Pr0201 b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | Pr0201 | |
Constellation | Cancer [1] | |
Right ascension | (α) | 08h 41m 44.0s[2] |
Declination | (δ) | +19° 16′ 37″[2] |
Apparent magnitude | (mV) | 12.15[2] |
Mass | (m) | 1.234 (± 0.034) [2] M☉ |
Radius | (r) | 1.167 (± 0.121) [2] R☉ |
Temperature | (T) | 6174 (± 50) K |
Metallicity | [Fe/H] | 0.187 |
Age | 0.578 (± 0.049)[2] Gyr | |
Physical characteristics | ||
Mass | (m) | 0.54 (± 0.039)[2] MJ |
Orbital elements | ||
Orbital period | (P) | 4.4264 (± 0.007) (days)[2] d |
Time of periastron | (T0) | 2455992.861 JD |
Discovery information | ||
Discovery date | 2012 | |
Discoverer(s) | Sam Quinn | |
Discovery method | Radial Velocity | |
Discovery site | University of Georgia | |
Discovery status | Confirmed |
Pr0201 b[2] (also written Pr 0201 b)[1] is an exoplanet orbiting around the F-type main sequence star Pr0201. Pr0201 b along with Pr0211 b are notable for being the first exoplanets discovered in the Beehive cluster located in the Constellation Cancer.[1][2] Since Pr0201 b has a mass of about 0.5 Jupiters and an orbital period of about 4 days, it is likely a hot Jupiter.
Discovery
Pr0201 b and Pr 0211 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 "Notes on Pr 0201 b". Exoplanet.eu. Retrieved 2017-01-02.
- ↑ "TWO "b"s IN THE BEEHIVE: THE DISCOVERY OF THE FIRST HOT JUPITERS IN AN OPEN CLUSTER". The American Astronomical Society. 2012-08-22.
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