Planet Oph 11 b
| Name | Oph 11 b | |
| Discovered in | 2007 | |
| M × sin i | 21 ± 3 MJ | |
| Semi-major axis | 243 ± 55 AU |  |
| Orbital period | 730000 ± 365000 days | |
| Eccentricity | — | |
| ω | — | |
| Tperi | — | |
| Radius | — | |
| Inclination | — | |
| Update | Dec. 14, 2011 | |
| Detection method | detected by imaging | |
| Molecules detected | — |
Star
| Name | Oph 11 | |
| Distance | 145 ± 20 pc | |
| Spectral type | M9 | |
| Apparent magnitude V | — | |
| Mass | 0.162 +0.005-0.005 MSun | |
| Age | 0.011 ± 0.002 Gyr | |
| Effective temperature | 2375 ± 175 K | |
| Radius | RSun | |
| Metallicity [Fe/H] | ||
| RA2000 | 16:22:25.0 | |
| Dec2000 | -24:05:14 | |
| Planetary system | 1 planet |
More data
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- Most recent references (ADS)
Related publications
The Exoplanet Handbook
May 22, 2012
Michael Perryman
Content
Content and Chapter 5
Defining and cataloging exoplanets: The exoplanet.eu database
Aug. 1, 2011
SCHNEIDER J., DEDIEU C., LE SIDANER P., SAVALLE R. & ZOLOTUKHIN I.
Astron. & Astrophys., 532, A79
paper arxiv
Density Estimation for Projected Exoplanet Quantities
May 6, 2011
BROWN R.
ApJ., 733, 68
paper
The Wide Brown Dwarf Binary Oph 1622–2405 and Discovery of a Wide, Low-Mass Binary in Ophiuchus (Oph 1623–2402): A New Class of Young Evaporating Wide Binaries?
April 22, 2011
CLOSE L., ZUCKERMAN B., SONG I., BARMAN T., MAROIS Ch. & 8 additional authors
ApJ., 660, 1492
paper