HD 80606 b is a transiting hot Jupiter orbiting
a G-type star (0.9 solar masses) in a 111-day orbit.
It was discovered by the radial velocity method in 2001
and a transit was identified in 2011.
Its orbit has a high eccentricity, 0.93226,
varying from 0.03 to 0.88 AU.
Due to the two types of observation
and its high eccentricity, it is of interest for
further study, e.g., determining characteristics of its atmosphere
using its light curve.
Characteristics: