Notes for HD 178911 B
Alias HIP 94075
by
Jean Schneider
update: 2O April 2003
The planets:
- Detection method: Radial Velocity
- Basic data:
| Name: |
HIP 94075 b |
| M.sini: |
6.292 ± 0.059 MJ |
| Semi-major axis: |
0.32 AU |
| Orbital period: |
71.487 ± 0.018 d. |
| Eccentricity: |
0.1243 ± 0.0075 |
| Omega (deg): |
175.6 ± 4.2 |
| T_peri (JD-2450000): |
306.45 ± 0.73 |
| Inclination: |
- |
- Remarks:
20 apr. 03: Planet in wide (a ~ 640 AU) binary system
(Eggenberger et al 2003)
Name HD 178911 B not in Simbad; HIP 94075 or ADS 12101
B instaed
- References:
- EGGENBERGER A., UDRY S. & MAYOR M., 2003
Planets in binaries.
in Scientific Frontiers in Research on Extrasolar Planets,
ASP Conference Series. D.Deming and S.Seager, eds.
paper
- ZUCKER S., NAEF D., LATHAM D., MAYOR M., MAZEH T., BEUZIT J.-L.,
DRUKIER G.,
PERRIER-BELLET C., QUELOZ D., SIVAN J.-P., TORRES G., & UDRY S., 2001d
A Planet Candidate in the Stellar Triple System HD 178911.
ApJ., 568, 363
paper
- Other Web pages:
The star:
- Distance: 46.73 pc
- Spectral type: G5
- Apparent magnitude: B = 8.71, V = 7.98
- Absolute luminosity: !.3 Lsun
- Coordinates (2000): RA = 19 09 03.1039 , DEC = +34 35 59.454
- Metallicity: [Fe/H]= 0.28
- Mass (M_sun): M= 0.87
- More data:
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Extra-solar Planets Catalog