Planet 1RXS 1609 b
| Name | 1RXS 1609 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2008 | ||
| Mass | 14.0 ( -3.0 +2.0 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 330.0 (± 0.0) AU | |
|
| Orbital Period | — | ||
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | 1.7 RJ | |
|
| Inclination | — | ||
| Update | 2018-11-15 | ||
| Detection Method | Imaging | ||
| Mass Detection Method | — | ||
| Radius Detection Method | — | ||
| Primary transit | — | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | — | ||
| Measured temperature | 1800.0 K | |
|
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | 4.0 | |
|
| Alternate Names | 1RXS J160929.1-210524 b, 1RXS J1609b, 1RXS J1609-2105b, RXJ 1609 |
Star
1RXS 1609| Name | 1RXS 1609 | ||
| Distance | 145.0 (± 20.0) pc | |
|
| Spectral type | K7V | ||
| Apparent magnitude V | — | ||
| Mass | 0.73 (± 0.05) MSun | |
|
| Age | 0.011 (± 0.002) Gyr | |
|
| Effective temperature | 4060.0 ( -200.0 +200.0 ) K | |
|
| Radius | 1.35 RSun | |
|
| Metallicity [Fe/H] | — | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 16:09:30.0 | ||
| Dec2000 | -21:04:58 | ||
| Alternate Names | 1RXS J160929, 1RXS J1609, 1RXS1609 | ||
| Planetary system | 1 planet |
Atmospheric parameters
Temperatures
| Data Source | Type | Result Value | Result Figure | Notes | Reference |
Molecules
| Molecule | Data Source | Type | Result Value | Result Figure | Notes | Reference |
| CO | Measurements | Detected | 2008 - LAFRENIERE D. | |||
| H2O | Measurements | Detected | 2008 - LAFRENIERE D. | |||
| K | Measurements | Detected | 2010 - LAFRENIERE D. | |||
Observability Predictor 
Remarks
Pecaut et al. (2012) have revised the age of Upper Scorpius to 11 Myr from the 5 Myr previously estimated. As a consequence, the estimation of the planet mass has increased to 14 Mjup from the previous estimates of 8 Mjup, putting this planet in the brown dwarf range.(Lafrenière et al. 2010): companions more massive than 1 Mjup, 2 Mjup and 4 Mjup are ruled out for separations ≳ 440 AU, 100 AU and 50 AU respectively.
(Lafrenière et al. 2008): spectral type L4+1-2
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Content
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