Observation data Epoch J2000 Equinox J2000 | |
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Constellation | Antlia |
Right ascension | 09 52 58.02763 |
Declination | −27° 19′ 55.8219″ |
Apparent magnitude (V) | 6.28 |
Characteristics | |
Spectral type | G1 V |
B−V color index | +0.62 |
Astrometry | |
Radial velocity (Rv) | 61.6±0.1 km/s |
Proper motion (μ) | RA: −278.245 mas/yr Dec.: +95.043 mas/yr |
Parallax (π) | 18.5634 ± 0.0256 mas |
Distance | 175.7 ± 0.2 ly (53.87 ± 0.07 pc) |
Absolute magnitude (MV) | +2.68 |
Details | |
Mass | 1.42 M☉ |
Radius | 2.59±0.11 R☉ |
Luminosity | 7.58 L☉ |
Surface gravity (log g) | 3.86 cgs |
Temperature | 5,940±110 K |
Metallicity | +0.15 dex |
Rotational velocity (v sin i) | 5.9±0.3 km/s |
Age | 2.75 Gyr |
Other designations | |
33 G. Antliae, CD−26° 7505, CPD−26°4079, HIP 48468, HR 3916, SAO 178130, WDS J09530-2720A | |
Database references | |
SIMBAD | data |
HD 85725, also known as HR 3916, is a yellow hued star located in the southern constellation Antlia. It has an apparent magnitude of 6.29, placing it near the limit for naked eye visibility. The object is relatively close at a distance of 176 light-years, but is receding with a heliocentric radial velocity of 61.6 km/s.
HD 85725 has a stellar classification of G1 V, which indicates that it is an ordinary G-type main-sequence star that is fusing hydrogen at its core. However, a low surface gravity of 7244 cm/s suggests that the object is instead an evolved subgiant.
At present it has 143% the mass of the Sun but is 2.59 times larger, which is not characteristic of a yellow dwarf. It shines at 7.6 times the luminosity of the Sun from its photosphere at a surface temperature of 5,940 K, which gives it a yellow glow. At an age of 2.75 billion years, HD 85725 is spinning leisurely with a projected rotational velocity of 5.9 km/s.
There is a 10th magnitude companion located 1.5″ away along a position angle of 25°. It appears to have a common proper motion with the star, suggesting physical relation.
References
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. ISSN 1063-7737. S2CID 255204555.
- ^ Houk, N. (1982). Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume_3. Declinations -40_ƒ0 to -26_ƒ0. Bibcode:1982mcts.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.
- ^ Nidever, David L.; Marcy, Geoffrey W.; Butler, R. Paul; Fischer, Debra A.; Vogt, Steven S. (August 2002). "Radial Velocities for 889 Late-Type Stars". The Astrophysical Journal Supplement Series. 141 (2): 503–522. arXiv:astro-ph/0112477. Bibcode:2002ApJS..141..503N. doi:10.1086/340570. eISSN 1538-4365. ISSN 0067-0049.
- ^ "BaSTI Home Page". basti.oa-abruzzo.inaf.it.
- ^ Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467. eISSN 1538-3881.
- ^ McDonald, I.; Zijlstra, A. A.; Watson, R. A. (October 2017). "Fundamental parameters and infrared excesses of Tycho-Gaia stars". Monthly Notices of the Royal Astronomical Society. 471 (1): 770–791. arXiv:1706.02208. Bibcode:2017MNRAS.471..770M. doi:10.1093/mnras/stx1433. ISSN 0035-8711.
- ^ Costa Silva, A. R.; Delgado Mena, E.; Tsantaki, M. (February 2020). "Chemical abundances of 1111 FGK stars from the HARPS-GTO planet search sample. III. Sulfur". Astronomy and Astrophysics. 634: A136. arXiv:1912.08659. Bibcode:2020A&A...634A.136C. doi:10.1051/0004-6361/201936523. ISSN 0004-6361.
- Delgado Mena, E.; Adibekyan, V.; Santos, N. C.; Tsantaki, M.; González Hernández, J. I.; Sousa, S. G.; Bertrán de Lis, S. (November 2021). "Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program". Astronomy & Astrophysics. 655: A99. arXiv:2109.04844. Bibcode:2021A&A...655A..99D. doi:10.1051/0004-6361/202141588. eISSN 1432-0746. ISSN 0004-6361. S2CID 237485512.
- ^ Saar, S. H.; Osten, R. A. (1 February 1997). "Rotation, turbulence and evidence for magnetic fields in southern dwarfs". Monthly Notices of the Royal Astronomical Society. 284 (4): 803–810. Bibcode:1997MNRAS.284..803S. doi:10.1093/mnras/284.4.803. eISSN 1365-2966. ISSN 0035-8711.
- "HD 85725". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 22 August 2017.
- Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (December 2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466–3471. Bibcode:2001AJ....122.3466M. doi:10.1086/323920. ISSN 0004-6256.
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