

Starts With A Bang #121 - Direct exoplanet imaging
Sep 6, 2025
Dr. Kielan Hoch, a postdoctoral researcher at the Space Telescope Science Institute, dives into the fascinating realm of exoplanets and their formation. He discusses groundbreaking imaging techniques, particularly those from the James Webb Space Telescope, that could one day help us see Earth-like worlds. Hoch also highlights the challenges faced by early-career scientists in securing funding and navigating a competitive landscape, stressing the need for systemic reform. This engaging conversation blends optimism and urgency as we ponder the future of exoplanet exploration.
AI Snips
Chapters
Transcript
Episode notes
Direct Imaging Targets Young Giant Planets
- Direct imaging favors young, self-luminous giant planets at tens-to-hundreds of AU from their star.
- These planets emit thermal infrared light, making spectroscopy of atmospheres possible without reflected starlight.
Spectra From Every Pixel Reveals Formation Clues
- Integral field spectrographs deliver spectra for every image pixel, letting us detect individual molecular lines.
- Those lines reveal atmospheric abundances and formation clues like core accretion versus gravitational collapse.
Transit And Imaging Offer Complementary Windows
- Transit spectroscopy and direct imaging are complementary but biased to different regimes.
- Direct imaging gives higher SNR, higher-resolution spectra for younger, wide-orbit objects useful for formation studies.