HAT-P-25 is a G-type main-sequence star about 985 light-years away. It has a very low flare activity.[4] The star is enriched in heavy elements, having about twice amount of metals compared to solar abundance.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Aries |
| Right ascension | 03h 13m 44.4981s[1] |
| Declination | +25° 11′ 50.689″[1] |
| Apparent magnitude (V) | 13.15[2] |
| Characteristics | |
| Spectral type | G5V |
| Astrometry | |
| Proper motion (μ) | RA: 13.490(21) mas/yr[1] Dec.: −13.684(16) mas/yr[1] |
| Parallax (π) | 3.3128 ± 0.0178 mas[1] |
| Distance | 985 ± 5 ly (302 ± 2 pc) |
| Details[3] | |
| Mass | 1.012+0.051 −0.051 M☉ |
| Radius | 0.919±0.034 R☉ |
| Surface gravity (log g) | 4.516+0.026 −0.025 cgs |
| Temperature | 5519+78 −76 K |
| Metallicity | 0.29±0.08 |
| Age | 3.2±2.3 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Planetary system
editIn 2010 a transiting hot Jupiter like planet was detected.[5] It has an equilibrium temperature of 1182±25 K.[3] The stability of orbits within circumstellar habitable zone is not significantly affected by the HAT-P-25b planet.[6]
| 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
edit- ^ 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 HAT-P-25 -- Star
- ^ 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
- ^ Evgenya L. Shkolnik, "AN ULTRAVIOLET INVESTIGATION OF ACTIVITY ON EXOPLANET HOST STARS", 2013
- ^ 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
- ^ Nikolaos Georgakarakos, Siegfried Eggl, and Ian Dobbs-Dixon, "Giant Planets: Good Neighbors for Habitable Worlds?", 2018
 | This main-sequence-star-related article is a stub. You can help Wikipedia by expanding it. |
 | This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it. |