Planet EGB 6 b

Detailed information about planet EGB 6 b and its parameters.

Planet

Name
EGB 6 b
Planet Status
Candidate
Discovered in
1989
Publication
Status
—
Update
2026-07-03
Mass
Mass*sin(i)
—
Semi-Major Axis
Orbital Period
—
Eccentricity
—
Angular distance
—
ω
—
Tperi
—
Radius
Inclination
—
Detection Method
Other
Mass Meas. Method
Theoretical
Radius Meas. Method
Theoretical
Primary transit
—
Secondary transit
—
λ
—
Impact Parameter b
—
Time Vr=0
—
Velocity Semiamplitude K
—
Calculated temperature
Measured temperature
—
Hottest point longitude
—
Geometric albedo
—
Surface gravity log(g/gH)
—
Alternate Names
—
Data Source Type Result Value Result Figure Notes Reference
Molecule Data Source Type Result Value Result Figure Notes Reference

Dopita & Liebert (1989) infer the presence of a photo-evaporating highly inflated (0.6 RSol = 6 RJup) gas giant planet (assumed mass 1030 g = 0.526 MJup) to explain the origin of EGB 6 planetary nebula. However neither planet ablation or exocomet evaporation are enough to account for the amount of ionized gas making up the nebula.

https://commons.wikimedia.org/wiki/File:A_Dead_Star%E2%80%99s_Shroud_(iotw2215a).tiff?page=1

Star

Name
EGB 6
Distance
751.7 pc
Spectral type
DA0.5
Apparent magnitude V
—
Apparent magnitude I
—
Apparent magnitude J
—
Apparent magnitude H
—
Apparent magnitude K
—
Mass
—
Age
—
Effective temperature
Radius
Metallicity [Fe/H]
—
Detected Disc
—
Magnetic Field
—
RA2000
09:52:59.0
Dec2000
+13:44:34.6
Alternate Names
PG 0950+139

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