Atmospheric Spectral Signatures

We focus on planets and moons orbiting stars bright enough for future atmosphere follow-up, especially Mini- to Super-Earths (rocky terrestrial planets of 0.5-10 Earth masses) orbiting in the “Habitable Zones” around their host stars.  We explore a wide diversity of planets from Mini-Neptunes to Lava Worlds in our team, and compare their spectral fingerprint to learn about planets and how they work. Prepare for transit observations of planets with the James Webb Space Telescope and the Extremely Large Telescopes

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Lisa Kaltenegger

Associate Professor, Director of the Carl Sagan Institute

All research areas

Accelerator Physics    Aesthetics & Media Studies    Algebra    Analysis    Analytical    Applied Mathematics    Astrophysics, General Relativity and Cosmology    Atmospheric Spectral Signatures    Bangla    Biogeochemistry and Ecosystem Science    Bioinorganic    Biological Physics    Biology Education Research    Bioorganic    Biophysical    Black Holes and Neutron Stars    Burmese    Chemical Biology    Chinese (Mandarin)    Cognition    Combinatorics and Discrete Geometry    Community and Urban Sociology    Community Ecology and Population Biology    Comparative and World Literature    Comparative Media Studies    Computational Social Science    Cosmology and the Distant Universe    Critical Studies of Race, Gender & Sexuality    Critical Studies of Race, Gender, and Sexuality    Critical Theory    Culture    Development    Disks and Jets    Early Modern Studies    Economy and Society    Engaging With Life on Earth    Evolutionary Patterns and Processes    Experimental Condensed Matter Physics    Experimental Elementary Particle Physics    Extreme Physics and Astrophysics of Compact Objects    Galaxies Across the Universe    Gender    Geometry    Habitable Environments    Hindi-Urdu    Indonesian    Inequality and Social Stratification    Inorganic    Intimate Organismal Interactions and Chemical Ecology    Japanese   
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