Planet LOri 167

Detailed information about planet LOri 167 and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

LOri 167

Planet Status

Confirmed

Discovered in

2005

Update

2024-06-17

Mass

17.0 (\begin{matrix} + 3.0 \\ - 2.0 \end{matrix})

M_J 1 publication

The young, wide and very low mass visual binary Lambda Orionis 167

Mass*sin(i)

—

Semi-Major Axis

—

Orbital Period

—

Eccentricity

—

ω

—

T_peri

—

Radius

1.84 (\pm 0.39)

R_J 1 publication

Variability in the Lambda Orionis cluster substellar domain

Inclination

—

Detection Method

Imaging

Mass Meas. Method

Spectrum

Radius Meas. Method

—

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

—

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

2125.0 K 1 publication

The young, wide and very low mass visual binary Lambda Orionis 167

Measured temperature

—

Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

LOri-CFHT 167, LOri-SOC 16

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

Franciosini & Sacco (2011): Spectral type M9-L2. Age 5 Myrs.

https://simbad.u-strasbg.fr/simbad/sim-id?Ident=LOri-CFHT+167

System without star

Distance

400.0 pc

RA₂₀₀₀

05:35:14.1

Dec₂₀₀₀

+09:54:07.9

Planet LOri 167

Planet

Basic informations 28 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks Some remarks

Other web pages Some pages

System without star

System informations 3 parameters

Planet LOri 167

Planet

Basic informations 28 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks Some remarks

Other web pages Some pages

System without star

System informations 3 parameters

Related publications

XMM-Newton observations of the young open cluster around λ Orionis

A deep look into the core of young clusters. II. λ Orionis

Spitzer: Accretion in Low-Mass Stars and Brown Dwarfs in the λ Orionis Cluster

The young, wide and very low mass visual binary Lambda Orionis 167

Variability in the Lambda Orionis cluster substellar domain