词条 | List of star extremes | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
释义 |
A star is a sphere that is mainly composed of hydrogen and plasma, held together by gravity and is able to produce light through nuclear fusion. Stars exhibit many diverse properties, resulting from different masses, volumes, velocities, stage in stellar evolution and even proximity to earth. Some of these properties are considered extreme and sometimes disproportionate by astronomers. Age and distance
Brightness and power
Size and mass
Motion
Star systems
See also
Notes1. ^{{cite journal|doi=10.1051/0004-6361/201628422|title=Characterisation of red supergiants in the Gaiaspectral range|journal=Astronomy & Astrophysics|volume=595|pages=A105|year=2016|last1=Dorda|first1=Ricardo|last2=González-Fernández|first2=Carlos|last3=Negueruela|first3=Ignacio}} 2. ^{{de icon}} "Innes' Sterne bei α Centauri", Astronomische Nachrichten, volume 206, 1918 {{bibcode|1918AN....206...97H}} 3. ^Harold L. Aden, "Alpha and Proxima Centauri", Astronomical Journal, vol. 39, issue 913, 1918 {{bibcode|1928AJ.....39...20A}} 4. ^{{cite journal |author=Kelly, Patrick L.|display-authors=etal|title=Extreme magnification of an individual star at redshift 1.5 by a galaxy-cluster lens |url=https://www.nature.com/articles/s41550-018-0430-3 |date=2 April 2018 |journal=Nature |volume=2 |issue=4 |pages=334–342 |doi=10.1038/s41550-018-0430-3 |accessdate=2 April 2018 |arxiv=1706.10279 |bibcode=2018NatAs...2..334K }} 5. ^{{cite web |last=Howell |first=Elizabeth |title=Rare Cosmic Alignment Reveals Most Distant Star Ever Seen |url=https://www.space.com/40171-cosmic-alignment-reveals-most-distant-star-yet.html |date=2 April 2018|work=Space.com |accessdate=2 April 2018 }} 6. ^{{cite news |last=Sanders |first=Robert |title=Hubble peers through cosmic lens to capture most distant star ever seen |url=http://news.berkeley.edu/2018/04/02/cosmic-lens-helps-hubble-capture-most-distant-star-ever-seen/ |date=2 April 2018 |work=Berkeley News |accessdate=2 April 2018 }} 7. ^{{cite web |last=Parks |first=Jake |title=Hubble spots farthest star ever seen |url=http://www.astronomy.com/news/2018/04/hubble-images-farthest-star-ever-seen |date=2 April 2018 |work=Astronomy |accessdate=2 April 2018 }} 8. ^{{cite journal | authors=P. A. Oesch, G. Brammer, P. G. van Dokkum, G. D. Illingworth, R. J. Bouwens, I. Labbe, M. Franx, I. Momcheva, M. L. N. Ashby, G. G. Fazio, V. Gonzalez, B. Holden, D. Magee, R. E. Skelton, R. Smit, L. R. Spitler, M. Trenti, S. P. Willner | title=A Remarkably Luminous Galaxy at z = 11.1 Measured with Hubble Space Telescope Grism Spectroscopy | journal=The Astrophysical Journal | volume=819 | issue=2 | pages=129 |arxiv=1603.00461 |bibcode=2016ApJ...819..129O |doi=10.3847/0004-637X/819/2/129 | year=2016 }} 9. ^ScienceDaily, [https://www.sciencedaily.com/releases/2013/03/130307145103.htm "Hubble Finds 'Birth Certificate' of Oldest Known Star"], 7 March 2013 10. ^An "average" star is a normal star which is larger than a red dwarf, but smaller than a giant star. Depending on the definition, this can also be called "Sun-like star". 11. ^Universe Today, "How Far is the Nearest Star?", Fraser Cain, 13 November 2009 (accessed 2010-11-02) 12. ^1 2 Not including stellar-mass black holes, or exotic stars 13. ^{{cite book|author=New Scientist|title=The Invisible Star Shows Up|url=https://books.google.com/books?id=XLlzpvKTIjMC&pg=PA538|year=1983|publisher=Reed Business Information|page=538}} 14. ^ NASA, "Where is the closest neutron star?", Laura Whitlock, 1 December 2005 (accessed 2010-11-01) 15. ^NASA Images, "Hubble Sees Bare Neutron Star Streaking Across Space" {{Webarchive|url=https://web.archive.org/web/20121102160337/http://www.nasaimages.org/luna/servlet/detail/NVA2~8~8~13120~113661:Hubble-Sees-Bare-Neutron-Star-Strea# |date=2012-11-02 }}, NASA, 9 November 2000 (accessed 2010-11-01) 16. ^RedOrbit, "The Motion of RX J185635-3754 - The Nearest Neutron Star to Earth", 8 February 2005 (accessed 2010-11-01) 17. ^Astronomy 122: Astronomy of Stars and Galaxies, "Lecture 19: Neutron Stars"{{dead link|date=January 2018 |bot=InternetArchiveBot |fix-attempted=yes }}, Sharon Morsink, University of Alberta, term:Winter 2011, published:2010 (accessed 2010-11-01) 18. ^1 2 Atlas of the Universe, "The Universe within 12.5 Light Years: The Nearest Stars", Richard Powell, 30 July 2006 (accessed 2010-11-01) 19. ^BBC News, "Hubble finds mass of white dwarf", Christine McGourty, 14 December 2005 (accessed 2010-11-01) 20. ^Universe Today, "What is the Nearest Star to the Sun?", Fraser Cain, 7 October 2009 (accessed 2010-11-02) 21. ^SpaceDaily, "The Closest Star System Found in a Century", Barbara K. Kennedy, 12 March 2013 22. ^1 2 3 By visual magnitude (m) 23. ^1 2 3 4 5 6 This is the appearance in the sky from Earth. 24. ^This does not include brightest stars due to outbursts 25. ^1 2 3 4 5 Other than the Sun 26. ^NOAO, "Astronomers Peg Brightness of History’s Brightest Star", 5 March 2003 (accessed 2010-10-25) 27. ^1 2 Luminosity here represents how bright a star is if all stars were equally far away, in visible light. 28. ^1 {{cite journal|last=Dieterich|first=Sergio B.|author2=Henry, Todd J. |author3=Jao, Wei-Chun |author4=Winters, Jennifer G. |author5=Hosey, Altonio D. |author6=Riedel, Adric R. |author7= Subasavage, John P. |title=The Solar Neighborhood XXXII. The Hydrogen Burning Limit|journal= The Astronomical Journal|year=2014|arxiv=1312.1736 |bibcode = 2014AJ....147...94D |doi = 10.1088/0004-6256/147/5/94 |volume=147 |issue=5|page=94}} 29. ^1 2 Energetic here is the total electromagnetic energy emitted by a star in all wavelengths. 30. ^{{Cite journal |last=Tramper |first=F. |last2=Straal |first2=S. M. |last3=Sanyal |first3=D. |last4=Sana |first4=H. |last5=de Koter |first5=A. |last6=Gräfener |first6=G. |last7=Langer |first7=N. |last8=Vink |first8=J. S. |last9=de Mink |first9=S. 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Martin, Francesco Pepe, Don Pollacco, Damien Ségransan, Barry Smalley, Stéphane Udry, Richard West |arxiv= 1706.08781 |journal= Astronomy & Astrophysics |volume= 604 |pages= L6 |id= EBLM_III |date= 12 June 2017 |bibcode= 2017A&A...604L...6V |doi=10.1051/0004-6361/201731107}} 44. ^Not including stellar black holes 45. ^1 2 Monthly Notices of the Royal Astronomical Society, "The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 Msun stellar mass limit", Paul A Crowther, Olivier Schnurr, Raphael Hirschi, Norhasliza Yusof, Richard J Parker, Simon P Goodwin, Hasan Abu Kassim, Volume 408, Issue 2, pp. 731–751, October 2010, {{doi|10.1111/j.1365-2966.2010.17167.x}} , {{bibcode|2010MNRAS.408..731C}} , {{ArXiv|1007.3284}} 46. ^{{Cite web|url=http://www.astro.gsu.edu/RECONS/TOP100.posted.htm|title=THE 100 NEAREST STAR SYSTEMS|website=www.astro.gsu.edu|access-date=2019-02-04}} 47. ^Astrophysical Journal Letters, "Brown Dwarfs in the Pleiades Cluster Confirmed by the Lithium Test", Rebolo, R.; Martin, E. 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