Zobrazeno 1 - 10
of 84
pro vyhledávání: '"Sarah M, Hörst"'
Autor:
Shannon M. MacKenzie, Alexandra Pontefract, R. Terik Daly, Jacob J. Buffo, Gordon R. Osinski, Christopher J. Cline II, Mark J. Cintala, Kathleen L. Craft, Mallory J. Kinczyk, Joshua Hedgepeth, Sarah M. Hörst, Abel Méndez, Ben K. D. Pearce, Angela M. Stickle, Steven D. Vance
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 8, p 176 (2024)
Evidence for the beneficial role of impacts in the creation of urable or habitable environments on Earth prompts the question of whether meteorite impacts could play a similar role at other potentially urable/habitable worlds like Enceladus, Europa,
Externí odkaz:
https://doaj.org/article/f9fd7c9d4c384a0b92f2970d944677b6
Autor:
Ben K. D. Pearce, Sarah M. Hörst, Christopher J. Cline, Mark J. Cintala, Chao He, Joshua A. Sebree, Shannon M. MacKenzie, R. Terik Daly, Alexandra J. Pontefract, Cara Pesciotta
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 3, p 68 (2024)
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 expe
Externí odkaz:
https://doaj.org/article/63ad791098954d2298c6b6a34d5eeab7
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 1, p 23 (2024)
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 have contained a vast inventory of life’s building blocks and thus may have seeded warm littl
Externí odkaz:
https://doaj.org/article/48a11a660c4d4ce38e0423f140e404ce
Publikováno v:
ACS Earth and Space Chemistry. 6:2295-2304
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e9f9eff914eea06d98a024825553df18
https://doi.org/10.1021/acsearthspacechem.2c00164
https://doi.org/10.1021/acsearthspacechem.2c00164
Autor:
Koyena Das, Thomas Gautier, Joseph Serigano, Cyril Szopa, Sarah M. Hörst, Maélie Coutelier, Sandrine Vinatier, Melissa G. Trainer
In Titan, the two major gases - dinitrogen (N2) and methane (CH4) are ionized and/or photolyzed at high altitudes by the sunlight and the energetic particles from Saturn's magnetosphere, resulting in rich atmospheric chemistry and a wide variety of c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0dcb5ed984a86f34ff46fd271a18d0e5
https://doi.org/10.5194/epsc2022-710
https://doi.org/10.5194/epsc2022-710
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::319b627fd25ed10a24c7fd6bc081a5ed
http://arxiv.org/abs/2209.09257
http://arxiv.org/abs/2209.09257
Autor:
Julianne I. Moses, Zarah L. Brown, Tommi T. Koskinen, Leigh N. Fletcher, Joseph Serigano, Sandrine Guerlet, Luke Moore, J. Hunter Waite, Lotfi Ben-Jaffel, Marina Galand, Joshua M. Chadney, Sarah M. Hörst, James A. Sinclair, Veronique Vuitton, Ingo Müller-Wodarg
Publikováno v:
Icarus. 391:115328
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4fb575443d01117d73c79e7931a72eac
https://doi.org/10.1016/j.icarus.2022.115328
https://doi.org/10.1016/j.icarus.2022.115328
Autor:
Jialin Li, Xinting Yu, Ella Sciamma-O’Brien, Chao He, Joshua A. Sebree, Farid Salama, Sarah M. Hörst, Xi Zhang
In Titan's nitrogen-methane atmosphere, photochemistry leads to the production of complex organic particles, forming Titan's thick haze layers. Laboratory-produced aerosol analogs, or "tholins", are produced in a number of laboratories; however, most
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6201646aefb0392fc51afa1da3c0c4be
http://arxiv.org/abs/2112.04904
http://arxiv.org/abs/2112.04904
Autor:
Natasha E. Batalha, E. M. May, Jayesh M. Goyal, Kristin S. Sotzen, Joseph J. Linden, Carey M. Lisse, Nikole K. Lewis, Sarah M. Hörst, Kathleen Mandt, Kevin B. Stevenson, Noam R. Izenberg, Calley L. Tinsman
The majority of exoplanets found to date have been discovered via the transit method, and transmission spectroscopy represents the primary method of studying these distant worlds. Currently, in-depth atmospheric characterization of transiting exoplan
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bd8ecc21ff26ae44d4a773f74a170bc2
http://arxiv.org/abs/2109.02714
http://arxiv.org/abs/2109.02714
Autor:
Sarah M. Hörst, Peter Gao, Nikole K. Lewis, Jonathan J. Fortney, Caroline V. Morley, Xinting Yu, Austin H. Dymont, Patricia McGuiggan, Véronique Vuitton, Chao He, Jeff A. Valenti, Julianne I. Moses, Diana Powell, Xi Zhang, Sarah E. Moran, Eliza M.-R. Kempton
Publikováno v:
NATURE ASTRONOMY, vol 5, iss 8
Nature Astronomy
Nature Astronomy, Nature Publishing Group, 2021
Nature Astronomy, vol 5, iss 8
Nature Astronomy
Nature Astronomy, Nature Publishing Group, 2021
Nature Astronomy, vol 5, iss 8
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3a94086cb78306c9f7951ba557ad6738
https://escholarship.org/uc/item/8714021c
https://escholarship.org/uc/item/8714021c