  | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Corvus |
| Right ascension | 12h 10m 07.48058s [1] |
| Declination | –22° 37′ 11.1620″ [1] |
| Apparent magnitude (V) | +3.024 [2] |
| Characteristics | |
| Spectral type | K2 III [3] |
| U−B color index | +1.458 [2] |
| B−V color index | +1.318 [2] |
| Astrometry | |
| Radial velocity (Rv) | +4.9 [4] km/s |
| Proper motion (μ) |
RA: –71.74
mas/
yr Dec.: +10.25 mas/ yr |
| Parallax (π) | 10.26 ± 0.16 mas [1] |
| Distance | 318 ± 5
ly (97 ± 2 pc) |
| Absolute magnitude (MV) | −1.82+0.15 −0.14 [5] |
| Details | |
| Mass | 3.2 [6] M☉ |
| Radius | 52 [7] R☉ |
| Surface gravity (log g) | 2.16 [8] cgs |
| Temperature | 4320 [8] K |
| Metallicity [Fe/H] | –0.13 [8] dex |
| Rotational velocity (v sin i) | 1.0 [6] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
Epsilon Corvi (ε Crv, ε Corvi) is a star in the southern constellation of Corvus. It has the traditional name Minkar /ˈmɪŋkɑːr/, from Arabic منقار minqar meaning "beak [of the crow]" [10] The apparent visual magnitude is +3.0 [2] and it is located at a distance of 318 light-years (97 parsecs) from Earth. [1]
In Chinese, 軫宿 (Zhěn Sù), meaning Chariot (asterism), refers to an asterism consisting of ε Corvi, γ Corvi, δ Corvi and β Corvi. [11] Consequently, ε Corvi itself is known as 軫宿二 (Zhěn Sù èr, English: the Second Star of Chariot.). [12]
Epsilon Corvi is a red giant with a stellar classification of K2 III, having consumed the hydrogen at its core and evolved away from the main sequence. It has about three times the Sun's mass. [6] The interferometry-measured angular diameter of this star is about 4.99 mas, [13] which, at its estimated distance, equates to a physical radius of about 52 times the radius of the Sun. [7] The effective temperature of the outer envelope is 4320 K, [8] giving it an orange hue that is characteristic of a K-type star. [14] Around 4 times as massive as the Sun, it spent much of its life as a main sequence star of spectral type B5V. [15]
References
- ^ a b c d van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv: 0708.1752, Bibcode: 2007A&A...474..653V, doi: 10.1051/0004-6361:20078357, S2CID 18759600
- ^ a b c d Celis S., L. (October 1975), "Photoelectric photometry of late-type variable stars", Astronomy and Astrophysics Supplement Series, 22: 9–17, Bibcode: 1975A&AS...22....9C
- ^ Houk, Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 4, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan, Bibcode: 1988mcts.book.....H
- ^ Wielen, R.; et al. (1999), "Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions", Veroeffentlichungen des Astronomischen Rechen-Instituts Heidelberg, 35 (35), Astronomisches Rechen-Institut Heidelberg: 1, Bibcode: 1999VeARI..35....1W
- ^ Carney, Bruce W.; et al. (March 2008), "Rotation and Macroturbulence in Metal-Poor Field Red Giant and Red Horizontal Branch Stars", The Astronomical Journal, 135 (3): 892–906, arXiv: 0711.4984, Bibcode: 2008AJ....135..892C, doi: 10.1088/0004-6256/135/3/892, S2CID 2756572
- ^ a b c Melo, C. H. F.; et al. (August 2005), "On the nature of lithium-rich giant stars. Constraints from beryllium abundances", Astronomy and Astrophysics, 439 (1): 227–235, arXiv: astro-ph/0504133, Bibcode: 2005A&A...439..227M, doi: 10.1051/0004-6361:20041805, S2CID 10580797
- ^
a
b Lang, Kenneth R. (2006),
Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.),
Birkhäuser,
ISBN
3-540-29692-1. The radius (R*) is given by:
- ^ a b c d McWilliam, Andrew (December 1990), "High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances", Astrophysical Journal Supplement Series, 74: 1075–1128, Bibcode: 1990ApJS...74.1075M, doi: 10.1086/191527
- ^ "MINKAR -- Variable Star", SIMBAD, Centre de Données astronomiques de Strasbourg, retrieved 2012-01-23
- ^ Al-Sufi, Book Of Fixed Stars, Constellation: The Crow
- ^ (in Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.
- ^ (in Chinese) 香港太空館 - 研究資源 - 亮星中英對照表 Archived January 30, 2011, at the Wayback Machine, Hong Kong Space Museum. Accessed on line November 23, 2010.
- ^ Richichi, A.; Percheron, I.; Khristoforova, M. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics, 431 (2): 773–777, Bibcode: 2005A&A...431..773R, doi: 10.1051/0004-6361:20042039
- ^ "The Colour of Stars", Australia Telescope, Outreach and Education, Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived from the original on 2012-03-18, retrieved 2012-01-16
- ^ Kaler, James B. (Jim), "Minkar", Stars, University of Illinois, retrieved 12 July 2015
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| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Corvus |
| Right ascension | 12h 10m 07.48058s [1] |
| Declination | –22° 37′ 11.1620″ [1] |
| Apparent magnitude (V) | +3.024 [2] |
| Characteristics | |
| Spectral type | K2 III [3] |
| U−B color index | +1.458 [2] |
| B−V color index | +1.318 [2] |
| Astrometry | |
| Radial velocity (Rv) | +4.9 [4] km/s |
| Proper motion (μ) |
RA: –71.74
mas/
yr Dec.: +10.25 mas/ yr |
| Parallax (π) | 10.26 ± 0.16 mas [1] |
| Distance | 318 ± 5
ly (97 ± 2 pc) |
| Absolute magnitude (MV) | −1.82+0.15 −0.14 [5] |
| Details | |
| Mass | 3.2 [6] M☉ |
| Radius | 52 [7] R☉ |
| Surface gravity (log g) | 2.16 [8] cgs |
| Temperature | 4320 [8] K |
| Metallicity [Fe/H] | –0.13 [8] dex |
| Rotational velocity (v sin i) | 1.0 [6] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
Epsilon Corvi (ε Crv, ε Corvi) is a star in the southern constellation of Corvus. It has the traditional name Minkar /ˈmɪŋkɑːr/, from Arabic منقار minqar meaning "beak [of the crow]" [10] The apparent visual magnitude is +3.0 [2] and it is located at a distance of 318 light-years (97 parsecs) from Earth. [1]
In Chinese, 軫宿 (Zhěn Sù), meaning Chariot (asterism), refers to an asterism consisting of ε Corvi, γ Corvi, δ Corvi and β Corvi. [11] Consequently, ε Corvi itself is known as 軫宿二 (Zhěn Sù èr, English: the Second Star of Chariot.). [12]
Epsilon Corvi is a red giant with a stellar classification of K2 III, having consumed the hydrogen at its core and evolved away from the main sequence. It has about three times the Sun's mass. [6] The interferometry-measured angular diameter of this star is about 4.99 mas, [13] which, at its estimated distance, equates to a physical radius of about 52 times the radius of the Sun. [7] The effective temperature of the outer envelope is 4320 K, [8] giving it an orange hue that is characteristic of a K-type star. [14] Around 4 times as massive as the Sun, it spent much of its life as a main sequence star of spectral type B5V. [15]
References
- ^ a b c d van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv: 0708.1752, Bibcode: 2007A&A...474..653V, doi: 10.1051/0004-6361:20078357, S2CID 18759600
- ^ a b c d Celis S., L. (October 1975), "Photoelectric photometry of late-type variable stars", Astronomy and Astrophysics Supplement Series, 22: 9–17, Bibcode: 1975A&AS...22....9C
- ^ Houk, Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 4, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan, Bibcode: 1988mcts.book.....H
- ^ Wielen, R.; et al. (1999), "Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions", Veroeffentlichungen des Astronomischen Rechen-Instituts Heidelberg, 35 (35), Astronomisches Rechen-Institut Heidelberg: 1, Bibcode: 1999VeARI..35....1W
- ^ Carney, Bruce W.; et al. (March 2008), "Rotation and Macroturbulence in Metal-Poor Field Red Giant and Red Horizontal Branch Stars", The Astronomical Journal, 135 (3): 892–906, arXiv: 0711.4984, Bibcode: 2008AJ....135..892C, doi: 10.1088/0004-6256/135/3/892, S2CID 2756572
- ^ a b c Melo, C. H. F.; et al. (August 2005), "On the nature of lithium-rich giant stars. Constraints from beryllium abundances", Astronomy and Astrophysics, 439 (1): 227–235, arXiv: astro-ph/0504133, Bibcode: 2005A&A...439..227M, doi: 10.1051/0004-6361:20041805, S2CID 10580797
- ^
a
b Lang, Kenneth R. (2006),
Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.),
Birkhäuser,
ISBN
3-540-29692-1. The radius (R*) is given by:
- ^ a b c d McWilliam, Andrew (December 1990), "High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances", Astrophysical Journal Supplement Series, 74: 1075–1128, Bibcode: 1990ApJS...74.1075M, doi: 10.1086/191527
- ^ "MINKAR -- Variable Star", SIMBAD, Centre de Données astronomiques de Strasbourg, retrieved 2012-01-23
- ^ Al-Sufi, Book Of Fixed Stars, Constellation: The Crow
- ^ (in Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.
- ^ (in Chinese) 香港太空館 - 研究資源 - 亮星中英對照表 Archived January 30, 2011, at the Wayback Machine, Hong Kong Space Museum. Accessed on line November 23, 2010.
- ^ Richichi, A.; Percheron, I.; Khristoforova, M. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics, 431 (2): 773–777, Bibcode: 2005A&A...431..773R, doi: 10.1051/0004-6361:20042039
- ^ "The Colour of Stars", Australia Telescope, Outreach and Education, Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived from the original on 2012-03-18, retrieved 2012-01-16
- ^ Kaler, James B. (Jim), "Minkar", Stars, University of Illinois, retrieved 12 July 2015
| Stars |
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| Galaxies |
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