WASP-107b

WASP-107b
Artist's impression of exoplanet WASP-107b.[1]
Discovery
Discovered byD. R. Anderson et al.
Discovery date2017
WASP-South
Orbital characteristics
0.0566 ± 0.0017 AU (8,470,000 ± 250,000 km)[2]
Eccentricity0.06 ± 0.04[2]
5.7214742 d[2]
StarWASP-107
Physical characteristics
0.96±0.03 RJ[2]
Mass0.096±0.005[2] MJ

WASP-107b is a super-Neptune exoplanet that orbits the star WASP-107. It lies 200 light-years away from Earth in the constellation Virgo.[3] Its discovery was announced in 2017 by a team led by D. R. Anderson via the WASP-South.[4]

  1. ^ heic1809 (2 May 2018). "Hubble detects helium in the atmosphere of an exoplanet for the first time". www.spacetelescope.org. Retrieved 4 May 2018.{{cite web}}: CS1 maint: numeric names: authors list (link)
  2. ^ a b c d e Piaulet, Caroline; Benneke, Björn; et al. (2021-01-18). "WASP-107b's Density Is Even Lower: A Case Study for the Physics of Planetary Gas Envelope Accretion and Orbital Migration". The Astronomical Journal. 161 (2): 70. arXiv:2011.13444. Bibcode:2021AJ....161...70P. doi:10.3847/1538-3881/abcd3c. ISSN 1538-3881. S2CID 227208673.
  3. ^ Reed, Nola (2 May 2018). "An Exoplanet First! Helium Spotted on Bizarre Comet-Like World". Space.com.
  4. ^ Anderson, D.R.; Cameron, A. Collier; et al. (August 2017). "The discoveries of WASP-91b, WASP-105b and WASP-107b: Two warm Jupiters and a planet in the transition region between ice giants and gas giants" (PDF). Astronomy & Astrophysics. 604 (A110): A110. arXiv:1701.03776. Bibcode:2017A&A...604A.110A. doi:10.1051/0004-6361/201730439. S2CID 58910823.