COLLOQUIUM 2024

Learning the Ages and Origins of Stars from their Vibrations

SpeakerMarc Hon, MIT Kavli Institute for Astrophysics and Space Research
Date/TimeWednesday, 21 February, 3pm
LocationConference room: S11-02-07
Registration Linkhttp://tinyurl.com/2t6ckjvm
HostProf Gong Jiangbin

Abstract

For centuries, the interiors of stars have been thought impossible to probe. Only in the past three decades has asteroseismology, the study of stellar oscillations, allowed us to peer through stellar atmospheres and probe the insides of stars. It is therefore the only method that allows the determination of a star’s mass, radius, and age based on its interior properties. I will discuss how we measure the vibrations of stars like our Sun and what we can learn about the lifetimes of such stars. Asteroseismology is emerging as a powerful tool in modern astronomy for studying the history of our Galaxy and for revealing new discoveries about planets outside our Solar System. This is now made possible by our ability to survey millions of stars across the sky from NASA’s space telescopes, as well as the growing influence of machine learning and AI in astronomy. I will showcase discoveries in Galactic archaeology and exoplanetary science, along with exploring the potential of AI in the survey era of asteroseismology.

Biography

Marc is an astronomer whose research interests lie at the intersection of stellar physics, Milky Way studies, exoplanetary science, and machine learning. He is currently a postdoctoral associate at the Massachusetts Institute of Technology working on NASA’s Transiting Exoplanet Survey Satellite mission. He was a NASA Hubble Fellow at the University of Hawaii from 2020 to 2023. Hailing from Malaysia, Marc obtained his education in Australia, where he earned a first class Honours and a PhD in physics.