WASP-95 Planetary system
In 2013, a planet was discovered around WASP-95. The planet, WASP-95b, is a hot Jupiter about 10% more massive than Jupiter , and completes an orbit round its star every two days. It was discovered by its transit of the star in 2013.[ 5] ± 40.4 K .[ 6]
References
↑ Roman, Nancy G. (1987). "Identification of a constellation from a position" . Publications of the Astronomical Society of the Pacific 99 (617): 695. Bibcode :1987PASP...99..695R . doi :10.1086/132034 Constellation record for this object at VizieR .1 2 3 4 5 6 Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties" . Astronomy and Astrophysics . 674 : A1. arXiv :2208.00211 Bibcode :2023A& A...674A...1G . doi :10.1051/0004-6361/202243940 S2CID 244398875 . Gaia DR3 record for this source at VizieR .1 2 3 "WASP-95" . SIMBAD Centre de données astronomiques de Strasbourg . Retrieved 30 December 2016 .1 2 Bonomo, A. S.; Desidera, S.; et al. (June 2017). "The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets". Astronomy & Astrophysics 602 : A107. arXiv :1704.00373 Bibcode :2017A& A...602A.107B . doi :10.1051/0004-6361/201629882 . S2CID 118923163 . ↑ Hellier, Coel; Anderson, D. R.; Collier Cameron, A.; Delrez, L.; et al. (2013). "Transiting Hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b" . Monthly Notices of the Royal Astronomical Society . 440 (3): 1982– 1992. arXiv :1310.5630 Bibcode :2014MNRAS.440.1982H . doi :10.1093/mnras/stu410 S2CID 54977201 . 1 2 Saha, Suman; Sengupta, Sujan (2021), "Critical Analysis of Tess Transit Photometric Data: Improved Physical Properties for Five Exoplanets", The Astronomical Journal , 162 (5): 221, arXiv :2109.11366 Bibcode :2021AJ....162..221S , doi :10.3847/1538-3881/ac294d S2CID 237605336
