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 14002.0 ( -5095.0 +4018.0 ) JD
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
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 5892.0 (± 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

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
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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.
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paper  arxiv

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Astrobiology, 12, 361
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Density Estimation for Projected Exoplanet Quantities
2011 BROWN R.
ApJ., 733, 68
paper

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ApJ., 734, 67
paper

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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.
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2011 MIGUEL Y.? GUILERA O. & BRUNINI A.
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paper

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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
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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