Astronomy:Pr0201 b

From HandWiki
Short description: Extrasolar planet in the constellation Cancer
Pr0201 b
Discovery
Discovered bySam Quinn
Discovery siteUniversity of Georgia
Discovery date2012
Radial velocity
Orbital characteristics
Orbital period4.4264 (± 0.007)[1] d
astron|astron|helion}}2,455,992.861
StarPr0201
Physical characteristics
Mass0.54 (± 0.039)[1] ||J}}}}}}


Pr0201 b[1] (also written Pr 0201 b)[2] 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 half of Jupiter and an orbital period of about 4 days, it is likely a hot Jupiter. Its host star, Pr0201, is rotationally variable and has a rotation period of 5.63 days.[3]

Discovery

Pr0201 b and Pr 0211 b were discovered in 2012 by Sam Quinn[1][2][4] and his colleagues while observing 53 stars in the Beehive cluster using the 1.5 m (4.9 ft; 1.6 yd) telescope at the University of Georgia in the United States.[2]

References

  1. 1.0 1.1 1.2 1.3 1.4 "Notes on Pr 0201 b". Extrasolar Planets Encyclopaedia. https://exoplanet.eu/catalog/pr_0201_b--1192/. 
  2. 2.0 2.1 2.2 2.3 Fazekas, Andrew (2012-09-21). "New Planets Found in Star Cluster - Would Have Dazzling Nights". National Geographic. http://news.nationalgeographic.com/news/2012/120920-new-planets-star-cluster-science-space-beehive-exoplanets/. 
  3. Kovács, Géza; Hartman, Joel D.; Bakos, Gáspár Á.; Quinn, Samuel N.; Penev, Kaloyan; Latham, David W.; Bhatti, Waqas; Csubry, Zoltán et al. (2014). "Stellar rotational periods in the planet hosting open cluster Praesepe". Monthly Notices of the Royal Astronomical Society 442 (3): 2081. doi:10.1093/mnras/stu946. Bibcode2014MNRAS.442.2081K. 
  4. Quinn, Samuel N.; White, Russel J.; Latham, David W.; Buchhave, Lars A.; Cantrell, Justin R.; Dahm, Scott E.; Fűrész, Gabor; Szentgyorgyi, Andrew H. et al. (2012-08-22). "Two 'b's in the Beehive: The Discovery of the First Hot Jupiters in an Open Cluster". The Astrophysical Journal (The American Astronomical Society) 756 (2): L33. doi:10.1088/2041-8205/756/2/L33. Bibcode2012ApJ...756L..33Q.