The "hot Saturn" class planet WASP-29b was discovered around WASP-29 in 2010.[5] The planet would have an equilibrium temperature of 960±30
K.[7] The planetary atmosphere has abundant
carbon monoxide but likely lacks
methane[8] and
sodium,[9] although the high and dense cloud deck of WASP-29b prevents high-quality spectroscopic measurements.[10]
A study in 2018 revealed the stability of planetary orbits in the habitable zone of WASP-29 is significantly affected by the WASP-29b planet.[11]
^
abcdeFontanive, Clémence; Daniella Bardalez Gagliuffi (2021), "The Census of Exoplanets in Visual Binaries: population trends from a volume-limited Gaia DR2 and literature search", Frontiers in Astronomy and Space Sciences, 8: 16,
arXiv:2101.12667,
Bibcode:
2021FrASS...8...16F,
doi:10.3389/fspas.2021.625250
^
abHellier, Coel; Anderson, D. R.; Collier Cameron, A.; Gillon, M.; Lendl, M.; Maxted, P. F. L.; Queloz, D.; Smalley, B.; Triaud, A. H. M. J.; West, R. G.; Brown, D. J. A.; Enoch, B.; Lister, T. A.; Pepe, F.; Pollacco, D.; Ségransan, D.; Udry, S. (2010). "WASP-29b: A SATURN-SIZED TRANSITING EXOPLANET". The Astrophysical Journal. 723 (1): L60–L63.
arXiv:1009.5318.
Bibcode:
2010ApJ...723L..60H.
doi:
10.1088/2041-8205/723/1/L60.
S2CID64119308.
^Dos Santos, L. A.; Bourrier, V.; Ehrenreich, D.; Sanz-Forcada, J.; López-Morales, M.; Sing, D. K.; García Muñoz, A.; Henry, G. W.; Lavvas, P.; Lecavelier Des Etangs, A.; Mikal-Evans, T.; Vidal-Madjar, A.; Wakeford, H. R. (2021), "HST PanCET program: Non-detection of atmospheric escape in the warm Saturn-sized planet WASP-29 B", Astronomy & Astrophysics, 649: A40,
arXiv:2103.15688,
Bibcode:
2021A&A...649A..40D,
doi:
10.1051/0004-6361/202140491,
S2CID232417342