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pro vyhledávání: '"Checlair, Jade H."'
Autor:
Checlair, Jade H., Villanueva, Geronimo L., Hayworth, Benjamin P. C., Olson, Stephanie L., Komacek, Thaddeus D., Robinson, Tyler D., Popovic, Predrag, Yang, Huanzhou, Abbot, Dorian S.
A critical question in astrobiology is whether exoEarth candidates (EECs) are Earth-like, in that they originate life that progressively oxygenates their atmospheres similarly to Earth. We propose answering this question statistically by searching fo
Externí odkaz:
http://arxiv.org/abs/2101.07378
Autor:
Checlair, Jade H., Hayworth, Benjamin P. C., Olson, Stephanie L., Komacek, Thaddeus D., Villanueva, Geronimo L., Popović, Predrag, Yang, Huanzhou, Abbot, Dorian S.
A critical question in the search for extraterrestrial life is whether exoEarths are Earth-like, in that they host life that progressively oxygenates their atmospheres roughly following Earth's oxygenation history. This question could be answered sta
Externí odkaz:
http://arxiv.org/abs/2008.03952
Terrestrial planets orbiting within the habitable zones of M-stars are likely to become tidally locked in a 1:1 spin:orbit configuration and are prime targets for future characterization efforts. An issue of importance for the potential habitability
Externí odkaz:
http://arxiv.org/abs/1910.06285
Autor:
Checlair, Jade H., Abbot, Dorian S., Webber, Robert J., Feng, Y. Katherina, Bean, Jacob L., Schwieterman, Edward W., Stark, Christopher C., Robinson, Tyler D., Kempton, Eliza, Alcabes, Olivia D. N., Apai, Daniel, Arney, Giada, Cowan, Nicolas, Domagal-Goldman, Shawn, Dong, Chuanfei, Fleming, David P., Fujii, Yuka, Graham, R. J., Guzewich, Scott D., Hasegawa, Yasuhiro, Hayworth, Benjamin P. C., Kane, Stephen R., Kite, Edwin S., Komacek, Thaddeus D., Kopparapu, Ravi K., Mansfield, Megan, Marounina, Nadejda, Montet, Benjamin T., Olson, Stephanie L., Paradise, Adiv, Popovic, Predrag, Rackham, Benjamin V., Ramirez, Ramses M., Rau, Gioia, Reinhard, Chris, Renaud, Joe, Rogers, Leslie, Walkowicz, Lucianne M., Warren, Alexandra, Wolf, Eric. T.
Provided that sufficient resources are deployed, we can look forward to an extraordinary future in which we will characterize potentially habitable planets. Until now, we have had to base interpretations of observations on habitability hypotheses tha
Externí odkaz:
http://arxiv.org/abs/1903.05211
Autor:
Wolf, Eric T., Kopparapu, Ravi, Airapetian, Vladimir, Fauchez, Thomas, Guzewich, Scott D., Kane, Stephen R., Pidhorodetska, Daria, Way, Michael J., Abbot, Dorian S., Checlair, Jade H., Davis, Christopher E., Del Genio, Anthony, Dong, Chaunfei, Eggl, Siegfried, Fleming, David P., Fujii, Yuka, Haghighipour, Nader, Heavens, Nicholas, Henning, Wade G., Kiang, Nancy Y., Lopez-Morales, Mercedes, Lustig-Yaeger, Jacob, Meadows, Vikki, Reinhard, Christopher T., Rugheimer, Sarah, Schwieterman, Edward W., Shields, Aomawa L., Sohl, Linda, Turbet, Martin, Wordsworth, Robin D.
While recently discovered exotic new planet-types have both challenged our imaginations and broadened our knowledge of planetary system workings, perhaps the most compelling objective of exoplanet science is to detect and characterize habitable and p
Externí odkaz:
http://arxiv.org/abs/1903.05012
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