HAT-P-30

HAT-P-30
Observation data
Epoch J2000      Equinox ICRS
Constellation Hydra
Right ascension 08h 15m 47.9802s
Declination +05° 50′ 12.351″
Apparent magnitude (V) 10.35
Characteristics
Evolutionary stage main sequence
Spectral type G0
Astrometry
Radial velocity (Rv)45.14±0.37 km/s
Proper motion (μ) RA: −17.231 mas/yr
Dec.: +23.875 mas/yr
Parallax (π)4.8037±0.0148 mas
Distance679 ± 2 ly
(208.2 ± 0.6 pc)
Details
Mass1.175±0.025 M☉
Radius1.314±0.015 R☉
Luminosity2.37±0.01 L☉
Surface gravity (log g)4.270±0.007 cgs
Temperature6,252±100 K
Metallicity [Fe/H]−0.079±0.079 dex
Rotational velocity (v sin i)3.6±0.4 km/s
Age4.1±0.6 Gyr
Other designations
HAT-P-30, BD+06 1909, TOI-490, TIC 455135327, WASP-51, GSC 00208-00722, 2MASS J08154797+0550121
Database references
SIMBADdata
Exoplanet Archivedata

HAT-P-30, also known as WASP-51, is the primary of a binary star system about 679 light-years away in the constellation Hydra. It is a G-type main-sequence star. HAT-P-30 has a similar concentration of heavy elements compared to the Sun.

The faint stellar companion was detected in 2013 at a projected separation of 3.842±0.007″.

Planetary system

In 2011 a transiting hot Jupiter planet, HAT-P-30b, was independently detected by two teams, the HATNet Project and the Wide Angle Search for Planets (WASP).

The planetary orbit is strongly misaligned with the equatorial plane of the star, the misalignment angle being equal to 73.5±9.0°.

Since 2022, an additional planet in the system is suspected based on transit timing variations.

The HAT-P-30 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination
(°)
Radius
b 0.723±0.023 MJ 0.04114±0.00030 2.8106006(4) <0.016 82.56±0.08 1.426±0.020 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 7 8 9 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. ↑ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000), "The Tycho-2 catalogue of the 2.5 million brightest stars", Astronomy and Astrophysics, 355: L27–L30, Bibcode:2000A&A...355L..27H, ISSN 0004-6361
  4. ↑ Ginski, C.; Mugrauer, M.; Seeliger, M.; Löhne, T. (November 2013), "The multiplicity status of three exoplanet host stars", Astronomy & Astrophysics, 559: 6, Bibcode:2013A&A...559A..71G, doi:10.1051/0004-6361/201322274
  5. 1 2 3 4 5 6 7 Bai, Lu; Gu, Shenghong; Wang, Xiaobin; Sun, Leilei; Kwok, Chi-Tai; Hui, Ho-Keung (2022), "WASP-35 and HAT-P-30/WASP-51: Reanalysis using TESS and Ground-based Transit Photometry", The Astronomical Journal, 163 (5): 208, arXiv:2203.02866, Bibcode:2022AJ....163..208B, doi:10.3847/1538-3881/ac5b6a, S2CID 247292453
  6. 1 2 Enoch, B.; Anderson, D. R.; Barros, S. C. C.; Brown, D. J. A.; Cameron, A. Collier; Faedi, F.; Gillon, M.; Hébrard, G.; Lister, T. A.; Queloz, D.; Santerne, A.; Smalley, B.; Street, R. A.; Triaud, A. H. M. J.; West, R. G.; Bouchy, F.; Bento, J.; Butters, O.; Fossati, L.; Haswell, C. A.; Hellier, C.; Holmes, S.; Jehen, E.; Lendl, M.; Maxted, P. F. L.; McCormac, J.; Miller, G. R. M.; Moulds, V.; Moutou, C.; et al. (2011), "WASP-35b, WASP-48b, and HAT-P-30b/WASP-51b: Two New Planets and an Independent Discovery of a Hat Planet", The Astronomical Journal, 142 (3): 86, arXiv:1104.2827, Bibcode:2011AJ....142...86E, doi:10.1088/0004-6256/142/3/86, S2CID 63996398
  7. ↑ "BD+06 1909", SIMBAD, Centre de données astronomiques de Strasbourg
  8. ↑ Wöllert, Maria; Brandner, Wolfgang (2015), "A Lucky Imaging search for stellar sources near 74 transit hosts", Astronomy & Astrophysics, 579: A129, arXiv:1506.05456, Bibcode:2015A&A...579A.129W, doi:10.1051/0004-6361/201526525, S2CID 118903879
  9. 1 2 Johnson, John Asher; Winn, J. N.; Bakos, G. Á.; Hartman, J. D.; Morton, T. D.; Torres, G.; Kovács, Géza; Latham, D. W.; Noyes, R. W.; Sato, B.; Esquerdo, G. A.; Fischer, D. A.; Marcy, G. W.; Howard, A. W.; Buchhave, L. A.; Fűrész, G.; Quinn, S. N.; Béky, B.; Sasselov, D. D.; Stefanik, R. P.; Lázár, J.; Papp, I.; Sári, P. (2011), "HAT-P-30b: A transiting hot Jupiter on a highly oblique orbit", The Astrophysical Journal, 735 (1): 24, arXiv:1103.3825, Bibcode:2011ApJ...735...24J, doi:10.1088/0004-637X/735/1/24, S2CID 53689766
  10. ↑ 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.