Zobrazeno 1 - 10
of 151
pro vyhledávání: '"Hörst, Sarah"'
Autor:
Horst, Sarah M.
The arrival of the Cassini-Huygens mission to the Saturn system ushered in a new era in the study of Titan. Armed with a variety of instruments capable of remote sensing and in situ investigations of Titan's atmosphere and surface, Cassini and Huygen
Externí odkaz:
http://hdl.handle.net/10150/145467
Autor:
Hamilton, Christopher W., McEwen, Alfred S., Keszthelyi, Laszlo, Carter, Lynn M., Davies, Ashley G., de Kleer, Katherine, Jessup, Kandis Lea, Jia, Xianzhe, Keane, James T., Mandt, Kathleen, Nimmo, Francis, Paranicas, Chris, Park, Ryan S., Perry, Jason E., Pommier, Anne, Radebaugh, Jani, Sutton, Sarah S., Vorburger, Audrey, Wurz, Peter, Borlina, Cauê, Haapala, Amanda F., DellaGiustina, Daniella N., Denevi, Brett W., Hörst, Sarah M., Kempf, Sascha, Khurana, Krishan K., Likar, Justin J., Masters, Adam, Mousis, Olivier, Polit, Anjani T., Bhushan, Aditya, Bland, Michael, Matsuyama, Isamu, Spencer, John
Jupiter's moon Io is a highly compelling target for future exploration that offers critical insight into tidal dissipation processes and the geology of high heat flux worlds, including primitive planetary bodies, such as the early Earth, that are sha
Externí odkaz:
http://arxiv.org/abs/2408.08334
Autor:
Pearce, Ben K. D., Hörst, Sarah M., Cline, Christopher J., Cintala, Mark J., He, Chao, Sebree, Joshua A., MacKenzie, Shannon M., Daly, R. Terik, Pontefract, Alexandra J., Pesciotta, Cara
Publikováno v:
2024 Planet. Sci. J. 5 68
Impacts are critical to producing the aqueous environments necessary to stimulate prebiotic chemistry on Titan's surface. Furthermore, organic hazes resting on the surface are a likely feedstock of biomolecules. In this work, we conduct impact experi
Externí odkaz:
http://arxiv.org/abs/2403.00029
Publikováno v:
(2024) Planet. Sci. J., 5, 23
Over 4 billion years ago, Earth is thought to have been a hazy world akin to Saturn's moon Titan. The organic hazes in the atmosphere at this time could contain a vast inventory of life's building blocks, and thus may have seeded warm little ponds fo
Externí odkaz:
http://arxiv.org/abs/2401.06212
Autor:
Moses, Julianne I., Brown, Zarah L., Koskinen, Tommi T., Fletcher, Leigh N., Serigano, Joseph, Guerlet, Sandrine, Moore, Luke, Waite Jr., J. Hunter, Ben-Jaffel, Lotfi, Galand, Marina, Chadney, Joshua M., Hörst, Sarah M., Sinclair, James A., Vuitton, Veronique, Müller-Wodarg, Ingo
During the Grand Finale stage of the Cassini mission, organic-rich ring material was discovered to be flowing into Saturn's equatorial upper atmosphere at a surprisingly large rate. Through a series of photochemical models, we have examined the conse
Externí odkaz:
http://arxiv.org/abs/2211.05253
Publikováno v:
ACS Earth and Space Chemistry 2022 6 (10), 2385-2399
A critical early stage for the origin of life on Earth may have involved the production of hydrogen cyanide (HCN) in a reducing, predominantly H$_2$ atmosphere. HCN is crucial for the origin of life as it is a possible precursor to several biomolecul
Externí odkaz:
http://arxiv.org/abs/2209.09257
Autor:
Moran, Sarah E., Hörst, Sarah M., He, Chao, Radke, Michael J., Sebree, Joshua A., Izenberg, Noam R., Vuitton, Véronique, Flandinet, Laurène, Orthous-Daunay, François-Régis, Wolters, Cédric
Triton is the largest moon of the Neptune system and possesses a thin nitrogen atmosphere with trace amounts of carbon monoxide and methane, making it of similar composition to that of the dwarf planet Pluto. Like Pluto and Saturn's moon Titan, Trito
Externí odkaz:
http://arxiv.org/abs/2112.11627
Autor:
Yu, Xinting, He, Chao, Zhang, Xi, Hörst, Sarah M., Dymont, Austin H., McGuiggan, Patricia, Moses, Julianne I., Lewis, Nikole K., Fortney, Jonathan J., Gao, Peter, Kempton, Eliza M. -R., Moran, Sarah E., Morley, Caroline V., Powell, Diana, Valenti, Jeff A., Vuitton, Véronique
Photochemical hazes are important opacity sources in temperate exoplanet atmospheres, hindering current observations from characterizing exoplanet atmospheric compositions. The haziness of an atmosphere is determined by the balance between haze produ
Externí odkaz:
http://arxiv.org/abs/2107.07069
Autor:
Moran, Sarah E., Hörst, Sarah M., Vuitton, Véronique, He, Chao, Lewis, Nikole K., Flandinet, Laurène, Moses, Julianne I., North, Nicole, Orthous-Daunay, François-Régis, Sebree, Joshua, Wolters, Cédric, Kempton, Eliza M. -R., Marley, Mark S., Morley, Caroline V., Valenti, Jeff A.
Publikováno v:
Planet. Sci. J. 1 17 (2020)
Very little experimental work has been done to explore the properties of photochemical hazes formed in atmospheres with very different compositions or temperatures than that of the outer solar system or of early Earth. With extrasolar planet discover
Externí odkaz:
http://arxiv.org/abs/2004.13794
Autor:
Sotzen, Kristin S., Stevenson, Kevin B., Sing, David K., Kilpatrick, Brian M., Wakeford, Hannah R., Filippazzo, Joseph C., Lewis, Nikole K., Hörst, Sarah M., López-Morales, Mercedes, Henry, Gregory W., Buchhave, Lars A., Ehrenreich, David, Fraine, Jonathan D., Muñoz, Antonio García, Jayaraman, Rahul, Lavvas, Panayotis, Etangs, Alain Lecavelier des, Marley, Mark S., Nikolov, Nikolay, Rathcke, Alexander D., Sanz-Forcada, Jorge
As part of the PanCET program, we have conducted a spectroscopic study of WASP-79b, an inflated hot Jupiter orbiting an F-type star in Eridanus with a period of 3.66 days. Building on the original WASP and TRAPPIST photometry of Smalley et al (2012),
Externí odkaz:
http://arxiv.org/abs/1911.02051