Magellanic Clouds

Short description: Two dwarf galaxies orbiting the Milky Way

The Large and Small Magellanic Clouds Small and Large Magellanic Clouds over Paranal Observatory

thumb|ALMA antennae bathed in red light. In the background are the southern Milky Way on the left and the Magellanic Clouds at the top.[1]]]

The Magellanic Clouds (Magellanic system[2][3] or Nubeculae Magellani[4]) are two irregular dwarf galaxies in the southern celestial hemisphere. Orbiting the Milky Way galaxy, these satellite galaxies are members of the Local Group. Because both show signs of a bar structure, they are often reclassified as Magellanic spiral galaxies.

The two galaxies are the following:

* Large Magellanic Cloud (LMC), about 163 kly (50 kpc) away
* Small Magellanic Cloud (SMC), about 206 kly (63 kpc) away

The Magellanic clouds are visible to the unaided eye from the Southern Hemisphere, but cannot be observed from the most northern latitudes.

## Contents

* 1 History
* 2 Characteristics
* 3 Mini Magellanic Cloud (MMC)
* 4 See also
* 5 References
* 6 Sources
* 7 External links

## History

The Magellanic Clouds have been known since ancient times to indigenous peoples across South America, Australia, and Africa, and from the first millennium in Western Asia. The first preserved mention of the Large Magellanic Cloud is believed to be in petroglyphs and rock drawings found in Chile . They may be the objects mentioned by the polymath Ibn Qutaybah (d. 889 CE), in his book on Al-Anwā̵’ (the stations of the Moon in pre-Islamic Arabian culture):

> "وأسفل من سهيل قدما سهيل . وفى مجرى قدمى سهيل، من خلفهما كواكب زهر كبار، لا ترى بالعراق، يسميها أهل تهامة الأعبار

> "And below Canopus, there are the feet of Canopus, and on their extension, behind them bright big stars, not seen in Iraq, the people of Tihama call them al-a‘bār."[5]

Later Al Sufi, a professional astronomer,[6] in 964 CE, in his Book of Fixed Stars, mentioned the same quote, but with a different spelling. Under Argo Navis, he quoted that "unnamed others have claimed that beneath Canopus there are two stars known as the 'feet of Canopus', and beneath those there are bright white stars that are unseen in Iraq nor Najd, and that the inhabitants of Tihama call them al-Baqar [cows], and Ptolemy did not mention any of this so we [Al-Sufi] do not know if this is true or false."[7] Both Ibn Qutaybah and Al-Sufi were probably quoting from the former's contemporary (and compatriot) and famed scientist Abu Hanifa Dinawari'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.

In Europe, the Clouds were first reported by 16th century Italian authors Peter Martyr d'Anghiera and Andrea Corsali, both based on Portuguese voyages.[8][9] Subsequently, they were reported by Antonio Pigafetta, who accompanied the expedition of Ferdinand Magellan on its circumnavigation of the world in 1519–1522.[10][4] However, naming the clouds after Magellan did not become widespread until much later. In Bayer's Uranometria they are designated as nubecula major and nubecula minor.[11][12] In the 1756 star map of the French astronomer Lacaille, they are designated as le Grand Nuage and le Petit Nuage ("the Large Cloud" and "the Small Cloud").[13][14] John Herschel 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.[15] In 1867 Cleveland Abbe suggested that they were separate satellites of the Milky Way.[16] Distances were first estimated by Ejnar Hertzsprung in 1913 using 1912 measurements of Cepheid variables in the SMC by Henrietta Leavitt.[17][18] Recalibration of the Cepheid scales allowed Harlow Shapley to refine the measurement,[19] and these were again revised in 1952 following further research.[20] As of 2023[update], 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.[21][22][23]

## Characteristics

The Large Magellanic Cloud (LMC). Small Magellanic Cloud (SMC). LMC and SMC rendered from Gaia EDR3 data with foreground stars removed

The Large Magellanic Cloud and its neighbour and relative, the Small Magellanic Cloud, are conspicuous objects in the southern hemisphere, looking like separated pieces of the Milky Way to the naked eye. Roughly 21° apart in the night sky, the true distance between them is roughly 75,000 light-years. Until the discovery of the Sagittarius Dwarf Elliptical Galaxy in 1994, they were the closest known galaxies to our own (since 2003, the Canis Major Dwarf Galaxy was discovered to be closer still, and is now considered the actual nearest neighbor). The LMC lies about 160,000 light years away,[24][25][26][27] while the SMC is around 200,000.[28] The LMC is about twice the diameter of the SMC (14,000 ly and 7,000 ly respectively). For comparison, the Milky Way is about 100,000 ly across.

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 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 NGC 3109 system, which is on the edge of the Local Group.

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.[29] Observation and theoretical evidence suggest that the Magellanic Clouds have both been greatly distorted by tidal 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 barred spiral galaxies.[30] Their gravity has affected the Milky Way as well, distorting the outer parts of the galactic disk.

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 helium compared to the Milky Way.[31] They are also more metal-poor than the Milky Way; the youngest stars in the LMC and SMC have a metallicity of 0.5 and 0.25 times solar, respectively.[32] Both are noted for their nebulae and young stellar populations, but as in our own galaxy their stars range from the very young to the very old, indicating a long stellar formation history.[33]

The Large Magellanic Cloud was the host galaxy to a supernova (SN 1987A), the brightest observed in over four centuries.

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 Milky Way.[34] 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 Andromeda Galaxy (and perhaps the Triangulum Galaxy) in the future.

In 2019, astronomers discovered the young star cluster Price-Whelan 1 using Gaia data. The star cluster has a low metallicity 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.[35]

## Mini Magellanic Cloud (MMC)

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 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.[36][37] This hypothesis was confirmed in 2023. The part of the SMC which is closer to Earth lies 196,000 lightyears (60 kiloparsecs) away, whereas the farther part lies 215,000 lightyears (66 kiloparsecs) away.[38]

## See also

* Astronomical surveys of the Magellanic Clouds
* Irregular galaxy
* Magellanic Stream
* Magellanic Bridge

## References

1. ↑ {{cite news |title=Media Advisory: Virtual Press Conference to Mark ALMA Inauguration |url=http://www.eso.org/public/announcements/ann13020/ |access-date=3 April 2013|newspaper=[[ESO}}
2. ↑ Tepper-García, Thor; Bland-Hawthorn, Joss; Pawlowski, Marcel S.; Fritz, Tobias K. (2019-09-01). "The Magellanic System: the puzzle of the leading gas stream". Monthly Notices of the Royal Astronomical Society 488 (1): 918–938. doi:10.1093/mnras/stz1659. ISSN 0035-8711.
3. ↑ "Magellanic System | UW-Madison Astronomy". http://www.astro.wisc.edu/wham-site/research-topics/research-magellanic-system/.
4. ↑ 4.0 4.1 Star Names: Their Lore and Meaning (Reprint ed.). New York City: Dover Publications Inc. 1963. pp. 294–295.
5. ↑ "Al-Anwaa, Ibn Qutaybah". http://shamela.ws/browse.php/book-9093#page-204.
6. ↑ "Observatoire de Paris (Abd-al-Rahman Al Sufi)". http://messier.obspm.fr/xtra/Bios/alsufi.html.
7. ↑ "Book of Fixed Stars, Al-Sufi (manuscript written and illustrated by his son)". http://bodley30.bodley.ox.ac.uk:8180/luna/servlet/detail/ODLodl~23~23~125630~142720?sort=Shelfmark,sort_order&qvq=q:ms.+marsh+144;sort:Shelfmark,sort_order;lc:ODLodl~29~29,ODLodl~7~7,ODLodl~6~6,ODLodl~14~14,ODLodl~8~8,ODLodl~23~23,ODLodl~1~1,ODLodl~24~24&mi=372&trs=436.
8. ↑ For Peter Martyr d'Anghiera's mention of the Magellanic clouds, see:
* Petrus Martyr de Anghiera (1574) De rebus Oceanicis et Orbe Novo [Concerning the ocean and the new world] (Cologne, (Germany): Geruinum Calenium (Gerwin Calenius), 1574), decade 3, book 1, p. 217. (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 [i.e., the southern celestial pole], scattered in the Milky Way like luminous patches throughout the whole sphere of the sky, within the breadth of its extent. [That is, nebulae appear in or beside the Milky Way throughout its entire length in the southern sky.])
* Humboldt, Alexander von, with E.C. Otte and B.H. Paul, trans., Cosmos: A Sketch of a Physical Description of the Universe (London, England: Henry G. Bohn, 1852), vol. 4, pp. 340–341.
* For further details of – and other editions of – Peter Martyr d'Anghiera's book De Orbe Novo, see Wikipedia's article: Decades of the New World
9. ↑ 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 Giuliano de' Medici, Duke of Nemours, mentioning the Magellanic clouds. This letter was translated into English by Richard Eden (c.1520–1576) and published in 1555. The relevant part of Corsali's letter (translated by Eden) appears in:
* Richard Eden, with Edward Arber, ed., The First Three English Books on America … (Birmingham, England: 1885), "Of the pole antarike and the starres abowt the same … ", p. 279. 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 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 [that is] opposite our north [celestial] pole, in order to know in what place and degree [of latitude] the south [celestial] pole was, we [measured our position during] the day using the sun, and observed [our position during] the night using an astrolabe, and saw clearly two clouds of reasonable bigness revolving around the location of the [southern celestial] pole, continually now rising and now falling, thus maintaining their continual course of circular motion, with a star always in the middle [between them], which revolves with them about 11 degrees from the [south celestial] pole.")
* See also: Kanas, Nick, Star Maps: History, Artistry, and Cartography, 2nd ed. (New York, New York: Springer Science + Business Media, 2012), § 4.3.2.2 Andreas Corsali, p. 118.
10. ↑ Pigafetta et al., with Lord Stanley of Alderley, trans., The First Voyage Round the World, by Magellan (London, England: Hakluyt Society, 1874), p. 66. 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 dimmed, … "
11. ↑ Bayer Johann (1603) Uranometria. Augsburg, (Germany): Christoph Mang. Star chart 49. The Large Magellanic Cloud (Nubecula major) appears below the chart's center and just above the fish Dorado; the Small Magellanic Cloud (Nubecula minor) appears to the left and below the chart's center and touches the right side of Hydrus the water snake.
12. ↑ Bayer, J., (1661) Uranometria, pl. Aaa (49) U.S. Naval Observatory; retrieved on 2009-09-05
13. ↑ de la Caille (1752). "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" (in French). Histoire de l'Académie Royale des Sciences, avec les Mémoires de Mathématique & de Physique de l'Académie Royale des Sciences: 539–592. https://www.biodiversitylibrary.org/item/88113#page/348/mode/1up. See the plate (Planisphere contenant des constellations celestes comprises entre le pole austral et le Tropique du Capricorne [Planisphere containing the celestial constellations included between the south [celestial] pole and the Tropic of Capricorn]) following p. 592. (The Large Magellanic Cloud (Le Grand Nuage) and the Small Magellanic Cloud (Le Petit Nuage) appear just below the center of the diagram.)
14. ↑ de Lacaille, N. L., (1756) Planisphere contenant les Constellations Celestes, Memoires Academie Royale des Sciences pour 1752. Linda Hall Library; retrieved on 2009-09-05
15. ↑ Herschel, John F.W. (1847). Results of Astronomical Observations Made During the Years 1834, 5, 6, 7, 8 at the Cape of Good Hope. London, England: Smith, Elder and Co.. pp. 151–165. https://books.google.com/books?id=8WBNAAAAcAAJ&pg=PA151.
16. ↑ Abbe, Cleveland (1867). "On the distribution of the nebulae in space". Monthly Notices of the Royal Astronomical Society 27 (7): 257–264. doi:10.1093/mnras/27.7.257a. https://babel.hathitrust.org/cgi/pt?id=nyp.33433110033127&view=1up&seq=269. From p. 262: "2. The Nebulae resolved and unresolved lie in general without [i.e., outside of] the Via Lactea [i.e., Milky Way], which is therefore essentially stellar. 3. The visible universe is composed of systems, of which the Via Lactea, the two Nubeculae [sic] [i.e., Magellanic Clouds], 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."
17. ↑ Hertzsprung, E. (1913). "Über die räumliche Verteilung der Veränderlichen vom δ Cephei-Typus" (in German). Astronomische Nachrichten 196 (4692): 201–208. Bibcode: 1913AN....196..201H. http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1913AN....196..201H. 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 [stars] that are treated above, the absolute brightness (the mean between the maximum and the minimum) of -7.3 m corresponds to a period of 6.6 days. Variable [stars] 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 p of the Small Magellanic Cloud, which is given by 5 log p = -7.3 - 13.0 = -20.3. One obtains p = 0.0001", corresponding to a distance of about 3000 lightyears. Since the galactic latitude of the Small Magellanic Cloud amounts to about - 45°, then it would lie — according to the foregoing — about 2000 lightyears from a plane [passing] through our Sun [and] lying parallel to the Milky Way and [it] would have to be regarded as lying outside the Milky Way.)
18. ↑ Leavitt, Henrietta S.; Pickering, Edward C. (March 3, 1912). "Periods of 25 Variable Stars in the Small Magellanic Cloud". Harvard College Observatory Circular no. 173.
* Summarized in German: Pickering, E.C.; Wendell, O.C. (1912). "Mitteilungen über veränderliche Sterne" (in German). Astronomische Nachrichten 192 (13): 219–226. doi:10.1002/asna.19121921303. Bibcode: 1912AN....192..219P. http://adsabs.harvard.edu/pdf/1912AN....192..219. See pp. 225-226.
19. ↑ Shapley, Harlow (1918). "Studies on the colors and magnitudes in stellar clusters. Seventh paper: The distances, distributions in space, and dimensions of 69 globular clusters". The Astrophysical Journal 48: 154–181. doi:10.1086/142423. https://babel.hathitrust.org/cgi/pt?id=hvd.32044059981803&view=1up&seq=172&skin=2021. See p. 155.
20. ↑ Leverington, David (2013). Encyclopedia of the History of Astronomy and Astrophysics. Cambridge: Cambridge University Press. pp. 231–232. ISBN 978-0-521-89994-9.
21. ↑ "Astronomers need to rename the Magellanic Clouds" Mia de los Reyes 12 September 2023 American Physical Society; retrieved 12 November 2023
22. ↑ McKie, Robin (12 November 2023). "'Violent colonialist' Magellan is unfit to keep his place in the night sky, say astronomers". The Observer (Guardian Media Group). https://www.theguardian.com/science/2023/nov/12/violent-colonialist-magellan-is-unfit-to-keep-his-place-in-the-night-sky-say-astronomers.
23. ↑ Ravisetti, Monisha (3 November 2023). "The Magellanic Clouds must be renamed, astronomers say". Space.com. https://www.space.com/astronomers-rename-magellanic-clouds-coalition.
24. ↑ "A Cosmic Zoo in the Large Magellanic Cloud". European Southern Observatory Press Release (European Southern Observatory): 21. 1 June 2010. Bibcode: 2010eso..pres...21.. http://www.eso.org/public/news/eso1021/. Retrieved 29 August 2010.
25. ↑ Macri, L. M. (2006). "A New Cepheid Distance to the Maser-Host Galaxy NGC 4258 and Its Implications for the Hubble Constant". The Astrophysical Journal 652 (2): 1133–1149. doi:10.1086/508530. Bibcode: 2006ApJ...652.1133M.
26. ↑ Freedman, Wendy L.; Madore, Barry F. "The Hubble Constant", Annual Review of Astronomy and Astrophysics, 2010
27. ↑ Majaess, Daniel J.; Turner, David G.; Lane, David J.; Henden, Arne; Krajci, Tom "Anchoring the Universal Distance Scale via a Wesenheit Template", Journal of the American Association of Variable Star Observers, 2010
28. ↑ "Little Galaxy Explored". Jet Propulsion Laboratory, California Institute of Technology. 5 January 2010. http://www.spitzer.caltech.edu/images/2875-ssc2010-02a1-Little-Galaxy-Explored.
29. ↑ Ferris, Timothy (December 2011). "Dancing in the Dark". National Geographic 220 (6): 118.
30. ↑ "The Large and Small Magellanic Clouds". Archived from the original on July 15, 2005. https://web.archive.org/web/20050715231207/http://www.aao.gov.au/images/captions/misc021.html.
31. ↑ http://home.insightbb.com/~lasweb/lessons/magellanic.htm Home.insightbb.com Retrieved on 2007-05-31
32. ↑ http://aa.springer.de/papers/8336003/2300925/sc6.htm Aa.springer.de Retrieved on 2007-05-31
33. ↑ Chaisson and McMillan
34. ↑ "Press release: Magellanic Clouds May Be Just Passing Through". Harvard University. January 9, 2007. https://www.cfa.harvard.edu/news/2007-02.
35. ↑ "IoW_20200109 - Gaia - Cosmos". https://www.cosmos.ESA.int/web/Gaia/iow_20200109.
36. ↑ Mathewson, D. S.; Ford, V. L.; Visvanathan, N. (1986). "The structure of the Small Magellanic Cloud". The Astrophysical Journal 301: 664. doi:10.1086/163932. Bibcode: 1986ApJ...301..664M.
37. ↑ http://iopscience.iop.org/1538-3881/122/1/220/200523.text.html The Astronomical Journal 122:220–231 July 2001
38. ↑ Murray, Claire E. ; et al. (14 December 2023) "A galactic eclipse: the Small Magellanic Cloud is forming stars in two, superimposed systems" arxiv.org

## Sources

* Eric Chaisson and Steve McMillan, Astronomy Today (Englewood Cliffs: Prentice-Hall, Inc., 1993), p. 550.
* Michael Zeilik, Conceptual Astronomy (New York: John Wiley & Sons, Inc., 1993), pp. 357–8.

## External links

* Magellanic Clouds Working Group
* ESO: VISTA Peeks Through the Small Magellanic Cloud’s Dusty Veil incl. Photos & Animations

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