Planet zet Her Ab
Detailed information about planet zet Her Ab and its parameters.
Planet
- Name
- zet Her Ab
- Planet Status
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- Discovered in
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                    Publication
 Status
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                    Published in a refereed paper
- Update
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- Mass
- Mass*sin(i)
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- Semi-Major Axis
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- Orbital Period
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- Eccentricity
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- Angular distance
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- ω
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- Tperi
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- Radius
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- Inclination
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- Detection Method
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- Mass Meas. Method
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- Radius Meas. Method
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- Primary transit
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- Secondary transit
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- λ
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- Impact Parameter b
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- Time Vr=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
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- Geometric albedo
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- Surface gravity log(g/gH)
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- Alternate Names
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| Data Source | Type | Result Value | Result Figure | Notes | Reference | 
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| Molecule | Data Source | Type | Result Value | Result Figure | Notes | Reference | 
|---|
The presence of a third body in Zeta Herculis binary system is suspected since early XX Century and increasingly investigated in late 80s-early 90s (e.g. Baize 1976, McCarthy 1983, Lebreton et al. 1993). Morel et al. (2001) infer a mass less than 50 MJup, compatible either with a brown dwarf or a giant planet. Orbital period is assumed to be equal or less than 12 years.
No link
Star
- Name
- zet Her A
- Distance
- Spectral type
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- Apparent magnitude V
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- Apparent magnitude I
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- Apparent magnitude J
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- Apparent magnitude H
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- Apparent magnitude K
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- Mass
- Age
- Effective temperature
- Radius
- Metallicity [Fe/H]
- Detected Disc
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- Magnetic Field
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- RA2000
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- Dec2000
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- Alternate Names
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Zeta Herculis forms a binary system with a late G to early K dwarf companion star 15 AUs away in eccentric orbit (P = 34.45 ± 0.005 yr, e = 0.462 ± 0.002, i = 131°).
No link
- Simbad
- Most recent references (ADS)