activity
20082025
most citedOptical Images of an Exosolar Planet 25 Light Years from Earth

853 citations · 3.5k across the 55 of their papers we have counts for

collaborators
Showing 2019Show all

10 papers · 1 filter

astro-ph.EP2019★ 13 cited

A Probabilistic Case For A Large Missing Carbon Sink On Mars After 3.5 Billion Years Ago

Andy W. Heard, Edwin S. Kite

Mars has a thin (6 mbar) CO2 atmosphere currently. There is strong evidence for paleolakes and rivers formed by warm climates on Mars, including after 3.5 billion years (Ga) ago, w…

astro-ph.EP2019★ 96 cited

Superabundance of Exoplanet Sub-Neptunes Explained by Fugacity Crisis

Edwin S. Kite, Bruce Fegley, Laura Schaefer +1

Transiting planets with radii 2-3 $R_\bigoplus$ are much more numerous than larger planets. We propose that this drop-off is so abrupt because at 3 $R_\bigoplus$, base-o…

astro-ph.EP2019★ 77 cited

Identifying Candidate Atmospheres on Rocky M dwarf Planets via Eclipse Photometry

Daniel D. B. Koll, Matej Malik, Megan Mansfield +4

Most rocky planets in the galaxy orbit a cool host star, and there is large uncertainty among theoretical models whether these planets can retain an atmosphere. The James Webb Spac…

astro-ph.EP2019★ 23 cited

Geochemistry constrains global hydrology on Early Mars

Edwin S. Kite, Mohit Melwani Daswani

Ancient hydrology is recorded by sedimentary rocks on Mars. The most voluminous sedimentary rocks that formed during Mars' Hesperian period are sulfate-rich rocks, explored by the…

astro-ph.EP2019★ 82 cited

Identifying Atmospheres on Rocky Exoplanets Through Inferred High Albedo

Megan Mansfield, Edwin S. Kite, Renyu Hu +4

The upcoming launch of the James Webb Space Telescope (JWST) means that we will soon have the capability to characterize the atmospheres of rocky exoplanets. However, it is still u…

astro-ph.EP2019★ 60 cited

Analyzing Atmospheric Temperature Profiles and Spectra of M dwarf Rocky Planets

Matej Malik, Eliza M. -R. Kempton, Daniel D. B. Koll +3

The James Webb Space Telescope (JWST) will open up the possibility of comprehensively measuring the emission spectra of rocky exoplanets orbiting M dwarfs to detect and characteriz…