MOUSIS, O.; ATKINSON, D.; AMATO, M.; ASLAM, S.; ATREYA, S.; BLANC, M.; BOLTON, S.; BRUGGER, B.; CALCUTT, S.; CAVALIÉ, T.; CHARNOZ, S.; COUSTENIS, A.; DELEUIL, M.; DOBRIJEVIC, M.; FERRI, F.; FLETCHER, L.; GAUTIER, D.; GUILLOT, T.; HARTOGH, P.; HOLLAND, A.

Metadatos

Mostrar el registro completo del ítem

Licencia de uso del documento

MOUSIS, O.
Univers, Théorie, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) [UTINAM]

ATKINSON, D.
Center for medical imaging

AMATO, M.

Idioma

Communication dans un congrès

Este ítem está publicado en

European Planetary Science Congress 2017, held 17-22 September, 2017 in Riga Latvia, id. EPSC2017-305, 2017-09-17, Riga.

Resumen en inglés

The Hera Saturn entry probe mission is proposed as an ESA M-class mission to be piggybacked on a NASA spacecraft sent to or past the Saturn system. Hera consists of an atmospheric probe built by ESA and released into the atmosphere of Saturn by its NASA companion Saturn Carrier-Relay spacecraft. Hera will perform in situ measurements of the chemical and isotopic composition as well as the structure and dynamics of Saturn's atmosphere using a single probe, with the goal of improving our understanding of the origin, formation, and evolution of Saturn, the giant planets and their satellite systems, with extrapolation to extrasolar planets. Hera will probe well into and possibly beneath the cloud-forming region of the troposphere, below the region accessible to remote sensing, to locations where certain cosmogenically abundant species are expected to be well mixed.< Leer menos

Orígen

Importado de Hal

Centros de investigación

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804