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61 Virginis b information


61 Virginis b
Artist's impression of 61 Virginis b as a hot super-Earth, with some sporadic volcanic activity.
Discovery
Discovered byVogt et al.
Discovery siteKeck Observatory
Anglo-Australian Observatory
Discovery date14 December 2009
Detection method
Radial velocity
Orbital characteristics
Apastron0.056163 AU
Periastron0.044239 AU
Semi-major axis
0.050201±0.000005 AU
Eccentricity0.12±0.11
Orbital period (sidereal)
4.2150±0.0006 d
101.16 h
Average orbital speed
130.01
Time of periastron
2453369.166
Argument of periastron
105±54
Star61 Virginis
Physical characteristics
Mean radius
~1.6 R🜨
Mass≥ 5.1 ME
Temperature1,054 K (781 °C; 1,438 °F)

61 Virginis b (abbreviated 61 Vir b) is an extrasolar planet, orbiting the 5th magnitude G-type star 61 Virginis, in Virgo. This planet has a minimum mass of 5.1 times that of Earth and is an example of a super-Earth planet. It orbits very close to the star, at a distance of 0.050201 AU with an eccentricity of 0.12. This planet was discovered on 14 December 2009 using the radial velocity method taken at Keck and Anglo-Australian Observatories.[1][2]

  1. ^ Vogt, Steven (2010). "A Super-Earth and two Neptunes Orbiting the Nearby Sun-like star 61 Virginis". The Astrophysical Journal. 708 (2): 1366–1375. arXiv:0912.2599. Bibcode:2010ApJ...708.1366V. doi:10.1088/0004-637X/708/2/1366. S2CID 1979253.
  2. ^ Tim Stephens (2009-12-14). "New planet discoveries suggest low-mass planets are common around nearby stars". UCSC News. UC Santa Cruz. Archived from the original on 23 December 2009. Retrieved 2009-12-14.

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