Planet WASP-80 b
Detailed information about planet WASP-80 b and its parameters.
Planet
- Name
- WASP-80 b
- Planet Status
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- Discovered in
-
- Update
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- Mass
- Mass*sin(i)
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—
- Semi-Major Axis
- Orbital Period
- Eccentricity
- ω
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—
- Tperi
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—
- Radius
- Inclination
- Detection Method
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- Mass Meas. Method
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—
- Radius Meas. Method
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—
- Primary transit
-
JD
- Secondary transit
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—
- λ
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—
- Impact Parameter b
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—
- Time Vr=0
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—
- Velocity Semiamplitude K
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—
- Calculated temperature
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—
- Measured temperature
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—
- Hottest point longitude
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—
- Geometric albedo
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—
- Surface gravity log(g/gH)
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—
- Alternate Names
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—
Data Source | Type | Result Value | Result Figure | Notes | Reference |
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Molecule | Data Source | Type | Result Value | Result Figure | Notes | Reference |
---|---|---|---|---|---|---|
C2H2 | ||||||
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
-
- Apparent magnitude V
-
- Mass
- Age
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—
- Effective temperature
- Radius
- Metallicity [Fe/H]
- Detected Disc
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—
- Magnetic Field
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—
- RA2000
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- Dec2000
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- Alternate Names
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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
- Simbad
- Most recent references (ADS)