Helium escaping from the atmosphere of a nearby rocky exoplanet orbiting in a habitable zone

C Collin Cherubim (Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA, USA.) S Shreyas Vissapragada (Carnegie Science Observatories, Pasadena, CA, USA.) T Tim Cunningham (Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA, USA.) A Annabella G. Meech (Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA, USA.) D David Charbonneau (Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA, USA.) R Robin Wordsworth (Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA, USA.) A Aaron Householder (Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA.) J Johanna Teske L Leonardo A. dos Santos N Nicole L. Wallack (Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA.) W William Misener (Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA.) Z Zifan Lin (Department of Physics, Washington University in St. Louis, St. Louis, MO, USA.) A Andrew McWilliam (Carnegie Science Observatories, Pasadena, CA, USA.) M Michael Zhang (Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA.) J Jason A. Dittmann (Department of Astronomy, University of Florida, Gainesville, FL, USA.) M Mercedes López-Morales (Space Telescope Science Institute, Baltimore, MD, USA.)

Abstract

Observations of highly irradiated gas giant exoplanets have shown helium escaping from their atmospheres. There is limited evidence for atmospheres on rocky exoplanets, perhaps because they have already escaped. We report near-infrared spectroscopic observations of LHS 1140b, a rocky exoplanet that orbits in the habitable zone of a nearby low-mass star. The transit spectra show absorption by helium escaping from the planet’s atmosphere. Helium absorption is detected in 2024 but not in 2025, indicating time-variable atmospheric escape. We interpret these results as indicating an upper atmosphere dominated by helium and depleted in hydrogen, with other volatile species trapped at lower altitudes, consistent with atmospheric fractionation models. No helium absorption is detected for LHS 1140c, a smaller and more strongly irradiated exoplanet in the same system.

Article Details

Journal Science
Volume / Issue Vol. 1, Issue 1
Published July 16, 2026
ISSN 0036-8075
Publisher American Association for the Advancement of Science

Journal Info

Science

American Association for the Advancement of Science

ISSN: 0036-8075 Social Sciences

Authors (16)

C

Collin Cherubim

Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA, USA.

S

Shreyas Vissapragada

Carnegie Science Observatories, Pasadena, CA, USA.

T

Tim Cunningham

Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA, USA.

A

Annabella G. Meech

Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA, USA.

D

David Charbonneau

Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA, USA.

R

Robin Wordsworth

Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA, USA.

A

Aaron Householder

Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA.

J

Johanna Teske

L

Leonardo A. dos Santos

N

Nicole L. Wallack

Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA.

W

William Misener

Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA.

Z

Zifan Lin

Department of Physics, Washington University in St. Louis, St. Louis, MO, USA.

A

Andrew McWilliam

Carnegie Science Observatories, Pasadena, CA, USA.

M

Michael Zhang

Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA.

J

Jason A. Dittmann

Department of Astronomy, University of Florida, Gainesville, FL, USA.

M

Mercedes López-Morales

Space Telescope Science Institute, Baltimore, MD, USA.