HAT-P-25

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HAT-P-25
Observation data
Epoch J2000      Equinox J2000
Constellation Aries
Right ascension 03h 10m 47.4136016557s[1]
Declination +25° 00′ 41.677262346″[1]
Apparent magnitude (V) 13.15[1]
Characteristics
Spectral type G5V
Astrometry
Proper motion (μ) RA: 13.49 mas/yr
Dec.: -13.586 mas/yr
Parallax (π)3.3009 ± 0.0466[1] mas
Distance990 ± 10 ly
(303 ± 4 pc)
Details[2]
Mass1.012+0.051
−0.051 M☉
Radius0.919±0.034 R☉
Surface gravity (log g)4.516+0.026
−0.025 cgs
Temperature5519+78
−76 K
Metallicity0.29±0.08
Age3.2±2.3 Gyr
Other designations
Gaia DR2 3668036348641580288, TYC 320-1027-1, GSC 0320-01027, 2MASS J14123753+0403359[1]
Database references
SIMBADdata

HAT-P-25 is a G-type main-sequence star about 990 light-years away. It has a very low flare activity.[3] The star is enriched in heavy elements, having about twice amount of metals compared to solar abundance.

Planetary system[]

In 2010 a transiting hot Jupiter like planet was detected.[4] It has an equilibrium temperature of 1182±25 K.[2] The stability of orbits within circumstellar habitable zone is not significantly affected by the HAT-P-25b planet.[5]

Size comparison of HAT-P-25 b and Jupiter
The HAT-P-25 planetary system[4][2]
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b 0.569+0.023
−0.022 MJ 		0.0466±0.0005 3.65281514+0.00000076
−0.00000075 		0.023+0.022
−0.014 		87.6±0.5° 1.135±0.048 RJ

References[]

  1. ^ a b c d e HAT-P-25 -- Star
  2. ^ a b c Wang, Xian-Yu; Wang, Songhu; Hinse, Tobias C.; Li, Kai; Wang, Yong-Hao; Laughlin, Gregory; Liu, Hui-Gen; Zhang, Hui; Wu, Zhen-Yu; Zhou, Xu; Zhou, Ji-Lin; Hu, Shao-Ming; Wu, Dong-Hong; Peng, Xi-Yan; Chen, Yuan-Yuan (2018), "Transiting Exoplanet Monitoring Project (TEMP). IV. Refined System Parameters, Transit Timing Variations and Orbital Stability of the Transiting Planetary System HAT-P-25", Publications of the Astronomical Society of the Pacific, 130 (988): 064401, arXiv:1805.01580, Bibcode:2018PASP..130f4401W, doi:10.1088/1538-3873/aab93e, S2CID 118993367
  3. ^ Evgenya L. Shkolnik, "AN ULTRAVIOLET INVESTIGATION OF ACTIVITY ON EXOPLANET HOST STARS", 2013
  4. ^ a b Quinn, S. N.; Bakos, G. Á.; Hartman, J.; Torres, G.; Kovács, G.; Latham, D. W.; Noyes, R. W.; Fischer, D. A.; Johnson, J. A.; Marcy, G. W.; Howard, A. W.; Szentgyorgyi, A.; Fűrész, G.; Buchhave, L. A.; Béky, B.; Sasselov, D. D.; Stefanik, R. P.; Perumpilly, G.; Everett, M.; Lázár, J.; Papp, I.; Sári, P. (2010), "HAT-P-25b: a Hot-Jupiter Transiting a Moderately Faint G Star", The Astrophysical Journal, 745: 80, arXiv:1008.3565, doi:10.1088/0004-637X/745/1/80, S2CID 119291022
  5. ^ Nikolaos Georgakarakos, Siegfried Eggl, and Ian Dobbs-Dixon, "Giant Planets: Good Neighbors for Habitable Worlds?", 2018

Coordinates: Sky map 03h 10m 47.4136s, +25° 00′ 41.6773″


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