:et al.
4488:Smith
4476:Graney
4459:
4096:(1969)
4094:et al.
4080:(2005)
4078:et al.
4025:(2003)
4023:et al.
3815:
3807:
3750:
3742:
3704:(23).
3671:
3663:
3616:
3608:
3600:
3574:Nature
3535:Icarus
3514:
3504:
3496:
3439:
3429:
3411:(2010)
3409:Graney
3399:, p. 5
3361:Icarus
3340:
3332:
3267:
3259:
3251:
3215:Nature
3160:(2004)
3158:et al.
3156:Kunde
3057:, p. 8
3011:(2004)
3009:et al.
2890:, p. 1
2858:
2850:
2777:
2769:
2761:
2735:Nature
2708:
2700:
2692:
2514:(1998)
2512:et al.
2510:Sieff
2215:(many
2040:oxygen
2030:) and
2006:) and
1748:plumes
1543:Jovian
1212:or an
1200:(EB),
1075:Ferrel
1071:Hadley
1017:. The
976:carbon
968:sulfur
951:belts.
876:comets
866:. The
854:, and
848:ethane
834:) and
828:arsine
808:oxygen
804:sulfur
796:carbon
786:) and
735:helium
733:) and
422:0.0975
94:, and
92:sulfur
82:, and
64:helium
9327:Titan
9316:Dione
9253:Pluto
9247:Ceres
9193:Earth
9186:Venus
9143:Stars
9036:SMARA
8736:Carpo
8677:Thebe
8662:Metis
8655:Inner
8647:Moons
8618:Rings
8450:video
8405:(PDF)
8367:(PDF)
8321:(PDF)
8301:(PDF)
8265:(PDF)
8229:(PDF)
8193:(PDF)
8155:(PDF)
8113:(PDF)
8077:(PDF)
8061:S2CID
8033:(PDF)
7895:(PDF)
7876:(PDF)
7861:(PDF)
7845:S2CID
7769:S2CID
7601:(PDF)
7571:(PDF)
7541:(PDF)
7390:S2CID
7345:S2CID
7254:S2CID
7152:(PDF)
7122:(PDF)
7075:S2CID
7024:S2CID
6977:S2CID
6951:arXiv
6924:S2CID
6898:arXiv
6832:(PDF)
6647:S2CID
6559:(PDF)
6543:S2CID
6497:(PDF)
6068:S2CID
6010:S2CID
5976:arXiv
5945:S2CID
5911:arXiv
5880:S2CID
5829:S2CID
5801:(9).
5704:S2CID
5670:arXiv
5579:S2CID
5485:S2CID
5422:S2CID
5388:arXiv
5357:S2CID
5290:S2CID
5238:S2CID
5210:(9).
4504:Irwin
3813:S2CID
3779:arXiv
3748:S2CID
3706:arXiv
3669:S2CID
3614:S2CID
3468:arXiv
3338:S2CID
3296:arXiv
3294:(9).
3265:S2CID
3007:West
2856:S2CID
2814:arXiv
2775:S2CID
2706:S2CID
2264:Notes
2235:probe
2169:orbit
1893:plume
1889:Probe
1844:JIRAM
1772:power
1704:Earth
1170:ochre
1079:Polar
947:zones
820:xenon
812:argon
760:water
589:0.011
569:Ratio
543:0.82
351:X-ray
151:zones
147:belts
139:jets,
131:zonal
84:water
9390:Coma
9321:Rhea
9286:Moon
9267:Eris
9200:Mars
8889:Past
8879:Juno
8137:ISBN
7968:OCLC
7958:ISBN
7934:OCLC
7924:ISBN
7761:PMID
7691:PMID
7525:OCLC
7515:ISBN
7492:ISBN
7427:ISSN
7382:PMID
7246:PMID
7199:ISBN
7193:and
7134:ISBN
7106:OCLC
7096:ISBN
7067:PMID
7016:PMID
6716:OCLC
6706:ISBN
6639:PMID
6599:ISSN
6535:ISSN
6481:ISSN
6441:PMID
6433:ISSN
6380:PMID
6344:PNAS
6325:2020
6313:NASA
6134:PMID
6126:ISSN
6060:ISSN
6002:ISSN
5937:ISSN
5821:ISSN
5771:PMID
5753:ISSN
5696:ISSN
5636:ISSN
5571:ISSN
5532:ISSN
5477:PMID
5469:ISSN
5414:ISSN
5349:ISSN
5282:ISSN
5230:ISSN
5121:2017
5014:2008
4457:ISBN
4380:2014
4372:NASA
4328:2017
3984:2015
3805:ISSN
3740:ISSN
3661:ISSN
3606:PMID
3598:ISSN
3512:PMID
3494:ISSN
3437:OCLC
3427:ISBN
3330:ISSN
3257:PMID
3249:ISSN
3181:2012
2848:ISSN
2786:2021
2767:PMID
2759:ISSN
2698:PMID
2690:ISSN
2421:2017
2338:The
2233:Juno
2049:The
1970:and
1923:and
1778:Juno
1763:and
1484:wake
1459:Juno
1419:and
1372:The
1247:2010
1235:2009
1077:and
983:jets
974:and
838:(GeH
830:(AsH
824:neon
818:and
778:S),
708:and
349:and
312:((NH
304:((NH
267:bars
242:and
200:Juno
177:and
117:and
62:and
46:The
9152:Sun
8425:doi
8387:doi
8351:doi
8285:doi
8249:doi
8213:doi
8175:doi
8163:102
8129:doi
8097:doi
8053:doi
8041:257
8017:doi
8005:162
7837:doi
7804:doi
7753:doi
7741:204
7722:doi
7710:103
7681:doi
7669:451
7646:doi
7634:149
7611:118
7581:113
7551:111
7466:hdl
7458:doi
7419:doi
7374:doi
7362:267
7337:doi
7325:116
7304:107
7285:doi
7236:doi
7224:305
7174:doi
7059:doi
7047:438
7008:doi
6996:268
6969:doi
6916:doi
6852:doi
6840:208
6816:doi
6784:doi
6751:doi
6670:103
6631:doi
6619:318
6591:doi
6525:hdl
6517:doi
6505:116
6473:doi
6425:doi
6370:PMC
6360:doi
6348:117
6118:doi
6106:117
6050:doi
5994:doi
5929:doi
5870:doi
5811:doi
5799:127
5761:PMC
5743:doi
5731:117
5688:doi
5626:hdl
5618:doi
5563:doi
5559:105
5524:doi
5461:doi
5449:555
5406:doi
5339:hdl
5329:doi
5317:123
5274:doi
5262:335
5220:doi
5208:127
4852:Go
4760:doi
4748:302
3797:doi
3732:hdl
3724:doi
3653:doi
3641:213
3590:doi
3578:403
3551:doi
3539:174
3502:PMC
3486:doi
3464:216
3377:doi
3322:hdl
3314:doi
3239:hdl
3231:doi
3219:555
2840:hdl
2832:doi
2810:125
2751:doi
2739:584
2682:doi
2670:204
2409:ESO
2155:of
2080:GRS
2026:(NH
2010:(CS
913:to
790:(PH
782:(NH
770:),
766:(CH
572:Sun
405:Sun
334:or
9426::
9291:Io
8695:Io
8423:.
8413:63
8411:.
8407:.
8385:.
8375:81
8373:.
8369:.
8349:.
8339:.
8329:60
8327:.
8323:.
8309:84
8307:.
8303:.
8283:.
8273:60
8271:.
8267:.
8247:.
8237:59
8235:.
8231:.
8211:.
8201:53
8199:.
8195:.
8173:.
8161:.
8157:.
8135:.
8127:.
8115:.
8095:.
8085:35
8083:.
8079:.
8059:.
8051:.
8039:.
8035:.
8015:.
8003:.
7966:.
7932:.
7843:.
7835:.
7825:68
7823:.
7802:.
7792:31
7790:.
7784:.
7767:.
7759:.
7751:.
7739:.
7720:.
7708:.
7689:.
7679:.
7667:.
7661:.
7644:.
7632:.
7609:.
7603:.
7579:.
7573:.
7549:.
7543:.
7523:.
7513:.
7464:.
7456:.
7444:.
7425:.
7417:.
7407:84
7405:.
7388:.
7380:.
7372:.
7360:.
7343:.
7335:.
7323:.
7302:.
7283:.
7273:71
7271:.
7252:.
7244:.
7234:.
7222:.
7216:.
7197:.
7189:.
7172:.
7162:26
7160:.
7154:.
7132:.
7104:.
7094:.
7073:.
7065:.
7057:.
7045:.
7039:.
7022:.
7014:.
7006:.
6994:.
6975:.
6967:.
6959:.
6947:47
6945:.
6939:.
6922:.
6914:.
6906:.
6894:19
6892:.
6871:38
6869:.
6850:.
6838:.
6834:.
6814:.
6804:51
6802:.
6782:.
6772:29
6770:.
6749:.
6739:38
6737:.
6731:.
6714:.
6704:.
6668:.
6662:.
6645:.
6637:.
6629:.
6617:.
6597:.
6589:.
6579:.
6569:53
6567:.
6561:.
6541:.
6533:.
6523:.
6515:.
6503:.
6499:.
6479:.
6471:.
6461:51
6459:.
6439:.
6431:.
6423:.
6413:47
6411:.
6378:.
6368:.
6358:.
6346:.
6342:.
6311:.
6240:^
6209:^
6194:^
6132:.
6124:.
6116:.
6104:.
6100:.
6066:.
6058:.
6048:.
6038:48
6036:.
6032:.
6008:.
6000:.
5992:.
5984:.
5972:49
5970:.
5966:.
5943:.
5935:.
5927:.
5919:.
5907:49
5905:.
5901:.
5878:.
5868:.
5860:.
5858:15
5856:.
5852:.
5827:.
5819:.
5809:.
5797:.
5793:.
5769:.
5759:.
5751:.
5741:.
5729:.
5725:.
5702:.
5694:.
5686:.
5678:.
5666:14
5664:.
5660:.
5648:^
5634:.
5624:.
5616:.
5604:.
5600:.
5577:.
5569:.
5557:.
5553:.
5530:.
5522:.
5510:.
5506:.
5483:.
5475:.
5467:.
5459:.
5447:.
5443:.
5420:.
5412:.
5404:.
5396:.
5384:14
5382:.
5378:.
5355:.
5347:.
5337:.
5327:.
5315:.
5311:.
5288:.
5280:.
5272:.
5260:.
5236:.
5228:.
5218:.
5206:.
5202:.
5165:^
5144:^
5129:^
5110:.
5048:^
4979:.
4967:^
4939:^
4888:^
4844:^
4814:^
4758:.
4746:.
4691:^
4618:^
4427:.
4369:.
4319:.
4290:^
4275:^
4211:^
4149:^
4102:^
4068:^
4053:^
3880:^
3837:^
3811:.
3803:.
3795:.
3787:.
3775:67
3773:.
3769:.
3746:.
3738:.
3730:.
3722:.
3714:.
3702:48
3700:.
3696:.
3681:^
3667:.
3659:.
3651:.
3639:.
3635:.
3612:.
3604:.
3596:.
3588:.
3576:.
3572:.
3549:.
3537:.
3533:.
3510:.
3500:.
3492:.
3484:.
3476:.
3462:.
3458:.
3435:.
3389:^
3375:.
3365:29
3363:.
3359:.
3336:.
3328:.
3320:.
3312:.
3304:.
3292:48
3290:.
3286:.
3263:.
3255:.
3247:.
3237:.
3229:.
3217:.
3213:.
3189:^
3134:^
3113:.
3089:^
3062:^
3033:^
3018:^
2999:^
2984:^
2967:^
2952:^
2935:^
2918:^
2895:^
2868:^
2854:.
2846:.
2838:.
2830:.
2822:.
2808:.
2804:.
2773:.
2765:.
2757:.
2749:.
2737:.
2733:.
2718:^
2704:.
2696:.
2688:.
2680:.
2668:.
2639:^
2620:^
2603:^
2584:^
2567:^
2532:^
2492:^
2474:^
2429:^
2407:.
2403:.
2309:,
2291:Mg
2289:/(
2287:RT
2285:=
2283:sh
2278:sh
2256:,
2034:(H
2002:(S
1973:11
1967:10
1927:.
1499:.
1115:,
1073:,
978:.
970:,
870:,
850:,
814:,
802:,
798:,
774:(H
762:,
656:He
652:He
639:Ne
635:Ne
622:Ar
618:Ar
551:/H
537:/H
520:/H
503:/H
489:/H
475:/H
473:Xe
461:/H
459:Kr
447:/H
445:Ar
433:/H
431:Ne
414:He
238:,
234:,
113:,
109:,
90:,
78:,
74:,
9127:e
9120:t
9113:v
8860:,
8566:e
8559:t
8552:v
8465::
8431:.
8427::
8419::
8395:.
8389::
8381::
8357:.
8353::
8335::
8291:.
8287::
8279::
8255:.
8251::
8243::
8219:.
8215::
8207::
8183:.
8177::
8169::
8145:.
8131::
8123::
8103:.
8099::
8091::
8067:.
8055::
8047::
8023:.
8019::
8011::
7994:.
7974:.
7940:.
7905:.
7885:.
7851:.
7839::
7831::
7812:.
7806::
7798::
7775:.
7755::
7747::
7728:.
7724::
7716::
7697:.
7683::
7675::
7652:.
7648::
7640::
7621:.
7617::
7591:.
7587::
7561:.
7557::
7531:.
7500:.
7474:.
7468::
7460::
7452::
7446:5
7433:.
7421::
7413::
7396:.
7376::
7368::
7351:.
7339::
7331::
7314:.
7310::
7291:.
7287::
7279::
7260:.
7238::
7230::
7207:.
7180:.
7176::
7168::
7142:.
7112:.
7081:.
7061::
7053::
7030:.
7010::
7002::
6983:.
6971::
6963::
6953::
6930:.
6918::
6910::
6900::
6881:.
6877::
6858:.
6854::
6846::
6822:.
6818::
6810::
6790:.
6786::
6778::
6759:.
6753::
6745::
6722:.
6691:.
6676::
6653:.
6633::
6625::
6605:.
6593::
6575::
6549:.
6527::
6519::
6511::
6487:.
6475::
6467::
6447:.
6427::
6419::
6386:.
6362::
6354::
6327:.
6140:.
6120::
6112::
6074:.
6052::
6044::
6016:.
5996::
5988::
5978::
5951:.
5931::
5923::
5913::
5886:.
5872::
5864::
5835:.
5813::
5805::
5777:.
5745::
5737::
5710:.
5690::
5682::
5672::
5642:.
5628::
5620::
5612::
5606:8
5585:.
5565::
5538:.
5526::
5518::
5512:8
5491:.
5463::
5455::
5428:.
5408::
5400::
5390::
5363:.
5341::
5331::
5323::
5296:.
5276::
5268::
5244:.
5222::
5214::
5123:.
5095:.
5069:.
5042:.
5016:.
4989:.
4961:.
4933:.
4911:.
4882:.
4792:.
4766:.
4762::
4754::
4612:.
4542:.
4465:.
4438:.
4408:.
4382:.
4330:.
3986:.
3953:.
3819:.
3799::
3791::
3781::
3754:.
3734::
3726::
3718::
3708::
3675:.
3655::
3647::
3620:.
3592::
3584::
3557:.
3553::
3545::
3518:.
3488::
3480::
3470::
3443:.
3383:.
3379::
3371::
3344:.
3324::
3316::
3308::
3298::
3271:.
3241::
3233::
3225::
3183:.
3146:.
3128:.
2994:.
2979:.
2913:.
2862:.
2842::
2834::
2826::
2816::
2788:.
2753::
2745::
2712:.
2684::
2676::
2527:.
2469:.
2423:.
2411:/
2324:j
2322:g
2318:T
2312:M
2301:R
2296:)
2293:j
2229:)
2219:)
2036:2
2028:3
2016:2
2012:2
2004:2
1780:)
1582:K
1456:(
1214:S
1210:N
915:N
911:N
840:4
832:3
792:3
784:3
776:2
768:4
728:2
723:H
721:(
673:H
671:/
669:D
654:/
637:/
620:/
602:N
600:/
598:N
585:C
583:/
581:C
549:S
535:P
518:O
501:N
487:C
418:H
416:/
380:3
375:H
373:(
318:2
316:)
314:4
306:4
271:K
20:)
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.