Pr0211 b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | Pr0211 | |
Constellation | Cancer [1] | |
Right ascension | (α) | 08h 42m 11.0s[2] |
Declination | (δ) | +19° 16′ 37″[2] |
Apparent magnitude | (mV) | 12.15[2] |
Mass | (m) | 0.935 (± 0.013) [2] M☉ |
Radius | (r) | 0.827 (± 0.012) [2] R☉ |
Age | 0.79 (± 0.03)[2] Gyr | |
Physical characteristics | ||
Mass | (m) | 1.88 (± 0.02)[2] MJ |
Orbital elements | ||
Semi-major axis | (a) | 0.03184 (± 0.00015) [2] AU |
Eccentricity | (e) | 0.017 (± 0.01)[2] |
Orbital period | (P) | 2.14609 (± 2e-05) (Julian Days)[2] d |
Discovery information | ||
Discovery date | 2012 | |
Discoverer(s) | Sam Quinn | |
Discovery method | Radial Velocity | |
Discovery site | University of Georgia | |
Discovery status | Confirmed |
Pr0211 b[2] (also written Pr 0211 b)[1] is a gas giant exoplanet orbiting around the Sun-like star Pr0211, a G-type main sequence star. Pr0211 b along with Pr0201 b are notable for being the first exoplanets discovered in the Beehive cluster located in the constellation Cancer.[1][2]
Discovery
Pr0211 b and Pr0201 b were discovered in 2012 by Sam Quinn[1][2][3] and his colleagues while observing 53 stars in the Beehive cluster using the 1.5 metres (4.9 ft; 1.6 yd) telescope at the University of Georgia in the United States.[1]
References
- 1 2 3 4 5 Fazekas, Andrew (2012-09-21). "New Planets Found in Star Cluster - Would Have Dazzling Nights". National Geographic News. NATIONAL GEOGRAPHIC. Retrieved 2016-05-30.
- 1 2 3 4 5 6 7 8 9 10 11 12 13 "Planet Pr 0211 b". Exoplanet.eu. Retrieved 2016-04-18.
- ↑ https://iopscience.iop.org/article/10.1088/2041-8205/756/2/L33/meta;jsessionid=22B1114FA9B7BAB2F3D65FC22C4045C4.c1
This article is issued from
Wikipedia.
The text is licensed under Creative Commons - Attribution - Sharealike.
Additional terms may apply for the media files.