WASP-26
Appearance
Observation data Epoch J2000 Equinox | |
---|---|
Constellation | Cetus |
Right ascension | 00h 18m 24.7008s[1] |
Declination | −15° 16′ 02.2775″[1] |
Apparent magnitude (V) | 11.30[2] |
Characteristics | |
Evolutionary stage | main sequence star |
Spectral type | G0V |
B−V color index | 0.32 |
J−H color index | 0.246 |
J−K color index | 0.411 |
Details Gyr | |
Other designations | |
WASP-26, TYC 5839-876-1, DENIS J001824.6-151601, 2MASS J00182469-1516022, Gaia DR2 2416782701664155008[7] | |
Database references | |
SIMBAD | data |
WASP-26 is a yellow
Cetus
.
Star characteristics
WASP-26 is an old star close to leaving the main sequence and is part of a wide binary. The binary's projected separation is 3800 astronomical units, its companion star being a red dwarf with an effective temperature of 4600K and a visual magnitude of 13.6.[3] WASP-26 produces a large amount of ultraviolet light due to frequent flares, with an average ultraviolet flux close to the F7 class main-sequence star WASP-1.[8]
Planetary system
The "
Rossiter-McLaughlin effect failed to determine the inclination of the planetary orbit to the equatorial plane of the parent star due to high stellar noise,[5] but an initial constraint of -34+36
−26° was published in 2012.[10]
−26° was published in 2012.[10]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 1.02±0.03 MJ | 0.0400±0.0003 | 2.75660±0.00001 | 0 | 82.5±0.5° | 1.216±0.047 RJ |
References
- ^ .
- Bibcode:2000A&A...355L..27H.
- ^ S2CID 55114421.
- ^ A. Bonfanti, S. Ortolani, and V. Nascimbeni, "Age consistency between exoplanet hosts and field stars", 2016
- ^ S2CID 31204371.
- ^ S2CID 53641330.
- ^ "WASP-26". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2022-02-19.
- ^ Evgenya L. Shkolnik, "AN ULTRAVIOLET INVESTIGATION OF ACTIVITY ON EXOPLANET HOST STARS", 2013
- S2CID 55842630.
- S2CID 17174530