WASP-94

Binary star system From Wikipedia, the free encyclopedia

WASP-94 is a binary star system located about 690 light-years (210 parsecs) away in the constellation Microscopium. It consists of two F-type stars separated by 15, corresponding to a projected separation of 2700 au. Both stars are known to host exoplanets.[3]

Quick facts Apparent magnitude (V), Characteristics ...
WASP-94
Observation data
Epoch J2000      Equinox J2000
Constellation Microscopium[1]
A
Right ascension 20h 55m 07.94435s[2]
Declination −34° 08 08.0075[2]
Apparent magnitude (V) 10.1[3]
B
Right ascension 20h 55m 09.15767s[4]
Declination −34° 08 07.9138[4]
Apparent magnitude (V) 10.5[3]
Characteristics
A
Evolutionary stage main sequence[2]
Spectral type F8[3]
B
Evolutionary stage subgiant[4]
Spectral type F9[3]
Astrometry
A
Radial velocity (Rv)−8.36±0.19[2] km/s
Proper motion (μ) RA: +26.500 mas/yr[2]
Dec.: −44.971 mas/yr[2]
Parallax (π)4.7498±0.0242 mas[2]
Distance687 ± 3 ly
(211 ± 1 pc)
B
Radial velocity (Rv)−8.30±0.20[4] km/s
Proper motion (μ) RA: +26.191 mas/yr[4]
Dec.: −44.702 mas/yr[4]
Parallax (π)4.7208±0.0165 mas[4]
Distance691 ± 2 ly
(211.8 ± 0.7 pc)
Details
A
Mass1.45±0.09[3] M
Radius1.62+0.05
−0.04
[3] R
Luminosity3.2[5] L
Surface gravity (log g)4.21±0.011[6] cgs
Temperature6194±5[6] K
Metallicity [Fe/H]+0.320±0.004[6] dex
Rotation19.5 d[3]
Rotational velocity (v sin i)4.2±0.5[3] km/s
Age2.3–2.8[6] Gyr
B
Mass1.24±0.09[3] M
Radius1.35±0.12[3] R
Luminosity2.2[7] L
Surface gravity (log g)4.30±0.015[6] cgs
Temperature6112±6[6] K
Metallicity [Fe/H]+0.305±0.005[6] dex
Rotation>45.5 d[3]
Rotational velocity (v sin i)<1.5[3] km/s
Age2.3–2.8[6] Gyr
Other designations
CD−34 14724, WASP-94, HJ 5234
A: TOI-107, TIC 92352620, TYC 7466-1400-1, 2MASS J20550794-3408079[8]
B: TIC 92352621, 2MASS J20550915-3408078[9]
Database references
SIMBADA
B
Exoplanet Archivedata
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The binary system was first observed by John Herschel in 1834 and catalogued as HJ 5234. The designation WASP-94 comes from the Wide Angle Search for Planets, and has been used since the system was found to host planets in 2014.[3] While the two stars have similar spectral types, they differ in elemental abundance  WASP-94A has fewer volatile elements and more refractory elements than WASP-94B.[6]

Planetary system

The two stars host a single known planet each. Both are hot Jupiters, gas giant planets completing orbits around their stars in just a few days.[3]

Diagram of the WASP-94 system

WASP-94Ab transits its host star, and it has also been detected by the radial velocity method.[3] As a result, both its size and mass are known, which show that it is a low-density planet with a highly inflated radius. It has an equilibrium temperature of 1508±75 K.[10] Its orbit is retrograde and misaligned with the rotation of its host star.[11] The atmosphere of WASP-94Ab appears to be relatively free of clouds, with sodium,[10] water vapor and carbon dioxide being detected.[12]

WASP-94Bb is a non-transiting planet that has been detected only by radial velocity, so it has no measured radius and true mass. Its minimum mass is 62% the mass of Jupiter.[3]

More information Companion (in order from star), Mass ...
The WASP-94 A planetary system[3]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.452+0.035
−0.032
 MJ
0.055±0.001 3.9501907+0.0000044
−0.0000030
<0.064[13] 88.7±0.7° 1.72+0.06
−0.05
 RJ
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More information Companion (in order from star), Mass ...
The WASP-94 B planetary system[3]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥0.618+0.028
−0.029
 MJ
0.0335+0.0006
−0.0005
2.00839±0.00024 0
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See also

Other systems with multiple planet-hosting stars:

References

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