WASP-61是一顆F型主序星,距離大約1,560光年。這顆恆星的年齡可能比太陽年輕,大約為3.8+1.8 −0.9億年。WASP-61的重元素含量很低,鐵豐度僅占太陽的40%[3]。
行星系統
2012年,觀測到一顆超級木星的行星WASP-61b在一個緊密的圓形軌道上凌日[5]。其平衡溫度為7003156500000000000♠1565±35 K[5]。
行星軌道與恆星的赤道平面對齊,錯位等於4.0+17.1 −18.4°[6]。
參考資料
- ^ 1.0 1.1 1.2 1.3 1.4 1.5 Brown, A. G. A.; Vallenari, A.; Prusti, T.; de Bruijne, J. H. J.; et al. Gaia Data Release 2. Summary of the contents and survey properties. Astronomy & Astrophysics. 2018. Bibcode:2018A&A...616A...1G. arXiv:1804.09365 . doi:10.1051/0004-6361/201833051. VizieR中此天体在盖亚望远镜第二批数据发布的记录
- ^ 2.0 2.1 Bonomo, A. S.; et al, The GAPS Programme with HARPS-N at TNG, Astronomy & Astrophysics, 2017, 602: A107, Bibcode:2017A&A...602A.107B, S2CID 118923163, arXiv:1704.00373 , doi:10.1051/0004-6361/201629882
- ^ 3.0 3.1 3.2 3.3 Andreasen, D. T.; Sousa, S. G.; Tsantaki, M.; Teixeira, G. D. C.; Mortier, A.; Santos, N. C.; Suárez-Andrés, L.; Delgado-Mena, E.; Ferreira, A. C. S., SWEET-Cat update and FASMA, Astronomy & Astrophysics, 2017, 600: A69, S2CID 119534579, arXiv:1703.06671 , doi:10.1051/0004-6361/201629967
- ^ WASP-61. SIMBAD. 斯特拉斯堡天文資料中心.
- ^ 5.0 5.1 5.2 Hellier, Coel; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G., Seven transiting hot-Jupiters from WASP-South, Euler and TRAPPIST: WASP-47b, WASP-55b, WASP-61b, WASP-62b, WASP-63b, WASP-66b & WASP-67b, Monthly Notices of the Royal Astronomical Society, 2012, 426 (1): 739–750, Bibcode:2012MNRAS.426..739H, S2CID 54713354, arXiv:1204.5095 , doi:10.1111/j.1365-2966.2012.21780.x
- ^ Brown, D. J. A.; Triaud, A. H. M. J.; Doyle, A. P.; Gillon, M.; Lendl, M.; Anderson, D. R.; Collier Cameron, A.; Hébrard, G.; Hellier, C.; Lovis, C.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Smalley, B., Rossiter–Mc Laughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems, Monthly Notices of the Royal Astronomical Society, 2016, 464: 810–839, arXiv:1610.00600 , doi:10.1093/mnras/stw2316
- ^ Stassun, Keivan G.; Collins, Karen A.; Gaudi, B. Scott, Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes, The Astronomical Journal, 2016, 153 (3): 136, Bibcode:2017AJ....153..136S, S2CID 119219062, arXiv:1609.04389 , doi:10.3847/1538-3881/aa5df3
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