Zobrazeno 1 - 10
of 49
pro vyhledávání: '"Mikhail Yu. Zolotov"'
Publikováno v:
Elements. 16:47-52
The ingredients to make an environment habitable (e.g., liquid water, chemical disequilibria, and organic molecules) are found throughout the solar system. Liquid water has existed transiently on some bodies and persistently as oceans on others. Mole
Autor:
Keisuke Fukushi, Yoshio Takahashi, Daigo Shoji, Masahiro Yoda, Shuukhaaz Ganbat, Yasuhito Sekine, Mikhail Yu. Zolotov, Davaadorj Davaasuren, Takuma Kitajima, Tuvshin Gerelmaa, Baasansuren Gankhurel
Publikováno v:
Journal of Geophysical Research: Planets. 126
Autor:
Shuukhaaz Ganbat, Davaadorj Davaasuren, Takuma Kitajima, Tuvshin Gerelmaa, Baasansuren Gankhurel, Yasuhito Sekine, Daigo Shoji, Yoshio Takahashi, Keisuke Fukushi, Mikhail Yu. Zolotov, Masahiro Yoda
Publikováno v:
Goldschmidt2021 abstracts.
Autor:
Cayman T. Unterborn, Camerian Millsaps, Steven Glaser, Susanne Neuer, Steffen Buessecker, Ariel D. Anbar, Mikhail Yu. Zolotov, Hilairy E. Hartnett, D. Glaser, Nuno C. Santos, Steven J. Desch, Joseph O'Rourke, Sara Imari Walker, Stephen R. Kane, Theresa Fisher, Carey M. Lisse
The search for life on exoplanets is one of the grand scientific challenges of our time. The strategy to date has been to find (e.g., through transit surveys like Kepler) earthlike exoplanets in their stars’ habitable zone, then use transmission sp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ecfac385af3ba46a9efc71ff42e952d
http://arxiv.org/abs/2004.03631
http://arxiv.org/abs/2004.03631
Autor:
Mikhail Yu. Zolotov
Publikováno v:
Reviews in Mineralogy and Geochemistry. 84:351-392
Autor:
Mikhail Yu. Zolotov
Publikováno v:
Icarus. 296:289-304
Bright materials have been reported in association with impact craters on Ceres. The abundant Na2CO3 and some ammonium salts, NH4HCO3 and/or NH4Cl, were detected in bright deposits within Occator crater with Dawn near infrared spectroscopy. The compo
Publikováno v:
Geochimica et Cosmochimica Acta. 199:58-74
Chondritic planetesimals are among the first planetary bodies that accreted inside and outside water snow line in the protoplanetary disk. CV3 carbonaceous chondrite parent body accreted relatively small amount of water ice, probably near the snow li
Autor:
Mikhail Yu. Zolotov
Chemical and phase compositions of the surface of Venus could reflect a history of gas–rock and fluid–rock interactions, recent and past climate changes, and a loss of water from the Earth’s sister planet. The concept of chemical weathering on
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::796f6dd225006eea1705f0ed3f8d9ea2
https://doi.org/10.1093/acrefore/9780190647926.013.146
https://doi.org/10.1093/acrefore/9780190647926.013.146
Publikováno v:
Icarus. 275:203-220
Numerical chemical models for water–basalt interaction have been used to constrain the formation of stratified mineralogical sequences of Noachian clay-bearing rocks exposed in the Mawrth Vallis region and in other places on cratered martian highla