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Magellanic Clouds

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degree the south pole was, we tooke the day with the soonne, and obserued the nyght with the Astrolabie, and sawe manifestly twoo clowdes of reasonable bygnesse mouynge abowt the place of the pole continually now rysynge and nowe faulynge, so keepynge theyr continuall course in circular mouying, with a starre euer in the myddest which is turned abowt with them abowte xi degrees from the pole." ("Here we saw a marvelous arrangement of stars, so that in the part of heaven opposite our north pole, in order to know in what place and degree the south pole was, we the day using the sun, and observed the night using an
765:(in Latin) From p. 217: "Assecuti sunt Portugallenses alterius poli gradum quintum & quinquagesimum amplius, ubi punctum, circumeuntes quasdam nubeculas licet intueri, veluti in lactea via sparsos fulgores per universum coeli globum intra eius spatii latitudinem." ("The Portuguese reached beyond the 55th degree of the other pole, where one may observe certain nebulae revolving around the point , scattered in the Milky Way like luminous patches throughout the whole sphere of the sky, within the breadth of its extent." ) 449: 346:
in the current observable universe. Since the sizes of relatively nearby galaxies are highly skewed, the average mass can be a misleading statistic. In terms of rank, the LMC appears to be the fourth most massive member of over 50 galaxies in the local group. Suggesting that the Magellanic cloud system is historically not a part of the Milky Way is evidence that the SMC has been in orbit about the LMC for a very long time. The Magellanic system seems most similar to the distinct
2210: 28: 2200: 2248: 1060:(the mean between the maximum and the minimum) of -7.3 m corresponds to a period of 6.6 days. Variable of the period 6.6 days have in the Small Magellanic Cloud a mean photographic star size of 14.5 m. If one assumes — according to the universal yellow color of the δ Cepheid variables — a color index of + 1.5 m, then the corresponding visual star size will equal 13.0 m. This consideration thus leads to a parallax 2272: 2260: 39: 2236: 500:
due to a past interaction with the LMC splitting the SMC, and that the two sections are still moving apart. They have dubbed this smaller remnant the Mini Magellanic Cloud. This hypothesis was confirmed in 2023. The part of the SMC which is closer to Earth lies 196,000 light-years (60 kiloparsecs) away, whereas the farther part lies 215,000 light-years (66 kiloparsecs) away.
1072:= 0.0001", corresponding to a distance of about 3000 light-years. Since the galactic latitude of the Small Magellanic Cloud amounts to about - 45°, then it would lie — according to the foregoing — about 2000 light-years from a plane through our Sun lying parallel to the Milky Way and would have to be regarded as lying outside the Milky Way.) 734: 353:
Astronomers have long assumed that the Magellanic Clouds have orbited the Milky Way at approximately their current distances, but evidence suggests that it is rare for them to come as close to the Milky Way as they are now. Observation and theoretical evidence suggest that the Magellanic Clouds have
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The total mass of these two galaxies is uncertain. Only a fraction of their gas seems to have coalesced into stars and they probably both have large dark matter halos. One recent estimate of the total mass of the LMC is about 1/10 that of the Milky Way. That would make the LMC rather a large galaxy
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Corsali said that his ship had passed the Cape of Good Hope ("the cape of Bona Speranza") and was at 37 degrees south latitude when he observed the Magellanic clouds: "Here we sawe a marueylous order of starres, so that in the parte of heauen contrary to owre northe pole, to know in what place and
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Astrophysicists D. S. Mathewson, V. L. Ford and N. Visvanathan proposed that the SMC may in fact be split in two, with a smaller section of this galaxy behind the main part of the SMC (as seen from Earth's perspective), and separated by about 30,000 light years. They suggest the reason for this is
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From p. 204: "Zunächst ergibt sich eine Parallaxe der kleinen Magellanschen Wolke. ... und als außerhalb der Milchstraße liegend zu betrachten sein." (First, a parallax of the Small Magellanic Cloud follows. According to the 13 δ Cepheid variable that are treated above, the absolute brightness
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in 1994, they were the closest known galaxies to our own. The LMC lies about 160,000 light years away, while the SMC is around 200,000. The LMC is about 70% larger than the diameter of the SMC (32,200 ly and 18,900 ly respectively). For comparison, the Milky Way is about 87,400 ly
824:, and saw clearly two clouds of reasonable bigness revolving around the location of the pole, continually now rising and now falling, thus maintaining their continual course of circular motion, with a star always in the middle , which revolves with them about 11 degrees from the pole.") 308:
to refine the measurement, and these were again revised in 1952 following further research. As of 2023, some astronomers believe the Magellanic Clouds should be renamed, alleging that Magellan was a murderer and neither an astronomer nor the discoverer of the dwarf galaxies.
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interaction with the Milky Way as they travel close to it. The LMC maintains a very clear spiral structure in radio-telescope images of neutral hydrogen. Streams of neutral hydrogen connect them to the Milky Way and to each other, and both resemble disrupted
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From p. 66: "The antarctic pole is not so covered with stars as the arctic, for there are to be seen there many small stars congregated together, which are like to two clouds a little separated from one another, and a little
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and belongs to the leading arm of the Magellanic Clouds. The existence of this star cluster suggests that the leading arm of the Magellanic Clouds is 90,000 light-years away from the Milky Way—closer than previously thought.
416:. If they are in orbit, that orbit takes at least 4 billion years. They are possibly on a first approach and we are witnessing the start of a galactic merger that may overlap with the Milky Way's expected merger with the 916:[Table of the apparent right ascensions and declinations of the southern stars contained within the Tropic of Capricorn; observed at the Cape of Good Hope during the period from 6 August 1751 to 18 July 1752]. 914:"Table des ascensions droites et des déclinaisons apparentes des étoiles australes renfermées dans le tropique cu Capricorne; observées au cap de Bonne-espérance, dans l'intervalle du 6 Août 1751, au 18 Juillet 1752" 231:
did not mention any of this so we do not know if this is true or false." Both Ibn Qutaybah and Al-Sufi were probably quoting from the former's contemporary (and compatriot) and famed scientist
888: 1027:, and the Nebulae, are individuals, and which are themselves composed of stars (either simple, multiple, or in clusters) and of gaseous bodies of both regular and irregular outlines." 288:
studied the Magellanic Clouds from South Africa, writing an 1847 report detailing 919 objects in the Large Magellanic Cloud and 244 objects in the Small Magellanic Cloud. In 1867
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Aside from their different structure and lower mass, they differ from our galaxy in two major ways. They are gas-rich; a higher fraction of their mass is hydrogen and
235:'s mostly lost work on Anwaa. Abu Hanifa was probably quoting earlier sources, which may be just travelers stories, and hence Al-Sufi's comments about their veracity. 1138:"Studies on the colors and magnitudes in stellar clusters. Seventh paper: The distances, distributions in space, and dimensions of 69 globular clusters" 412:
Measurements with the Hubble Space Telescope, announced in 2006, suggest the Magellanic Clouds may be moving too fast to be long term companions of the
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on its circumnavigation of the world in 1519–1522. However, naming the clouds after Magellan did not become widespread until much later. In Bayer's
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Macri, L. M.; et al. (2006). "A New Cepheid Distance to the Maser-Host Galaxy NGC 4258 and Its Implications for the Hubble Constant".
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From 1515 to 1517, Andrea Corsali sailed to the East Indies and China in a Portuguese ship. In 1516, Andrea Corsali sent a letter to
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Histoire de l'Académie Royale des Sciences, avec les Mémoires de Mathématique & de Physique de l'Académie Royale des Sciences
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ALMA antennae bathed in red light. In the background are the southern Milky Way on the left and the Magellanic Clouds at the top.
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there are two stars known as the 'feet of Canopus', and beneath those there are bright white stars that are unseen in
2170: 992: 624: 2165: 1393: 170:وأسفل من سهيل قدما سهيل . وفى مجرى قدمى سهيل، من خلفهما كواكب زهر كبار، لا ترى بالعراق، يسميها أهل تهامة الأعبار 1082: 448: 2010: 1904: 1417: 926:
Planisphere contenant des constellations celestes comprises entre le pole austral et le Tropique du Capricorne
2015: 1812: 1277: 808:(c.1520–1576) and published in 1555. The relevant part of Corsali's letter (translated by Eden) appears in: 69: 816: 2302: 762: 1019:, which is therefore essentially stellar. 3. The visible universe is composed of systems, of which the 879:) appears to the left and below the chart's center and touches the right side of Hydrus the water snake. 2292: 2226: 1820: 1244: 946: 243: 19: 1546:
Mathewson, D. S.; Ford, V. L.; Visvanathan, N. (1986). "The structure of the Small Magellanic Cloud".
1198: 850: 831:, 2nd ed. (New York, New York: Springer Science + Business Media, 2012), § 4.3.2.2 Andreas Corsali, 805: 273: 977:
Results of Astronomical Observations Made During the Years 1834, 5, 6, 7, 8 at the Cape of Good Hope
394:, but as in our own galaxy their stars range from the very young to the very old, indicating a long 2110: 1840: 1802: 923: 913: 787: 177:, there are the feet of Canopus, and on their extension, behind them bright big stars, not seen in 2040: 2005: 1797: 1656: 1580: 292:
suggested that they were separate satellites of the Milky Way. Distances were first estimated by
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Tepper-García, Thor; Bland-Hawthorn, Joss; Pawlowski, Marcel S.; Fritz, Tobias K. (2019-09-01).
1952: 1947: 1594:"A galactic eclipse: the Small Magellanic Cloud is forming stars in two, superimposed systems" 875:) appears below the chart's center and just above the fish Dorado; the Small Magellanic Cloud ( 651: 470: 455: 322: 318: 120: 106: 975: 832: 815:... (Birmingham, England: 1885), "Of the pole antarike and the starres abowt the same ... ", 777: 673: 2180: 2105: 2055: 2050: 1716: 1635: 1213:"'Violent colonialist' Magellan is unfit to keep his place in the night sky, say astronomers" 2297: 2060: 2045: 1914: 1555: 1457: 1325: 1281: 1222: 1107: 1050: 360: 325:, are conspicuous objects in the southern hemisphere, looking like separated pieces of the 92: 868: 378:
compared to the Milky Way. They are also more metal-poor than the Milky Way; the youngest
8: 2276: 2125: 1730: 232: 199: 132: 128: 32: 1559: 1329: 1285: 1111: 1054: 2264: 2252: 2213: 2120: 2075: 1909: 1710: 1649: 1508: 1472: 1341: 1315: 669: 586: 391: 255: 163: 114: 1359: 2199: 2185: 2175: 2000: 1957: 1888: 1873: 1444: 1175: 606: 524: 519: 486: 432: 421: 301: 297: 293: 251: 96: 1376: 1345: 761:(Cologne, (Germany): Geruinum Calenium (Gerwin Calenius), 1574), decade 3, book 1, 544: 2203: 2135: 1995: 1563: 1522: 1333: 1149: 1115: 1095: 1004: 929:
pole and the Tropic of Capricorn]) following p. 592. (The Large Magellanic Cloud (
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From p. 262: "2. The Nebulae resolved and unresolved lie in general without the
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Majaess, Daniel J.; Turner, David G.; Lane, David J.; Henden, Arne; Krajci, Tom
804:, mentioning the Magellanic clouds. This letter was translated into English by 782:
For further details of – and other editions of – Peter Martyr d'Anghiera's book
713: 2130: 2020: 1893: 1845: 1785: 1396:. Jet Propulsion Laboratory, California Institute of Technology. 5 January 2010 428: 395: 330: 305: 289: 247: 1009: 735:"Book of Fixed Stars, Al-Sufi (manuscript written and illustrated by his son)" 2286: 2115: 2070: 1860: 1850: 1780: 1119: 665: 610: 368: 285: 1990: 601: 572: 2240: 2085: 2035: 1967: 1883: 1878: 1790: 1504: 1217: 1194: 155: 62: 1985: 1545: 1269: 1041:[On the spatial distribution of variable of the δ Cepheid type]. 2030: 2025: 1835: 1704: 1698: 1320: 570: 438: 383: 355: 334: 333:
apart in the night sky, the true distance between them is roughly 75,000
260: 88: 1980: 250:, both based on Portuguese voyages. Subsequently, they were reported by 1723: 1593: 204: 144: 27: 367:
has affected the Milky Way as well, distorting the outer parts of the
2145: 2080: 1975: 1898: 1830: 1825: 1684: 1672: 1039:"Über die räumliche Verteilung der Veränderlichen vom δ Cephei-Typus" 821: 769: 754:
For Peter Martyr d'Anghiera's mention of the Magellanic clouds, see:
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of 0.5 and 0.25 times solar, respectively. Both are noted for their
326: 77: 545:"Media Advisory: Virtual Press Conference to Mark ALMA Inauguration" 1737: 1567: 1337: 1154: 591: 406: 347: 152: 2140: 2100: 2095: 1377:"Anchoring the Universal Distance Scale via a Wesenheit Template" 661: 364: 228: 208: 203:, mentioned the same quote, but with a different spelling. Under 194: 174: 1636:
ESO: VISTA Peeks Through the Small Magellanic Cloud’s Dusty Veil
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http://iopscience.iop.org/1538-3881/122/1/220/200523.text.html
1505:"Press release: Magellanic Clouds May Be Just Passing Through" 1381:
Journal of the American Association of Variable Star Observers
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An early possible mention of the Large Magellanic Cloud is in
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The Magellanic clouds are visible to the unaided eye from the
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Leavitt, Henrietta S.; Pickering, Edward C. (March 3, 1912).
573:"The Magellanic System: the puzzle of the leading gas stream" 148: 73: 1641: 1083:"Periods of 25 Variable Stars in the Small Magellanic Cloud" 38: 1174:. Cambridge: Cambridge University Press. pp. 231–232. 379: 242:, the Clouds were reported by 16th century Italian authors 216: 212: 207:, he quoted that "unnamed others have claimed that beneath 178: 2235: 774:
Cosmos: A Sketch of a Physical Description of the Universe
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Encyclopedia of the History of Astronomy and Astrophysics
980:. London, England: Smith, Elder and Co. pp. 151–165. 845:
Pigafetta et al., with Lord Stanley of Alderley, trans.,
549: 1620:(New York: John Wiley & Sons, 1993), pp. 357–8. 1458:
http://home.insightbb.com/~lasweb/lessons/magellanic.htm
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Ferris, Timothy (December 2011). "Dancing in the Dark".
1245:"The Magellanic Clouds must be renamed, astronomers say" 1064:
of the Small Magellanic Cloud, which is given by 5 log
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In 2019, astronomers discovered the young star cluster
2224: 1613:(Englewood Cliffs: Prentice-Hall, 1993), p. 550. 1473:
http://aa.springer.de/papers/8336003/2300925/sc6.htm
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The Large Magellanic Cloud was the host galaxy to a
1592:Murray, Claire E. ; et al. (14 December 2023) 1195:"Astronomers need to rename the Magellanic Clouds" 409:), the brightest observed in over four centuries. 997:Monthly Notices of the Royal Astronomical Society 949:Planisphere contenant les Constellations Celestes 776:(London, England: Henry G. Bohn, 1852), vol. 4, 578:Monthly Notices of the Royal Astronomical Society 350:system, which is on the edge of the Local Group. 2284: 1093: 272:. In the 1756 star map of the French astronomer 937:) appear just below the center of the diagram.) 902:U.S. Naval Observatory; retrieved on 2009-09-05 714:"Observatoire de Paris (Abd-al-Rahman Al Sufi)" 197:, a professional astronomer, in 964 CE, in his 1583:The Astronomical Journal 122:220–231 July 2001 494: 304:. Recalibration of the Cepheid scales allowed 1657: 1299: 993:"On the distribution of the nebulae in space" 847:The First Voyage Round the World, by Magellan 829:Star Maps: History, Artistry, and Cartography 510:Astronomical surveys of the Magellanic Clouds 1352: 1270:"A Cosmic Zoo in the Large Magellanic Cloud" 1163: 911: 650: 123:(SMC), about 206 kly (63 kpc) away 1369: 1364:Annual Review of Astronomy and Astrophysics 1274:European Southern Observatory Press Release 1169: 1036: 964:Linda Hall Library; retrieved on 2009-09-05 849:(London, England: Hakluyt Society, 1874), 284:("the Large Cloud" and "the Small Cloud"). 151:. They may be the objects mentioned by the 1664: 1650: 625:"Magellanic System | UW-Madison Astronomy" 1319: 1242: 1153: 1008: 600: 590: 16:Two dwarf galaxies orbiting the Milky Way 1098:[Reports about variable stars]. 1096:"Mitteilungen über veränderliche Sterne" 973: 867:. Augsburg, (Germany): Christoph Mang. 813:The First Three English Books on America 37: 26: 18: 1746:) may be read as "within" or "part of". 1437:"The Large and Small Magellanic Clouds" 1135: 1094:Pickering, E.C.; Wendell, O.C. (1912). 646: 644: 131:, but cannot be observed from the most 31:Small and Large Magellanic Clouds over 2285: 1414: 1243:Ravisetti, Monisha (3 November 2023). 811:Richard Eden, with Edward Arber, ed., 1645: 1358:Freedman, Wendy L.; Madore, Barry F. 1305: 1210: 953:Memoires Academie Royale des Sciences 23:The Large and Small Magellanic Clouds 1087:Harvard College Observatory Circular 1068:= -7.3 - 13.0 = -20.3. One obtains 990: 802:Giuliano de' Medici, Duke of Nemours 641: 321:and its neighbour and relative, the 254:, who accompanied the expedition of 102:The two galaxies are the following: 1197:Mia de los Reyes 12 September 2023 339:Sagittarius Dwarf Elliptical Galaxy 296:in 1913 using 1912 measurements of 13: 1752: 1638:—including photos & animations 1609:Eric Chaisson and Steve McMillan, 933:) and the Small Magellanic Cloud ( 657:Star Names: Their Lore and Meaning 489:data with foreground stars removed 312: 14: 2314: 1624: 1211:McKie, Robin (12 November 2023). 757:Petrus Martyr de Anghiera (1574) 437:data. The star cluster has a low 95:, they are often reclassified as 2270: 2258: 2246: 2234: 2209: 2208: 2198: 478: 463: 447: 1631:Magellanic Clouds Working Group 1586: 1574: 1539: 1515: 1497: 1488: 1466: 1451: 1429: 1408: 1386: 1262: 1236: 1204: 1188: 1129: 1075: 1030: 984: 967: 940: 905: 882: 857: 839: 759:De rebus Oceanicis et Orbe Novo 354:both been greatly distorted by 91:. Because both show signs of a 1523:"IoW_20200109 - Gaia - Cosmos" 794: 768:Humboldt, Alexander von, with 748: 727: 706: 680: 617: 564: 537: 219:, and that the inhabitants of 1: 2171:Andromeda–Milky Way collision 1671: 1278:European Southern Observatory 530: 337:. Until the discovery of the 162:(the stations of the Moon in 70:southern celestial hemisphere 1201:; retrieved 12 November 2023 974:Herschel, John F.W. (1847). 871:The Large Magellanic Cloud ( 786:, see Knowledge's article: 329:to the naked eye. Roughly 21 158:(d. 889 CE), in his book on 7: 1170:Leverington, David (2013). 947:de Lacaille, N. L., (1756) 503: 495:Mini Magellanic Cloud (MMC) 147:and rock drawings found in 10: 2319: 1603: 485:LMC and SMC rendered from 382:in the LMC and SMC have a 138: 2194: 2158: 1966: 1938: 1927: 1859: 1811: 1803:Galactic Center filaments 1771: 1764: 1750: 1679: 1548:The Astrophysical Journal 1308:The Astrophysical Journal 1199:American Physical Society 1142:The Astrophysical Journal 1100:Astronomische Nachrichten 1043:Astronomische Nachrichten 276:, they are designated as 1394:"Little Galaxy Explored" 1136:Shapley, Harlow (1918). 1120:10.1002/asna.19121921303 1037:Hertzsprung, E. (1913). 991:Abbe, Cleveland (1867). 827:See also: Kanas, Nick, 788:Decades of the New World 688:"Al-Anwaa, Ibn Qutaybah" 1798:Supermassive black hole 1485:Retrieved on 2007-05-31 1463:Retrieved on 2007-05-31 1092:Summarized in German: 1010:10.1093/mnras/27.7.257a 772:and B.H. Paul, trans., 264:they are designated as 244:Peter Martyr d'Anghiera 2091:Sagittarius Spheroidal 1953:Small Magellanic Cloud 1948:Large Magellanic Cloud 1905:Pisces-Eridanus stream 1758: 471:Small Magellanic Cloud 456:Large Magellanic Cloud 361:barred spiral galaxies 323:Small Magellanic Cloud 319:Large Magellanic Cloud 191: 121:Small Magellanic Cloud 109:(LMC), about 163  107:Large Magellanic Cloud 43: 35: 24: 1756: 1717:Laniakea Supercluster 1494:Chaisson and McMillan 1360:"The Hubble Constant" 920:(in French): 539–592. 912:de la Caille (1752). 602:10.1093/mnras/stz1659 168: 41: 30: 22: 1757:The Milky Way Galaxy 1618:Conceptual Astronomy 1223:Guardian Media Group 863:Bayer Johann (1603) 1731:Observable universe 1560:1986ApJ...301..664M 1418:National Geographic 1330:2006ApJ...652.1133M 1286:2010eso..pres...21. 1280:: 21. 1 June 2010. 1112:1912AN....192..219P 1055:1913AN....196..201H 392:stellar populations 233:Abu Hanifa Dinawari 200:Book of Fixed Stars 164:pre-Islamic Arabian 129:Southern Hemisphere 87:are members of the 56:Nubeculae Magellani 33:Paranal Observatory 2303:Milky Way Subgroup 2076:Pisces Overdensity 1910:Sagittarius Stream 1821:Carina–Sagittarius 1759: 1711:Virgo Supercluster 1692:Milky Way subgroup 1527:www.cosmos.esa.int 1511:. January 9, 2007. 1509:Harvard University 1478:2007-06-07 at the 1461:Home.insightbb.com 960:2009-05-09 at the 898:2011-07-22 at the 889:Bayer, J., (1661) 670:Dover Publications 256:Ferdinand Magellan 133:northern latitudes 85:satellite galaxies 44: 36: 25: 2293:Magellanic Clouds 2222: 2221: 2186:Zone of Avoidance 2154: 2153: 2001:Canes Venatici II 1958:Magellanic Bridge 1940:Magellanic Clouds 1923: 1922: 1889:Magellanic Stream 1874:Fimbulthul stream 1447:on July 15, 2005. 1181:978-0-521-89994-9 1049:(4692): 201–208. 525:Magellanic Stream 520:Magellanic Bridge 424:) in the future. 422:Triangulum Galaxy 420:(and perhaps the 396:stellar formation 302:Henrietta Leavitt 298:Cepheid variables 294:Ejnar Hertzsprung 252:Antonio Pigafetta 97:Magellanic spiral 52:Magellanic system 48:Magellanic Clouds 2310: 2275: 2274: 2273: 2263: 2262: 2261: 2251: 2250: 2249: 2239: 2238: 2230: 2212: 2211: 2204:Astronomy portal 2202: 1996:Canes Venatici I 1936: 1935: 1841:Scutum–Centaurus 1769: 1768: 1747: 1745: 1736: 1729: 1722: 1715: 1709: 1703: 1697: 1690: 1666: 1659: 1652: 1643: 1642: 1616:Michael Zeilik, 1597: 1590: 1584: 1578: 1572: 1571: 1543: 1537: 1536: 1534: 1533: 1519: 1513: 1512: 1501: 1495: 1492: 1486: 1470: 1464: 1455: 1449: 1448: 1443:. Archived from 1433: 1427: 1426: 1412: 1406: 1405: 1403: 1401: 1390: 1384: 1373: 1367: 1356: 1350: 1349: 1323: 1321:astro-ph/0608211 1314:(2): 1133–1149. 1303: 1297: 1296: 1294: 1292: 1266: 1260: 1259: 1257: 1255: 1240: 1234: 1233: 1231: 1229: 1208: 1202: 1192: 1186: 1185: 1167: 1161: 1159: 1157: 1133: 1127: 1124:See pp. 225-226. 1123: 1079: 1073: 1058: 1034: 1028: 1014: 1012: 988: 982: 981: 971: 965: 944: 938: 921: 909: 903: 886: 880: 861: 855: 843: 837: 798: 792: 752: 746: 745: 743: 741: 731: 725: 724: 722: 720: 710: 704: 703: 701: 699: 690:. Archived from 684: 678: 677: 648: 639: 638: 636: 635: 621: 615: 614: 604: 594: 568: 562: 561: 559: 557: 541: 515:Irregular galaxy 482: 467: 451: 418:Andromeda Galaxy 181:, the people of 2318: 2317: 2313: 2312: 2311: 2309: 2308: 2307: 2283: 2282: 2281: 2271: 2269: 2259: 2257: 2247: 2245: 2233: 2225: 2223: 2218: 2190: 2166:Alternate names 2150: 1962: 1930: 1919: 1869:Aquarius Stream 1855: 1807: 1773:Galactic Center 1760: 1748: 1743: 1741: 1740: 1734: 1727: 1720: 1713: 1707: 1701: 1695: 1688: 1675: 1670: 1627: 1611:Astronomy Today 1606: 1601: 1600: 1591: 1587: 1579: 1575: 1544: 1540: 1531: 1529: 1521: 1520: 1516: 1503: 1502: 1498: 1493: 1489: 1480:Wayback Machine 1471: 1467: 1456: 1452: 1435: 1434: 1430: 1413: 1409: 1399: 1397: 1392: 1391: 1387: 1374: 1370: 1357: 1353: 1304: 1300: 1290: 1288: 1268: 1267: 1263: 1253: 1251: 1241: 1237: 1227: 1225: 1209: 1205: 1193: 1189: 1182: 1168: 1164: 1134: 1130: 1106:(13): 219–226. 1080: 1076: 1035: 1031: 989: 985: 972: 968: 962:Wayback Machine 945: 941: 910: 906: 900:Wayback Machine 887: 883: 862: 858: 844: 840: 799: 795: 753: 749: 739: 737: 733: 732: 728: 718: 716: 712: 711: 707: 697: 695: 694:on 24 July 2017 686: 685: 681: 649: 642: 633: 631: 623: 622: 618: 569: 565: 555: 553: 543: 542: 538: 533: 506: 497: 490: 483: 474: 468: 459: 452: 315: 313:Characteristics 141: 17: 12: 11: 5: 2316: 2306: 2305: 2300: 2295: 2280: 2279: 2267: 2255: 2243: 2220: 2219: 2217: 2216: 2206: 2195: 2192: 2191: 2189: 2188: 2183: 2178: 2176:Baade's Window 2173: 2168: 2162: 2160: 2156: 2155: 2152: 2151: 2149: 2148: 2143: 2138: 2133: 2131:Ursa Major III 2128: 2123: 2118: 2113: 2108: 2103: 2098: 2093: 2088: 2083: 2078: 2073: 2068: 2063: 2058: 2053: 2048: 2043: 2038: 2033: 2028: 2023: 2018: 2016:Coma Berenices 2013: 2008: 2003: 1998: 1993: 1988: 1983: 1978: 1972: 1970: 1964: 1963: 1961: 1960: 1955: 1950: 1944: 1942: 1933: 1925: 1924: 1921: 1920: 1918: 1917: 1912: 1907: 1902: 1896: 1894:Monoceros Ring 1891: 1886: 1881: 1876: 1871: 1865: 1863: 1857: 1856: 1854: 1853: 1848: 1846:Near 3 kpc Arm 1843: 1838: 1833: 1828: 1823: 1817: 1815: 1809: 1808: 1806: 1805: 1800: 1795: 1794: 1793: 1786:Sagittarius A* 1783: 1777: 1775: 1766: 1762: 1761: 1751: 1749: 1683: 1681: 1677: 1676: 1669: 1668: 1661: 1654: 1646: 1640: 1639: 1633: 1626: 1625:External links 1623: 1622: 1621: 1614: 1605: 1602: 1599: 1598: 1585: 1573: 1568:10.1086/163932 1538: 1514: 1496: 1487: 1483:Aa.springer.de 1465: 1450: 1428: 1407: 1385: 1368: 1351: 1338:10.1086/508530 1298: 1261: 1235: 1203: 1187: 1180: 1162: 1155:10.1086/142423 1128: 1126: 1125: 1074: 1029: 1003:(7): 257–264. 983: 966: 939: 935:Le Petit Nuage 931:Le Grand Nuage 904: 893:, pl. Aaa (49) 881: 877:Nubecula minor 873:Nubecula major 869:Star chart 49. 856: 838: 836: 835: 825: 793: 791: 790: 780: 766: 747: 726: 705: 679: 672:Inc. pp.  640: 629:astro.wisc.edu 616: 585:(1): 918–938. 563: 535: 534: 532: 529: 528: 527: 522: 517: 512: 505: 502: 496: 493: 492: 491: 484: 477: 475: 469: 462: 460: 453: 446: 429:Price-Whelan 1 314: 311: 306:Harlow Shapley 300:in the SMC by 290:Cleveland Abbe 282:le Petit Nuage 278:le Grand Nuage 270:nubecula minor 266:nubecula major 248:Andrea Corsali 140: 137: 125: 124: 118: 15: 9: 6: 4: 3: 2: 2315: 2304: 2301: 2299: 2296: 2294: 2291: 2290: 2288: 2278: 2268: 2266: 2256: 2254: 2244: 2242: 2237: 2232: 2231: 2228: 2215: 2207: 2205: 2201: 2197: 2196: 2193: 2187: 2184: 2182: 2179: 2177: 2174: 2172: 2169: 2167: 2164: 2163: 2161: 2157: 2147: 2144: 2142: 2139: 2137: 2134: 2132: 2129: 2127: 2126:Ursa Major II 2124: 2122: 2119: 2117: 2116:Triangulum II 2114: 2112: 2109: 2107: 2104: 2102: 2099: 2097: 2094: 2092: 2089: 2087: 2084: 2082: 2079: 2077: 2074: 2072: 2069: 2067: 2064: 2062: 2059: 2057: 2054: 2052: 2049: 2047: 2044: 2042: 2039: 2037: 2034: 2032: 2029: 2027: 2024: 2022: 2019: 2017: 2014: 2012: 2009: 2007: 2004: 2002: 1999: 1997: 1994: 1992: 1989: 1987: 1984: 1982: 1979: 1977: 1974: 1973: 1971: 1969: 1965: 1959: 1956: 1954: 1951: 1949: 1946: 1945: 1943: 1941: 1937: 1934: 1932: 1926: 1916: 1913: 1911: 1908: 1906: 1903: 1900: 1897: 1895: 1892: 1890: 1887: 1885: 1882: 1880: 1877: 1875: 1872: 1870: 1867: 1866: 1864: 1862: 1858: 1852: 1851:Far 3 kpc Arm 1849: 1847: 1844: 1842: 1839: 1837: 1834: 1832: 1829: 1827: 1824: 1822: 1819: 1818: 1816: 1814: 1810: 1804: 1801: 1799: 1796: 1792: 1791:Fermi bubbles 1789: 1788: 1787: 1784: 1782: 1781:Sagittarius A 1779: 1778: 1776: 1774: 1770: 1767: 1763: 1755: 1739: 1732: 1725: 1718: 1712: 1706: 1700: 1693: 1686: 1682: 1678: 1674: 1667: 1662: 1660: 1655: 1653: 1648: 1647: 1644: 1637: 1634: 1632: 1629: 1628: 1619: 1615: 1612: 1608: 1607: 1595: 1589: 1582: 1577: 1569: 1565: 1561: 1557: 1553: 1549: 1542: 1528: 1524: 1518: 1510: 1506: 1500: 1491: 1484: 1481: 1477: 1474: 1469: 1462: 1459: 1454: 1446: 1442: 1441:www.mq.edu.au 1438: 1432: 1424: 1420: 1419: 1411: 1395: 1389: 1382: 1378: 1372: 1365: 1361: 1355: 1347: 1343: 1339: 1335: 1331: 1327: 1322: 1317: 1313: 1309: 1302: 1287: 1283: 1279: 1275: 1271: 1265: 1250: 1246: 1239: 1224: 1220: 1219: 1214: 1207: 1200: 1196: 1191: 1183: 1177: 1173: 1166: 1156: 1151: 1147: 1143: 1139: 1132: 1121: 1117: 1113: 1109: 1105: 1102:(in German). 1101: 1097: 1091: 1090: 1088: 1084: 1078: 1071: 1067: 1063: 1056: 1052: 1048: 1045:(in German). 1044: 1040: 1033: 1026: 1022: 1018: 1011: 1006: 1002: 998: 994: 987: 979: 978: 970: 963: 959: 956: 954: 950: 943: 936: 932: 928: 927: 919: 915: 908: 901: 897: 894: 892: 885: 878: 874: 870: 866: 860: 852: 848: 842: 834: 830: 826: 823: 818: 814: 810: 809: 807: 803: 797: 789: 785: 781: 779: 775: 771: 767: 764: 760: 756: 755: 751: 736: 730: 715: 709: 693: 689: 683: 675: 671: 667: 663: 659: 658: 653: 647: 645: 630: 626: 620: 612: 608: 603: 598: 593: 588: 584: 580: 579: 574: 567: 552: 551: 546: 540: 536: 526: 523: 521: 518: 516: 513: 511: 508: 507: 501: 488: 481: 476: 472: 466: 461: 457: 450: 445: 444: 443: 440: 436: 435: 430: 425: 423: 419: 415: 410: 408: 404: 399: 397: 393: 389: 385: 381: 377: 372: 370: 369:galactic disk 366: 362: 357: 351: 349: 343: 340: 336: 332: 328: 324: 320: 310: 307: 303: 299: 295: 291: 287: 286:John Herschel 283: 279: 275: 271: 267: 263: 262: 257: 253: 249: 245: 241: 236: 234: 230: 226: 222: 218: 214: 210: 206: 202: 201: 196: 190: 188: 184: 180: 176: 171: 167: 165: 161: 157: 154: 150: 146: 136: 134: 130: 122: 119: 116: 112: 108: 105: 104: 103: 100: 98: 94: 93:bar structure 90: 86: 82: 79: 75: 71: 67: 64: 61: 57: 53: 49: 40: 34: 29: 21: 2277:Solar System 2181:In mythology 2121:Ursa Major I 2086:Reticulum II 1939: 1915:Virgo Stream 1884:Helmi stream 1879:Gaia Sausage 1831:Orion–Cygnus 1826:Norma–Cygnus 1742:Each arrow ( 1617: 1610: 1588: 1576: 1551: 1547: 1541: 1530:. Retrieved 1526: 1517: 1499: 1490: 1482: 1468: 1460: 1453: 1445:the original 1440: 1431: 1422: 1416: 1410: 1398:. Retrieved 1388: 1380: 1371: 1363: 1354: 1311: 1307: 1301: 1273: 1264: 1252:. Retrieved 1248: 1238: 1226:. Retrieved 1218:The Observer 1216: 1206: 1190: 1171: 1165: 1145: 1141: 1131: 1103: 1099: 1086: 1077: 1069: 1065: 1061: 1046: 1042: 1032: 1024: 1020: 1016: 1000: 996: 986: 976: 969: 952: 948: 942: 934: 930: 925: 917: 907: 890: 884: 876: 872: 864: 859: 846: 841: 828: 812: 806:Richard Eden 796: 784:De Orbe Novo 783: 778:pp. 340–341. 773: 758: 750: 738:. Retrieved 729: 717:. Retrieved 708: 696:. Retrieved 692:the original 682: 664: ed.). 656: 652:Allen, R. H. 632:. Retrieved 628: 619: 582: 576: 566: 554:. Retrieved 548: 539: 498: 433: 426: 411: 400: 373: 352: 344: 316: 281: 277: 269: 265: 259: 237: 224: 198: 192: 186: 172: 169: 159: 156:Ibn Qutaybah 142: 126: 101: 55: 51: 47: 45: 2298:Local Group 2265:Outer space 2253:Spaceflight 2031:Eridanus II 2006:Canis Major 1705:Local Sheet 1699:Local Group 1254:12 November 1228:12 November 1160:See p. 155. 1148:: 154–181. 891:Uranometria 865:Uranometria 439:metallicity 384:metallicity 335:light-years 261:Uranometria 145:petroglyphs 89:Local Group 2287:Categories 2136:Ursa Minor 1991:Boötes III 1724:Local Hole 1532:2020-01-09 1289:Retrieved 1023:, the two 1021:Via Lactea 1017:Via Lactea 955:pour 1752. 854:dimmed..." 634:2022-06-14 592:1901.05636 531:References 390:and young 223:call them 205:Argo Navis 185:call them 173:And below 166:culture): 99:galaxies. 58:) are two 2146:Willman 1 2081:Pisces II 1986:Boötes II 1976:Antlia II 1929:Satellite 1899:Palomar 5 1765:Structure 1685:Milky Way 1673:Milky Way 1596:arxiv.org 1425:(6): 118. 1400:29 August 1291:29 August 1249:Space.com 1089:no. 173. 1025:Nubeculae 822:astrolabe 770:E.C. Otte 611:0035-8711 487:Gaia EDR3 414:Milky Way 403:supernova 398:history. 327:Milky Way 160:Al-Anwā̵’ 113:(50  78:Milky Way 60:irregular 2214:Category 2106:Sculptor 2041:Hercules 2021:Crater 2 1981:Boötes I 1931:galaxies 1738:Universe 1680:Location 1476:Archived 1346:15728812 958:Archived 922:See the 896:Archived 666:New York 654:(1963). 504:See also 407:SN 1987A 363:. Their 348:NGC 3109 342:across. 274:Lacaille 225:al-Baqar 187:al-a‘bār 153:polymath 83:, these 74:Orbiting 66:galaxies 2227:Portals 2159:Related 2141:Virgo I 2111:Sextans 2101:Segue 2 2096:Segue 1 2071:Phoenix 1836:Perseus 1604:Sources 1556:Bibcode 1554:: 664. 1326:Bibcode 1282:Bibcode 1108:Bibcode 1051:Bibcode 924:plate ( 833:p. 118. 817:p. 279. 763:p. 217. 719:22 July 674:294–295 662:Reprint 556:3 April 388:nebulae 365:gravity 229:Ptolemy 209:Canopus 195:Al Sufi 175:Canopus 139:History 68:in the 2056:Leo IV 2051:Leo II 2036:Fornax 2011:Carina 1968:Dwarfs 1901:stream 1733:  1726:  1719:  1694:  1687:  1383:, 2010 1366:, 2010 1344:  1178:  851:p. 66. 740:22 Feb 609:  473:(SMC). 458:(LMC). 431:using 376:helium 240:Europe 227:, and 221:Tihama 193:Later 183:Tihama 117:) away 81:galaxy 2241:Stars 2066:Leo T 2061:Leo V 2046:Leo I 2026:Draco 1342:S2CID 1316:arXiv 698:4 Sep 587:arXiv 380:stars 356:tidal 149:Chile 63:dwarf 1861:Halo 1813:Disk 1402:2010 1293:2010 1256:2023 1230:2023 1176:ISBN 742:2017 721:2011 700:2017 607:ISSN 558:2013 454:The 434:Gaia 317:The 280:and 268:and 246:and 217:Najd 215:nor 213:Iraq 179:Iraq 76:the 46:The 1564:doi 1552:301 1423:220 1334:doi 1312:652 1150:doi 1116:doi 1104:192 1047:196 1005:doi 597:doi 583:488 550:ESO 238:In 115:kpc 111:kly 54:or 2289:: 1562:. 1550:. 1525:. 1507:. 1439:. 1421:. 1379:, 1362:, 1340:. 1332:. 1324:. 1310:. 1276:. 1272:. 1247:. 1221:. 1215:. 1146:48 1144:. 1140:. 1114:. 1085:. 1001:27 999:. 995:. 951:, 668:: 643:^ 627:. 605:. 595:. 581:. 575:. 547:. 371:. 135:. 72:. 2229:: 1744:→ 1735:→ 1728:→ 1721:→ 1714:→ 1708:→ 1702:→ 1696:→ 1689:→ 1665:e 1658:t 1651:v 1570:. 1566:: 1558:: 1535:. 1404:. 1348:. 1336:: 1328:: 1318:: 1295:. 1284:: 1258:. 1232:. 1184:. 1158:. 1152:: 1122:. 1118:: 1110:: 1070:p 1066:p 1062:p 1057:. 1053:: 1013:. 1007:: 744:. 723:. 702:. 676:. 660:( 637:. 613:. 599:: 589:: 560:. 405:( 331:° 189:. 50:(

Index



Paranal Observatory

irregular
dwarf
galaxies
southern celestial hemisphere
Orbiting
Milky Way
galaxy
satellite galaxies
Local Group
bar structure
Magellanic spiral
Large Magellanic Cloud
kly
kpc
Small Magellanic Cloud
Southern Hemisphere
northern latitudes
petroglyphs
Chile
polymath
Ibn Qutaybah
pre-Islamic Arabian
Canopus
Iraq
Tihama
Al Sufi

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