Planet IRAS 16253-2429

Detailed information about planet IRAS 16253-2429 and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

IRAS 16253-2429

Planet Status

Confirmed

Discovered in

2004

Publication Status

—

Update

2024-08-09

Mass

32.0

M_J 1 publication

IRAS 16253-2429: the first proto-brown dwarf binary candidate identified through the dynamics of jets

Mass*sin(i)

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Semi-Major Axis

—

Orbital Period

—

Eccentricity

—

Angular distance

—

ω

—

T_peri

—

Radius

—

Inclination

—

Detection Method

Imaging, Other, Kinematic

Mass Meas. Method

—

Radius Meas. Method

—

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

—

Time V_r=0

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Velocity Semiamplitude K

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Calculated temperature

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Measured temperature

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Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

IRAS 16253

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference
H2
H2	Modeling	Detected				2016 - HSIEH T.-H.

Part of ρ Oph star forming region, IRAS 16253-2429 is a class 0 source with internal luminosity of ∼0.08-0.09 L_Sol classified as proto-brown dwarf binary with a gas and dust envelope of 18 to 32 M_Jup. Individual masses are likely about 32 M_Jup and estimated separation likely equal or less than 0.50 arcseconds (<62 AUs at 125 pc).

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