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Binary star system in the constellation Hydra
HR 4458 is a binary star system in the equatorial constellation of Hydra . It has the Gould designation 289 G. Hydrae ; HR 4458 is the Bright Star Catalogue designation. At a distance of 31.13 light years , it is the closest star system to the Solar System within this constellation. This object is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.97. It is moving closer to the Earth with a heliocentric radial velocity of −22 km/s.
The primary component is K-type main-sequence star with a stellar classification of K0 V. It is around five billion years old with 84% of the Sun's radius . The star is radiating 37% of the Sun's luminosity from its photosphere at an effective temperature of 5,241 K. It has been examined for the presence of an infrared excess , but none was detected.
There is a common proper motion companion at an angular separation of 16.2″, corresponding to a projected separation of 162.5 AU . This is a white dwarf star with a classification of DC8. The orbital period of the pair is estimated as 1,110 years.
References
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^ Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data . Bibcode :1986EgUBV........0M .
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Holmberg, J.; et al. (July 2009), "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics", Astronomy and Astrophysics , 501 (3): 941–947, arXiv :0811.3982 , Bibcode :2009A&A...501..941H , doi :10.1051/0004-6361/200811191 , S2CID 118577511 .
^ Johnson, H. M.; Wright, C. D. (183). "Predicted infrared brightness of stars within 25 parsecs of the sun" . Astrophysical Journal Supplement Series . 53 (2): 643–711. Bibcode :1983ApJS...53..643J . doi :10.1086/190905 .
^ Eiroa, C.; et al. (July 2013). "DUst around NEarby Stars. The survey observational results". Astronomy & Astrophysics . 555 : A11. arXiv :1305.0155 . Bibcode :2013A&A...555A..11E . doi :10.1051/0004-6361/201321050 . S2CID 377244 .
^ Ramírez, I.; et al. (September 2012). "Lithium Abundances in nearby FGK Dwarf and Subgiant Stars: Internal Destruction, Galactic Chemical Evolution, and Exoplanets". The Astrophysical Journal . 756 (1): 46. arXiv :1207.0499 . Bibcode :2012ApJ...756...46R . doi :10.1088/0004-637X/756/1/46 . S2CID 119199829 .
Martínez-Arnáiz, R.; et al. (September 2010). "Chromospheric activity and rotation of FGK stars in the solar vicinity. An estimation of the radial velocity jitter" (PDF). Astronomy and Astrophysics . 520 : A79. arXiv :1002.4391 . Bibcode :2010A&A...520A..79M . doi :10.1051/0004-6361/200913725 . S2CID 43455849 . Archived from the original (PDF) on 2017-09-22. Retrieved 2018-11-04.
^ Mamajek, Eric E.; Hillenbrand, Lynne A. (November 2008). "Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics". The Astrophysical Journal . 687 (2): 1264–1293. arXiv :0807.1686 . Bibcode :2008ApJ...687.1264M . doi :10.1086/591785 . S2CID 27151456 .
"HD 100623" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved May 6, 2019.
^ Rodriguez, David R.; et al. (2015). "Stellar multiplicity and debris discs: An unbiased sample" . Monthly Notices of the Royal Astronomical Society . 449 (3): 3160. arXiv :1503.01320 . Bibcode :2015MNRAS.449.3160R . doi :10.1093/mnras/stv483 .
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