Research
The field of exoplanets -- the study of planetary systems beyond our solar system -- is one of the fastest-moving areas in astrophysics today. Astronomers have now discovered more than 6,000 extrasolar planets, and most orbit stars that will one day evolve into white dwarfs. Our own Sun will follow this path in about five billion years. What will happen to the solar system then? And more broadly, what becomes of planets, asteroids, and moons when their stars exhaust their fuel and leave the main sequence? These are the questions at the heart of my research.
I use a range of techniques to investigate the remains of planetary systems around white dwarfs. With telescopes such as TESS and ZTF — and soon LSST — I search for planets and fragments that cross in front of white dwarfs. Spectroscopic data from the Hubble Space Telescope, the Keck Telescope, the Very Large Telescope, and the Dark Energy Spectroscopic Instrument (DESI) allow me to study the fingerprints of rocky material that pollute white dwarf atmospheres. I also use the James Webb Space Telescope and the Spitzer Space Telescope to explore the dusty disks that surround these stellar remnants.
You can learn more about my work at the
NOIRLab Story Series. Recently, together with Dr. Aaron Meisner, we launched a citizen science project,
Exo-Asteroid — an open invitation to help search for asteroids around dead stars.