ProfessorTim Bedding

ARC Laureate Fellow

Faculty of Science

  • 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 SUPERVISION
    Asteroseismic Analysis and Modeling of Red-Giant Stars
  • RESEARCH-BASED DEGREE SUPERVISION
    Asteroseismology and pulsation timing of the A-type stars observed by Kepler
  • RESEARCH-BASED DEGREE SUPERVISION
    Asteroseismology of 20,000 Kepler red giants
  • RESEARCH-BASED DEGREE SUPERVISION
    Asteroseismology of bright star with the SONG telescopes and TESS
  • RESEARCH-BASED DEGREE SUPERVISION
    Asteroseismology of gamma Doradus stars with Kepler
  • RESEARCH-BASED DEGREE SUPERVISION
    Asteroseismology of intermediate- and high-mass stars
  • RESEARCH-BASED DEGREE SUPERVISION
    Asteroseismology of Long Period Variable Stars
  • RESEARCH-BASED DEGREE SUPERVISION
    Asteroseismology: Probing the Interior of Stars Using Stellar Oscillations
  • RESEARCH-BASED DEGREE SUPERVISION
    Astrophysics of Rotational Twists
  • RESEARCH-BASED DEGREE SUPERVISION
    Characterisation of the old open cluster NGC1901 with asteroseismology and gyrochronology
  • RESEARCH-BASED DEGREE SUPERVISION
    Chemical Evolution of the Milky Way and Chemical Tagging
  • RESEARCH-BASED DEGREE SUPERVISION
    COMBINING INTERFEROMETRY AND ASTEROSEISMOLOGY FOR PRECISE STELLAR PARAMETER DETERMINATION
  • RESEARCH-BASED DEGREE SUPERVISION
    Developing Tools For Probing Stellar Interiors With Asteroseismology
  • RESEARCH-BASED DEGREE SUPERVISION
    Ensemble Asteroseismology with Kepler and TESS
  • RESEARCH-BASED DEGREE SUPERVISION
    Pixels, photometry, and population studies: variable stars across four years of Kepler data
  • RESEARCH-BASED DEGREE SUPERVISION
    TESS asteroseismology of open clusters red giant
  • RESEARCH-BASED DEGREE SUPERVISION
    Validating Models of the Solar Corona