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.

WASP-88
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
Distance1,830 ± 20 ly
(560 ± 6 pc)
Position (relative to WASP-88)
ComponentWASP-88B
Epoch of observation2017
Angular distance3.350±0.015
Position angle355.5±0.5°
Projected separation1877±8 AU
Details
WASP-88
Mass1.450±0.050 M
Radius2.08+0.12
0.06
 R
Surface gravity (log g)4.24±0.06 cgs
Temperature6450±61 K
Metallicity [Fe/H]0.03±0.04 dex
Rotational velocity (v sin i)8.4±0.8 km/s
Age3.0±1.3 Gyr
WASP-88B
Mass0.11+0.03
0.02
 M
Temperature2844+155
209
 K
Other designations
Gaia DR2 6482103014085857024, 2MASS J20380268-4827434
Database references
SIMBADdata

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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