Hydrogen escaping from a pair of exoplanets smaller than Neptune

R. O. Parke Loyd (), Ethan Schreyer, James E. Owen, James G. Rogers, Madelyn I. Broome, Evgenya L. Shkolnik, Ruth Murray-Clay, David J. Wilson, Sarah Peacock, Johanna Teske, Hilke E. Schlichting, Girish M. Duvvuri, Allison Youngblood, P. Christian Schneider, Kevin France, Steven Giacalone, Natasha E. Batalha, Adam C. Schneider, Isabella Longo, Travis Barman and David R. Ardila
Additional contact information
R. O. Parke Loyd: Eureka Scientific
Ethan Schreyer: Imperial College London
James E. Owen: Imperial College London
James G. Rogers: University of Cambridge
Madelyn I. Broome: University of California
Evgenya L. Shkolnik: Arizona State University
Ruth Murray-Clay: University of California
David J. Wilson: University of Colorado
Sarah Peacock: University of Maryland Baltimore County
Johanna Teske: Carnegie Institution for Science
Hilke E. Schlichting: University of California
Girish M. Duvvuri: University of Colorado
Allison Youngblood: University of Colorado
P. Christian Schneider: Hamburger Sternwarte
Kevin France: University of Colorado
Steven Giacalone: California Institute of Technology
Natasha E. Batalha: NASA Ames Research Center
Adam C. Schneider: Flagstaff Station
Isabella Longo: University of Colorado
Travis Barman: University of Arizona
David R. Ardila: California Institute of Technology

Nature, 2025, vol. 638, issue 8051, 636-639

Abstract: Abstract Exoplanet surveys have shown a class of abundant exoplanets smaller than Neptune on close,

Date: 2025
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DOI: 10.1038/s41586-024-08490-x

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