Zobrazeno 1 - 10
of 36
pro vyhledávání: '"Hamano, Keiko"'
Mars, Venus and Earth are expected to have started in a hot molten state. Here, we discuss how these three terrestrial planets diverged in their evolution and what mechanisms could be the cause. We discuss that early-on after magma ocean crystallizat
Externí odkaz:
http://arxiv.org/abs/2404.09420
Autor:
Ramirez, Ramses M., Abbot, Dorian S., Fujii, Yuka, Hamano, Keiko, Kite, Edwin, Levi, Amit, Lingam, Manasvi, Lueftinger, Theresa, Robinson, Tyler D., Rushby, Andrew, Schaefer, Laura, Tasker, Elizabeth, Vladilo, Giovanni, Wordsworth, Robin D.
The habitable zone (HZ) is the region around a star(s) where standing bodies of water could exist on the surface of a rocky planet. The classical HZ definition makes a number of assumptions common to the Earth, including assuming that the most import
Externí odkaz:
http://arxiv.org/abs/1903.03706
Autor:
Giri, Chaitanya, Jia, Tony Z., Cleaves II, H. James, Usui, Tomohiro, Bodas, Dhananjay, Carr, Christopher, Chen, Huan, Fujii, Yuka, Furukawa, Yoshihiro, Genda, Hidenori, Gillams, Richard J., Hamano, Keiko, Kameda, Shingo, Krishnamurthy, Ramanarayanan, Meinert, Cornelia, Meringer, Markus, Paknikar, Kishore, Rajamani, Sudha, Shivaji, Sisinthy, Steele, Andrew, Taniguchi, Masateru, Yabuta, Hikaru, Yamagishi, Akihiko
Since its inception six decades ago, astrobiology has diversified immensely to encompass several scientific questions including the origin and evolution of Terran life, the organic chemical composition of extraterrestrial objects, and the concept of
Externí odkaz:
http://arxiv.org/abs/1810.06026
The water content of magma oceans is widely accepted as a key factor that determines whether a terrestrial planet is habitable. Water ocean mass is determined as a result not only of water delivery and loss, but also of water partitioning among sever
Externí odkaz:
http://arxiv.org/abs/1804.09294
Autor:
Henning, Wade G., Renaud, Joseph P., Saxena, Prabal, Whelley, Patrick L., Mandell, Avi M., Matsumura, Soko, Glaze, Lori S., Hurford, Terry A., Livengood, Timothy A., Hamilton, Christopher W., Efroimsky, Michael, Makarov, Valeri V., Berghea, Ciprian T., Guzewich, Scott D., Tsigaridis, Kostas, Arney, Giada N., Cremons, Daniel R., Kane, Stephen R., Bleacher, Jacob E., Kopparapu, Ravi K., Kohler, Erika, Lee, Yuni, Rushby, Andrew, Kuang, Weijia, Barnes, Rory, Richardson, Jacob A., Driscoll, Peter, Schmerr, Nicholas C., Del Genio, Anthony D., Davies, Ashley Gerard, Kaltenegger, Lisa, Elkins-Tanton, Linda, Fujii, Yuka, Schaefer, Laura, Ranjan, Sukrit, Quintana, Elisa, Barclay, Thomas S., Hamano, Keiko, Petro, Noah E., Kendall, Jordan D., Lopez, Eric D., Sasselov, Dimitar D.
Highly volcanic exoplanets, which can be variously characterized as 'lava worlds', 'magma ocean worlds', or 'super-Ios' are high priority targets for investigation. The term 'lava world' may refer to any planet with extensive surface lava lakes, whil
Externí odkaz:
http://arxiv.org/abs/1804.05110
Autor:
Henning, Wade G., Renaud, Joseph P., Mandell, Avi M., Saxena, Prabal, Hurford, Terry A., Matsumura, Soko, Glaze, Lori S., Livengood, Timothy A., Airapetian, Vladimir, Asphaug, Erik, Teske, Johanna K., Schwieterman, Edward, Efroimsky, Michael, Makarov, Valeri V., Berghea, Ciprian T., Bleacher, Jacob, Rushby, Andrew, Lee, Yuni, Kuang, Weijia, Barnes, Rory, Dong, Chuanfei, Driscoll, Peter, Domagal-Goldman, Shawn D., Schmerr, Nicholas C., Del Genio, Anthony D., Jensen, Adam G., Kaltenegger, Lisa, Elkins-Tanton, Linda, Shock, Everett L., Sohl, Linda E., Quintana, Elisa, Schaefer, Laura, Barclay, Thomas S., Fujii, Yuka, Hamano, Keiko, Petro, Noah E., Lopez, Eric D., Sasselov, Dimitar D.
The geophysics of extrasolar planets is a scientific topic often regarded as standing largely beyond the reach of near-term observations. This reality in no way diminishes the central role of geophysical phenomena in shaping planetary outcomes, from
Externí odkaz:
http://arxiv.org/abs/1804.05094
Autor:
Ramirez, Ramses M., Abbot, Dorian S., Airapetian, Vladimir, Fujii, Yuka, Hamano, Keiko, Levi, Amit, Robinson, Tyler D., Schaefer, Laura, Wolf, Eric T., Wordsworth, Robin D.
This is a white paper in response to the National Academy of Sciences "Exoplanet Science Strategy" call. We summarize recent advances in theoretical habitability studies and argue that such studies will remain important for guiding and interpreting o
Externí odkaz:
http://arxiv.org/abs/1803.00215
We present the thermal evolution and emergent spectra of solidifying terrestrial planets along with the formation of steam atmospheres. The lifetime of a magma ocean and its spectra through a steam atmosphere depends on the orbital distance of the pl
Externí odkaz:
http://arxiv.org/abs/1505.03552
Autor:
Giri, Chaitanya, Jia, Tony, James, H, Ii, Cleaves, Usui, Tomohiro, Bodas, Dhananjay, Carr, Christopher, Chen, Huan, Fujii, Yuka, Furukawa, Yoshihiro, Genda, Hidenori, Gillams, Richard, Hamano, Keiko, Kameda, Shingo, Krishnamurthy, Ramanarayanan, Meinert, Cornelia, Meringer, Markus, Paknikar, Kishore, Rajamani, Sudha, Shivaji, Sisinthy, Steele, Andrew, Taniguchi, Masateru, Yabuta, Hikaru, Yamagishi, Akihiko
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2592::8159698398d08bd4c2baeefcfcecf660
https://hal.archives-ouvertes.fr/hal-02323543/document
https://hal.archives-ouvertes.fr/hal-02323543/document
Autor:
Giri, Chaitanya, Jia, Tony, James, H, Ii, Cleaves, Usui, Tomohiro, Bodas, Dhananjay, Carr, Christopher, Chen, Huan, Fujii, Yuka, Furukawa, Yoshihiro, Genda, Hidenori, Gillams, Richard, Hamano, Keiko, Kameda, Shingo, Krishnamurthy, Ramanarayanan, Meinert, Cornelia, Meringer, Markus, Paknikar, Kishore, Rajamani, Sudha, Shivaji, Sisinthy, Steele, Andrew, Taniguchi, Masateru, Yabuta, Hikaru, Yamagishi, Akihiko
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::8159698398d08bd4c2baeefcfcecf660
https://hal.science/hal-02323543
https://hal.science/hal-02323543