Results 11 to 20 of about 108,558 (304)
Are NH3 and CO2 Ice Present on Miranda?
Published near-IR spectra of the four largest classical Uranian satellites display the presence of discrete deposits of CO _2 ice, along with subtle absorption features around 2.2 μ m.
Riley A. DeColibus +2 more
doaj +1 more source
A CO2 Cycle on Ariel? Radiolytic Production and Migration to Low-latitude Cold Traps
CO _2 ice is present on the trailing hemisphere of Ariel but is mostly absent from its leading hemisphere. The leading/trailing hemispherical asymmetry in the distribution of CO _2 ice is consistent with radiolytic production of CO _2 , formed by charged
Richard J. Cartwright +13 more
doaj +1 more source
GEOLOGICAL MAPPING OF PLUTO AND CHARON USING NEW HORIZONS DATA [PDF]
Pluto and Charon exhibit strikingly different surface appearances, despite their similar densities and presumed bulk compositions. Systematic mapping has revealed that much of Pluto’s surface can be attributed to surface-atmosphere interactions and the ...
J. M. Moore +14 more
doaj +1 more source
Indirect ultraviolet photodesorption from CO:N2 binary ices - an efficient grain-gas process [PDF]
UV ice photodesorption is an important non-thermal desorption pathway in many interstellar environments that has been invoked to explain observations of cold molecules in disks, clouds and cloud cores. Systematic laboratory studies of the photodesorption
Bertin, Mathieu +9 more
core +5 more sources
Ice Nucleation on a Corrugated Surface [PDF]
Heterogeneous ice nucleation is a key process in many environmental and technical fields and is of particular importance in modeling atmospheric behavior and the Earth's climate. Despite an improved understanding of how water binds at solid surfaces, no clear picture has emerged to describe how 3D ice grows from the first water layer, nor what makes a ...
Chenfang Lin +5 more
openaire +4 more sources
Molecules, ices and astronomy [PDF]
Molecules in interstellar gas and in interstellar ices play a fundamental role in astronomy. However, the formation of the simplest molecule, molecular hydrogen, is still not fully understood.
Brown, W A +4 more
core +1 more source
Crystallization Kinetics of Vitreous Magnesium Sulfate Hydrate and Implications for Europa’s Surface
Brines consistent with that expected for Europa’s global subsurface ocean have been shown to form vitreous salt hydrates when frozen. We report experiments examining the crystallization kinetics of vitreous MgSO _4 hydrate in order to better understand ...
Paul V. Johnson +2 more
doaj +1 more source
The effects of methanol on the trapping of volatile ice components [PDF]
The evaporation of icy mantles, which have been formed on the surface of dust grains, is acknowledged to give rise to the rich chemistry that has been observed in the vicinity of hot cores and corinos.
Adriaens +50 more
core +1 more source
Cosmic-ray-mediated Formation of Benzene on the Surface of Saturn's Moon Titan [PDF]
The aromatic benzene molecule (C_6H_6)—a central building block of polycyclic aromatic hydrocarbon molecules—is of crucial importance for the understanding of the organic chemistry of Saturn's largest moon, Titan. Here, we show via laboratory experiments
Kaiser, Ralf I. +6 more
core +1 more source
Water formation on bare grains: When the chemistry on dust impacts interstellar gas [PDF]
Context. Water together with O2 are important gas phase ingredients to cool dense gas in order to form stars. On dust grains, H2 O is an important constituent of the icy mantle in which a complex chemistry is taking place, as revealed by hot core ...
Akai +53 more
core +4 more sources

