HAT-P-30

G-type main-sequence star From Wikipedia, the free encyclopedia

HAT-P-30, also known as WASP-51, is the primary of a binary star system about 679 light-years away in the constellation Hydra. It is a G-type main-sequence star. HAT-P-30 has a similar concentration of heavy elements compared to the Sun.

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HAT-P-30
Observation data
Epoch J2000      Equinox J2000
Constellation Hydra[1]
Right ascension 08h 15m 47.9802s[2]
Declination +05° 50 12.351[2]
Apparent magnitude (V) 10.35[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type G0[4]
Astrometry
Radial velocity (Rv)45.14±0.37[2] km/s
Proper motion (μ) RA: −17.231 mas/yr[2]
Dec.: +23.875 mas/yr[2]
Parallax (π)4.8037±0.0148 mas[2]
Distance679 ± 2 ly
(208.2 ± 0.6 pc)
Details
Mass1.175±0.025[5] M
Radius1.314±0.015[5] R
Luminosity2.37±0.01[2] L
Surface gravity (log g)4.270±0.007[5] cgs
Temperature6,252±100[5] K
Metallicity [Fe/H]−0.079±0.079[5] dex
Rotational velocity (v sin i)3.6±0.4[6] km/s
Age4.1±0.6[2] Gyr
Other designations
HAT-P-30, BD+06 1909, TOI-490, TIC 455135327, WASP-51, GSC 00208-00722, 2MASS J08154797+0550121[7]
Database references
SIMBADdata
Exoplanet Archivedata
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The faint stellar companion was detected in 2013 at a projected separation of 3.842±0.007″.[8]

Planetary system

In 2011 a transiting hot Jupiter planet, HAT-P-30b, was independently detected by two teams, the HATNet Project[9] and the Wide Angle Search for Planets (WASP).[6]

The planetary orbit is strongly misaligned with the equatorial plane of the star, the misalignment angle being equal to 73.5±9.0°.[9]

Since 2022, an additional planet in the system is suspected based on transit timing variations.[5]

More information Companion (in order from star), Mass ...
The HAT-P-30 planetary system[5]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination
(°)
Radius
b 0.723±0.023 MJ 0.04114±0.00030 2.8106006(4) <0.016[10] 82.56±0.08 1.426±0.020 RJ
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References

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