Planet HD 62509 b
| Name | HD 62509 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2006 | ||
| Mass | 2.9 (± 0.1) MJ | ||
| Mass*sin(i) | 2.9 (± 0.1) MJ |  |
|
| Semi-Major Axis | 1.69 (± 0.03) AU | |
|
| Orbital Period | 589.64 (± 0.81) JD | |
|
| 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 | — | ||
| Molecules | |||
| 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.
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2014
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in "Magnetic fields throughout stellar evolution" IAU Symposium 302
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2012
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Michael Perryman
Content
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2010
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2010
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abstract
