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Artist’s illustration of a young red dwarf stripping away a planet’s atmosphere. Credit: NASA, ESA, and D. Player (STScI)
Reference: “GJ 1252b: A Hot Terrestrial Super-Earth with No Atmosphere” by Ian J. M. Crossfield, Matej Malik, Michelle L. Hill, Stephen R. Kane, Bradford Foley, Alex S. Polanski, David Coria, Jonathan Brande, Yanzhe Zhang, Katherine Wienke, Laura Kreidberg, Nicolas B. Cowan, Diana Dragomir, Varoujan Gorjian, Thomas Mikal-Evans, Björn Benneke, Jessie L. Christiansen, Drake Deming and Farisa Y. Morales, 23 September 2022, The Astrophysical Journal Letters.
DOI: 10.3847/2041-8213/ac886b
The research was led by Ian Crossfield at the University of Kansas. It included scientists from UC Riverside as well as NASA’s Jet Propulsion Laboratory (JPL), California Institute of Technology (Caltech), University of Maryland, Carnegie Institution for Science, Max Planck Institute for Astronomy, McGill University, University of New Mexico, and the University of Montreal.
Hill’s work on this project was supported by a grant from the Future Investigators in NASA Earth and Space Science and Technology program.
Original Text (This is the original text for your reference.)
Artist’s illustration of a young red dwarf stripping away a planet’s atmosphere. Credit: NASA, ESA, and D. Player (STScI)
Reference: “GJ 1252b: A Hot Terrestrial Super-Earth with No Atmosphere” by Ian J. M. Crossfield, Matej Malik, Michelle L. Hill, Stephen R. Kane, Bradford Foley, Alex S. Polanski, David Coria, Jonathan Brande, Yanzhe Zhang, Katherine Wienke, Laura Kreidberg, Nicolas B. Cowan, Diana Dragomir, Varoujan Gorjian, Thomas Mikal-Evans, Björn Benneke, Jessie L. Christiansen, Drake Deming and Farisa Y. Morales, 23 September 2022, The Astrophysical Journal Letters.
DOI: 10.3847/2041-8213/ac886b
The research was led by Ian Crossfield at the University of Kansas. It included scientists from UC Riverside as well as NASA’s Jet Propulsion Laboratory (JPL), California Institute of Technology (Caltech), University of Maryland, Carnegie Institution for Science, Max Planck Institute for Astronomy, McGill University, University of New Mexico, and the University of Montreal.
Hill’s work on this project was supported by a grant from the Future Investigators in NASA Earth and Space Science and Technology program.
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