Astronomy:HD 88809
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Short description: Star in the constellation of Antlia
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Antlia[1] |
| Right ascension | 10h 13m 45.9269s[2] |
| Declination | −40° 20′ 45.683″[2] |
| Apparent magnitude (V) | 5.893±0.009[3] |
| Characteristics | |
| Spectral type | K1 III[4] |
| U−B color index | +1.25[5] |
| B−V color index | +1.21[5] |
| Astrometry | |
| Radial velocity (Rv) | 19.96±0.76[2] km/s |
| Proper motion (μ) | RA: −79.460[2] mas/yr Dec.: +2.511[2] mas/yr |
| Parallax (π) | 7.2269 ± 0.0909[2] mas |
| Distance | 451 ± 6 ly (138 ± 2 pc) |
| Absolute magnitude (MV) | +0.09[1] |
| Position (relative to HD 88809A)[6] | |
| Component | HD 88809B |
| Epoch of observation | J2000.0 |
| Angular distance | 4.9″ |
| Position angle | 105° |
| Observed separation (projected) | 676.2 AU {{{projsepref}}} |
| Details | |
| Mass | 1.29+1.20 −0.4[7] M☉ |
| Radius | 17.7[8] R☉ |
| Luminosity | 117±8[7] L☉ |
| Temperature | 4,410±110[7] K |
| Metallicity [Fe/H] | −0.2[7] dex |
| Rotational velocity (v sin i) | <1.3[9] km/s |
| Age | 4.9[10] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 88809 is a star located in the southern constellation Antlia. With an apparent magnitude of 5.89[3] it is barely visible to the naked eye under ideal conditions. The star is located at a distance of around 451 light years[2] but is drifting away at a heliocentric radial velocity of almost 20 km/s.[2]
HD 88809 has a classification of K1 III[4] which indicates that it is an evolved early K-type giant star that has exhausted hydrogen at its core and left the main sequence. It has an angular diameter of 1.15 mas,[11] which yields a diameter of 17.07[12] times that of the Sun at its estimated distance. At present HD 88809 has 129%[7] the mass of the Sun and shines with a luminosity approximately 117[7] times that of the Sun and has a surface temperature of 4,410 K,[7] which gives it an orange glow of a K-type star. HD 88809 has a faint 13th magnitude companion located approximately 4.9″ away.[6]
References
- ↑ 1.0 1.1 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A XHIP record for this object at VizieR.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 3.0 3.1 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355: L27–L30. ISSN 0004-6361. Bibcode: 2000A&A...355L..27H.
- ↑ 4.0 4.1 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. https://ui.adsabs.harvard.edu/abs/1982mcts.book.....H/abstract.
- ↑ 5.0 5.1 Mermilliod, J. -C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data: 0. Bibcode: 1986EgUBV........0M.
- ↑ 6.0 6.1 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. doi:10.1086/323920. ISSN 0004-6256. Bibcode: 2001AJ....122.3466M.
- ↑ 7.0 7.1 7.2 7.3 7.4 7.5 7.6 Charbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R. et al. (January 2020). "Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era". Astronomy & Astrophysics 633: A34. doi:10.1051/0004-6361/201936360. ISSN 0004-6361. Bibcode: 2020A&A...633A..34C.
- ↑ Hon, Marc; Huber, Daniel; Kuszlewicz, James S.; Stello, Dennis; Sharma, Sanjib; Tayar, Jamie; Zinn, Joel C.; Vrard, Mathieu et al. (2021). "A "Quick Look" at All-sky Galactic Archeology with TESS: 158,000 Oscillating Red Giants from the MIT Quick-look Pipeline". The Astrophysical Journal 919 (2): 131. doi:10.3847/1538-4357/ac14b1. Bibcode: 2021ApJ...919..131H.
- ↑ De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (January 2014). "A catalog of rotational and radial velocities for evolved stars: V. Southern stars⋆⋆⋆". Astronomy & Astrophysics 561: A126. doi:10.1051/0004-6361/201220762. ISSN 0004-6361. Bibcode: 2014A&A...561A.126D.
- ↑ "Digital Demo Room - Stellar Structure and Evolution Simulator". http://rainman.astro.illinois.edu/ddr/stellar/intermediate.html.
- ↑ Stassun, Keivan G.; Collins, Karen A.; Gaudi, B. Scott (3 March 2017). "Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes". The Astronomical Journal 153 (3): 136. doi:10.3847/1538-3881/aa5df3. ISSN 0004-6256. Bibcode: 2017AJ....153..136S.
- ↑ Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, 1 (3rd ed.), Birkhäuser, ISBN 3-540-29692-1, https://books.google.com/books?id=OvTjLcQ4MCQC&pg=PA41. The radius (R*) is given by:
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