Planet WISE J0413-4750

Detailed information about planet WISE J0413-4750 and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

WISE J0413-4750

Planet Status

Confirmed

Discovered in

2012

Update

2024-07-14

Mass

32.04 (\pm 14.76)

M_J 1 publication

A Search for Predicted Astrometric Microlensing Events by Nearby Brown Dwarfs

Mass*sin(i)

—

Semi-Major Axis

—

Orbital Period

—

Eccentricity

—

ω

—

T_peri

—

Radius

—

Inclination

—

Detection Method

Imaging

Mass Meas. Method

Theoretical

Radius Meas. Method

—

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

—

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

527.0 (\pm 47.0)

K 1 publication

An HST survey of 33 T8 to Y1 brown dwarfs: NIR photometry and multiplicity of the coldest isolated objects

Measured temperature

—

Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

WISE J041358.14-475039.3

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

Spectral type T9. Luberto etal. 2022 : mJ=19.71, predicted microlensing event at 2031.8453 ± 0.2811 with theta min= 63.16+/_ 29.1 mas.

No link

System without star

Distance

22.0 (\pm 3.0)

RA₂₀₀₀

04:13:58.1

Dec₂₀₀₀

-47:50:39.3

Planet WISE J0413-4750

Planet

Basic informations 28 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 WISE J0413-4750

Planet

Basic informations 28 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

An HST survey of 33 T8 to Y1 brown dwarfs: NIR photometry and multiplicity of the coldest isolated objects

A Search for Predicted Astrometric Microlensing Events by Nearby Brown Dwarfs

Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function