List of star extremes explained
A star is a massive luminous spheroid astronomical object made of plasma that is held together by its own gravity. Stars exhibit great diversity in their properties (such as mass, volume, velocity, stage in stellar evolution, and distance from Earth) and some of the outliers are so disproportionate in comparison with the general population that they are considered extreme. This is a list of such stars.
Records that are regarded as authoritative and unlikely to change at any given point are recorded on a white background, while those that could change with new information and/or discoveries are recorded on a grey background.
Age and distance
Nearest stars by typeTitle | Object | Date | Data | Comments | Notes | Refs | See more |
---|
Nearest sun-like star | Alpha Centauri A & B | 1839 | 1.34pc | This was the third star whose parallax was determined. Before Alpha Centauri, the record was held by 61 Cygni, the first star whose parallax was determined. | [8] | | |
Nearest normal star | Alpha Centauri C (Proxima Centauri) | 1915 | 1.3pc | Before Proxima, the title had been held by Alpha Centauri A & B. | | [9] | |
Nearest red dwarf | Before Proxima, the title had been held by Barnard's Star | |
Nearest degenerate star | Sirius B | 1852 | 8.6ly | This is also the nearest white dwarf. | [10] | | |
Nearest subdwarf | Kapteyn's Star | 1898 | 12.83ly | Kapteyn's star is either a sdM1 subdwarf[11] or a M1.5V main-sequence star.[12] [13] WISEA 1810−1010 is the nearest undisputed subdwarf, at 29.03ly. [14] | | [15] | |
Nearest borderline subgiant | Procyon | | 11.5ly | All stars closer to the Sun are either main sequence or dwarf stars. | | | |
Nearest undisputed subgiant | Delta Pavonis | | 19.9ly | A subgiant, but only slightly brighter than the Sun. | | | |
Nearest "true" giant star | Pollux | | 33.8ly | | | | |
Nearest red giant | Arcturus | | 36.7ly | | | |
Nearest supergiant | Canopus | | 309ly | While it is frequently described as a yellow supergiant, especially in evolutionary terms,[16] it is classified as a bright giant based on spectrum.[17] | | | |
Nearest carbon star | CW Leonis | | 310ly | | | | |
Nearest F-type star | Procyon A | | 11.46ly | | | [18] | |
Nearest A-type star | Sirius A | | 8.6ly | | | | |
Nearest B-type star | Regulus A | | 79.3ly | | | [19] | |
Nearest O-type star | Zeta Ophiuchi | | 366ly | | | [20] | |
Nearest Wolf–Rayet star | Gamma Velorum | | 1080ly | | | | |
Nearest neutron star | RX J1856.35-3754 | 2000 | 400ly | | | [21] [22] [23] | |
Nearest white dwarf | Sirius B | 1852 | 8.6ly | Sirius B is also the second white dwarf discovered, after 40 Eridani B. | | [24] [25] [26] | |
Nearest brown dwarf | | 2013 | 6.5ly | This is a pair of brown dwarfs in a binary system, with no other stars. | | [27] | |
|
Brightness and power
Size and mass
Title | Object | Date | Data | Comments | Notes | Refs | See more |
---|
Largest apparent size star | Sun | prehistoric | | The apparent size of the Sun was first measured by Eratosthenes in the 3rd century BC,[44] 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 BC, as the great circle of the Sun (the orbit of the Earth)[45] | Reported for reference
| | |
Largest extrasolar 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. | | [46] | |
Smallest apparent size star | Thousands of neutron stars located on the other side of the galaxy, likely impossible to resolve. | | | | | | |
Largest star | WOH G64 | 2009 | | Consistent with the upper limit for red supergiants of roughly based on the four largest stars measured in a survey, which is consistent with the current stellar evolutionary theory.[47] | | [48] [49] [50] [51] | List of largest known stars |
Smallest star | | 2017 | | | [52] | [53] [54] [55] | List of smallest stars |
Most massive star | BAT99-98 or R136a1 | 2014, 2022 | , | This exceeds the predicted limit of, previously believed to be the limit of stellar mass, according to the leading star formation theories. R136a1 considered the most massive known by the scientific community. | [56] | [57] [58] | List of most massive stars |
Least massive normal star | SCR 1845–6357 A | | | | | [59] | List of least massive stars |
|
Most massive stars by typeTitle | Object | Date | Data | Comments | Notes | Refs | See more |
---|
Most massive brown dwarf | SDSS J010448.46+153501.8 | 2017 | 90 MJupiter | This is at the limit between brown dwarfs and red dwarfs.[60] [61] | | [62] | |
Most massive degenerate star | The most massive type of degenerate star is the neutron star. See Most massive neutron star for this recordholder. |
Most massive neutron star | PSR J0740+6620 | 2019 | 2.14 MSun | Several candidates exist which have a higher mass, however their mass has been measured by less precise methods and as such their mass value is regarded as less certain. | | [63] | List of most massive neutron stars |
Most massive neutron star (disputed) | PSR J1748-2021B | 2015 | 2.548 MSun | | | [64] |
Most massive white dwarf | RE J0317-853/ZTF J1901+1458 | 1998/2020 | 1.35 MSun | | | [65] [66] | |
|
Motion
Star systems
Title | Object | Date | Data | Comments | Notes | Refs | See more |
---|
Least stars in a star system | There are many single star systems. |
Most stars in a star system | | | Nonuple star system[81] | System contains at least nine stars. | [82] | | |
Stars in the closest orbit around one another | There are many stars that are in contact binary systems (where two or more stars are in physical contact with each other). |
Stars in the most distant orbit around one another | Fomalhaut A/B/C | | ~0.77pc | | | | |
Nearest multiple star system | Alpha Centauri | 1839 | 1.3pc | This was one of the first three stars to have its distance measured.[83] [84] | | [85] | |
Nearest binary star system | Luhman 16 | 2013 | 1.998pc | Brown dwarf binary system. The nearest non-brown dwarf binary is Sirius, and the nearest composed entirely of main-sequence stars is Luyten 726-8. | | | |
Nearest trinary star system | Alpha Centauri | 1839 | 1.38pc | Also nearest multiple star system, and nearest star system of any type | | | |
Nearest quaternary star system | Gliese 570 | | 5.88pc | K4 star orbited by a pair of M stars, all orbited by a T7 brown dwarf. | | | |
Nearest quintenary star system | V1054 Ophiuchi | | 6.46pc | M3 star orbited by a pair of pair of M4 stars, together orbited by an M3.5 star, all orbited by an M7 star. | | | |
Nearest sextenary star system | Castor | 1718 | 15.6pc | A1 star orbited by a red dwarf, both orbited by another A star orbited by a red dwarf, all orbited by two red dwarfs orbiting each other. | | | |
Nearest septenary star system | Nu Scorpii | | 150pc | A B3V star orbited by an unknown-type star, both orbited by another unknown star, together orbited by another unknown star, all orbited by a B9III star orbiting a pair of stars which are a B9III and unknown star. | | | | |
External links
Notes and References
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- Harold L. Aden, "Alpha and Proxima Centauri", Astronomical Journal, vol. 39, issue 913, 1918
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- Not including stellar-mass black holes or exotic stars
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- By visual magnitude (m)
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