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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
776:(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." ) 460: 357:
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
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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.
1083:= 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.) 745: 364:
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
835:, 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.") 319:
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.
427:. 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 927:[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]. 925:"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" 242:
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
899: 1038:, 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." 299:
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
246:'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. 1149:"Studies on the colors and magnitudes in stellar clusters. Seventh paper: The distances, distributions in space, and dimensions of 69 globular clusters" 423:
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
2176: 1003: 17: 635: 2171: 1404: 181:وأسفل من سهيل قدما سهيل . وفى مجرى قدمى سهيل، من خلفهما كواكب زهر كبار، لا ترى بالعراق، يسميها أهل تهامة الأعبار 1093: 459: 2016: 1910: 1428: 937:
Planisphere contenant des constellations celestes comprises entre le pole austral et le Tropique du Capricorne
2021: 1818: 1288: 819:(c.1520–1576) and published in 1555. The relevant part of Corsali's letter (translated by Eden) appears in: 80: 827: 2308: 773: 1030:, which is therefore essentially stellar. 3. The visible universe is composed of systems, of which the 890:) appears to the left and below the chart's center and touches the right side of Hydrus the water snake. 2298: 2232: 1826: 1255: 957: 254: 30: 1557:
Mathewson, D. S.; Ford, V. L.; Visvanathan, N. (1986). "The structure of the Small Magellanic Cloud".
1209: 861: 842:, 2nd ed. (New York, New York: Springer Science + Business Media, 2012), § 4.3.2.2 Andreas Corsali, 816: 284: 988:
Results of Astronomical Observations Made During the Years 1834, 5, 6, 7, 8 at the Cape of Good Hope
405:, but as in our own galaxy their stars range from the very young to the very old, indicating a long 2116: 1846: 934: 924: 798: 188:, there are the feet of Canopus, and on their extension, behind them bright big stars, not seen in 2046: 2011: 1808: 1667: 1591: 303:
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).
1958: 1953: 1605:"A galactic eclipse: the Small Magellanic Cloud is forming stars in two, superimposed systems" 886:) appears below the chart's center and just above the fish Dorado; the Small Magellanic Cloud ( 662: 481: 466: 333: 329: 131: 117: 986: 843: 826:... (Birmingham, England: 1885), "Of the pole antarike and the starres abowt the same ... ", 788: 684: 2186: 2111: 2061: 2056: 1727: 1646: 1224:"'Violent colonialist' Magellan is unfit to keep his place in the night sky, say astronomers" 2303: 2066: 2051: 1920: 1566: 1468: 1336: 1292: 1233: 1118: 1061: 371: 336:, are conspicuous objects in the southern hemisphere, looking like separated pieces of the 103: 879: 389:
compared to the Milky Way. They are also more metal-poor than the Milky Way; the youngest
8: 2282: 2131: 1741: 243: 210: 143: 139: 43: 1570: 1340: 1296: 1122: 1065: 2270: 2258: 2219: 2126: 2081: 1915: 1721: 1660: 1519: 1483: 1352: 1326: 680: 597: 402: 266: 174: 125: 1370: 2205: 2191: 2181: 2006: 1963: 1894: 1879: 1455: 1186: 617: 535: 530: 497: 443: 432: 312: 308: 304: 262: 107: 1387: 1356: 772:(Cologne, (Germany): Geruinum Calenium (Gerwin Calenius), 1574), decade 3, book 1, 555: 2209: 2141: 2001: 1574: 1533: 1344: 1160: 1126: 1106: 1015: 940:
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
815:, mentioning the Magellanic clouds. This letter was translated into English by 793:
For further details of – and other editions of – Peter Martyr d'Anghiera's book
724: 2136: 2026: 1899: 1851: 1796: 1407:. Jet Propulsion Laboratory, California Institute of Technology. 5 January 2010 439: 406: 341: 316: 300: 258: 1020: 746:"Book of Fixed Stars, Al-Sufi (manuscript written and illustrated by his son)" 2292: 2121: 2076: 1866: 1856: 1791: 1130: 676: 621: 379: 296: 1996: 612: 583: 2246: 2091: 2041: 1973: 1889: 1884: 1801: 1515: 1228: 1205: 166: 73: 1991: 1556: 1280: 1052:[On the spatial distribution of variable of the δ Cepheid type]. 2036: 2031: 1841: 1715: 1709: 1331: 581: 449: 394: 366: 345: 344:
apart in the night sky, the true distance between them is roughly 75,000
271: 99: 1986: 261:, both based on Portuguese voyages. Subsequently, they were reported by 1734: 1604: 215: 155: 38: 378:
has affected the Milky Way as well, distorting the outer parts of the
2151: 2086: 1981: 1904: 1836: 1831: 1695: 1683: 1050:"Über die räumliche Verteilung der Veränderlichen vom δ Cephei-Typus" 832: 780: 765:
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
337: 88: 556:"Media Advisory: Virtual Press Conference to Mark ALMA Inauguration" 1748: 1578: 1348: 1165: 602: 417: 358: 163: 2146: 2106: 2101: 1388:"Anchoring the Universal Distance Scale via a Wesenheit Template" 672: 375: 239: 219: 214:, mentioned the same quote, but with a different spelling. Under 205: 185: 1647:
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
1516:"Press release: Magellanic Clouds May Be Just Passing Through" 1392:
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).
584:"The Magellanic System: the puzzle of the leading gas stream" 159: 84: 1652: 1094:"Periods of 25 Variable Stars in the Small Magellanic Cloud" 49: 1185:. Cambridge: Cambridge University Press. pp. 231–232. 390: 253:, the Clouds were reported by 16th century Italian authors 227: 223: 218:, he quoted that "unnamed others have claimed that beneath 189: 2241: 785:
Cosmos: A Sketch of a Physical Description of the Universe
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Encyclopedia of the History of Astronomy and Astrophysics
991:. London, England: Smith, Elder and Co. pp. 151–165. 856:
Pigafetta et al., with Lord Stanley of Alderley, trans.,
560: 1631:(New York: John Wiley & Sons, 1993), pp. 357–8. 1469:
http://home.insightbb.com/~lasweb/lessons/magellanic.htm
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Ferris, Timothy (December 2011). "Dancing in the Dark".
1256:"The Magellanic Clouds must be renamed, astronomers say" 1075:
of the Small Magellanic Cloud, which is given by 5 log
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In 2019, astronomers discovered the young star cluster
2230: 1624:(Englewood Cliffs: Prentice-Hall, 1993), p. 550. 1484:
http://aa.springer.de/papers/8336003/2300925/sc6.htm
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The Large Magellanic Cloud was the host galaxy to a
1603:Murray, Claire E. ; et al. (14 December 2023) 1206:"Astronomers need to rename the Magellanic Clouds" 420:), the brightest observed in over four centuries. 1008:Monthly Notices of the Royal Astronomical Society 960:Planisphere contenant les Constellations Celestes 787:(London, England: Henry G. Bohn, 1852), vol. 4, 589:Monthly Notices of the Royal Astronomical Society 361:system, which is on the edge of the Local Group. 2290: 1104: 283:. In the 1756 star map of the French astronomer 948:) appear just below the center of the diagram.) 913:U.S. Naval Observatory; retrieved on 2009-09-05 725:"Observatoire de Paris (Abd-al-Rahman Al Sufi)" 208:, a professional astronomer, in 964 CE, in his 1594:The Astronomical Journal 122:220–231 July 2001 505: 315:. Recalibration of the Cepheid scales allowed 1668: 1310: 1004:"On the distribution of the nebulae in space" 858:The First Voyage Round the World, by Magellan 840:Star Maps: History, Artistry, and Cartography 521:Astronomical surveys of the Magellanic Clouds 1363: 1281:"A Cosmic Zoo in the Large Magellanic Cloud" 1174: 922: 661: 134:(SMC), about 206 kly (63 kpc) away 1380: 1375:Annual Review of Astronomy and Astrophysics 1285:European Southern Observatory Press Release 1180: 1047: 975:Linda Hall Library; retrieved on 2009-09-05 860:(London, England: Hakluyt Society, 1874), 295:("the Large Cloud" and "the Small Cloud"). 162:. They may be the objects mentioned by the 1675: 1661: 636:"Magellanic System | UW-Madison Astronomy" 1330: 1253: 1164: 1019: 611: 601: 27:Two dwarf galaxies orbiting the Milky Way 1109:[Reports about variable stars]. 1107:"Mitteilungen über veränderliche Sterne" 984: 878:. Augsburg, (Germany): Christoph Mang. 824:The First Three English Books on America 48: 37: 29: 1757:) may be read as "within" or "part of". 1448:"The Large and Small Magellanic Clouds" 1146: 1105:Pickering, E.C.; Wendell, O.C. (1912). 657: 655: 142:, but cannot be observed from the most 42:Small and Large Magellanic Clouds over 14: 2291: 1425: 1254:Ravisetti, Monisha (3 November 2023). 822:Richard Eden, with Edward Arber, ed., 1656: 1369:Freedman, Wendy L.; Madore, Barry F. 1316: 1221: 964:Memoires Academie Royale des Sciences 34:The Large and Small Magellanic Clouds 1098:Harvard College Observatory Circular 1079:= -7.3 - 13.0 = -20.3. One obtains 1001: 813:Giuliano de' Medici, Duke of Nemours 652: 332:and its neighbour and relative, the 265:, who accompanied the expedition of 113:The two galaxies are the following: 1208:Mia de los Reyes 12 September 2023 350:Sagittarius Dwarf Elliptical Galaxy 307:in 1913 using 1912 measurements of 24: 1763: 1649:—including photos & animations 1620:Eric Chaisson and Steve McMillan, 944:) and the Small Magellanic Cloud ( 668:Star Names: Their Lore and Meaning 500:data with foreground stars removed 323: 25: 2320: 1635: 1222:McKie, Robin (12 November 2023). 768:Petrus Martyr de Anghiera (1574) 448:data. The star cluster has a low 106:, they are often reclassified as 2276: 2264: 2252: 2240: 2215: 2214: 2204: 489: 474: 458: 1642:Magellanic Clouds Working Group 1597: 1585: 1550: 1526: 1508: 1499: 1477: 1462: 1440: 1419: 1397: 1273: 1247: 1215: 1199: 1140: 1086: 1041: 995: 978: 951: 916: 893: 868: 850: 770:De rebus Oceanicis et Orbe Novo 365:both been greatly distorted by 102:. Because both show signs of a 1534:"IoW_20200109 - Gaia - Cosmos" 805: 779:Humboldt, Alexander von, with 759: 738: 717: 691: 628: 575: 548: 230:, and that the inhabitants of 13: 1: 2177:Andromeda–Milky Way collision 1682: 1289:European Southern Observatory 541: 348:. Until the discovery of the 173:(the stations of the Moon in 81:southern celestial hemisphere 1212:; retrieved 12 November 2023 985:Herschel, John F.W. (1847). 882:The Large Magellanic Cloud ( 797:, see Knowledge's article: 340:to the naked eye. Roughly 21 169:(d. 889 CE), in his book on 7: 1181:Leverington, David (2013). 958:de Lacaille, N. L., (1756) 514: 506:Mini Magellanic Cloud (MMC) 158:and rock drawings found in 10: 2325: 1614: 496:LMC and SMC rendered from 393:in the LMC and SMC have a 149: 2200: 2164: 1972: 1944: 1933: 1865: 1817: 1782: 1775: 1761: 1690: 1559:The Astrophysical Journal 1319:The Astrophysical Journal 1210:American Physical Society 1153:The Astrophysical Journal 1111:Astronomische Nachrichten 1054:Astronomische Nachrichten 287:, they are designated as 1405:"Little Galaxy Explored" 1147:Shapley, Harlow (1918). 1131:10.1002/asna.19121921303 1048:Hertzsprung, E. (1913). 1002:Abbe, Cleveland (1867). 838:See also: Kanas, Nick, 799:Decades of the New World 699:"Al-Anwaa, Ibn Qutaybah" 1809:Supermassive black hole 1496:Retrieved on 2007-05-31 1474:Retrieved on 2007-05-31 1103:Summarized in German: 1021:10.1093/mnras/27.7.257a 783:and B.H. Paul, trans., 275:they are designated as 255:Peter Martyr d'Anghiera 2097:Sagittarius Spheroidal 1959:Small Magellanic Cloud 1954:Large Magellanic Cloud 1911:Pisces-Eridanus stream 1769: 482:Small Magellanic Cloud 467:Large Magellanic Cloud 372:barred spiral galaxies 334:Small Magellanic Cloud 330:Large Magellanic Cloud 202: 132:Small Magellanic Cloud 120:(LMC), about 163  118:Large Magellanic Cloud 54: 46: 35: 1767: 1728:Laniakea Supercluster 1505:Chaisson and McMillan 1371:"The Hubble Constant" 931:(in French): 539–592. 923:de la Caille (1752). 613:10.1093/mnras/stz1659 179: 52: 41: 33: 1768:The Milky Way Galaxy 1629:Conceptual Astronomy 1234:Guardian Media Group 874:Bayer Johann (1603) 1742:Observable universe 1571:1986ApJ...301..664M 1429:National Geographic 1341:2006ApJ...652.1133M 1297:2010eso..pres...21. 1291:: 21. 1 June 2010. 1123:1912AN....192..219P 1066:1913AN....196..201H 403:stellar populations 244:Abu Hanifa Dinawari 211:Book of Fixed Stars 175:pre-Islamic Arabian 140:Southern Hemisphere 98:are members of the 67:Nubeculae Magellani 44:Paranal Observatory 2309:Milky Way Subgroup 2082:Pisces Overdensity 1916:Sagittarius Stream 1827:Carina–Sagittarius 1770: 1722:Virgo Supercluster 1703:Milky Way subgroup 1538:www.cosmos.esa.int 1522:. January 9, 2007. 1520:Harvard University 1489:2007-06-07 at the 1472:Home.insightbb.com 971:2009-05-09 at the 909:2011-07-22 at the 900:Bayer, J., (1661) 681:Dover Publications 267:Ferdinand Magellan 144:northern latitudes 96:satellite galaxies 55: 47: 36: 2299:Magellanic Clouds 2228: 2227: 2192:Zone of Avoidance 2160: 2159: 2007:Canes Venatici II 1964:Magellanic Bridge 1946:Magellanic Clouds 1929: 1928: 1895:Magellanic Stream 1880:Fimbulthul stream 1458:on July 15, 2005. 1192:978-0-521-89994-9 1060:(4692): 201–208. 536:Magellanic Stream 531:Magellanic Bridge 435:) in the future. 433:Triangulum Galaxy 431:(and perhaps the 407:stellar formation 313:Henrietta Leavitt 309:Cepheid variables 305:Ejnar Hertzsprung 263:Antonio Pigafetta 108:Magellanic spiral 63:Magellanic system 59:Magellanic Clouds 16:(Redirected from 2316: 2281: 2280: 2279: 2269: 2268: 2267: 2257: 2256: 2255: 2245: 2244: 2236: 2218: 2217: 2210:Astronomy portal 2208: 2002:Canes Venatici I 1942: 1941: 1847:Scutum–Centaurus 1780: 1779: 1758: 1756: 1747: 1740: 1733: 1726: 1720: 1714: 1708: 1701: 1677: 1670: 1663: 1654: 1653: 1627:Michael Zeilik, 1608: 1601: 1595: 1589: 1583: 1582: 1554: 1548: 1547: 1545: 1544: 1530: 1524: 1523: 1512: 1506: 1503: 1497: 1481: 1475: 1466: 1460: 1459: 1454:. Archived from 1444: 1438: 1437: 1423: 1417: 1416: 1414: 1412: 1401: 1395: 1384: 1378: 1367: 1361: 1360: 1334: 1332:astro-ph/0608211 1325:(2): 1133–1149. 1314: 1308: 1307: 1305: 1303: 1277: 1271: 1270: 1268: 1266: 1251: 1245: 1244: 1242: 1240: 1219: 1213: 1203: 1197: 1196: 1178: 1172: 1170: 1168: 1144: 1138: 1135:See pp. 225-226. 1134: 1090: 1084: 1069: 1045: 1039: 1025: 1023: 999: 993: 992: 982: 976: 955: 949: 932: 920: 914: 897: 891: 872: 866: 854: 848: 809: 803: 763: 757: 756: 754: 752: 742: 736: 735: 733: 731: 721: 715: 714: 712: 710: 701:. Archived from 695: 689: 688: 659: 650: 649: 647: 646: 632: 626: 625: 615: 605: 579: 573: 572: 570: 568: 552: 526:Irregular galaxy 493: 478: 462: 429:Andromeda Galaxy 192:, the people of 21: 18:Magellanic Cloud 2324: 2323: 2319: 2318: 2317: 2315: 2314: 2313: 2289: 2288: 2287: 2277: 2275: 2265: 2263: 2253: 2251: 2239: 2231: 2229: 2224: 2196: 2172:Alternate names 2156: 1968: 1936: 1925: 1875:Aquarius Stream 1861: 1813: 1784:Galactic Center 1771: 1759: 1754: 1752: 1751: 1745: 1738: 1731: 1724: 1718: 1712: 1706: 1699: 1686: 1681: 1638: 1622:Astronomy Today 1617: 1612: 1611: 1602: 1598: 1590: 1586: 1555: 1551: 1542: 1540: 1532: 1531: 1527: 1514: 1513: 1509: 1504: 1500: 1491:Wayback Machine 1482: 1478: 1467: 1463: 1446: 1445: 1441: 1424: 1420: 1410: 1408: 1403: 1402: 1398: 1385: 1381: 1368: 1364: 1315: 1311: 1301: 1299: 1279: 1278: 1274: 1264: 1262: 1252: 1248: 1238: 1236: 1220: 1216: 1204: 1200: 1193: 1179: 1175: 1145: 1141: 1117:(13): 219–226. 1091: 1087: 1046: 1042: 1000: 996: 983: 979: 973:Wayback Machine 956: 952: 921: 917: 911:Wayback Machine 898: 894: 873: 869: 855: 851: 810: 806: 764: 760: 750: 748: 744: 743: 739: 729: 727: 723: 722: 718: 708: 706: 705:on 24 July 2017 697: 696: 692: 660: 653: 644: 642: 634: 633: 629: 580: 576: 566: 564: 554: 553: 549: 544: 517: 508: 501: 494: 485: 479: 470: 463: 326: 324:Characteristics 152: 28: 23: 22: 15: 12: 11: 5: 2322: 2312: 2311: 2306: 2301: 2286: 2285: 2273: 2261: 2249: 2226: 2225: 2223: 2222: 2212: 2201: 2198: 2197: 2195: 2194: 2189: 2184: 2182:Baade's Window 2179: 2174: 2168: 2166: 2162: 2161: 2158: 2157: 2155: 2154: 2149: 2144: 2139: 2137:Ursa Major III 2134: 2129: 2124: 2119: 2114: 2109: 2104: 2099: 2094: 2089: 2084: 2079: 2074: 2069: 2064: 2059: 2054: 2049: 2044: 2039: 2034: 2029: 2024: 2022:Coma Berenices 2019: 2014: 2009: 2004: 1999: 1994: 1989: 1984: 1978: 1976: 1970: 1969: 1967: 1966: 1961: 1956: 1950: 1948: 1939: 1931: 1930: 1927: 1926: 1924: 1923: 1918: 1913: 1908: 1902: 1900:Monoceros Ring 1897: 1892: 1887: 1882: 1877: 1871: 1869: 1863: 1862: 1860: 1859: 1854: 1852:Near 3 kpc Arm 1849: 1844: 1839: 1834: 1829: 1823: 1821: 1815: 1814: 1812: 1811: 1806: 1805: 1804: 1797:Sagittarius A* 1794: 1788: 1786: 1777: 1773: 1772: 1762: 1760: 1694: 1692: 1688: 1687: 1680: 1679: 1672: 1665: 1657: 1651: 1650: 1644: 1637: 1636:External links 1634: 1633: 1632: 1625: 1616: 1613: 1610: 1609: 1596: 1584: 1579:10.1086/163932 1549: 1525: 1507: 1498: 1494:Aa.springer.de 1476: 1461: 1439: 1418: 1396: 1379: 1362: 1349:10.1086/508530 1309: 1272: 1246: 1214: 1198: 1191: 1173: 1166:10.1086/142423 1139: 1137: 1136: 1085: 1040: 1014:(7): 257–264. 994: 977: 950: 946:Le Petit Nuage 942:Le Grand Nuage 915: 904:, pl. Aaa (49) 892: 888:Nubecula minor 884:Nubecula major 880:Star chart 49. 867: 849: 847: 846: 836: 804: 802: 801: 791: 777: 758: 737: 716: 690: 683:Inc. pp.  651: 640:astro.wisc.edu 627: 596:(1): 918–938. 574: 546: 545: 543: 540: 539: 538: 533: 528: 523: 516: 513: 507: 504: 503: 502: 495: 488: 486: 480: 473: 471: 464: 457: 440:Price-Whelan 1 325: 322: 317:Harlow Shapley 311:in the SMC by 301:Cleveland Abbe 293:le Petit Nuage 289:le Grand Nuage 281:nubecula minor 277:nubecula major 259:Andrea Corsali 151: 148: 136: 135: 129: 26: 9: 6: 4: 3: 2: 2321: 2310: 2307: 2305: 2302: 2300: 2297: 2296: 2294: 2284: 2274: 2272: 2262: 2260: 2250: 2248: 2243: 2238: 2237: 2234: 2221: 2213: 2211: 2207: 2203: 2202: 2199: 2193: 2190: 2188: 2185: 2183: 2180: 2178: 2175: 2173: 2170: 2169: 2167: 2163: 2153: 2150: 2148: 2145: 2143: 2140: 2138: 2135: 2133: 2132:Ursa Major II 2130: 2128: 2125: 2123: 2122:Triangulum II 2120: 2118: 2115: 2113: 2110: 2108: 2105: 2103: 2100: 2098: 2095: 2093: 2090: 2088: 2085: 2083: 2080: 2078: 2075: 2073: 2070: 2068: 2065: 2063: 2060: 2058: 2055: 2053: 2050: 2048: 2045: 2043: 2040: 2038: 2035: 2033: 2030: 2028: 2025: 2023: 2020: 2018: 2015: 2013: 2010: 2008: 2005: 2003: 2000: 1998: 1995: 1993: 1990: 1988: 1985: 1983: 1980: 1979: 1977: 1975: 1971: 1965: 1962: 1960: 1957: 1955: 1952: 1951: 1949: 1947: 1943: 1940: 1938: 1932: 1922: 1919: 1917: 1914: 1912: 1909: 1906: 1903: 1901: 1898: 1896: 1893: 1891: 1888: 1886: 1883: 1881: 1878: 1876: 1873: 1872: 1870: 1868: 1864: 1858: 1857:Far 3 kpc Arm 1855: 1853: 1850: 1848: 1845: 1843: 1840: 1838: 1835: 1833: 1830: 1828: 1825: 1824: 1822: 1820: 1816: 1810: 1807: 1803: 1802:Fermi bubbles 1800: 1799: 1798: 1795: 1793: 1792:Sagittarius A 1790: 1789: 1787: 1785: 1781: 1778: 1774: 1766: 1750: 1743: 1736: 1729: 1723: 1717: 1711: 1704: 1697: 1693: 1689: 1685: 1678: 1673: 1671: 1666: 1664: 1659: 1658: 1655: 1648: 1645: 1643: 1640: 1639: 1630: 1626: 1623: 1619: 1618: 1606: 1600: 1593: 1588: 1580: 1576: 1572: 1568: 1564: 1560: 1553: 1539: 1535: 1529: 1521: 1517: 1511: 1502: 1495: 1492: 1488: 1485: 1480: 1473: 1470: 1465: 1457: 1453: 1452:www.mq.edu.au 1449: 1443: 1435: 1431: 1430: 1422: 1406: 1400: 1393: 1389: 1383: 1376: 1372: 1366: 1358: 1354: 1350: 1346: 1342: 1338: 1333: 1328: 1324: 1320: 1313: 1298: 1294: 1290: 1286: 1282: 1276: 1261: 1257: 1250: 1235: 1231: 1230: 1225: 1218: 1211: 1207: 1202: 1194: 1188: 1184: 1177: 1167: 1162: 1158: 1154: 1150: 1143: 1132: 1128: 1124: 1120: 1116: 1113:(in German). 1112: 1108: 1102: 1101: 1099: 1095: 1089: 1082: 1078: 1074: 1067: 1063: 1059: 1056:(in German). 1055: 1051: 1044: 1037: 1033: 1029: 1022: 1017: 1013: 1009: 1005: 998: 990: 989: 981: 974: 970: 967: 965: 961: 954: 947: 943: 939: 938: 930: 926: 919: 912: 908: 905: 903: 896: 889: 885: 881: 877: 871: 863: 859: 853: 845: 841: 837: 834: 829: 825: 821: 820: 818: 814: 808: 800: 796: 792: 790: 786: 782: 778: 775: 771: 767: 766: 762: 747: 741: 726: 720: 704: 700: 694: 686: 682: 678: 674: 670: 669: 664: 658: 656: 641: 637: 631: 623: 619: 614: 609: 604: 599: 595: 591: 590: 585: 578: 563: 562: 557: 551: 547: 537: 534: 532: 529: 527: 524: 522: 519: 518: 512: 499: 492: 487: 483: 477: 472: 468: 461: 456: 455: 454: 451: 447: 446: 441: 436: 434: 430: 426: 421: 419: 415: 410: 408: 404: 400: 396: 392: 388: 383: 381: 380:galactic disk 377: 373: 368: 362: 360: 354: 351: 347: 343: 339: 335: 331: 321: 318: 314: 310: 306: 302: 298: 297:John Herschel 294: 290: 286: 282: 278: 274: 273: 268: 264: 260: 256: 252: 247: 245: 241: 237: 233: 229: 225: 221: 217: 213: 212: 207: 201: 199: 195: 191: 187: 182: 178: 176: 172: 168: 165: 161: 157: 147: 145: 141: 133: 130: 127: 123: 119: 116: 115: 114: 111: 109: 105: 104:bar structure 101: 97: 93: 90: 86: 82: 78: 75: 72: 68: 64: 60: 51: 45: 40: 32: 19: 2283:Solar System 2187:In mythology 2127:Ursa Major I 2092:Reticulum II 1945: 1921:Virgo Stream 1890:Helmi stream 1885:Gaia Sausage 1837:Orion–Cygnus 1832:Norma–Cygnus 1753:Each arrow ( 1628: 1621: 1599: 1587: 1562: 1558: 1552: 1541:. Retrieved 1537: 1528: 1510: 1501: 1493: 1479: 1471: 1464: 1456:the original 1451: 1442: 1433: 1427: 1421: 1409:. Retrieved 1399: 1391: 1382: 1374: 1365: 1322: 1318: 1312: 1284: 1275: 1263:. Retrieved 1259: 1249: 1237:. Retrieved 1229:The Observer 1227: 1217: 1201: 1182: 1176: 1156: 1152: 1142: 1114: 1110: 1097: 1088: 1080: 1076: 1072: 1057: 1053: 1043: 1035: 1031: 1027: 1011: 1007: 997: 987: 980: 963: 959: 953: 945: 941: 936: 928: 918: 901: 895: 887: 883: 875: 870: 857: 852: 839: 823: 817:Richard Eden 807: 795:De Orbe Novo 794: 789:pp. 340–341. 784: 769: 761: 749:. Retrieved 740: 728:. Retrieved 719: 707:. Retrieved 703:the original 693: 675: ed.). 667: 663:Allen, R. H. 643:. Retrieved 639: 630: 593: 587: 577: 565:. Retrieved 559: 550: 509: 444: 437: 422: 411: 384: 363: 355: 327: 292: 288: 280: 276: 270: 248: 235: 209: 203: 197: 183: 180: 170: 167:Ibn Qutaybah 153: 137: 112: 66: 62: 58: 56: 2304:Local Group 2271:Outer space 2259:Spaceflight 2037:Eridanus II 2012:Canis Major 1716:Local Sheet 1710:Local Group 1265:12 November 1239:12 November 1171:See p. 155. 1159:: 154–181. 902:Uranometria 876:Uranometria 450:metallicity 395:metallicity 346:light-years 272:Uranometria 156:petroglyphs 100:Local Group 2293:Categories 2142:Ursa Minor 1997:Boötes III 1735:Local Hole 1543:2020-01-09 1300:Retrieved 1034:, the two 1032:Via Lactea 1028:Via Lactea 966:pour 1752. 865:dimmed..." 645:2022-06-14 603:1901.05636 542:References 401:and young 234:call them 216:Argo Navis 196:call them 184:And below 177:culture): 110:galaxies. 69:) are two 2152:Willman 1 2087:Pisces II 1992:Boötes II 1982:Antlia II 1935:Satellite 1905:Palomar 5 1776:Structure 1696:Milky Way 1684:Milky Way 1607:arxiv.org 1436:(6): 118. 1411:29 August 1302:29 August 1260:Space.com 1100:no. 173. 1036:Nubeculae 833:astrolabe 781:E.C. Otte 622:0035-8711 498:Gaia EDR3 425:Milky Way 414:supernova 409:history. 338:Milky Way 171:Al-Anwā̵’ 124:(50  89:Milky Way 71:irregular 2220:Category 2112:Sculptor 2047:Hercules 2027:Crater 2 1987:Boötes I 1937:galaxies 1749:Universe 1691:Location 1487:Archived 1357:15728812 969:Archived 933:See the 907:Archived 677:New York 665:(1963). 515:See also 418:SN 1987A 374:. Their 359:NGC 3109 353:across. 285:Lacaille 236:al-Baqar 198:al-a‘bār 164:polymath 94:, these 85:Orbiting 77:galaxies 2233:Portals 2165:Related 2147:Virgo I 2117:Sextans 2107:Segue 2 2102:Segue 1 2077:Phoenix 1842:Perseus 1615:Sources 1567:Bibcode 1565:: 664. 1337:Bibcode 1293:Bibcode 1119:Bibcode 1062:Bibcode 935:plate ( 844:p. 118. 828:p. 279. 774:p. 217. 730:22 July 685:294–295 673:Reprint 567:3 April 399:nebulae 376:gravity 240:Ptolemy 220:Canopus 206:Al Sufi 186:Canopus 150:History 79:in the 2062:Leo IV 2057:Leo II 2042:Fornax 2017:Carina 1974:Dwarfs 1907:stream 1744:  1737:  1730:  1705:  1698:  1394:, 2010 1377:, 2010 1355:  1189:  862:p. 66. 751:22 Feb 620:  484:(SMC). 469:(LMC). 442:using 387:helium 251:Europe 238:, and 232:Tihama 204:Later 194:Tihama 128:) away 92:galaxy 2247:Stars 2072:Leo T 2067:Leo V 2052:Leo I 2032:Draco 1353:S2CID 1327:arXiv 709:4 Sep 598:arXiv 391:stars 367:tidal 160:Chile 74:dwarf 1867:Halo 1819:Disk 1413:2010 1304:2010 1267:2023 1241:2023 1187:ISBN 753:2017 732:2011 711:2017 618:ISSN 569:2013 465:The 445:Gaia 328:The 291:and 279:and 257:and 228:Najd 226:nor 224:Iraq 190:Iraq 87:the 57:The 1575:doi 1563:301 1434:220 1345:doi 1323:652 1161:doi 1127:doi 1115:192 1058:196 1016:doi 608:doi 594:488 561:ESO 249:In 126:kpc 122:kly 65:or 2295:: 1573:. 1561:. 1536:. 1518:. 1450:. 1432:. 1390:, 1373:, 1351:. 1343:. 1335:. 1321:. 1287:. 1283:. 1258:. 1232:. 1226:. 1157:48 1155:. 1151:. 1125:. 1096:. 1012:27 1010:. 1006:. 962:, 679:: 654:^ 638:. 616:. 606:. 592:. 586:. 558:. 382:. 146:. 83:. 2235:: 1755:→ 1746:→ 1739:→ 1732:→ 1725:→ 1719:→ 1713:→ 1707:→ 1700:→ 1676:e 1669:t 1662:v 1581:. 1577:: 1569:: 1546:. 1415:. 1359:. 1347:: 1339:: 1329:: 1306:. 1295:: 1269:. 1243:. 1195:. 1169:. 1163:: 1133:. 1129:: 1121:: 1081:p 1077:p 1073:p 1068:. 1064:: 1024:. 1018:: 755:. 734:. 713:. 687:. 671:( 648:. 624:. 610:: 600:: 571:. 416:( 342:° 200:. 61:( 20:)

Index

Magellanic Cloud


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

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