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WASP-37

From Wikipedia, the free encyclopedia
Star in constellation of Virgo
WASP-37
Observation data
Epoch J2000      Equinox
ConstellationVirgo
Right ascension14h 47m 46.5618s
Declination01° 03′ 53.8024″
Apparent magnitude (V)12.704
Characteristics
Evolutionary stagemain sequence star
Spectral typeG2V
U−Bcolor index0.022
B−Vcolor index0.628
V−Rcolor index0.337
J−Hcolor index0.378
J−Kcolor index0.406
Astrometry
Radial velocity (Rv)7.927±0.0042 km/s
Proper motion (μ)RA: -28.082±0.069mas/yr
Dec.: 18.018±0.062mas/yr
Parallax (π)2.5183±0.0493 mas
Distance1,300 ± 30 ly
(397 ± 8 pc)
Details[1]
Mass0.926+0.039
−0.034
 M
Radius1.071+0.019
−0.018
 R
Surface gravity (log g)4.346+0.023
−0.021
 cgs
Temperature5795+69
−64
 K
Metallicity [Fe/H]-0.098+0.05
−0.06
 dex
Rotational velocity (v sin i)2.4±1.6[2] km/s
Age10.31+4.01
−2.55
[3] Gyr
Other designations
WASP-37, DENIS J144746.5+010354, 2MASS J14474655+0103538, Gaia DR2 3652176997218325888[4]
Database references
SIMBADdata

WASP-37 is a yellowmain sequencestar in theconstellation ofVirgo.

Star characteristics

[edit]

WASP-37 has a low metallicity of just 40% of solar,[5] and is likely older than Sun.[2] WASP-37 does not have noticeable flare activity.[6]

Planetary system

[edit]

The "Hot Jupiter" class planet WASP-37b was discovered around WASP-37 in 2010.[5] The study in 2018 has found the stability of orbits in habitable zone of WASP-37 is not significantly affected by WASP-37b planet.[7]

The WASP-37 planetary system[5][7][8]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b1.79±0.17 MJ0.045±0.0023.5774807±0.0000019088.78°1.16+0.07
−0.06
 RJ

References

[edit]
  1. ^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
  2. ^abBrown, 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.
  3. ^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.
  4. ^WASP-37 -- Star
  5. ^abcSimpson, 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 1.8MJEXOPLANET 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.
  6. ^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.
  7. ^abGeorgakarakos, 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.
  8. ^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.
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