Stimulated desorption of atoms and molecules in the outer solar system



Título del documento: Stimulated desorption of atoms and molecules in the outer solar system
Revista: Brazilian journal of physics
Base de datos: PERIÓDICA
Número de sistema: 000156873
ISSN: 0103-9733
Autors: 1
Institucions: 1University of Virginia, Engineering Phyics, Charlottesville, Virginia. Estados Unidos de América
Any:
Període: Sep
Volum: 29
Número: 3
Paginació: 444-449
País: Brasil
Idioma: Inglés
Tipo de documento: Artículo
Enfoque: Analítico
Resumen en inglés Laboratory data is needed on electronically-induced desorption from low-temperature solids: ices, organics, hydrated salts, glasses and certain minerals. Many bodies in the outer solar system are bombarded by relatively intense fluxes of fast ions and electrons as well as solar UV photons. This can cause both changes in their optical reflectance as well as desorption of atoms and molecules from their surfaces. Stimulated desorption produces Na and K 'atmospheres' above the 'rocky' surfaces of the moon and Mercury and H2O, H2 and O2 'atmospheres' about icy outer-solar system bodies. Since theses bodies contain other surface materials, direct detection by spacecraft or remote detection by telescopes of the desorbed atoms and molecules can be used, along with laboratory data, to determine the surface composition and geological processes occurring on distant bodies. This paper describes the relevance of stimulated desorption to the ambient neutrals and plasma in Saturn's magnetosphere, in preparation for CASSINI's arrival, and to the production of atmospheres on the moons of Jupiter being studied by the Galileo spacecraft
Disciplines Física y astronomía
Paraules clau: Astronomía,
Física atómica y molecular,
Desorbción,
Atomos,
Moléculas,
Sólidos a baja temperatura,
Magnetósfera,
Saturno
Keyword: Physics and astronomy,
Astronomy,
Atomic and molecular physics,
Desorption,
Atoms,
Molecules,
Low temperature solids,
Magnetosphere,
Saturn
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