HD 88809
Star in the constellation of Antlia
HD 88809 is a star located in the southern constellation Antlia . With an apparent magnitude of 5.89[ 2] it is barely visible to the naked eye under ideal conditions. The star is located at a distance of around 451 light years [ 1] but is drifting away at a heliocentric radial velocity of almost 20 km/s.[ 1]
HD 88809 has a classification of K1 III[ 3] 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 ,[ 10] which yields a diameter of 17.07[ 6] times that of the Sun at its estimated distance. At present HD 88809 has 129%[ 5] the mass of the Sun and shines with a luminosity approximately 117[ 5] times that of the Sun and has a surface temperature of 4,410 K ,[ 5] which gives it an orange glow of a K-type star. HD 88809 has a faint 13th magnitude companion located approximately 4.9″ away.[ 9]
References
^ a b c d e f g h 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 .
^ a b Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics . 355 : L27–L30. Bibcode :2000A&A...355L..27H . ISSN 0004-6361 .
^ a b 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 .
^ a b Mermilliod, J. -C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data : 0. Bibcode :1986EgUBV........0M .
^ a b c d Charbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R.; Palacios, A.; Ottoni, G. (January 2020). "Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era" . Astronomy & Astrophysics . 633 : A34. arXiv :1910.12732 . Bibcode :2020A&A...633A..34C . doi :10.1051/0004-6361/201936360 . ISSN 0004-6361 .
^ a b Lang, Kenneth R. (2006), Astrophysical formulae , Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser , ISBN 3-540-29692-1 . The radius (R* ) is given by:
2
⋅ ⋅ -->
R
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=
(
138
⋅ ⋅ -->
1.15
⋅ ⋅ -->
10
− − -->
3
)
AU
0.0046491
AU
/
R
⨀ ⨀ -->
≈ ≈ -->
34.14
⋅ ⋅ -->
R
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{\displaystyle {\begin{aligned}2\cdot R_{*}&={\frac {(138\cdot 1.15\cdot 10^{-3})\ {\text{AU}}}{0.0046491\ {\text{AU}}/R_{\bigodot }}}\\&\approx 34.14\cdot R_{\bigodot }\end{aligned}}}
^ 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. arXiv :1312.3474 . Bibcode :2014A&A...561A.126D . doi :10.1051/0004-6361/201220762 . ISSN 0004-6361 .
^ "Digital Demo Room - Stellar Structure and Evolution Simulator" . rainman.astro.illinois.edu .
^ a b 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 .
^ 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. arXiv :1609.04389 . Bibcode :2017AJ....153..136S . doi :10.3847/1538-3881/aa5df3 . ISSN 0004-6256 .