ProfessorTim Bedding
ARC Laureate Fellow
Faculty of Science
Research projects & supervision summary
Project Opportunities
Title: Asteroseismology: probing inside stars using stellar oscillations
Summary of opportunity:
Measuring oscillations in stars like the Sun using asteroseismology is a powerful new method for exploring their internal structures and testing physical theories.
Opportunity synopsis:
Asteroseismology involves using the oscillation frequencies of a star to measure its internal properties. Measuring stellar oscillations is a beautiful physics experiment: a star is a gaseous sphere and will oscillate in many different modes when suitably excited. The frequencies of these oscillations depend on the sound speed inside the star, which in turn depends on density, temperature, gas motion and other properties of the stellar interior. This analysis, called asteroseismology, yields information such as composition, age, mixing and internal rotation that cannot be obtained in any other way and is completely analogous to the seismological study of the interior of the Earth.
Many stars, including the Sun, are observed to oscillate. Asteroseismology is a new and rapidly developing field and there are several possible PhD projects, depending on the preference of the student. The projects will use observations from NASA’s Kepler and TESS spacecrafts.
RESEARCH PROJECTS & ACTIVITIES
- RESEARCH-BASED DEGREE SUPERVISIONAsteroseismic Analysis and Modeling of Red-Giant Stars
- RESEARCH-BASED DEGREE SUPERVISIONAsteroseismology and pulsation timing of the A-type stars observed by Kepler
- RESEARCH-BASED DEGREE SUPERVISIONAsteroseismology of 20,000 Kepler red giants
- RESEARCH-BASED DEGREE SUPERVISIONAsteroseismology of bright star with the SONG telescopes and TESS
- RESEARCH-BASED DEGREE SUPERVISIONAsteroseismology of gamma Doradus stars with Kepler
- RESEARCH-BASED DEGREE SUPERVISIONAsteroseismology of intermediate- and high-mass stars
- RESEARCH-BASED DEGREE SUPERVISIONAsteroseismology of Long Period Variable Stars
- RESEARCH-BASED DEGREE SUPERVISIONAsteroseismology: Probing the Interior of Stars Using Stellar Oscillations
- RESEARCH-BASED DEGREE SUPERVISIONAstrophysics of Rotational Twists
- RESEARCH-BASED DEGREE SUPERVISIONCharacterisation of the old open cluster NGC1901 with asteroseismology and gyrochronology
- RESEARCH-BASED DEGREE SUPERVISIONChemical Evolution of the Milky Way and Chemical Tagging
- RESEARCH-BASED DEGREE SUPERVISIONCOMBINING INTERFEROMETRY AND ASTEROSEISMOLOGY FOR PRECISE STELLAR PARAMETER DETERMINATION
- RESEARCH-BASED DEGREE SUPERVISIONDeveloping Tools For Probing Stellar Interiors With Asteroseismology
- RESEARCH-BASED DEGREE SUPERVISIONEnsemble Asteroseismology with Kepler and TESS
- RESEARCH-BASED DEGREE SUPERVISIONPixels, photometry, and population studies: variable stars across four years of Kepler data
- RESEARCH-BASED DEGREE SUPERVISIONTESS asteroseismology of open clusters red giant
- RESEARCH-BASED DEGREE SUPERVISIONValidating Models of the Solar Corona