Planet EGB 6 b
Detailed information about planet EGB 6 b and its parameters.
Planet
- Name
- EGB 6 b
- Mass
- Mass*sin(i)
-
—
- Semi-Major Axis
- Orbital Period
-
—
- Eccentricity
-
—
- ω
-
—
- Tperi
-
—
- Radius
- Inclination
-
—
- Primary transit
-
—
- Secondary transit
-
—
- λ
-
—
- Impact Parameter b
-
—
- Time Vr=0
-
—
- Velocity Semiamplitude K
-
—
- Calculated temperature
- Measured temperature
-
—
- Hottest point longitude
-
—
- Surface gravity log(g/gH)
-
—
| 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
No remarks
No link
- Simbad
- Most recent references (ADS)