Results 221 to 223 of about 171,532 (223)

Retention of Habitable Atmospheres in Planetary Systems

The ability of a planet to retain an atmosphere influences whether water can be stable as a liquid at the planet's surface. A planet's atmospheric state is the result of source, loss, and modification processes that have acted on the atmosphere over time. The loss of atmosphere to space is therefore an important component in assessing planetary surface
Brain, David, Berta-Thompson, Zachory, Chaffin, Michael, Chaufray, Jean-Yves, Cohen, Ofer, Cravens, Thomas, France, Kevin, Futaana, Yoshifumi, Garcia-Sage, Katherine, Glocer, Alex, Holmstrom, Mats, Jarvinen, Riku, Kistler, Lynn, Kopparapu, Ravikumar, Leblanc, François, Ma, Yingjuan, Marsh, Dan, Merkel, Aimee, Osten, Rachel, Peterson, William, Peticolas, Laura, Ramstad, Robin, Sakai, Shotaro, Seki, Kanako, Stevenson, Kevin, Strangeway, Robert, Terada, Naoki, Vidotto, Aline   +27 more
openaire   +1 more source

Salt partitioning between water and high-pressure ices. Implication for the dynamics and habitability of icy moons and water-rich planetary bodies

, 2017
B. Journaux, I. Daniel, S. Petitgirard, H. Cardon, J. Perrillat, R. Caracas, M. Mezouar   +6 more
semanticscholar   +1 more source

Constraints on planetary habitability from interior modelling

2013
Noack, L., Godolt, M., von Paris, Philip, Plesa, A.-C., Stracke, Barbara, Breuer, D., Rauer, H.   +6 more
openaire   +3 more sources