Planet 2MASS J0414+2811
Detailed information about planet 2MASS J0414+2811 and its parameters.
Planet
- Name
- 2MASS J0414+2811
- 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
- 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 M6.25. Circumbinary substellar companion to V773 Tau multiple system.
No link
Star
- Name
- V773 Tau (ABC)
- Distance
- 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
- Effective temperature
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- 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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Highly complex multiple system. Primary component is V773 Tau A (spT K3Ve, mA = 1.54 MSol) with a nearly equal but lower-mass companion at 0.336 AUs (mAb = 1.32 MSol, P = 51.1003 d, e = 0.271). A third star, V773 Tau B (mB = 1.2 MSol) lies 15.2 AUs away tracing a mildly eccentric orbit (e = 0.1), itself close binary with a nearly equal component (P = 63 d, e > 0.3) and likely surrounded by a circumbinary disk. A fifth star lies in outer, more eccentric orbit (V773 Tau C, spT M0.5, P = 560 y, e = 0.38) and finally an outer brown dwarf traces an orbit that encompasses all of the stellar components 2,800 AUs away (Harris et al. 2012, Kenworthy et al. 2022).
No link
- Simbad
- Most recent references (ADS)