Gliese 293

Gliese 293
           Gliese 293
Location of Gliese 293 in the constellation Volans

Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Volans[1]
Right ascension 07h 53m 08.1439s[2]
Declination −67° 47′ 31.382″[2]
Apparent magnitude (V) 13.96[3]
Characteristics
Evolutionary stage white dwarf[4]
Spectral type DC8.8,[4] or DC10.3[5]
Apparent magnitude (B) 14.75[6]
Apparent magnitude (RKC) 13.58[3]
Apparent magnitude (IKC) 13.20[3]
Apparent magnitude (J) 12.726±0.023[7]
Apparent magnitude (H) 12.476±0.026[7]
Apparent magnitude (KS) 12.362±0.024[7]
Astrometry
Proper motion (μ) RA: 1,467.123 mas/yr[2]
Dec.: −1,489.721 mas/yr[2]
Parallax (π)122.4130±0.0114 mas[2]
Distance26.644 ± 0.002 ly
(8.1691 ± 0.0008 pc)
Absolute magnitude (MV)14.47±0.04[3]
Details
Mass0.59±0.01[3] M
Radius0.0128[3][note 1] R
Surface gravity (log g)8.00±0.02[3] cgs
Temperature5,700±90[3] K
Age2.65±0.10[3][note 2] Gyr
Other designations
GJ 293, EGGR 56, L 97-12, LAWD 26, LFT 555, LHS 34, LTT 2981, PLX 1882, WD 0752-676, 2MASS J07530814-6747314[8]
Database references
SIMBADdata

Gliese 293 (or WD 0752-676, or LHS 34, or L 97-12) is a nearby white dwarf star, located 26.64 light-years away in the constellation Volans. It is the nearest star in this constellation.[9]: 84 

Distance

Gliese 293 is the 12th-nearest known white dwarf.[10] A trigonometric parallax of Gliese 293 was included in the YPC (Yale Parallax Catalog), and subsequently it was measured more precisely in CTIOPI (Cerro Tololo Inter-American Observatory (CTIO) Parallax Investigation) 0.9 m telescope program, and by Gaia.

Gliese 293 parallax measurements
Source Paper Parallax, mas Distance, pc Distance, ly Ref.
YPC van Altena et al., 1995 141.2±8.4 7.08±0.42 23.10±1.37 [11]
CTIOPI 0.9 m TSN-21 (Subasavage et al., 2009) 126.25±1.34 7.92±0.08 25.83±0.27 [3]
Gaia DR3 Gaia Collaboration 2023 122.4130±0.0114 8.1691±0.0008 26.644±0.002 [2]

Physical parameters

The mass of Gliese 293 is 0.59±0.01 Solar masses,[3] and its surface gravity is 108.00±0.02 cm/s2,[3] or approximately 102,000 times Earth's, corresponding to a radius of 8,887 kilometres (5,522 miles), or 139% of Earth's.

Gliese 293 has a temperature of 5,700±90 K,[3] almost like the Sun, and a cooling age, i.e. age as a degenerate star (not including its lifetime as a main-sequence star and a giant star) of 2.65±0.10 Gyr[3] It has a white appearance due to similar temperature to Sun.

See also

Notes

  1. ^ From surface gravity and mass.
  2. ^ White dwarf cooling age, i.e. age as degenerate star (not including lifetime as main-sequence star and as giant star)

References

  1. ^ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific. 99 (617): 695. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Constellation record for this object at VizieR.
  2. ^ a b c d e Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  3. ^ a b c d e f g h i j k l m n Subasavage, John P.; Jao, Wei-Chun; Henry, Todd J.; Bergeron, P.; Dufour, P.; Ianna, Philip A.; Costa, Edgardo; Méndez, René A. (2009). "The Solar Neighborhood. XXI. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the 25 Parsec White Dwarf Sample". The Astronomical Journal. 137 (6): 4547. arXiv:0902.0627. Bibcode:2009AJ....137.4547S. doi:10.1088/0004-6256/137/6/4547.
  4. ^ a b Holberg, J. B.; Sion; Oswalt; McCook; Foran; Subasavage (2008). "A New Look at the Local White Dwarf Population". The Astronomical Journal. 135 (4): 1225–1238. Bibcode:2008AJ....135.1225H. doi:10.1088/0004-6256/135/4/1225. S2CID 122855486.
  5. ^ Sion, Edward M.; Holberg; Oswalt; McCook; Wasatonic (2009). "The White Dwarfs within 20 Parsecs of the Sun: Kinematics and Statistics". The Astronomical Journal. 138 (6): 1681–1689. arXiv:0910.1288. Bibcode:2009AJ....138.1681S. doi:10.1088/0004-6256/138/6/1681. S2CID 119284418.
  6. ^ Zacharias, N.; Monet, D. G.; Levine, S. E.; Urban, S. E.; Gaume, R.; Wycoff, G. L. (2004). "The Naval Observatory Merged Astrometric Dataset (NOMAD)". American Astronomical Society Meeting Abstracts. 205. Bibcode:2004AAS...205.4815Z.
  7. ^ a b c Cutri, R. M.; Skrutskie, M. F.; Van Dyk, S.; Beichman, C. A.; Carpenter, J. M.; Chester, T.; Cambresy, L.; Evans, T.; Fowler, J.; Gizis, J.; Howard, E.; Huchra, J.; Jarrett, T.; Kopan, E. L.; Kirkpatrick, J. D.; Light, R. M.; Marsh, K. A.; McCallon, H.; Schneider, S.; Stiening, R.; Sykes, M.; Weinberg, M.; Wheaton, W. A.; Wheelock, S.; Zacarias, N. (2003). "VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)". Vizier Online Data Catalog. Bibcode:2003yCat.2246....0C.
  8. ^ "GJ 293 -- White Dwarf". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2011-10-30.
  9. ^ Kirkpatrick, J. Davy; Marocco, Federico; et al. (April 2024). "The Initial Mass Function Based on the Full-sky 20 pc Census of ~3600 Stars and Brown Dwarfs". The Astrophysical Journal Supplement Series. 271 (2): 55. arXiv:2312.03639. Bibcode:2024ApJS..271...55K. doi:10.3847/1538-4365/ad24e2.
  10. ^ Reylé, Céline; Jardine, Kevin; Fouqué, Pascal; Caballero, Jose A.; Smart, Richard L.; Sozzetti, Alessandro (30 April 2021). "The 10 parsec sample in the Gaia era". Astronomy & Astrophysics. 650: A201. arXiv:2104.14972. Bibcode:2021A&A...650A.201R. doi:10.1051/0004-6361/202140985. S2CID 233476431. Data available at https://gruze.org/10pc/ Archived 12 March 2023 at the Wayback Machine
  11. ^ Van Altena, W. F.; Lee, J. T.; Hoffleit, E. D. (1995). The general catalogue of trigonometric [stellar] parallaxes. Bibcode:1995gcts.book.....V.