HD 130322 b
HD 130322 b is an exoplanet that orbits the main sequence star HD 130322 every 10.70875 days . Due to its high mass , it is assumed that it is a gas planet .
discovery
The planet was determined using the radial velocity method by Michel Mayor , Stephan Udry , Francesco Pepe et al. discovered in 2000 .
Circulation and mass
The planet orbits its star at a distance of approx. 0.091 astronomical units and has a mass of approx. 346.5 Earth masses or 1.09 Jupiter masses.
See also
Web links
- The exoplanet in the "Encyclopedia of Extrasolar Planets"