Planet GG Tau Ad

Detailed information about planet GG Tau Ad and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

GG Tau Ad

Planet Status

Candidate

Discovered in

2020

Publication Status

Published in a refereed paper

Update

2024-07-09

Mass

0.053

M_J 1 publication

Planet-induced spirals in the circumbinary disk of GG Tauri A

Mass*sin(i)

—

Semi-Major Axis

450.0 AU 1 publication

Planet-induced spirals in the circumbinary disk of GG Tauri A

Orbital Period

—

Eccentricity

—

Angular distance

—

ω

—

T_peri

—

Radius

—

Inclination

—

Detection Method

Imaging, Kinematic

Mass Meas. Method

Theoretical

Radius Meas. Method

—

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

—

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

—

Measured temperature

—

Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

—

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

No remarks

No link

Star

Name

GG Tau A

Distance

150.0 pc 1 publication

The Coevality of Young Binary Systems

Spectral type

K7Ve

Apparent magnitude V

13.4

Apparent magnitude I

—

Apparent magnitude J

—

Apparent magnitude H

—

Apparent magnitude K

—

Mass

0.73 M_Sun 1 publication

The Coevality of Young Binary Systems

Age

0.0015 Gyr 1 publication

A test of pre-main-sequence evolutionary models across the stellar/substellar boundary based on spectra of the young quadruple GG Tauri

Effective temperature

4060.0 K 1 publication

The Coevality of Young Binary Systems

Radius

1.63 R_Sun

Metallicity [Fe/H]

-0.07 1 publication

Stellar Properties for a Comprehensive Collection of Star-forming Regions in the SDSS APOGEE-2 Survey

Detected Disc

Imaging

Magnetic Field

—

RA₂₀₀₀

04:32:30.4

Dec₂₀₀₀

+17:31:40.5

Alternate Names

GG Tauri is a quintuple system whose primary component (GG Tau A or Aa, spT K7V or M0.5Ve) is itself binary made of a late type K star and an early M dwarf (GG Tau Ab, spT M0.5V) about 35 AUs away tracing an eccentric orbit (e = 0.28, i = 143°). Companion star GG Tau Ab too is binary with a second M dwarf (GG Tau Ab1, spT M3V) about 4.5 AUs away. The secondary component GG Tau B (spT M5.5V) lies about 1500AUs away from GG Tau A and hosts a substellar companion (GG Tau Bb, spT M7.5V) about 14 AUs away or less.

No link