Planet 47 Uma d
| Name | 47 Uma d | |
| Discovered in | 2010 | |
| M × sin i | 1.64 ( -0.48 +0.29 ) MJ |  |
| Semi-major axis | 11.6 ( -2.9 +2.9 ) AU | |
| Orbital period | 14002.0 ( -5095.0 +5095.0 ) day | |
| Eccentricity | 0.16 ( -0.16 +0.16 ) | |
| ω | 110.0 ( -160.0 +160.0 ) deg | |
| Tperi | 1736.0 ( -5051.0 +5051.0 ) JD | |
| Radius | — | |
| Inclination | — | |
| Update | March 10, 2010 | |
| Detection method | detected by radial velocity | |
| Molecules detected | — | |
| Primary transit | — | |
| Secondary transit | — | |
| Anomaly angle | — | |
| Time Vr=0 | — | |
| Calculated temperature | — | |
| Measured temperature | — | |
| Hottest point longitute | — | |
| Surface gravity log(g/gH) | — |
Remarks
7 Mar. 2010: According to Gregory & Fischer (2010), "the three-planet model is found to be 105 times more probable than the next most probable model which is a two-planet model."Star
| Name | 47 Uma | |
| Distance | 13.97 (± 1.91) pc | |
| Spectral type | G0V | |
| Apparent magnitude V | 5.1 | |
| Mass | 1.03 (± 0.05) MSun | |
| Age | 7.4 (± 1.9) Gyr | |
| Effective temperature | 5892.0 (± 70.0) K | |
| Radius | 1.24 (± 0.04) RSun | |
| Metallicity [Fe/H] | — | |
| RA2000 | 10:59:29.0 | |
| Dec2000 | +40:25:46 | |
| Planetary system | 3 planets |
More data
- Simbad
- Most recent references (ADS)
Related publications
A Mid-Infrared Search for Substellar Companions of Nearby Planet-Host Stars
March 4, 2014
HULSEBUS A., MARENGO M., CARSON J. & STAPELFELDT K.
ApJ, 784, 41
paper arxiv
Gravitational scattering by giant planets
March 3, 2014
LAAKSO T., RANTALA J. & KAASALAINEN M.
MNRAS, submitted
arxiv
Planetary Candidates Observed by Kepler IV: Planet Sample From Q1-Q8 (22 Months)
Dec. 20, 2013
BURKE Ch., BRYSON S., MULLALLY F., ROWE J., CHRISTIANSEN J. et al.
ApJ. Suppl., 210, 19
paper arxiv
Taxonomy of the extrasolar planet
April 21, 2012
PLAVALOVA E.
Astrobiology, 12, 361
paper arxiv
A Uniformly Derived Catalogue of Exoplanets from Radial Velocities
Feb. 10, 2012
HOLLIS M., BALAN S., LEVER G. & LAHAV O.
MNRAS
arxiv
The Exoplanet Handbook
May 22, 2012
Michael Perryman
Content
Content and Chapter 5
On the Ages of Planetary Systems with Mean Motion Resonances
Oct. 17, 2011
KORISKI Sh. & ZUCKER Sh.
ApJ. Letters, 741, L23
paper arxiv
The diversity of planetary system architectures: contrasting theory with observations
Oct. 5, 2011
MIGUEL Y.? GUILERA O. & BRUNINI A.
MNRAS, 417, 314
paper
Estimation of the XUV radiation onto close planets and their evaporation
Sept. 16, 2011
SANZ-FORCADA J., MICELA G., RIBAS I., POLLOCK A., EIROA C. & 2 additional authors
Astron. & Astrophys., 532, A6
paper arxiv
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
Exozodiacal Dust Levels for Nearby Main-sequence Stars: A Survey with the Keck Interferometer Nuller
May 26, 2011
MILLAN-GABET R., SEARBYN E., MENNESSON B., TRAUB W., BARRY R. & 10 additional authors
ApJ., 734, 67
paper
Chromospheric activity of stars with planets
May 12, 2011
CANTO MARTINS B., DAS CHAGAS M., ALVES S., LEAO I., de SOUZA NETO L. & MEDEIROS J.
Astron. & Astrophys., 530, A73
paper arxiv
Density Estimation for Projected Exoplanet Quantities
May 6, 2011
BROWN R.
ApJ., 733, 68
paper
The Exoplanet Orbit Database
April 23, 2011
WRIGHT J., FAKHOURI O., MARCY G., HAN E., FENG Y., JOHNSON A., HOWARD A., VALENTI J., ANDERSON J. & PISKUNOV N.
PASP, 123, 412
paper arxiv
Quantization of Planetary Systems and its Dependency on Stellar Rotation
March 8, 2011
ZOGHBI J.-P.
Publ. Astron. Soc. Australia
arxiv
Forming Close-in Earth-like Planets Via a Collision-merger Mechanism in Late-stage Planet Formation
Dec. 22, 2010
JI J., JIN Sh. & TINNEY Ch.
ApJ. Letters, 727, L5
paper
The barycentric motion of exoplanet host stars - Tests of solar spin-orbit coupling
Dec. 14, 2010
PERRYMAN M. & SCHULZE-HARTUNG T.
Astron. & Astrophys., 525, A65
paper
The Hill stability of the possible moons of extrasolar planets
Sept. 11, 2010
DONNISON J.
MNRAS, 406, 1918
paper
A Bayesian periodogram finds evidence for three planets in 47 Ursae Majoris
March 22, 2010
GREGORY Ph. & FISCHER D.
MNRAS, 403, 731
paper