Observation data Epoch J2000 Equinox J2000 | |
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Constellation | Hydra |
Right ascension | 08 41 43.33591 |
Declination | −15° 56′ 36.1727″ |
Apparent magnitude (V) | 4.866 |
Characteristics | |
Spectral type | K0 III CNII |
U−B color index | +0.92 |
B−V color index | +1.07 |
Astrometry | |
Radial velocity (Rv) | −1.98±0.12 km/s |
Proper motion (μ) | RA: 3.676 mas/yr Dec.: -97.743 mas/yr |
Parallax (π) | 15.9089 ± 0.1297 mas |
Distance | 205 ± 2 ly (62.9 ± 0.5 pc) |
Absolute magnitude (MV) | +0.81 |
Details | |
Mass | 1.72±0.46 M☉ |
Radius | 11.10+0.15 −0.69 R☉ |
Luminosity | 54.445+0.536 −0.457 L☉ |
Surface gravity (log g) | 2.8 cgs |
Temperature | 4,688±5 K |
Metallicity | −0.01 dex |
Rotational velocity (v sin i) | 1.7 km/s |
Other designations | |
9 Hya, BD−15°2554, FK5 2684, HD 74137, HIP 42662, HR 3441, SAO 154552 | |
Database references | |
SIMBAD | data |
9 Hydrae is a single star in the equatorial constellation of Hydra, located 205 light years away from the Sun. It is visible to the naked eye as a faint, yellow-orange hued star with an apparent visual magnitude of 4.87. This body is moving closer to the Sun with a heliocentric radial velocity of −2 km/s.
This is an aging giant star with a stellar classification of K0 III CNII, where the suffix notation indicates an overabundance of cyanogen in the spectrum. It is a red clump giant, which indicates it is on the horizontal branch and is generating energy through helium fusion at its core. The star has 1.7 times the mass of the Sun but, as a consequence of evolving away from the main sequence, its envelope has swollen to 11 times the Sun's radius. It is radiating 54 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,688 K.
References
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ Høg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode:2000A&A...355L..27H.
- ^ Houk, N.; Smith-Moore, M. (1988). "Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars. Volume 4, Declinations -26°.0 to -12°.0". Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars. 4. Bibcode:1988mcts.book.....H.
- ^ Johnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99. Bibcode:1966CoLPL...4...99J.
- Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015, S2CID 119257644.
- ^ Massarotti, Alessandro; Latham, David W.; Stefanik, Robert P.; Fogel, Jeffrey (2008). "Rotational and Radial Velocities for a Sample of 761 Hipparcos Giants and the Role of Binarity". The Astronomical Journal. 135 (1): 209–231. Bibcode:2008AJ....135..209M. doi:10.1088/0004-6256/135/1/209.
- ^ Allende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: masses, radii and effective temperatures". Astronomy and Astrophysics. 352: 555–562. arXiv:astro-ph/9911002. Bibcode:1999A&A...352..555A.
- ^ "9 Hya". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved April 26, 2019.
- Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
- Alves, David R. (August 2000), "K-Band Calibration of the Red Clump Luminosity", The Astrophysical Journal, 539 (2): 732–741, arXiv:astro-ph/0003329, Bibcode:2000ApJ...539..732A, doi:10.1086/309278, S2CID 16673121.
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