Planet 47 Uma d
| Name | 47 Uma d | ||
| Planet Status | Confirmed | ||
| Discovered in | 2010 | ||
| Mass | — | ||
| Mass*sin(i) | 1.64 ( -0.48 +0.29 ) MJ |  |
|
| Semi-Major Axis | 11.6 ( -2.9 +2.1 ) AU | |
|
| Orbital Period | 14002.0 ( -5095.0 +4018.0 ) day | |
|
| Eccentricity | 0.16 ( -0.16 +0.09 ) | |
|
| ω | 110.0 ( -160.0 +132.0 ) deg | |
|
| Tperi | 2451736.0 ( -5051.0 +6783.0 ) JD | |
|
| Radius | — | ||
| Inclination | — | ||
| Update | 2014-08-27 | ||
| Detection Method | Radial Velocity | ||
| Mass Detection Method | — | ||
| Radius Detection Method | — | ||
| 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 | 5892.0 (± 70.0) 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
On the Dynamics of Comets in Extrasolar Planetary Systems
2019
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arxiv
Impact of Gas Giant Instabilities on Habitable Planets
2018
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MNRAS, submitted
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Exocomets in the 47 UMa System: Theoretical Simulations including Water Transport
2018
CUNTZ M., LOIBNEGGER B. & DVORAK R.
Astron. J., 156, 290
paper 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
Taxonomy of the extrasolar planet
2012
PLAVALOVA E.
Astrobiology, 12, 361
paper arxiv
A Uniformly Derived Catalogue of Exoplanets from Radial Velocities
2012
HOLLIS M., BALAN S., LEVER G. & LAHAV O.
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paper arxiv
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
Density Estimation for Projected Exoplanet Quantities
2011
BROWN R.
ApJ., 733, 68
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
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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
The Exoplanet Handbook
2011
Michael Perryman
Content
Content and Chapter 5
The barycentric motion of exoplanet host stars - Tests of solar spin-orbit coupling
2011
PERRYMAN M. & SCHULZE-HARTUNG T.
Astron. & Astrophys., 525, A65
paper
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
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
Quantization of Planetary Systems and its Dependency on Stellar Rotation
2011
ZOGHBI J.-P.
Publ. Astron. Soc. Australia, 28, 177
paper arxiv ADS
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
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
The Hill stability of the possible moons of extrasolar planets
2010
DONNISON J.
MNRAS, 406, 1918
paper
A Bayesian periodogram finds evidence for three planets in 47 Ursae Majoris
2010
GREGORY Ph. & FISCHER D.
MNRAS, 403, 731
paper
arxiv
Models of the in situ formation of detected extrasolar giant planets
2000
BODENHEIMER P., HUBICKYI O. & LISSAUER J.
Icarus, 143, 2
paper
arxiv
Solar-type stars with planetary companions: 51 Pegasi and 47 Ursae Majoris
1997
FUHRMANN K., PFEIFFER M. & BERNKOPF J.
Astron. & Astrophys., 326, 1081
paper
