List of star extremes
Stars are luminous balls of plasma which illuminate the universe. They come in various sizes and arrangements; their properties depending on their initial mass and their stage of stellar evolution.
Age and distance
Title | Object | Date | Data | Comments | Notes | Refs | See more |
---|---|---|---|---|---|---|---|
Nearest star | Sun | prehistoric (3rd century BC) |
1 AU | Our local star's distance was first determined in the 3rd century BC by Aristarchus of Samos | Reported for reference | ||
Second nearest star | Proxima Centauri | 1915 | 1.30 pc | Also called Alpha Centauri C, it is the outlying star in a trinary star system. This is currently the nearest known neighbouring star to our own Sun. This star was discovered in 1915, and its parallax was determined at the time, when enough observations were established. | [NB 1] | [1][2] | List of nearest stars |
Most distant star | Stars in UDFj-39546284 | 2011 | z=11.9 | ||||
Oldest star | HD 140283 | ±0.8 billion years 14.5 | the "Methuselah star" | [3] | List of oldest stars | ||
Youngest | |||||||
Title | Object | Date | Data | Comments | Notes | Refs | See more |
---|---|---|---|---|---|---|---|
Nearest "average" star | Alpha Centauri A & B |
Prehistoric | 1.34 parsecs (4.4 ly) | This was the third star whose parallax was determined. Before Alpha Cen, the record was held by 61 Cygni, the first star whose parallax was determined. | [NB 1][NB 2][NB 3] | ||
Nearest normal star | Alpha Centauri C (Proxima Centauri) |
1915 | 1.30 parsecs (4.2 ly) | Before Proxima, the title had been held by Alpha Centauri A&B. | [NB 1][NB 3] | ||
Nearest red dwarf | Proxima Centauri | 1915 | 1.30 parsecs (4.2 ly) | [4][5] | |||
Nearest degenerate star | Sirius B | 1852 | 8.6 light-years (2.6 pc) | This is also the nearest white dwarf | [NB 4] | ||
Nearest neutron star | RX J185635-3754 | 2000 | 200 light-years (61 pc) | [6][7][8] | |||
Nearest white dwarf | Sirius B | 1852 | 8.6 light-years (2.6 pc) | Sirius B is also the first white dwarf discovered. | [4][9] | ||
Nearest flare star | Proxima Centauri (Alpha Centauri C) |
1.30 parsecs (4.2 ly) | α Cen C is also the nearest neighbouring star. | [10] | |||
Nearest brown dwarf | Luhman 16 | 2013 | 6.5 light-years (2.0 pc) | This is a pair of brown dwarfs in a binary system, with no other stars. | [11] | ||
Brightness and power
Title | Object | Date | Data | Comments | Notes | Refs | See more |
---|---|---|---|---|---|---|---|
Brightest star | Sun | prehistoric | m=−26.74 | Reported for reference [NB 5][NB 6] |
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Brightest star other than the Sun | Sirius (Alpha Canis Majoris) |
prehistoric | m=−1.46 | See also: Historical brightest stars |
[NB 5][NB 6][NB 7][NB 1] | List of brightest stars | |
Brightest star in a transient event | Progenitor of SN 1006 | 1006 | m=−7.5 | This was a supernova, and its remnant (SNR) is catalogued as PKS 1459-41 | [NB 5][NB 6][NB 1] | [12] | |
Dimmest star | [NB 5][NB 6] | ||||||
Most luminous star | R136a1 | 2010 | V=−12.5 | [NB 8] | [13] | List of most luminous stars | |
Most luminous star in a transient event | Progenitor of GRB 080916C | 2008 | V=-40 | The star exploded in a gamma-ray burst with the total energy equal to 9,000 supernovae | [NB 8] | List of gamma-ray bursts | |
Least luminous normal star | 2MASS J0523-1403 | 2013 | V=20.6 | [NB 3][NB 8] | [14] | ||
Most energetic star | R136a1 | 2010 | B= | [NB 9] | [13] | ||
Most energetic star in a transient event | Progenitor of GRB 080916C | 2008 | [NB 9] | ||||
Least energetic normal star | 2MASS J0523-1403 | 2013 | L=0.000126LSun | [NB 3][NB 9] | [14] | ||
Hottest Normal Star | Melnick 34 | T=~ 63000 K | |||||
Coolest normal star | 2MASS J0523-1403 | 2013 | T=2074K | [14] | |||
Title | Object | Date | Data | Comments | Notes | Refs | See more |
---|---|---|---|---|---|---|---|
Hottest degenerate star | KPD 0005+5106 H1504+65 |
2008 |
200000 K 200000 K |
[15][16] | |||
Hottest neutron star | At least 100,000K | ||||||
Hottest white dwarf | KPD 0005+5106 | 2008 | 200000 K | [17] | |||
Hottest PG 1159 star/GW Vir star | RX J2117+3412 | 1999 | 170000 K | [18] | |||
Coolest brown dwarf | WISE 1828+2650 | ≤300 K | |||||
Size and mass
Title | Object | Date | Data | Comments | Notes | Refs | See more |
---|---|---|---|---|---|---|---|
Largest apparent size star | Sun | prehistoric (3rd century BCE) |
31.6′ – 32.7′ | The apparent size of the Sun was first measured by Eratosthenes in the 3rd Century BCE,[19] who was the second person to measure the distance to the Sun. However, Thales of Miletus provided a measurement for the real size of the Sun in the 6th Century BCE, as 1⁄720 the great circle of the Sun (the orbit of the Earth) [20] | Reported for reference [NB 6] |
||
Largest apparent size star | R Doradus | 1997 | 0.057" | This replaced Betelgeuse as the largest, Betelgeuse having been the first star other than the Sun to have its apparent size measured. | [NB 6][NB 1] | [21] | |
Smallest apparent size star | [NB 6] | ||||||
Most voluminous star | Westerlund 1 BKS AS | 2013 | r=1,951-2,544 RSun | This star is a strong radio source, with uncertain variability, leading it to have wildly varying size estimates. | List of largest stars | ||
Least voluminous normal star | 2MASS J0523-1403 | 2013 | r=0.086 RSun | [NB 3] | [22] | ||
Most massive star | R136a1 | 2010 | 315 MSun | This exceeds the predicted limit of 150 solar masses, previously believed to be the limit of stellar mass, according to the leading star formation theories. | [NB 10] | [13] | List of most massive stars |
Least massive normal star | [NB 3] | List of least massive stars | |||||
Title | Object | Date | Data | Comments | Notes | Refs | See more |
---|---|---|---|---|---|---|---|
Most massive brown dwarf | PPl 15 | 1996 | 80 MJupiter | This is at the limit between brown dwarfs and red dwarfs.[23][24] | [23][25][26][27] | ||
Most massive degenerate star | The most massive type of degenerate star is the neutron star. See Most massive neutron star for this recordholder. [NB 4] | ||||||
Most massive neutron star | PSR J1614−2230 | 2010 | 1.97 MSun | This millisecond pulsar greatly exceeds the predicted limit of neutron star size of roughly 1.5 solar masses. The previous titleholder only massed of 1.67 solar masses. | [28][29][30] | ||
Most massive white dwarf | RE J0317-853 | 1998 | 1.35 MSun | [31][32] | |||
Title | Object | Date | Data | Comments | Notes | Refs | See more |
---|---|---|---|---|---|---|---|
Least massive brown dwarf | List of least massive stars | ||||||
Least massive degenerate star | The least massive type of degenerate star is the white dwarf. See Least massive white dwarf for this recordholder. [NB 4] | ||||||
Least massive neutron star | |||||||
Least massive white dwarf | SDSS J091709.55+463821.8 (WD J0917+4638) |
2007 | 0.17 MSun | [33][34][35][36] | |||
Motion
Title | Object | Date | Data | Comments | Notes | Refs | See more |
---|---|---|---|---|---|---|---|
Highest proper motion | Barnard's Star | 10.3 "/yr | This is also the fourth closest star to Earth | [37][38] | |||
Lowest proper motion | |||||||
Highest radial velocity | |||||||
Lowest radial velocity | |||||||
Highest peculiar motion | |||||||
Lowest peculiar motion | |||||||
Highest rotational speed of a normal star | [NB 3] | ||||||
Lowest rotational speed | |||||||
Planetary systems
Main article: List of extrasolar planet extremes
Star systems
Title | Object | Date | Data | Comments | Notes | Refs | See more |
---|---|---|---|---|---|---|---|
Least stars in a star system | There are many stars in single star systems | ||||||
Most stars in a star system | Septuple star system | Both are called 7-star systems in the 1997 MSC,[39] and appear in the 2008 MSC.[40] | [NB 11] | [39][40] | |||
Stars in the closest orbit around one another | There are many stars that are contact binaries, where the stars are in physical contact with each other | ||||||
Stars in the most distant orbit around one another | [NB 11] | ||||||
Nearest multiple star system | Alpha Centauri | 1839 | 1.30 parsecs (4.2 ly) | This was one of the first three stars to have its distance measured.[41][42] | [4][43] | ||
Title | Object | Date | Data | Comments | Notes | Refs | See more |
---|---|---|---|---|---|---|---|
Shortest period black hole binary system | MAXI J1659-152 | 2013 | 2.4 hours | This exceeds the preceding recordholder by about one hour (Swift J1753.5-0127 with a 3.2 hour period) | [44] | ||
Notes
- 1 2 3 4 5 6 Other than the Sun
- ↑ 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".
- 1 2 3 4 5 6 7 A normal star is a star that is past its protostar period, in its main fusion period, before becoming a degenerate star, black hole, or post-stellar nebula, and is not a failed star (brown dwarf).
- 1 2 3 Not including stellar-mass black holes, or exotic stars
- 1 2 3 4 By visual magnitude (m)
- 1 2 3 4 5 6 7 This is the appearance in the sky from Earth.
- ↑ This does not include brightest stars due to outbursts
- 1 2 3 Luminosity here represents how bright a star is if all stars were equally far away, in visible light.
- 1 2 3 Energetic here is the total electromagnetic energy emitted by a star in all wavelengths.
- ↑ Not including stellar black holes
- 1 2 The allowable distance between components of a star system is debated.
References
- ↑ (German) "Innes' Sterne bei α Centauri", Astronomische Nachrichten, volume 206, 1918 Bibcode: 1918AN....206...97H
- ↑ Harold L. Aden, "Alpha and Proxima Centauri", Astronomical Journal, vol. 39, issue 913, 1918 Bibcode: 1928AJ.....39...20A
- ↑ ScienceDaily, "Hubble Finds 'Birth Certificate' of Oldest Known Star", 7 March 2013
- 1 2 3 Atlas of the Universe, "The Universe within 12.5 Light Years: The Nearest Stars", Richard Powell, 30 July 2006 (accessed 2010-11-01)
- ↑ Universe Today, "How Far is the Nearest Star?", Fraser Cain, 13 November 2009 (accessed 2010-11-02)
- ↑ NASA Images, "Hubble Sees Bare Neutron Star Streaking Across Space", NASA, 9 November 2000 (accessed 2010-11-01)
- ↑ RedOrbit, "The Motion of RX J185635-3754 - The Nearest Neutron Star to Earth", 8 February 2005 (accessed 2010-11-01)
- ↑ Astronomy 122: Astronomy of Stars and Galaxies, "Lecture 19: Neutron Stars", Sharon Morsink, University of Alberta, term:Winter 2011, published:2010 (accessed 2010-11-01)
- ↑ BBC News, "Hubble finds mass of white dwarf", Christine McGourty, 14 December 2005 (accessed 2010-11-01)
- ↑ Universe Today, "What is the Nearest Star to the Sun?", Fraser Cain, 7 October 2009 (accessed 2010-11-02)
- ↑ SpaceDaily, "The Closest Star System Found in a Century", Barbara K. Kennedy, 12 March 2013
- ↑ NOAO, "Astronomers Peg Brightness of History’s Brightest Star", 5 March 2003 (accessed 2010-10-25)
- 1 2 3 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
- 1 2 3 Dieterich, Sergio B.; Henry, Todd J.; Jao, Wei-Chun; Winters, Jennifer G.; Hosey, Altonio D.; Riedel, Adric R.; Subasavage, John P. (2014). "The Solar Neighborhood XXXII. The Hydrogen Burning Limit". arXiv:1312.1736. Bibcode:2014AJ....147...94D. doi:10.1088/0004-6256/147/5/94.
- ↑ http://adsabs.harvard.edu//abs/2011hst..prop12483W
- ↑ http://rd.springer.com/article/10.1007%2Fs10509-011-0617-x
- ↑ Thaindian News, "Astronomers discover Universes hottest white dwarf", ANI, 13 December 2008 (accessed 2010-11-09)
- ↑ 11th European Workshop on White Dwarfs, ASP Conference Series #169, "RX J2117+3412, the hottest known pulsating PG 1159 star", Vauclair, G.; Moskalik, P.; The Wet Team, 1999, ISBN 1-886733-91-0 , Bibcode: 1999ASPC..169...96V , pg.96
- ↑ http://www.csus.edu/indiv/o/oreyd/papers/Chapterfour.html
- ↑ Internet Encyclopedia of Philosophy, "Thales of Miletus (c. 620 BCE – c. 546 BCE)", Patricia O’Grady, 17 September 2004 (accessed 2010-10-25)
- ↑ ESO, "The Biggest Star in the Sky", 11 March 1997 (accessed 2010-10-25)
- ↑ Katy, Garmany. "NOAO/SOAR: Where do stars end and brown dwarfs begin?". National Optical Astronomy Observatory. Retrieved 14 December 2013.
- 1 2 Astrophysical Journal Letters, "Brown Dwarfs in the Pleiades Cluster Confirmed by the Lithium Test", Rebolo, R.; Martin, E. L.; Basri, G.; Marcy, G. W.; Zapatero-Osorio, M. R., v.469, p.L53, September 1996, doi:10.1086/310263 , Bibcode: 1996ApJ...469L..53R , arXiv:astro-ph/9607002
- ↑ Astronomical Society of the Pacific Conference Series, 'In Cool Stars, Stellar Systems, and the Sun: Ninth Cambridge Workshop', "An I. K Survey of the Pleiades", Jameson, R. F.; Hodgkin, S. T.; Pinfield, D. J., vol. 109, p. 363, eds. R. Pallavicini, A. K. Dupree, 1996, Bibcode: 1996ASPC..109..363J
- ↑ SIMBAD, "Cl* Melotte 22 IPMBD 23" (accessed 2010-11-11)
- ↑ Astronomy and Astrophysics, "Brown dwarfs in the Pleiades cluster: a CCD-based R, I survey", Zapatero Osorio, M. R.; Rebolo, R.; Martin, E. L., v.317, p.164-170, January 1997, Bibcode: 1997A&A...317..164Z , arXiv:astro-ph/9604079
- ↑ Astronomical Society of the Pacific Conference Series, 'Proceedings of the 9th Cambridge workshop', "Lithium, rotation and activity in young clusters", Soderblom, D. R., volume 109, p.315, eds. Roberto Pallavicini, Andrea K. Dupree, October 1995, Bibcode: 1996ASPC..109..315S
- ↑ Science Daily, "Astronomers Discover Most Massive Neutron Star Yet Known; Discovery Has Broad Implications for Astrophysics, Nuclear Physics", 27 October 2010 (accessed 30-10-2010)
- ↑ SpaceRef.com, "Astronomers discover most massive neutron star yet known", NRAO, 27 October 2010 (accessed 2010-10-30)
- ↑ Space.com, "Most Massive Neutron Star Breaks Cosmic Record ", Charles Q. Choi, 27 October 2010 (accessed 10-30-2010)
- ↑ Bulletin of the American Astronomical Society, "The Record Breaking Magnetic White Dwarf RE J0317-853", Burleigh, M. R.; Jordan, S., Vol. 29, p.1234, January 1998, Bibcode: 1998AAS...191.1511B
- ↑ Wolfram Scienceworld, "White Dwarf", Eric W. Weisstein, 2007 (accessed 2010-30-10)
- ↑ CfA, "Cosmic Weight Loss: The Lowest Mass White Dwarf", 17 April 2007 (accessed 2010-10-30)
- ↑ JUMK.de, "Special Stars: SDSS J091709.55+463821.8" (accessed 2010-10-30)
- ↑ The Astrophysical Journal Letters, "No Neutron Star Companion to the Lowest Mass SDSS White Dwarf", Marcel Agüeros et al., Volume 700, Issue 2, pp. L123-L126, August 2009, doi:10.1088/0004-637X/700/2/L123 , Bibcode: 2009ApJ...700L.123A , arXiv:0906.5109
- ↑ Internet Encyclopedia of Science, "White Dwarf", David Darling (accessed 10-30-2010)
- ↑ Hayden Planetarium, "Stellar Orbits", Sébastien Lépine, Brian Abbott (accessed 2010-11-20)
- ↑ Ohio State University, Astronomy 143: The History of the Universe (Fall 2009); "Stars and Galaxies in Motion", Barbara Sue Ryden, 15 October 2009 (accessed 2010-11-20)
- 1 2 Astronomy & Astrophysics Supplement Series, "MSC - a catalogue of physical multiple stars", Tokovinin, A. A., Vol. 124, July 1997, pp.75-84, July 1997, doi:10.1051/aas:1997181 , Bibcode: 1997A&AS..124...75T , VizieR (accessed 2010-10-27)
- 1 2 Monthly Notices of the Royal Astronomical Society, "A catalogue of multiplicity among bright stellar systems", Eggleton, P. P.; Tokovinin, A. A., Volume 389, Issue 2, pp. 869-879, September 2008, doi:10.1111/j.1365-2966.2008.13596.x , Bibcode: 2008MNRAS.389..869E , arXiv:0806.2878v1 , VizieR (accessed 2010-10-27)
- ↑ "Report of the Council of the Society to the Nineteenth Annual General Meeting", Monthly Notices of the Royal Astronomical Society, Vol. 4 No. 20, 8 February 1839, Royal Astronomical Society, Bibcode: 1836MNRAS...4....3M
- ↑ Kentucky New Era, "A Problem That The Star Sharps Are Trying To Solve", New York World, 3 July 1895 (accessed 22 March 2010)
- ↑ Universe Today, "Distance to Nearest Star", Fraser Cain, 30 December 2009 (accessed 2010-11-02)
- ↑ SpaceDaily, "Black hole-star pair orbiting at dizzying speed", 22 March 2013
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