Exoplanetary Scratchpad

[SysBP Img]

Gamma Leporis is also known as Gl 216, HR 1983, and HD 38393. It is a double or triple star system, including a yellow white main sequence star A, a distant orange dwarf companion B at 864 AU. A distant star may or may not be gravitationally bound. This is sometimes called star C, or LTT 2368, or VB 1 (Van Biesbroeck 1). The star system may be 2.7 Billion Years old and is a member of the Sirius group. A has 1.2 times the Sun's mass and 1.3 its diameter. B has 63% of its mass, but about the same diameter. It is a BY Draconis variable star known as AK Leporis. The star is one of the top 100 target stars for the Terrestrial Planet finder mission.

Gamma Leporis System Web PagesEdit

Gamma Leporis System In the NewsEdit

Sample (Year)Edit

See AlsoEdit

Ad blocker interference detected!

Wikia is a free-to-use site that makes money from advertising. We have a modified experience for viewers using ad blockers

Wikia is not accessible if you’ve made further modifications. Remove the custom ad blocker rule(s) and the page will load as expected.