HAT-P-26
HAT-P-26 is a K-type main-sequence star about 302 light-years away. Survey in 2015 did not find any stellar companions on orbit around it.[4]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Virgo |
Right ascension | 14h 12m 37.5330s[1] |
Declination | +04° 03′ 36.1177″[1] |
Apparent magnitude (V) | 11.76[1] |
Characteristics | |
Spectral type | K1V |
Astrometry | |
Parallax (π) | 10.7960 ± 0.0561[1] mas |
Distance | 302 ± 2 ly (92.6 ± 0.5 pc) |
Details[2] | |
Mass | 0.81 M☉ |
Radius | 0.78 R☉ |
Temperature | 5079±88 K |
Metallicity | -0.04±0.08[3] |
Rotational velocity (v sin i) | 1.8 km/s |
Other designations | |
Database references | |
SIMBAD | data |
Planetary system
In 2010 a transiting hot Neptune like planet was detected.[3] The transiting planet HAT-P-26b was detected by the HATNet Project using telescopes located in Hawaii and Arizona. The planet is likely formed by pebble accretion mechanism.[5]
The transmission spectrum of the HAT-P-26b was taken in the 2015, with best fit favouring either cloudless atmosphere or atmosphere with low-lying cloud deck.[6] The atmospheric composition of the planet was measured in 2019, and the water vapor volume fraction of 1.5+2.1
−0.9% was detected. The HAT-P-26 is carbon depleted, C/O ratio been constrained to less than 0.33. Also, atmosphere contains light metal hydrides.[7]. The measured planetary temperature is equal to 563+58
−54 K.
In 2019, the transit timing variation analysis of HAT-P-26b, has indicated a presence of the second planet in the system on the wide, 1141-days orbit.[8]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | >0.0585±0.00717 MJ | 0.0479±0.0006 | 4.234516±0.000015 | 0.124±0.060 | 88.6±0.9° | 0.5647±0.0517 RJ |
c (unconfirmed) | — | — | 1141 | — | — | — |
References
- HAT-P-26 -- High proper-motion Star
- D. Ehrenreich and J.-M. Désert, "Mass-loss rates for transiting exoplanets", A&A 529, A136 (2011)
- HAT-P-26b: A LOW-DENSITY NEPTUNE-MASS PLANET TRANSITING A K STAR, 2010, arXiv:1010.1008
- A Lucky Imaging search for stellar companions to transiting planet host stars, 2015, arXiv:1507.01938
- Mohamad Ali-Dib, Gunjan Lakhlani, "Possible formation pathways for the low-density Neptune-mass planet HAT-P-26b"
- A SEARCH FOR WATER IN THE ATMOSPHERE OF HAT-P-26b USING LDSS-3C, 2015, arXiv:1511.08226
- The Metal-Rich Atmosphere of the Neptune HAT-P-26b, 2019, arXiv:1903.09151
- Indications for transit timing variations in the exo-Neptune HAT-P-26b, 2019, arXiv:1904.06360
- Planet HAT-P-26 b on exoplanet.eu