|
Links
news
people
research
reprints
courses
|
Dr. Fegley and Dr. Lodders apply
chemistry to key problems in astronomy, cosmochemistry, and planetary
science. Experimental studies and theoretical models are used to
study a wide range of problems related to the chemistry taking place in
these environments:
-
atmospheres and circumstellar envelopes around cool stars
-
brown dwarfs (so-called failed stars)
-
extrasolar gas giant planets
-
Jupiter's satellite Io
-
meteorite parent bodies
-
the gas giant planets Jupiter, Saturn, Neptune, Uranus
-
the lower atmosphere and surface of Venus
-
the solar nebula
-
Titan, which is Saturn's largest satellite
A list of some of our ongoing and recent projects is given below.
-
atmospheric chemistry of the brown dwarf Gliese 229 B
-
formation of silicon carbide grains around red giant stars
-
iron metal oxidation in the solar nebula
-
the oxygen isotope mixing
(OIM) model for the composition of Mars
-
tremolite decomposition on Venus
-
volcanic gas chemistry on Io
|