Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Virgo |
Right ascension | 13h 41m 49.0302s [1] |
Declination | −00° 07′ 41.0337″ [1] |
Apparent magnitude (V) | 10.41 |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | F8 [2] |
Astrometry | |
Radial velocity (Rv) | -2.82 [1] km/s |
Proper motion (μ) |
RA: -24.685
[1]
mas/
yr Dec.: -4.687 [1] mas/ yr |
Parallax (π) | 3.9522 ± 0.0692 mas [1] |
Distance | 830 ± 10
ly (253 ± 4 pc) |
Orbit [3] | |
Primary | WASP-54A |
Companion | WASP-54B |
Semi-major axis (a) | 5.728±0.006" (1450 AU) |
Details [4] | |
WASP-54A | |
Mass | 1.213±0.032 M☉ |
Radius | 1.828+0.091 −0.081 R☉ |
Surface gravity (log g) | 4.00±0.02 [5] cgs |
Temperature | 6100±100 K |
Metallicity [Fe/H] | -0.27±0.08 dex |
Rotational velocity (v sin i) | 4.0±0.8 km/s |
Age | 6.9+1.0 −1.9 Gyr |
WASP-54B | |
Mass | 0.19±0.01 [3] M☉ |
Temperature | 3216+26 −25 [3] K |
Other designations | |
Database references | |
SIMBAD | data |
WASP-54, also known as BD+00 3088, is a
binary star system about 825 light-years away. The primary, WASP-54A, is a
F-type main-sequence star, accompanied by the
red dwarf WASP-54B on a wide orbit. WASP-54 is depleted in heavy elements, having 55% of the solar abundance of iron.
[4] The age of WASP-54 is slightly older than the Sun's at 6.9+1.0
−1.9 billion years.
[4]
A multiplicity survey in 2017 did detect a red dwarf stellar companion WASP-54B 5.7″ away from WASP-54A. [6] The companion was proven to be co-moving in 2020. [3]
In 2012 a transiting hot Jupiter planet b was detected on a tight, mildly eccentric [4] orbit around WASP-54A. [7]
Planetary equilibrium temperature is 1742+49
−69
K.
[7]
Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 0.606±0.018 MJ | 0.04988+0.00043 −0.00045 |
3.6936411±0.0000059 | <0.06 | 84.97±0.61 ° | 1.653+0.090 −0.083 RJ |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Virgo |
Right ascension | 13h 41m 49.0302s [1] |
Declination | −00° 07′ 41.0337″ [1] |
Apparent magnitude (V) | 10.41 |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | F8 [2] |
Astrometry | |
Radial velocity (Rv) | -2.82 [1] km/s |
Proper motion (μ) |
RA: -24.685
[1]
mas/
yr Dec.: -4.687 [1] mas/ yr |
Parallax (π) | 3.9522 ± 0.0692 mas [1] |
Distance | 830 ± 10
ly (253 ± 4 pc) |
Orbit [3] | |
Primary | WASP-54A |
Companion | WASP-54B |
Semi-major axis (a) | 5.728±0.006" (1450 AU) |
Details [4] | |
WASP-54A | |
Mass | 1.213±0.032 M☉ |
Radius | 1.828+0.091 −0.081 R☉ |
Surface gravity (log g) | 4.00±0.02 [5] cgs |
Temperature | 6100±100 K |
Metallicity [Fe/H] | -0.27±0.08 dex |
Rotational velocity (v sin i) | 4.0±0.8 km/s |
Age | 6.9+1.0 −1.9 Gyr |
WASP-54B | |
Mass | 0.19±0.01 [3] M☉ |
Temperature | 3216+26 −25 [3] K |
Other designations | |
Database references | |
SIMBAD | data |
WASP-54, also known as BD+00 3088, is a
binary star system about 825 light-years away. The primary, WASP-54A, is a
F-type main-sequence star, accompanied by the
red dwarf WASP-54B on a wide orbit. WASP-54 is depleted in heavy elements, having 55% of the solar abundance of iron.
[4] The age of WASP-54 is slightly older than the Sun's at 6.9+1.0
−1.9 billion years.
[4]
A multiplicity survey in 2017 did detect a red dwarf stellar companion WASP-54B 5.7″ away from WASP-54A. [6] The companion was proven to be co-moving in 2020. [3]
In 2012 a transiting hot Jupiter planet b was detected on a tight, mildly eccentric [4] orbit around WASP-54A. [7]
Planetary equilibrium temperature is 1742+49
−69
K.
[7]
Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 0.606±0.018 MJ | 0.04988+0.00043 −0.00045 |
3.6936411±0.0000059 | <0.06 | 84.97±0.61 ° | 1.653+0.090 −0.083 RJ |