WASP-10b

WASP-10b is an extrasolar planet discovered in 2008 by SuperWASP using the transit method. It takes about 3 days to orbit around WASP-10. Follow-up radial velocity observations showed that it is three times more massive than Jupiter, while the transit observations showed that its radius is only 8% larger than Jupiter's, giving the planet a density more similar to the Moon than a normal gas giant.[1][2] It is currently the only confirmed planet around WASP-10, as WASP-10c is still unconfirmed.[3]

See also

  • SuperWASP

References

  1. ^ Johnson; Winn, Joshua N.; Cabrera, Nicole E.; Carter, Joshua A. (2009). "A SMALLER RADIUS FOR THE TRANSITING EXOPLANET WASP-10b". The Astrophysical Journal Letters. 692 (2): L100–L104. arXiv:0812.0029. Bibcode:2009ApJ...692L.100J. doi:10.1088/0004-637X/692/2/L100. S2CID 14858840.
  2. ^ Christian; Gibson, N. P.; Simpson, E. K.; Street, R. A.; Skillen, I.; Pollacco, D.; Collier Cameron, A.; Joshi, Y. C.; et al. (December 29, 2008). "WASP-10b: a 3MJ, gas-giant planet transiting a late-type K star". Monthly Notices of the Royal Astronomical Society. 392 (4): 1585–1590. arXiv:0806.1482. Bibcode:2009MNRAS.392.1585C. doi:10.1111/j.1365-2966.2008.14164.x. S2CID 862722.
  3. ^ "Extrasolar Planets Encyclopaedia - WASP-10". Extrasolar Planets Encyclopaedia. Archived from the original on 2011-01-03.

External links

Media related to WASP-10b at Wikimedia Commons