Planet HD 99492 d
Detailed information about planet HD 99492 d and its parameters.
Planet
- Name
- HD 99492 d
- Planet Status
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- Discovered in
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- Update
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- Mass
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MJ
- Mass*sin(i)
- Semi-Major Axis
-
AU
- Orbital Period
- Eccentricity
- ω
- Tperi
- Radius
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—
- Inclination
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—
- Detection Method
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- Mass Meas. Method
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- Radius Meas. Method
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—
- Primary transit
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—
- 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
- 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 |
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Originally reported as exoplanet candidate, Kane et al. (2016) found that associated radial velocity signal was related to stellar activity. Original designation was "HD 99492 c" but this has been transferred to the new exoplanet candidate detected by Stalport et al. (2023), hence the unconfirmed planet is here labelled as "83 Leo Bd/HD 99492 d" for its putative separation.
See also Planets in Binaries webpage.
No link
Star
- Name
- HD 99492
- Distance
- Spectral type
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- Apparent magnitude V
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- Mass
- Age
- 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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The evolved K-type primary star 83 Leo A lies about 515 AUs away (Raghavan et al. 2006).
No link
- Simbad
- Most recent references (ADS)