Planet HD 62509 b
| Name | HD 62509 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2006 | ||
| Mass | 2.9 ( -0.1 +0.1 ) MJ | ||
| Mass*sin(i) | 2.9 ( -0.1 +0.1 ) MJ | ||
| Semi-Major Axis | 1.69 (± 0.03) AU |  |
|
| Orbital Period | 589.64 (± 0.81) day | |
|
| Eccentricity | 0.02 (± 0.03) | ||
| ω | 354.58 (± 95.65) deg | |
|
| Tperi | 2447739.02 (± 4.5) JD | |
|
| Radius | — | ||
| Inclination | — | ||
| Update | 2015-08-21 | ||
| Detection Method | Radial Velocity | ||
| Mass Detection Method | — | ||
| Radius Detection Method | — | ||
| Primary transit | — | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 46.0 (± 1.6) m/s | ||
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
HD 62509| Name | HD 62509 | ||
| Distance | 10.34 (± 1.0) pc | |
|
| Spectral type | K0IIIb | ||
| Apparent magnitude V | 1.15 | ||
| Mass | 1.47 (± 0.45) MSun | |
|
| Age | — | ||
| Effective temperature | 4666.0 (± 95.0) K | |
|
| Radius | 9.3 RSun | |
|
| Metallicity [Fe/H] | 0.19 | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 07:45:18.0 | ||
| Dec2000 | +28:01:34 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Observability Predictor 
Remarks
The planet was first suspected by Hatzes & Cochran (1993)
05 Feb 2014: Aurière et al. (2013) suggest that that the apparent RV variation could be due to a stable weak dipolar magnetic field of the star.
Related publications
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2018
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Astron. & Astrophys., submitted
arxiv
Asteroseismic masses of retired planet-hosting A-stars using SONG
2017
STELLO D., HUBER D., GRUNDAHL F., LLOYD J., IRELAND M. et al.
MNRAS, 472, 4110
paper arxiv
Feasibility of spectro-polarimetric characterization of exoplanetary atmospheres with direct observing instruments
2017
TAKAHASHI J., MATSUO T. & ITOH Y.
Astron. & Astrophys., 599, A56
paper
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2015
TRIFONOV T., REFFERT S., ZECHMEISTER M., REINERS A. & QUIRRENBACH A.
Astron. & Astrophys., 582, A54
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2015
WITTENMYER R., GAO D., HU Sh., VILLAVER E., ENDL M. & WRIGHT D.
PASP, in press
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Pollux: a stable weak dipolar magnetic field but no planet ?
2014
AURIERE M., KONSTANTINOVA-ANTOVA R., ESPAGNET O., PETIT P., ROUDIER Th. et al.
in "Magnetic fields throughout stellar evolution" IAU Symposium 302
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2012
HOLLIS M., BALAN S., LEVER G. & LAHAV O.
MNRAS, 423, Issue 3, 2800-2814
paper arxiv
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2012
CARLBERG J., CUNHA K., SMITH V. & MAJEWSKI S.
ApJ, 757, 109
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2012
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Astron. & Astrophys.
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Taxonomy of the extrasolar planet
2012
PLAVALOVA E.
Astrobiology, 12, 361
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2011
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ApJ., 737, 66
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The Exoplanet Orbit Database
2011
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2011
QUIRRENBACH A., REFFERT S. & BERGMANN C.
arxiv
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2011
ZOGHBI J.-P.
Publ. Astron. Soc. Australia, 28, 177
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2011
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2011
BROWN R.
ApJ., 733, 68
paper
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2011
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Astron. & Astrophys., 532, A79
paper arxiv
The Exoplanet Handbook
2011
Michael Perryman
Content
Content and Chapter 5
The Hill stability of the possible moons of extrasolar planets
2010
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MNRAS, 406, 1918
paper
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2010
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paper
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Astron. & Astrophys., 522, A13
preprint
Coronal properties of planet-bearing stars
2010
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2009
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paper
Terrestrial planet formation in low eccentricity warm-Jupiter systems
2009
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Extrasolar planets around intermediate mass stars
2008
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Physica Scripta, T130, 014004
paper
Abundance Stratification of Exoplanet Host Stars
2008
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Astron. & Astrophys.
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2008
KASHYAP V., DRAKE J. & SAAR S.
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2008
WALKER G.
New Astronomy
preprint
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2007
MARCHI S.
ApJ., 666, 475
arxiv
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2007
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paper
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2007
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paper
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2007
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2006
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2006
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2006
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Long-period radial velocity variations in three K giants
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HATZES A. & COCHRAN W.
ApJ., 413, 339
abstract
