WASP-29

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WASP-29
Observation data
Epoch J2000       Equinox J2000
Constellation Phoenix [1]
Right ascension 23h 51m 31.08391s [2]
Declination −39° 54′ 24.2582″ [2]
Apparent magnitude  (V)11.33 [3]
Characteristics
WASP-29A
Evolutionary stage main sequence star
Spectral type K4V [4]
B−V color index 0.82
J−H color index 0.478
J−K color index 0.570
WASP-29B
Spectral type M3V [4]
Astrometry
Radial velocity (Rv)24.31±0.20 [2] km/s
Proper motion (μ)RA: −56.767(14) mas/yr [2]
Dec.: −88.988(13) mas/yr [2]
Parallax (π)11.4349±0.0151  mas [2]
Distance 285.2 ± 0.4  ly
(87.5 ± 0.1  pc)
Position (relative to WASP-29A) [4]
ComponentWASP-29B
Epoch of observation 2021
Angular distance 125.2″
Projected separation 10994 AU
Details [5]
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 [Fe/H]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 [4]   M☉
Other designations
CD−40 15273, TOI-192, TIC 183537452, WASP-29, TYC 8015-1020-1, 2MASS J23513108-3954241, DENIS J235131.0-395423 [3]
WASP-29A: Gaia DR3 6534414719318886144
WASP-29B: Gaia DR3 6534426740931264896
Database references
SIMBAD data
Exoplanet Archive 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. [4] The star system kinematically belongs to the thin disk of the Milky Way. [6] The primary is an old star with small starspot activity and low x-ray flux. [7]

Planetary system

The "hot Saturn" class planet WASP-29b was discovered around WASP-29 in 2010. [6] The planet would have an equilibrium temperature of 960±30 K. [8] The planetary atmosphere has abundant carbon monoxide but likely lacks methane [9] and sodium, [10] although the high and dense cloud deck of WASP-29b prevents high-quality spectroscopic measurements. [11]

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. [12]

The WASP-29 planetary system [8]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b0.243+0.020
−0.019  MJ 		0.0470±0.00253.92271218(25)<0.059 [5] 89.468+0.018
−0.017 ° 		0.775±0.031  RJ

References

  1. ↑ 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.
  2. 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.
  3. 1 2 "WASP-29". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 5 November 2023.
  4. 1 2 3 4 5 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 625250: 16, arXiv: 2101.12667 , Bibcode:2021FrASS...8...16F, doi: 10.3389/fspas.2021.625250
  5. 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.
  6. 1 2 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.
  7. ↑ 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
  8. 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
  9. ↑ Matthew Hardin, Joseph Harrington, K. Stevenson, "WASP-29b: Another Cool Exoplanet With Abundant CO?"
  10. ↑ A Gemini ground-based transmission spectrum of WASP-29b: a featureless spectrum from 515 to 720 nm
  11. ↑ 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
  12. ↑ 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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