Planet WASP-80 b

Detailed information about planet WASP-80 b and its parameters.

Planet

Name
WASP-80 b
Planet Status
Confirmed
Discovered in
2013
Publication
Status
—
Update
2026-06-09
Mass
Mass*sin(i)
—
Semi-Major Axis
Orbital Period
Eccentricity
Angular distance
—
ω
—
Tperi
—
Radius
Inclination
Detection Method
Primary Transit
Mass Meas. Method
—
Radius Meas. Method
—
Primary transit
2456125.41751 ( +5.2e-05 -6.7e-05 ) JD
Secondary transit
—
λ
—
Impact Parameter b
—
Time Vr=0
—
Velocity Semiamplitude K
—
Calculated temperature
—
Measured temperature
—
Hottest point longitude
—
Geometric albedo
—
Surface gravity log(g/gH)
—
Alternate Names
TOI-5801.01
Data Source Type Result Value Result Figure Notes Reference
Molecule Data Source Type Result Value Result Figure Notes Reference
CCH
Measurements Detected 2022 - CARLEO I.
CH4
Measurements Detected 2023 - BELL T.
Measurements Detected 2022 - CARLEO I.
Measurements Detected 2017 - SEDAGHATI E.
CO
Measurements Detected 2017 - SEDAGHATI E.
Measurements Detected 2022 - CARLEO I.
CO2
Measurements Detected 2022 - CARLEO I.
H
Measurements Detected 2017 - SEDAGHATI E.
Modeling Detected 2023 - FOSSATI L.
H2O
Measurements Detected 2022 - CARLEO I.
Measurements Detected 2017 - SEDAGHATI E.
HCN
Measurements Detected 2022 - CARLEO I.
He
Measurements Detected 2017 - SEDAGHATI E.
Measurements Detected 2023 - FOSSATI L.
Measurements Detected 2021 - FOSSATI L.
Measurements Detected 2021 - FOSSATI L.
K
Measurements Detected 2017 - SEDAGHATI E.
Na
Measurements Detected 2017 - SEDAGHATI E.
NH3
Measurements Detected 2022 - CARLEO I.

No remarks

No link

Star

Name
WASP-80
Distance
Spectral type
K7V
Apparent magnitude V
11.881
Apparent magnitude I
—
Apparent magnitude J
—
Apparent magnitude H
—
Apparent magnitude K
—
Mass
Age
—
Effective temperature
Radius
Metallicity [Fe/H]
Detected Disc
—
Magnetic Field
—
RA2000
20:12:40.0
Dec2000
-02:08:44.2
Alternate Names
2MASS J20124017-0208391

Bohn et al. (2020) detect a candidate faint source 2.132 arcseconds away (106 AUs at 49.8 pc), either a very low-mass star or an L to early T-type brown dwarf whose physical association has to be confirmed.

No link