Planet 2MASS J0414+2811

Detailed information about planet 2MASS J0414+2811 and its parameters.

Planet

Name
2MASS J0414+2811
Planet Status
Confirmed
Discovered in
2004
Publication
Status
Published in a refereed paper
Update
2025-08-16
Mass
Mass*sin(i)
Semi-Major Axis
Orbital Period
Eccentricity
Angular distance
23.43 arcsec
ω
Tperi
Radius
Inclination
Detection Method
Imaging
Mass Meas. Method
Spectrum
Radius Meas. Method
Primary transit
Secondary transit
λ
Impact Parameter b
Time Vr=0
Velocity Semiamplitude K
Calculated temperature
Measured temperature
Hottest point longitude
Geometric albedo
Surface gravity log(g/gH)
Alternate Names
V773 Tau (ABC)b, 2MASS J04141188+2811535
Data Source Type Result Value Result Figure Notes Reference
Molecule Data Source Type Result Value Result Figure Notes Reference

Spectral type M6.25. Circumbinary substellar companion to V773 Tau multiple system.

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Star

Name
V773 Tau (ABC)
Distance
Spectral type
K3e+K3+K3+K3+M4
Apparent magnitude V
Apparent magnitude I
Apparent magnitude J
Apparent magnitude H
Apparent magnitude K
Mass
Age
Effective temperature
Radius
Metallicity [Fe/H]
Detected Disc
Magnetic Field
RA2000
04:14:12.9
Dec2000
+28:12:12.4
Alternate Names
HD 283447, HIP 19762, GHE 1, HBC 367

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).

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