Planet WISE J1738+2732

Detailed information about planet WISE J1738+2732 and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

WISE J1738+2732

Planet Status

Confirmed

Discovered in

2011

Update

2024-07-14

Mass

16.0 (\pm 5.0)

M_J 1 publication

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

Mass*sin(i)

—

Semi-Major Axis

—

Orbital Period

—

Eccentricity

—

ω

—

T_peri

—

Radius

0.92

R_J

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

400.0 (\pm 20.0)

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 J173835.53+273259.0

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

Spectral type Y0. Age 8.2 ± 0.4 Gyrs.

No link

System without star

Distance

9.0 pc

RA₂₀₀₀

17:38:35.5

Dec₂₀₀₀

+27:32:59.1

Planet WISE J1738+2732

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 J1738+2732

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

WISE Y Dwarfs As Probes of the Brown Dwarf-Exoplanet Connection

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

The First Hundred Brown Dwarfs Discovered by the Wide-field Infrared Survey Explorer (WISE)