Star in constellation of Virgo
WASP-37 is a G-type main-sequence star about 1,240 light-years away in the constellation of Virgo .
Star characteristics
WASP-37 has a low metallicity of just 40% of solar,[ 4] and is likely older than the Sun.[ 7] WASP-37 does not have noticeable flare activity.[ 9]
Planetary system
The hot Jupiter class planet WASP-37b was discovered around WASP-37 in 2010.[ 4] A study in 2018 found that the stability of orbits in the habitable zone of WASP-37 is not significantly affected by WASP-37b.[ 10]
References
^ 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 .
^ a b c d 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 .
^ a b "WASP-37" . SIMBAD . Centre de données astronomiques de Strasbourg .
^ a b c d Simpson, E. K.; Faedi, F.; Barros, S. C. C.; Brown, D. J. A.; Cameron, A. Collier; Hebb, L.; Pollacco, D.; Smalley, B.; Todd, I.; Butters, O. W.; Hébrard, G.; McCormac, J.; Miller, G. R. M.; Santerne, A.; Street, R. A.; Skillen, I.; Triaud, A. H. M. J.; Anderson, D. R.; Bento, J.; Boisse, I.; Bouchy, F.; Enoch, B.; Haswell, C. A.; Hellier, C.; Holmes, S.; Horne, K.; Keenan, F. P.; Lister, T. A.; Maxted, P. F. L.; et al. (2011). "WASP-37b: A 1.8 M J Exoplanet Transiting a Metal-poor Star". The Astronomical Journal . 141 (1): 8. arXiv :1008.3096 . Bibcode :2011AJ....141....8S . doi :10.1088/0004-6256/141/1/8 . S2CID 20036137 .
^ Brown, A. G. A. ; et al. (Gaia collaboration ) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ Wang, Xian-Yu; Wang, Yong-Hao; Wang, Songhu; Wu, Zhen-Yu; Rice, Malena; Zhou, Xu; Hinse, Tobias C.; Liu, Hui-Gen; Ma, Bo; Peng, Xiyan; Zhang, Hui; Yu, Cong; Zhou, Ji-Lin; Laughlin, Gregory (2021), "Transiting Exoplanet Monitoring Project (TEMP). VI. The Homogeneous Refinement of System Parameters for 39 Transiting Hot Jupiters with 127 New Light Curves", The Astrophysical Journal Supplement Series , 255 (1): 15, arXiv :2105.14851 , Bibcode :2021ApJS..255...15W , doi :10.3847/1538-4365/ac0835 , S2CID 235253975
^ a b Brown, D. J. A. (2014). "Discrepancies between isochrone fitting and gyrochronology for exoplanet host stars?" . Monthly Notices of the Royal Astronomical Society . 442 (2): 1844– 1862. arXiv :1406.4402 . Bibcode :2014MNRAS.442.1844B . doi :10.1093/mnras/stu950 . S2CID 56052792 .
^ Maxted, P. F. L.; Koen, C.; Smalley, B. (2011). "UBV(RI)C photometry of transiting planet hosting stars" . Monthly Notices of the Royal Astronomical Society . 418 (2): 1039– 1042. arXiv :1108.0349 . Bibcode :2011MNRAS.418.1039M . doi :10.1111/j.1365-2966.2011.19554.x . S2CID 117056033 .
^ Shkolnik, Evgenya L. (2013). "An Ultraviolet Investigation of Activity on Exoplanet Host Stars". The Astrophysical Journal . 766 (1): 9. arXiv :1301.6192 . Bibcode :2013ApJ...766....9S . doi :10.1088/0004-637X/766/1/9 . S2CID 118415788 .
^ Georgakarakos, Nikolaos; Eggl, Siegfried; Dobbs-Dixon, Ian (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 . S2CID 119522834 .
^ 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 .
^ Mallonn, M.; von Essen, C.; Herrero, E.; Alexoudi, X.; Granzer, T.; Sosa, M.; Strassmeier, K. G.; Bakos, G.; Bayliss, D.; Brahm, R.; Bretton, M.; Campos, F.; Carone, L.; Colón, K. D.; Dale, H. A.; Dragomir, D.; Espinoza, N.; Evans, P.; Garcia, F.; Gu, S.-H.; Guerra, P.; Jongen, Y.; Jordán, A.; Kang, W.; Keles, E.; Kim, T.; Lendl, M.; Molina, D.; Salisbury, M.; et al. (2019). "Ephemeris refinement of 21 hot Jupiter exoplanets with high timing uncertainties". Astronomy & Astrophysics . 622 : A81. arXiv :1812.05882 . Bibcode :2019A&A...622A..81M . doi :10.1051/0004-6361/201834194 . S2CID 92990448 .