Planet Kepler-132 Ab
Detailed information about planet Kepler-132 Ab and its parameters.
Planet
- Name
- Kepler-132 Ab
- Planet Status
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- Discovered in
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- Update
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- Mass
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- Mass*sin(i)
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- Semi-Major Axis
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0.0643 AU 2 publications number of publications
- Orbital Period
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- Eccentricity
- ω
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- Tperi
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- Radius
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- Inclination
- 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
- Time Vr=0
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- Velocity Semiamplitude K
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- Calculated temperature
- 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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12 Feb 2024:
The parent star is a binary separated by 0.9'' with a position angle 97° (Howell et al. 2011 AJ 142) . One does not know around which stellar component the planet is orbiting (Lissauer et al. 2014 ApJ 784)
31 Jul. 2024: See also Planets in Binaries webpage.
No link
Star
- Name
- Kepler-132 A
- 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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12 Feb 2024:
The parent star is a binary separated by 0.9'' with a position angle 97° (Howell et al. 2011 AJ 142).
31 Jul. 2024: Furlan et al. (2017) provide a separation of 0.876 arcseconds for the companion star. Estimated luminosity is compatible with a G dwarf.
2 Ago. 2024: Michel & Mugrauer (2024) confirm a Solar-type G dwarf companion 330 AUs away.
No link
- Simbad
- Most recent references (ADS)