Astronomy:HAT-P-25
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Observation data Equinox J2000.0]] (ICRS) | |
---|---|
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 |
Distance | 990 ± 10 ly (303 ± 4 pc) |
Details[2] | |
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 |
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]
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
- ↑ 1.0 1.1 1.2 1.3 1.4 HAT-P-25 -- Star
- ↑ 2.0 2.1 2.2 Wang, Xian-Yu; Wang, Songhu; Hinse, Tobias C.; Li, Kai; Wang, Yong-Hao; Laughlin, Gregory; Liu, Hui-Gen; Zhang, Hui et al. (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, doi:10.1088/1538-3873/aab93e, Bibcode: 2018PASP..130f4401W
- ↑ Evgenya L. Shkolnik, "AN ULTRAVIOLET INVESTIGATION OF ACTIVITY ON EXOPLANET HOST STARS", 2013
- ↑ 4.0 4.1 Quinn, S. N.; Bakos, G. Á.; Hartman, J.; Torres, G.; Kovács, G.; Latham, D. W.; Noyes, R. W.; Fischer, D. A. et al. (2010), "HAT-P-25b: a Hot-Jupiter Transiting a Moderately Faint G Star", The Astrophysical Journal 745: 80, doi:10.1088/0004-637X/745/1/80
- ↑ Nikolaos Georgakarakos, Siegfried Eggl, and Ian Dobbs-Dixon, "Giant Planets: Good Neighbors for Habitable Worlds?", 2018
Coordinates: 03h 10m 47.4136s, +25° 00′ 41.6773″
Original source: https://en.wikipedia.org/wiki/HAT-P-25.
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