38 Virginis

38 Virginis is an F-type main sequence star in the constellation of Virgo. It is around 108 light years distant from the Earth.[2][1]

38 Virginis
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Virgo
Right ascension  12h 53m 11.1564s[1]
Declination −03° 33′ 11.1482″[1]
Apparent magnitude (V) 6.11
Characteristics
Spectral type F6V[2]
B−V color index 0.49[2]
Astrometry
Proper motion (μ) RA: −262.638±0.113[1] mas/yr
Dec.: −3.853±0.100[1] mas/yr
Parallax (π)30.0702 ± 0.0541[1] mas
Distance108.5 ± 0.2 ly
(33.26 ± 0.06 pc)
Absolute magnitude (MV)6.11
Details
Mass1.18 ± 0.12[2] M☉
Radius1.45 ± 0.07[2] R☉
Luminosity3.48[note 1] L☉
Temperature6557 ± 96[2] K
Metallicity [Fe/H]0.07[2] dex
Age1.9+0.6
−0.7[2] Gyr
Other designations
BD−02 3593, HD 111998, HIP 62875, HR 4891, WDS J12532-0333AB[3]
Database references
SIMBADdata

Nomenclature

The name 38 Virginis derives from the star being the 38th star in order of right ascension catalogued in the constellation Virgo by Flamsteed in his star catalogue. The designation b of 38 Virginis b derives from the order of discovery and is given to the first planet orbiting a given star, followed by the other lowercase letters of the alphabet.[4] In the case of 38 Virginis, only one was discovered, which was designated b.[2]

Stellar characteristics

38 Virginis is an F-type main sequence star that is approximately 118% the mass of and 145% the radius of the Sun. It has a temperature of 6557 K and is about 1.9 billion years old. In comparison, the Sun is about 4.6 billion years old[5] and has a temperature of 5778 K.[6]

The star is metal-rich, with a metallicity ([Fe/H]) of 0.07 dex, or 117% the solar amount. Its luminosity (L☉) is 3.48 times that of the Sun.

A companion star is cataloged in the CCDM at a separation of half an arcsecond.[7]

Planetary system
The 38 Virginis planetary system[2]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b 4.51 ± 0.5 MJ 1.82 ± 0.07 825.9 ± 6.2 0.03 ± 0.04 — ~4.51 RJ

The star is known to host one exoplanet, 38 Virginis b, discovered in 2016. This planet has a relatively low eccentricity out of any long-period giant exoplanet discovered, with an eccentricity of 0.03. The planet has a mass of around 4.5 times that of the planet Jupiter.[2] Its orbit very likely puts it and any moons it may have in the habitable zone of its star.

Notes
  1. From , where is the luminosity, is the radius, is the effective surface temperature and is the Stefan–Boltzmann constant.
gollark: You can probably obfuscate JS pretty well just by using a bunch of modern JS libraries and a bundler.
gollark: It's technically not *necessary*, but that doesn't make it *not useful*.
gollark: The problem is that I want:- some extensions to the "standard" markdown things - wikilinks, primarily- to use this with virtual DOM
gollark: ...
gollark: I'm implementing a thing in which I expect users will want advanced features like "headers" and "the ability to have links".

References
  1. 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.
  2. Borgniet, S.; et al. (2017). "Extrasolar planets and brown dwarfs around AF-type stars. IX. The HARPS southern sample". Astronomy and Astrophysics. 599. A57. arXiv:1608.08257. Bibcode:2017A&A...599A..57B. doi:10.1051/0004-6361/201628805.
  3. "38 Virginis". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-10-19.
  4. Hessman, F. V.; Dhillon, V. S.; Winget, D. E.; Schreiber, M. R.; Horne, K.; Marsh, T. R.; Guenther, E.; Schwope, A.; Heber, U. (2010). "On the naming convention used for multiple star systems and extrasolar planets". arXiv:1012.0707 [astro-ph.SR].
  5. Fraser Cain (16 September 2008). "How Old is the Sun?". Universe Today. Retrieved 19 February 2011.
  6. Fraser Cain (15 September 2008). "Temperature of the Sun". Universe Today. Retrieved 19 February 2011.
  7. J. Dommanget; et al. (February 2002), Catalog of Components of Double & Multiple Stars, Observations et Travaux, Societe Astronomique de France

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.