Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Phoenix |
Right ascension | 23 51 31.08391 |
Declination | −39° 54′ 24.2582″ |
Apparent magnitude (V) | 11.33 |
Characteristics | |
WASP-29A | |
Evolutionary stage | main sequence star |
Spectral type | K4V |
B−V color index | 0.82 |
J−H color index | 0.478 |
J−K color index | 0.570 |
WASP-29B | |
Spectral type | M3V |
Astrometry | |
Radial velocity (Rv) | 24.31±0.20 km/s |
Proper motion (μ) | RA: −56.767(14) mas/yr Dec.: −88.988(13) mas/yr |
Parallax (π) | 11.4349 ± 0.0151 mas |
Distance | 285.2 ± 0.4 ly (87.5 ± 0.1 pc) |
Position (relative to WASP-29A) | |
Component | WASP-29B |
Epoch of observation | 2021 |
Angular distance | 125.2″ |
Projected separation | 10994 AU |
Details | |
WASP-29A | |
Mass | 0.825±0.033 M☉ |
Radius | 0.808±0.044 R☉ |
Surface gravity (log g) | 4.5±0.2 cgs |
Temperature | 4800±150 K |
Metallicity | 0.11±0.14 dex |
Rotational velocity (v sin i) | 1.50±0.60 km/s |
Age | 14+0 −7 Gyr |
WASP-29B | |
Mass | 0.38 M☉ |
Other designations | |
CD−40 15273, TOI-192, TIC 183537452, WASP-29, TYC 8015-1020-1, 2MASS J23513108-3954241, DENIS J235131.0-395423 | |
WASP-29A: Gaia DR3 6534414719318886144 | |
WASP-29B: Gaia DR3 6534426740931264896 | |
Database references | |
SIMBAD | data |
WASP-29 is a binary star system 285 light-years (87 parsecs) away in the constellation of Phoenix. The primary star is a K-type main-sequence star. Its comoving companion, a red dwarf star, was discovered in 2021. The star system kinematically belongs to the thin disk of the Milky Way. The primary is an old star with small starspot activity and low x-ray flux.
Planetary system
The "hot Saturn" class planet WASP-29b was discovered around WASP-29 in 2010. The planet would have an equilibrium temperature of 960±30 K. The planetary atmosphere has abundant carbon monoxide but likely lacks methane and sodium, although the high and dense cloud deck of WASP-29b prevents high-quality spectroscopic measurements.
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.
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 0.243+0.020 −0.019 MJ |
0.0470±0.0025 | 3.92271218(25) | <0.059 | 89.468+0.018 −0.017° |
0.775±0.031 RJ |
References
- ^ 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.
- ^ "WASP-29". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 5 November 2023.
- ^ Fontanive, 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
- ^ 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.; 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. S2CID 64119308.
- 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, S2CID 232417342
- ^ 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
- Matthew Hardin, Joseph Harrington, K. Stevenson, "WASP-29b: Another Cool Exoplanet With Abundant CO?"
- A Gemini ground-based transmission spectrum of WASP-29b: a featureless spectrum from 515 to 720 nm
- Wong, Ian; Chachan, Yayaati; Knutson, Heather A.; Henry, Gregory W.; Adams, Danica; Kataria, Tiffany; Benneke, Björn; Gao, Peter; Deming, Drake; López-Morales, Mercedes; Sing, David K.; Alam, Munazza K.; Ballester, Gilda E.; Barstow, Joanna K.; Buchhave, Lars A.; Dos Santos, Leonardo A.; Fu, Guangwei; Muñoz, Antonio García; MacDonald, Ryan J.; Mikal-Evans, Thomas; Sanz-Forcada, Jorge; Wakeford, Hannah R. (2022), "The Hubble PanCET Program: A Featureless Transmission Spectrum for WASP-29b and Evidence of Enhanced Atmospheric Metallicity on WASP-80b", The Astronomical Journal, 164 (1): 30, arXiv:2205.10765, Bibcode:2022AJ....164...30W, doi:10.3847/1538-3881/ac7234, S2CID 248987053
- Georgakarakos, Nikolaos; Eggl, Siegfried; Dobbs-Dixon, Ian (April 2018). "Giant Planets: Good Neighbors for Habitable Worlds?". The Astrophysical Journal. 856 (2): 155. arXiv:1804.02183. Bibcode:2018ApJ...856..155G. doi:10.3847/1538-4357/aaaf72.
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