WASP-88
WASP-88 is a F-type main-sequence star. Its surface temperature is 6450±61 K. WASP-88 is similar to the Sun in its concentration of heavy elements, with a metallicity Fe/H index of 0.03±0.04, and is younger at an age of 3.0±1.3 billion years.
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Indus |
Right ascension | 20h 38m 02.6870s |
Declination | −48° 27′ 43.4255″ |
Apparent magnitude (V) | 11.39 |
Characteristics | |
Evolutionary stage | main-sequence star or subgiant star |
Spectral type | F6 |
Astrometry | |
Radial velocity (Rv) | −5.1±0.6 km/s |
Proper motion (μ) | RA: 5.890 mas/yr Dec.: −4.892 mas/yr |
Parallax (π) | 1.7844 ± 0.0185 mas |
Distance | 1,830 ± 20 ly (560 ± 6 pc) |
Position (relative to WASP-88) | |
Component | WASP-88B |
Epoch of observation | 2017 |
Angular distance | 3.350±0.015″ |
Position angle | 355.5±0.5° |
Projected separation | 1877±8 AU |
Details | |
WASP-88 | |
Mass | 1.450±0.050 M☉ |
Radius | 2.08+0.12 −0.06 R☉ |
Surface gravity (log g) | 4.24±0.06 cgs |
Temperature | 6450±61 K |
Metallicity [Fe/H] | 0.03±0.04 dex |
Rotational velocity (v sin i) | 8.4±0.8 km/s |
Age | 3.0±1.3 Gyr |
WASP-88B | |
Mass | 0.11+0.03 −0.02 M☉ |
Temperature | 2844+155 −209 K |
Other designations | |
Database references | |
SIMBAD | data |
A multiplicity survey did detect a candidate red dwarf companion to WASP-88 in 2020, with a 1.65% probability of it being an unrelated background star.
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