Planet V* V2384 Ori a

Detailed information about planet V* V2384 Ori a and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

V* V2384 Ori a

Planet Status

Confirmed

Discovered in

2006

Publication Status

Published in a refereed paper

Update

2019-03-19

Mass

56.7 (\pm 4.8)

M_J 1 publication

Discovery of two young brown dwarfs in an eclipsing binary system

Mass*sin(i)

—

Semi-Major Axis

0.0398 (\pm 0.001)

AU 1 publication

Discovery of two young brown dwarfs in an eclipsing binary system

Orbital Period

—

Eccentricity

0.3225 (\pm 0.006)

1 publication

Discovery of two young brown dwarfs in an eclipsing binary system

Angular distance

—

ω

215.4 (\pm 1.1)

deg 1 publication

Discovery of two young brown dwarfs in an eclipsing binary system

T_peri

—

Radius

6.52 (\pm 0.33)

R_J 1 publication

Discovery of two young brown dwarfs in an eclipsing binary system

Inclination

88.8 (\pm 0.1)

deg 1 publication

Discovery of two young brown dwarfs in an eclipsing binary system

Detection Method

Radial Velocity

Mass Meas. Method

Radial Velocity

Radius Meas. Method

Primary Transit

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

—

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

—

Measured temperature

—

Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

2MASS J05352184-0546085 a

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

Stassun et al. 2006 : V* V2384 Ori is an eclipsing binary of 2 brown dwarfs. The parameters of the system are fitted from radial velocity and light-curve data. They are given in the individual pages of the two components. Note that V* V2384 Ori b, the less massive of the pair is the hotter.

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