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59 Virgin

59 Virgin ( lat. 59 Virginis , GJ 504 ) - a star located in the constellation Virgo at a distance of about 57.3 light-years from us. Visible gloss +5.19 m [2] . At least one exoplanet (or brown dwarf ) is drawn around the star.

59 Virgin
Star
Yellow dwarf.jpg
Yellow dwarf in the view of the artist.
Observational data
( Age J2000.0 )
Type ofSingle star
Right ascension
Declination
Distance57.27 ± 0.26 St. years (17.56 ± 0.08 pc ) [1]
Visible magnitude ( V )5.191 ± 0.005 [2]
ConstellationVirgo
Astrometry
Radial velocity ( R v )-25.9 [3] km / s
Own movement (μ)RA: -333.83 [3]
Dec: 190.24 [3]
Parallax (π)56.95 ± 0.26 [3] mas
Absolute magnitude (V)4.08 ± 0.01 [4]
Specifications
Spectral classG0V [3]
physical characteristics
Weight1.16 ± 0.05 [2] M ☉
Radius1.36 ± 0.04 [2] R ☉
Age0.160 +0.35
−0.06 [1] ,
4.5 +2.0
−1.5 [2] ,
or 2.5 +1.0
−0.7 billion [5] years
Temperature6205 ± 20 [5] K
Luminosity2.15 ± 0.15 [1] L ☉
Metallicity[Fe / H] = 0.28 ± 0.03 [1]
Rotationperiod - 3.33 days. [five]
Other designations
BD +10 2531 , CCDM J13168 + 0925A , HD 115383 , HIC 64792 , HIP 64792 , HR 5011 , IRAS 13142 + 0941 , NLTT 33523 , PPM 159616 , 1RXS J131646.6 + 092530 , SAO 119847 , 2MASS J13164653 + 0925269 09 1600, ASCC 1045052, CSI +10 2531 1, EUVE J1316 + 09.4, 2EUVE J1316 + 09.4, 2E 1314.3 + 0941, 1ES 1314 + 09.6, GC 17975, GCRV 7894, GJ 504, IDS 13118 + 0957 A, LSPM J1316 + 0925, N30 3043, PLX 3034, ROT 1948, RX J1316.7 + 0925, SKY # 24535, SPOCS # 560, TD1 16736, TYC 891-624-1, UBV 12004, USNO-B1.0 0994-00226172, uvby98 100115383 , WDS J13168 + 0925A, YZ 9 4809 59 Virginis
Database Information
SIMBADdata
Sources: [3]

Content

Features

59 Virgin received this designation thanks to John Flemstead , who entered it into his star catalog in the 18th century .

59 Virgo is a yellow dwarf , somewhat larger, massive and hotter than the Sun. Its spectral class is G0V [1] , temperature is 6205 ± 20 K [5] , radius is 1.36 ± 0.04 solar [2] , mass is 1.16 ± 0.05 solar [2] , and luminosity is 2.15 ± 0.15 solar [1] . The period of axial rotation of the star is defined as 3.33 days (it is possible, however, that it is twice as large) [5] .

Researchers paid great attention to the age of the star, since it is needed to estimate the mass and other parameters of its satellite. In 2013, a score of 0.16 +0.35 was published
−0.60 billion years [1] , in 2015 - 4.5 +2.0
−1.5 billion years [2] , and in 2017 - 2.5 +1.0
−0.7 billion years [5] (for comparison: the age of our Sun is estimated at 4.57 billion years).

Estimates of the age of a star based on its rotation speed and its position on the Hertzsprung-Russell diagram diverge significantly. This can be explained by the fact that it absorbed the hot Jupiter circulating around it, which increased its rotation speed and chromospheric activity [5] .

Planet System

In 2011, an international group of astronomers, photographing a star with the 8.2-meter Subaru telescope, discovered the planet GJ 504 b . The discovery was published in 2013. The distance of GJ 504 b from the mother star in the projection onto the celestial sphere is 43.5 a. that is, 1.5 times the radius of the orbit of Neptune (the real distance in space may be even greater) [1] [6] . Thus, the planet receives very little light from the star. Nevertheless, it is rather hot: 271 ± 10 ° C [7] . Its mass, according to initial estimates, is 3–9 masses of Jupiter, and according to a later estimate, it is 20–30 masses of Jupiter, and in this case it is no longer a planet, but a brown dwarf [2] [7] [5] . The radius of the object is estimated at 0.96 ± 0.07 of the radius of Jupiter [7] .

Planet
Weight
( M J )
Radius
( R J )
Circulation period
( days )
Semimajor axis
orbits ( a.u. )
Eccentricity
orbits
b3-300.96 ± 0.07 [7]?≥43.5?

Notes

  1. ↑ 1 2 3 4 5 6 7 8 Kuzuhara, M .; Tamura, M .; Kudo, T. et el. Direct Imaging of a Cold Jovian Exoplanet in Orbit around the Sun-like Star GJ 504 // The Astrophysical Journal: journal. - 2013 .-- Vol. 774 , no. 1 . - DOI : 10.1088 / 0004-637X / 774/1/11 . - . - arXiv : 1307.2886 .
  2. ↑ 1 2 3 4 5 6 7 8 9 Fuhrmann, K .; Chini, R. On the age of Gliese 504 (Eng.) // The Astrophysical Journal. - 2015. - Vol. 806 , no. 2 . - DOI : 10.1088 / 0004-637X / 806/2/163 . - .
  3. ↑ 1 2 3 4 5 6 SIMBAD (English) . - 59 Virgin in the SIMBAD database . Date of treatment August 8, 2013.
  4. ↑ Park, Sunkyung; Kang, Wonseok; Lee, Jeong-Eun; Lee, Sang-Gak. Wilson-Bappu Effect: Extended to Surface Gravity // The Astronomical Journal. - 2013 .-- Vol. 146 , no. 4 . - P. 73 . - DOI : 10.1088 / 0004-6256 / 146/4/73 . - . - arXiv : 1307.0592 . (Absolute magnitudes of stars are given in band V according to Hipparcos ).
  5. ↑ 1 2 3 4 5 6 7 8 D'Orazi, V .; Desidera, S .; Gratton, RG et al. A critical reassessment of the fundamental properties of GJ 504: chemical composition and age // Astronomy & Astrophysics: journal. - 2017 .-- Vol. 598 . - DOI : 10.1051 / 0004-6361 / 201629283 . - . - arXiv : 1609.02530 .
  6. ↑ Astronomers removed the planet in the wrong place
  7. ↑ 1 2 3 4 Skemer, AJ; Morley, CV; Zimmerman, NT et al. The LEECH Exoplanet Imaging Survey: Characterization of the Coldest Directly Imaged Exoplanet, GJ 504 b, and Evidence for Superstellar Metallicity // The Astrophysical Journal: journal. - 2016. - Vol. 817 , no. 2 . - DOI : 10.3847 / 0004-637X / 817/2/166 . - . - arXiv : 1511.09183 .

See also

  • List of Virgo constellation stars

Links

  • 59 Virgin in the Encyclopedia of Extrasolar Planets
  • 59 Virgo on the Planet Systems website
  • Astronomers Image Lowest-mass Exoplanet Around a Sun-like Star . NASA (August 5, 2013). Archived on June 29, 2017.
  • The Subaru telescope received images of an exoplanet, the “double” of Jupiter. RIA News
Source - https://ru.wikipedia.org/w/index.php?title=59_Virgo&oldid=100041522


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Clever Geek | 2019