Planet 47 Uma d
| Name | 47 Uma d | ||
| Planet Status | Confirmed | ||
| Discovered in | 2010 | ||
| Mass | 1.64 ( -0.48 +0.29 ) MJ | ||
| Mass*sin(i) | 1.64 ( -0.48 +0.29 ) MJ | ||
| Semi-Major Axis | 11.6 ( -2.9 +2.1 ) AU |  |
|
| Orbital Period | 14002 ( -5095 +4018 ) day | |
|
| Eccentricity | 0.16 ( -0.16 +0.09 ) | ||
| ω | 110 ( -160 +132 ) deg | |
|
| Tperi | 2.45174e+06 ( -5051 +6783 ) JD | |
|
| Radius | — | ||
| Inclination | — | ||
| Update | 2014-08-27 | ||
| Detection Method | Radial Velocity | ||
| Mass Detection Method | — | ||
| Radius Detection Method | — | ||
| Molecules | — | ||
| Primary transit | — | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
47 Uma| 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 (± 70) K | |
|
| Radius | 1.24 (± 0.04) RSun | |
|
| Metallicity [Fe/H] | 0.0 | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 10:59:29.0 | ||
| Dec2000 | +40:25:46 | ||
| Alternate Names | |||
| Planetary system | 3 planets |
Observability Predictor 
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."Related publications
Impact of Gas Giant Instabilities on Habitable Planets
2018
SEPPEUR S.
MNRAS, submitted
arxiv
Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars
2015
SPINA L., MELENDEZ J. & RAMIREZ I.
Astron. & Astrophys., submitted
arxiv ADS
Planetary Candidates Observed by Kepler IV: Planet Sample From Q1-Q8 (22 Months)
2014
BURKE Ch., BRYSON S., MULLALLY F., ROWE J., CHRISTIANSEN J. et al.
ApJ. Suppl., 210, 19
paper arxiv
Gravitational scattering by giant planets
2014
LAAKSO T., RANTALA J. & KAASALAINEN M.
MNRAS, submitted
arxiv
A Mid-Infrared Search for Substellar Companions of Nearby Planet-Host Stars
2014
HULSEBUS A., MARENGO M., CARSON J. & STAPELFELDT K.
ApJ, 784, 41
paper arxiv
A Uniformly Derived Catalogue of Exoplanets from Radial Velocities
2012
HOLLIS M., BALAN S., LEVER G. & LAHAV O.
MNRAS, 423, Issue 3, 2800-2814
paper arxiv
Taxonomy of the extrasolar planet
2012
PLAVALOVA E.
Astrobiology, 12, 361
paper arxiv
Density Estimation for Projected Exoplanet Quantities
2011
BROWN R.
ApJ., 733, 68
paper
Exozodiacal Dust Levels for Nearby Main-sequence Stars: A Survey with the Keck Interferometer Nuller
2011
MILLAN-GABET R., SEARBYN E., MENNESSON B., TRAUB W., BARRY R. & 10 additional authors
ApJ., 734, 67
paper
Defining and cataloging exoplanets: The exoplanet.eu database
2011
SCHNEIDER J., DEDIEU C., LE SIDANER P., SAVALLE R. & ZOLOTUKHIN I.
Astron. & Astrophys., 532, A79
paper arxiv
The barycentric motion of exoplanet host stars - Tests of solar spin-orbit coupling
2011
PERRYMAN M. & SCHULZE-HARTUNG T.
Astron. & Astrophys., 525, A65
paper
The diversity of planetary system architectures: contrasting theory with observations
2011
MIGUEL Y.? GUILERA O. & BRUNINI A.
MNRAS, 417, 314
paper
On the Ages of Planetary Systems with Mean Motion Resonances
2011
KORISKI Sh. & ZUCKER Sh.
ApJ. Letters, 741, L23
paper arxiv
The Exoplanet Handbook
2011
Michael Perryman
Content
Content and Chapter 5
Chromospheric activity of stars with planets
2011
CANTO MARTINS B., DAS CHAGAS M., ALVES S., LEAO I., de SOUZA NETO L. & MEDEIROS J.
Astron. & Astrophys., 530, A73
paper arxiv
Quantization of Planetary Systems and its Dependency on Stellar Rotation
2011
ZOGHBI J.-P.
Publ. Astron. Soc. Australia, 28, 177
paper arxiv ADS
The Exoplanet Orbit Database
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
Forming Close-in Earth-like Planets Via a Collision-merger Mechanism in Late-stage Planet Formation
2011
JI J., JIN Sh. & TINNEY Ch.
ApJ. Letters, 727, L5
paper
Estimation of the XUV radiation onto close planets and their evaporation
2011
SANZ-FORCADA J., MICELA G., RIBAS I., POLLOCK A., EIROA C. & 2 additional authors
Astron. & Astrophys., 532, A6
paper arxiv ADS
A Bayesian periodogram finds evidence for three planets in 47 Ursae Majoris
2010
GREGORY Ph. & FISCHER D.
MNRAS, 403, 731
paper
arxiv
The Hill stability of the possible moons of extrasolar planets
2010
DONNISON J.
MNRAS, 406, 1918
paper
Solar-type stars with planetary companions: 51 Pegasi and 47 Ursae Majoris
1997
FUHRMANN K., PFEIFFER M. & BERNKOPF J.
Astron. & Astrophys., 326, 1081
paper
