Planet KPNO-Tau 2
Detailed information about planet KPNO-Tau 2 and its parameters.
Planet
- Name
- KPNO-Tau 2
- Planet Status
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- Discovered in
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Publication
Status -
Published in a refereed paper
- Update
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- Mass
- Mass*sin(i)
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—
- Semi-Major Axis
- Orbital Period
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—
- Eccentricity
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—
- Angular distance
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arcsec
- ω
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—
- Tperi
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—
- Radius
- 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
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—
- Calculated temperature
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2927.0 K
- 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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Spectral type M7.5e. L = 0.01 LSol. Member of Taurus-Auriga star-forming region. Age 1-2 Myr.
Joncour et al. (2017) deem KPNO-Tau 2 and KPNO-Tau 12 to be gravitationally bound to protostar IRAS 04158+2805 being located 22,288 and 80,679 AUs away respectively. Likely physical association to close binary LkCa 7 (1470 arcseconds away, ~191,000 AUs at 130 pc) could increase system complexity.
No link
Star
- Name
- IRAS 04158+2805
- Distance
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130.0 pc
- Spectral type
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- Apparent magnitude V
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—
- Apparent magnitude I
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- Apparent magnitude J
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—
- Apparent magnitude H
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- Apparent magnitude K
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—
- Mass
- Age
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—
- Effective temperature
- Radius
- Metallicity [Fe/H]
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- 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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Likely tertiary companion of young binary LkCa 7 1470 arcseconds away (~191,000 AUs at 130 pc). LkCa 7 is a pair of M-type protostars (m1 = 0.64 MSol and m2 = 0.33 MSol) separated by 148 AUs (Kraus et al. 2011).
No link
- Simbad
- Most recent references (ADS)