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] although a red dwarf companion with a temperature 4000+100
−350 K is suspected on wide orbit.[5]
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.[6]
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.[7] 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.[8] 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.[9]
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)
- Hartman, J. D.; Bakos, G. Á.; Kipping, D. M.; Torres, G.; Kovács, G.; Noyes, R. W.; Latham, D. W.; Howard, A. W.; Fischer, D. A.; Johnson, J. A.; Marcy, G. W.; Isaacson, H.; Quinn, S. N.; Buchhave, L. A.; Béky, B.; Sasselov, D. D.; Stefanik, R. P.; Esquerdo, G. A.; Everett, M.; Perumpilly, G.; Lázár, J.; Papp, I.; Sári, P. (2010), "HAT-P-26b: A LOW-DENSITY NEPTUNE-MASS PLANET TRANSITING A K STAR", The Astrophysical Journal, 728 (2): 138, arXiv:1010.1008, doi:10.1088/0004-637X/728/2/138, S2CID 119228956
- Wöllert, Maria; Brandner, Wolfgang; Bergfors, Carolina; Henning, Thomas (2015), "A Lucky Imaging search for stellar companions to transiting planet host stars", Astronomy & Astrophysics, 575: A23, arXiv:1507.01938, doi:10.1051/0004-6361/201424091, S2CID 119250579
- Piskorz, Danielle; Knutson, Heather A.; Ngo, Henry; Muirhead, Philip S.; Batygin, Konstantin; Crepp, Justin R.; Hinkley, Sasha; Morton, Timothy D. (2015), "Friends of Hot Jupiters. III. An Infrared Spectroscopic Search for Low-Mass Stellar Companions", The Astrophysical Journal, 814 (2): 148, arXiv:1510.08062, doi:10.1088/0004-637X/814/2/148, S2CID 11525988
- Mohamad Ali-Dib, Gunjan Lakhlani, "Possible formation pathways for the low-density Neptune-mass planet HAT-P-26b"
- Stevenson, Kevin B.; Bean, Jacob L.; Seifahrt, Andreas; Gilbert, Gregory J.; Line, Michael R.; Désert, Jean-Michel; Fortney, Jonathan J. (2015), "A SEARCH FOR WATER IN THE ATMOSPHERE OF HAT-P-26b USING LDSS-3C", The Astrophysical Journal, 817 (2): 141, arXiv:1511.08226, doi:10.3847/0004-637X/817/2/141, S2CID 118394486
- MacDonald, Ryan J.; Madhusudhan, Nikku (2019), "The Metal-Rich Atmosphere of the Neptune HAT-P-26b", Monthly Notices of the Royal Astronomical Society, 486: 1292–1315, arXiv:1903.09151, doi:10.1093/mnras/stz789, S2CID 85459516
- von Essen, C.; Wedemeyer, S.; Sosa, M. S.; Hjorth, M.; Parkash, V.; Freudenthal, J.; Mallonn, M.; Miculán, R. G.; Zibecchi, L.; Cellone, S.; Torres, A. F. (2019), "Indications for transit timing variations in the exo-Neptune HAT-P-26b", Astronomy & Astrophysics, 628: A116, arXiv:1904.06360, doi:10.1051/0004-6361/201731966, S2CID 118674293
- Planet HAT-P-26 b on exoplanet.eu