| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Corvus |
| Right ascension | 12h 20m 55.71287s [1] |
| Declination | –13° 33′ 56.6100″ [1] |
| Apparent magnitude (V) | +5.14 [2] |
| Characteristics | |
| Spectral type | K0 III [3] |
| U−B color index | +0.93 [4] |
| B−V color index | +1.048±0.003 [2] |
| Astrometry | |
| Radial velocity (Rv) | +14.0±0.7 [2] km/s |
| Proper motion (μ) |
RA: –4.93
[1]
mas/
yr Dec.: +9.86 [1] mas/ yr |
| Parallax (π) | 16.21 ± 0.29 mas [1] |
| Distance | 201 ± 4
ly (62 ± 1 pc) |
| Absolute magnitude (MV) | 1.18 [2] |
| Details | |
| Mass | 1.76 [5] M☉ |
| Radius | 9.92+0.11 −0.16 [6] R☉ |
| Luminosity | 43±1 [6] L☉ |
| Surface gravity (log g) | 3.01 [7] cgs |
| Temperature | 4,707+38 −27 [6] K |
| Metallicity [Fe/H] | 0.00±0.05 [8] dex |
| Rotational velocity (v sin i) | 0.0 [9] km/s |
| Age | 1.97 [5] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HR 4699 is a single [11] star in the southern constellation of Corvus. It is orange in hue and is dimly visible to the naked eye with an apparent visual magnitude of +5.14. [2] This star is located at a distance of approximately 201 light years from the Sun based on parallax. [1] It is drifting further away with a radial velocity of +14 km/s, after come to within 45.1 light-years some four million years ago. [2]
This is an aging giant star with a stellar classification of K0 III, [3] having exhausted the supply of hydrogen at its core then cooled and expanded to almost ten [6] times the Sun's radius. It is nearly two [5] billion years old with 1.76 times the mass of the Sun. [5] The star is radiating 43 times the luminosity of the Sun from its photosphere at an effective temperature of 4,707 K. [6]
- ^ a b c d e f 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. S2CID 18759600.
- ^ a b c d e f 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.
- ^ a b Houk, Nancy; Smith-Moore, M. (1978). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 4. Ann Arbor: Dept. of Astronomy, University of Michigan. Bibcode: 1988mcts.book.....H.
- ^ Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode: 1986EgUBV........0M.
- ^ a b c d Luck, R. Earle (2015). "Abundances in the Local Region. I. G and K Giants". The Astronomical Journal. 150 (3): 88. arXiv: 1507.01466. Bibcode: 2015AJ....150...88L. doi: 10.1088/0004-6256/150/3/88. S2CID 118505114.
- ^ a b c d e 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.
- ^ Luck, R. Earle; Heiter, Ulrike (June 2007). "Giants in the Local Region". The Astronomical Journal. 133 (6): 2464–2486. Bibcode: 2007AJ....133.2464L. doi: 10.1086/513194.
- ^ Gáspár, András; et al. (2016). "The Correlation between Metallicity and Debris Disk Mass". The Astrophysical Journal. 826 (2): 171. arXiv: 1604.07403. Bibcode: 2016ApJ...826..171G. doi: 10.3847/0004-637X/826/2/171. S2CID 119241004.
- ^ Massarotti, Alessandro; et al. (January 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. S2CID 121883397.
- ^ "HD 107418". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-12-07.
- ^ 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.
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| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Corvus |
| Right ascension | 12h 20m 55.71287s [1] |
| Declination | –13° 33′ 56.6100″ [1] |
| Apparent magnitude (V) | +5.14 [2] |
| Characteristics | |
| Spectral type | K0 III [3] |
| U−B color index | +0.93 [4] |
| B−V color index | +1.048±0.003 [2] |
| Astrometry | |
| Radial velocity (Rv) | +14.0±0.7 [2] km/s |
| Proper motion (μ) |
RA: –4.93
[1]
mas/
yr Dec.: +9.86 [1] mas/ yr |
| Parallax (π) | 16.21 ± 0.29 mas [1] |
| Distance | 201 ± 4
ly (62 ± 1 pc) |
| Absolute magnitude (MV) | 1.18 [2] |
| Details | |
| Mass | 1.76 [5] M☉ |
| Radius | 9.92+0.11 −0.16 [6] R☉ |
| Luminosity | 43±1 [6] L☉ |
| Surface gravity (log g) | 3.01 [7] cgs |
| Temperature | 4,707+38 −27 [6] K |
| Metallicity [Fe/H] | 0.00±0.05 [8] dex |
| Rotational velocity (v sin i) | 0.0 [9] km/s |
| Age | 1.97 [5] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HR 4699 is a single [11] star in the southern constellation of Corvus. It is orange in hue and is dimly visible to the naked eye with an apparent visual magnitude of +5.14. [2] This star is located at a distance of approximately 201 light years from the Sun based on parallax. [1] It is drifting further away with a radial velocity of +14 km/s, after come to within 45.1 light-years some four million years ago. [2]
This is an aging giant star with a stellar classification of K0 III, [3] having exhausted the supply of hydrogen at its core then cooled and expanded to almost ten [6] times the Sun's radius. It is nearly two [5] billion years old with 1.76 times the mass of the Sun. [5] The star is radiating 43 times the luminosity of the Sun from its photosphere at an effective temperature of 4,707 K. [6]
- ^ a b c d e f 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. S2CID 18759600.
- ^ a b c d e f 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.
- ^ a b Houk, Nancy; Smith-Moore, M. (1978). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 4. Ann Arbor: Dept. of Astronomy, University of Michigan. Bibcode: 1988mcts.book.....H.
- ^ Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode: 1986EgUBV........0M.
- ^ a b c d Luck, R. Earle (2015). "Abundances in the Local Region. I. G and K Giants". The Astronomical Journal. 150 (3): 88. arXiv: 1507.01466. Bibcode: 2015AJ....150...88L. doi: 10.1088/0004-6256/150/3/88. S2CID 118505114.
- ^ a b c d e 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.
- ^ Luck, R. Earle; Heiter, Ulrike (June 2007). "Giants in the Local Region". The Astronomical Journal. 133 (6): 2464–2486. Bibcode: 2007AJ....133.2464L. doi: 10.1086/513194.
- ^ Gáspár, András; et al. (2016). "The Correlation between Metallicity and Debris Disk Mass". The Astrophysical Journal. 826 (2): 171. arXiv: 1604.07403. Bibcode: 2016ApJ...826..171G. doi: 10.3847/0004-637X/826/2/171. S2CID 119241004.
- ^ Massarotti, Alessandro; et al. (January 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. S2CID 121883397.
- ^ "HD 107418". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-12-07.
- ^ 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.
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