This page describes exoplanet orbital and physical parameters.
Plot of equatorial spin velocity vs. mass for planets comparing Beta Pictoris b to the Solar System planets.
Sizes of Kepler Planet Candidates – based on 2,740 candidates orbiting 2,036 stars as of 4 November 2013[update] (NASA).
Plots of exoplanet density and radius. Top: Density vs. Radius. Bottom: Diffusity=1/Density vs. Radius. Units: Radius in Jupiter radii (RJup). Density in g/cm3. Diffusity in cm3/g. These plots show that there are a wide range of densities for planets between Earth and Neptune size, then the planets of 0.6 RJup size are very low-density and there are very few of them, then the gas giants have a large range of densities.
An exoplanet or extrasolar planet is a planet outside the Solar System. The first confirmed detection of an exoplanet was in 1992 around a pulsar, and the first detection around a main-sequence star w
Comparison of the size of exoplanets orbiting Kepler-37 to Mercury, Mars and Earth
Exoplanet HIP 65426b is the first discovered planet around star HIP 65426.
Coronagraphic image of AB Pictoris showing a companion (bottom left), which is either a brown dwarf or a massive planet. The data were obtained on 16 March 2003 with NACO on the VLT, using a 1.4 arcsec occulting mask on top of AB Pictoris.
The three known planets of the star HR 8799, as imaged by the Hale Telescope. The light from the central star was blanked out by a vector vortex coronagraph.