Planet Calar 3

Detailed information about planet Calar 3 and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

Calar 3

Mass

55.0 (\pm 15.0)

M_J 2 publications

Near-infrared low-resolution spectroscopy of Pleiades L-type brown dwarfs
Brown Dwarfs in the Pleiades Cluster Confirmed by the Lithium Test

Mass*sin(i)

—

Semi-Major Axis

—

Orbital Period

—

Eccentricity

—

ω

—

T_peri

—

Radius

—

Inclination

—

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

—

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

2584.0 (\pm 100.0)

K 2 publications

The seven sisters DANCe. II. Proper motions and the lithium rotation-activity connection for G and K Pleiades
Near-infrared low-resolution spectroscopy of Pleiades L-type brown dwarfs

Measured temperature

—

Hottest point longitude

—

Surface gravity log(g/g_H)

—

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

Spectral type M8.0±0.5. Age 110 Myrs. Member of Pleiades Cluster.

No link

System without star

Distance

180.8 pc

RA₂₀₀₀

03:51:25.6

Dec₂₀₀₀

+23:45:21.5

Planet Calar 3

Planet

Basic informations 20 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks Some remarks

Other web pages No page

System without star

System informations 3 parameters

Planet Calar 3

Planet

Basic informations 20 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks Some remarks

Other web pages No page

System without star

System informations 3 parameters

Related publications

The seven sisters DANCe. II. Proper motions and the lithium rotation-activity connection for G and K Pleiades

Near-infrared low-resolution spectroscopy of Pleiades L-type brown dwarfs

Brown Dwarfs in the Pleiades Cluster Confirmed by the Lithium Test

Spectroscopy of new substellar candidates in the Pleiades: toward a spectral sequence for young brown dwarfs