Richard E. Young, was a planetary scientist from NASA’s Ames Research Center. After graduating from UC Berkeley, he went to NASA Ames to work on advanced planetary mission concepts, which inspired him to seek and earn a Ph.D. from UCLA, working with Prof. Gerald (Jerry) Schubert, in 1972. After a short post-doc at the National Center for Atmospheric Research (NCAR), Rich returned to Ames to work on Venus' atmosphere with Jim Pollack, and joined the Theoretical Studies Branch of the Space Science Division in 1976. During his career Rich conducted research into a broad variety of topics ranging from interior structural and thermal models of the Moon, Mercury, Mars, Uranus, and Neptune, to 3D atmospheric dynamics of free and forced planetary-scale waves and zonally averaged flows, and the radiative properties of terrestrial volcanic hazes. He was among the first to develop general circulation models for Venus to try to explain its four-day superrotation – perhaps the most challenging goal for understanding deep planetary atmospheres. He participated in three major planetary missions including Pioneer Venus, the Venus Vega mission, and the Galileo Jupiter mission for which he served as the entry probe chief scientist. Later in his career Rich managed the Planetary Systems Branch for five years. He retired in 2006, but remained active in science by educating the public about the reality and challenge of climate change on Earth. He passed away unexpectedly on January 16, 2013.
Biographical information from Young's NASA obituary.