| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Crater |
| Right ascension | 11h 03m 14.87973s [1] |
| Declination | −11° 18′ 12.4981″ [1] |
| Apparent magnitude (V) | 5.50 [2] |
| Characteristics | |
| Spectral type | G7-IIIb [3] |
| B−V color index | +0.94 [2] |
| Astrometry | |
| Radial velocity (Rv) | −8.90 ± 0.10 [4] km/s |
| Proper motion (μ) |
RA: −81.61
[1]
mas/
yr Dec.: −108.01 [1] mas/ yr |
| Parallax (π) | 9.63 ± 0.69 mas [1] |
| Distance | 340 ± 20
ly (104 ± 7 pc) |
| Details [4] | |
| Mass | 2.43 ± 0.15 M☉ |
| Radius | 10.10 ± 0.76 R☉ |
| Luminosity | 64.6 L☉ |
| Surface gravity (log g) | 3.05 ± 0.07 cgs |
| Temperature | 5029 ± 34 K |
| Metallicity [Fe/H] | −0.04 ± 0.03 dex |
| Rotational velocity (v sin i) | 2.27 ± 0.45 km/s |
| Age | 0.68 ± 0.13 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 95808 is a double star in the constellation of Crater. Its apparent magnitude is 5.50, [2] but interstellar dust makes it appear 0.11 magnitudes dimmer than it should be. [4] It is located some 340 light-years (104 parsecs) away, based on parallax. [1]
HD 95808 is a G-type giant star. At an age of 680 million years old, it has swelled up to a radius of 10.1 times that of the Sun, and it is 2.43 times as massive. It emits 64.6 times as much energy as the Sun at a surface temperature of 5,029 K. [4]
References
- ^ a b c d e f van Leeuwen, F.; et al. (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 Corben, P. M. (1966). "Photoelectric magnitudes and colours for bright southern stars". Monthly Notes of the Astron. Soc. Southern Africa. 25: 44. Bibcode: 1966MNSSA..25...44C.
- ^ Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars". The Astrophysical Journal Supplement Series. 71: 245. Bibcode: 1989ApJS...71..245K. doi: 10.1086/191373.
- ^ a b c d Jofré, E.; Petrucci, R.; Saffe, C.; Saker, L.; de la Villarmois, E. Artur; Chavero, C.; Gómez, M.; Mauas, P. J. D. (2015). "Stellar parameters and chemical abundances of 223 evolved stars with and without planets". Astronomy & Astrophysics. 574: A50. arXiv: 1410.6422. Bibcode: 2015A&A...574A..50J. doi: 10.1051/0004-6361/201424474. S2CID 53666931.
 | This giant-star-related article is a stub. You can help Wikipedia by expanding it. |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Crater |
| Right ascension | 11h 03m 14.87973s [1] |
| Declination | −11° 18′ 12.4981″ [1] |
| Apparent magnitude (V) | 5.50 [2] |
| Characteristics | |
| Spectral type | G7-IIIb [3] |
| B−V color index | +0.94 [2] |
| Astrometry | |
| Radial velocity (Rv) | −8.90 ± 0.10 [4] km/s |
| Proper motion (μ) |
RA: −81.61
[1]
mas/
yr Dec.: −108.01 [1] mas/ yr |
| Parallax (π) | 9.63 ± 0.69 mas [1] |
| Distance | 340 ± 20
ly (104 ± 7 pc) |
| Details [4] | |
| Mass | 2.43 ± 0.15 M☉ |
| Radius | 10.10 ± 0.76 R☉ |
| Luminosity | 64.6 L☉ |
| Surface gravity (log g) | 3.05 ± 0.07 cgs |
| Temperature | 5029 ± 34 K |
| Metallicity [Fe/H] | −0.04 ± 0.03 dex |
| Rotational velocity (v sin i) | 2.27 ± 0.45 km/s |
| Age | 0.68 ± 0.13 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 95808 is a double star in the constellation of Crater. Its apparent magnitude is 5.50, [2] but interstellar dust makes it appear 0.11 magnitudes dimmer than it should be. [4] It is located some 340 light-years (104 parsecs) away, based on parallax. [1]
HD 95808 is a G-type giant star. At an age of 680 million years old, it has swelled up to a radius of 10.1 times that of the Sun, and it is 2.43 times as massive. It emits 64.6 times as much energy as the Sun at a surface temperature of 5,029 K. [4]
References
- ^ a b c d e f van Leeuwen, F.; et al. (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 Corben, P. M. (1966). "Photoelectric magnitudes and colours for bright southern stars". Monthly Notes of the Astron. Soc. Southern Africa. 25: 44. Bibcode: 1966MNSSA..25...44C.
- ^ Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars". The Astrophysical Journal Supplement Series. 71: 245. Bibcode: 1989ApJS...71..245K. doi: 10.1086/191373.
- ^ a b c d Jofré, E.; Petrucci, R.; Saffe, C.; Saker, L.; de la Villarmois, E. Artur; Chavero, C.; Gómez, M.; Mauas, P. J. D. (2015). "Stellar parameters and chemical abundances of 223 evolved stars with and without planets". Astronomy & Astrophysics. 574: A50. arXiv: 1410.6422. Bibcode: 2015A&A...574A..50J. doi: 10.1051/0004-6361/201424474. S2CID 53666931.
|
| This giant-star-related article is a stub. You can help Wikipedia by expanding it. |