Pr0211 c

Pr0211 c
Exoplanet List of exoplanets
Parent star
Star Pr0211
Constellation Cancer
Right ascension (α) 08h 42m 11.0s[1]
Declination (δ) +19° 16′ 37″[1]
Apparent magnitude (mV) 12.15[1]
Mass (m) 0.935 (± 0.013) [1] M☉
Radius (r) 0.827 (± 0.012) [1] R☉
Age 0.79 (± 0.03)[1] Gyr
Physical characteristics
Mass(m)7.95 (± 0.25)[1] MJ
Orbital elements
Semi-major axis(a) 5.8 ( -1.4 +2.9 )[1] AU
Eccentricity (e) 0.7 (± 0.1)[1]
Orbital period(P) 5300.0 ( -1800.0 +4450.0 ) (Julian Days)[1] d
Discovery information
Discovery date 18 February 2016
Discoverer(s) Sam Quinn
Discovery method Radial Velocity
Discovery site University of Georgia
Discovery status Confirmed

Pr0211 c'[1], sometimes written as Pr 0211 c, is a gas giant exoplanet orbiting around the Sun-like star Pr0211, a G-type main sequence star. Pr0211 c and two other planets, Pr0211 b and Pr0201 b are notable for being one of the first exoplanets discovered in the Beehive cluster located in the constellation Cancer, and for being the first multi-planet system discovered in an open cluster.[1]

Discovery

Pr0211 c was discovered in 2016 by Luca Malavolta[1][2] and his colleagues while observing its host star with the HARPS-N spectrograph on the 3.6 metres (12 ft; 3.9 yd) Italian Telescopio Nazionale Galileo (TNG) in La Palma, and the Tillinghast Reflector Echelle Spectrograph (TRES) mounted at the 1.5 metres (4.9 ft; 1.6 yd) telescope at the University of Georgia in the United States.

References

  1. 1 2 3 4 5 6 7 8 9 10 11 12 13 "Planet Pr 0211 c". Exoplanet.eu. Retrieved 2016-04-18.
  2. ↑ The GAPS programme with HARPS-N at TNG XI. Pr 0211 in M 44: the first multi-planet system in an open cluster


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