U Antliae
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Antlia |
Right ascension | 10h 35m 12.852s[1] |
Declination | −39° 33′ 45.32″[1] |
Apparent magnitude (V) | 5.505 |
Characteristics | |
Spectral type | N:v |
U−B color index | 7.1 |
B−V color index | 2.88 |
Variable type | LB |
Astrometry | |
Radial velocity (Rv) | 37 km/s |
Proper motion (μ) | RA: −31.02 ± 0.56[1] mas/yr Dec.: 3.50 ± 0.53[1] mas/yr |
Parallax (π) | 3.73 ± 0.54[1] mas |
Distance | approx. 900 ly (approx. 270 pc) |
Absolute magnitude (MV) | −5.22[2] |
Details | |
Mass | 1.04 M☉ |
Radius | 350 R☉ |
Luminosity | 5819[3] L☉ |
Temperature | 3317[3] K |
Age | ? years |
Other designations | |
Database references | |
SIMBAD | data |
Coordinates: 10h 35m 12.8507s, −39° 33′ 45.319″
U Antliae (U Ant) is a star in the constellation Antlia.
U Antliae is a red C-type carbon star and is an irregular variable star that varies between magnitudes 5.27 and 6.04.[4] Approximately 900 light years from Earth, it shines with a luminosity approximately 5819 times that of the Sun and has a surface temperature of 3317 K.[3] It is surrounded by two shells of dust, thought to have been ejected 14,000 and 10,000 years ago.[5]
References
- 1 2 3 4 5 van Leeuwen, F. (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.Vizier catalog entry
- ↑ Guandalini, R.; Cristallo, S. (2013). "Luminosities of carbon-rich asymptotic giant branch stars in the Milky Way". Astronomy & Astrophysics. 555: 7. arXiv:1305.4203. Bibcode:2013A&A...555A.120G. doi:10.1051/0004-6361/201321225. A120.
- 1 2 3 McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (2012). "Fundamental Parameters and Infrared Excesses of Hipparcos Stars". Monthly Notices of the Royal Astronomical Society. 427 (1): 343–57. arXiv:1208.2037. Bibcode:2012MNRAS.427..343M. doi:10.1111/j.1365-2966.2012.21873.x.
- ↑ Otero, Sebastian (3 November 2011). "U Antliae". AAVSO Website. American Association of Variable Star Observers. Retrieved 25 July 2014.
- ↑ Izumiura, H.; Waters, L. B. F. M.; de Jong, T.; Loup, C.; Bontekoe, Tj. R.; Kester, D. J. M. (1997). "A double dust shell surrounding the carbon star U Antliae". Astronomy and Astrophysics. 323: 449–60. Bibcode:1997A&A...323..449I.
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