![]() Size comparison of WASP-14b with Jupiter. | |
Discovery | |
---|---|
Discovered by | Cameron et al. ( SuperWASP) |
Discovery site | SAAO |
Discovery date | April 1, 2008 |
Transit | |
Orbital characteristics | |
0.037+0.001 −0.002 AU | |
Eccentricity | 0.095+0.004 −0.007 |
2.243756+5E-6 −1E-6 d | |
Inclination | 84.79+0.52 −0.67 |
254.9+0.92 −1.72 | |
Star | WASP-14 |
Physical characteristics | |
Mean radius | 1.259+0.08 −0.058 RJ |
Mass | 7.725+0.43 −0.67 MJ |
Mean
density | 5,133 kg/m3 (8,652 lb/cu yd) |
126.2
m/s2 (414
ft/s2) 12.87 g | |
Temperature | 2800 |
WASP-14b is an extrasolar planet discovered in 2008 by SuperWASP using the transit method. Follow-up radial velocity measurements showed that the mass of WASP-14b is almost eight times larger than that of Jupiter. The radius found by the transit observations show that it has a radius 25% larger than Jupiter. This makes WASP-14b one of the densest exoplanets known. [1] Its radius best fits the model of Jonathan Fortney. [2]
First calculation of WASP-14b's Rossiter–McLaughlin effect and so spin-orbit angle was −14 ± 17 degrees. [3] It is too eccentric for its age and so is possibly pulled into its orbit by another planet. [1] The study in 2012 has updated spin-orbit angle to 33.1±7.4°. [4]
Media related to
WASP-14b at Wikimedia Commons
![]() Size comparison of WASP-14b with Jupiter. | |
Discovery | |
---|---|
Discovered by | Cameron et al. ( SuperWASP) |
Discovery site | SAAO |
Discovery date | April 1, 2008 |
Transit | |
Orbital characteristics | |
0.037+0.001 −0.002 AU | |
Eccentricity | 0.095+0.004 −0.007 |
2.243756+5E-6 −1E-6 d | |
Inclination | 84.79+0.52 −0.67 |
254.9+0.92 −1.72 | |
Star | WASP-14 |
Physical characteristics | |
Mean radius | 1.259+0.08 −0.058 RJ |
Mass | 7.725+0.43 −0.67 MJ |
Mean
density | 5,133 kg/m3 (8,652 lb/cu yd) |
126.2
m/s2 (414
ft/s2) 12.87 g | |
Temperature | 2800 |
WASP-14b is an extrasolar planet discovered in 2008 by SuperWASP using the transit method. Follow-up radial velocity measurements showed that the mass of WASP-14b is almost eight times larger than that of Jupiter. The radius found by the transit observations show that it has a radius 25% larger than Jupiter. This makes WASP-14b one of the densest exoplanets known. [1] Its radius best fits the model of Jonathan Fortney. [2]
First calculation of WASP-14b's Rossiter–McLaughlin effect and so spin-orbit angle was −14 ± 17 degrees. [3] It is too eccentric for its age and so is possibly pulled into its orbit by another planet. [1] The study in 2012 has updated spin-orbit angle to 33.1±7.4°. [4]
Media related to
WASP-14b at Wikimedia Commons