Marc Pinsonneault
Professor of Astronomy
B.S., University of Texas at Austin
Ph.D., Yale University
My research concentrates on stellar structure and evolution; because
many areas of astronomy are influenced by stellar evolution theory, this
has led me to investigate a range of subjects. Broadly speaking, my interests
can be divided into studies of stellar physics and applications of stellar
models to problems of broad astrophysical interest. On the stellar physics side,
I am particularly interested in physical processes, such as microscopic diffusion and
stellar rotation, which are neglected in standard stellar models. Consideration of
these effects can strongly alter some of the predictions of stellar evolution theory.
The rapidly advancing field of asteroseismology is also now providing us with novel
diagnostics of internal stellar properties, especially in cool stars. Examples include
the surface helium abundance, convection zone depth, core mass, and core rotation.
On the applications side, I am interested in rotation as a population diagnostic, precision
estimates of stellar properties from photometry, and calibrating stellar models and
population studies using the asteroseismic tools above. Current
research interests include solar models; helioseismology and asteroseismology;
stellar populations; cosmology (big bang nucleosynthesis, ages of globular
clusters); angular momentum evolution in stars. I am working with both the Kepler Asteroseismology Science Consortium (KASC)
and the APOGEE survey of the 3rd Sloan Digital Sky Survey (SDSS.) The intersection
between the two (APOKASC) will be a rich treasury combining both abundance and seismic data on
a large sample (10,000 stars) in cool Kepler field dwarfs and giants.
Ohio State Astronomy
Department home page
Marc Pinsonneault (pinsonneault.1@osu.edu)
Updated: 2013 January 14