26 citations · 65 across the 7 of their papers we have counts for
7 papers
Comparing NASA Discovery and New Frontiers Class Mission Concepts for the Io Volcano Observer (IVO)
Christopher W. Hamilton, Alfred S. McEwen, Laszlo Keszthelyi +31
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, inclu…
Towards Prebiotic Chemistry on Titan: Impact experiments on organic haze particles
Ben K. D. Pearce, Sarah M. Hörst, Christopher J. Cline +7
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 li…
Organic hazes as a source of life's building blocks to warm little ponds on the Hadean Earth
Ben K. D. Pearce, Sarah M Hörst, Joshua A. Sebree +1
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…
Triton Haze Analogues: the Role of Carbon Monoxide in Haze Formation
Sarah E. Moran, Sarah M. Hörst, Chao He +7
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 tha…
Optical Constants of Titan Haze Analogue from 0.4 to 3.5 μm: Determined Using Vacuum Spectroscopy
Chao He, Sarah M. Horst, Michael Radke +1
Titan's thick atmosphere is primarily composed of nitrogen and methane. Complex chemistry happening in Titan's atmosphere produces optically thick organic hazes. These hazes play s…
A Cross-Laboratory Comparison Study of Titan Haze Analogs: Surface Energy
Jialin Li, Xinting Yu, Ella Sciamma-O'Brien +5
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,…