RT Journal Article
T1 Silicates versus sulphur - searching for clues about ionian vulcanism with Canaricam
A1 Martín Luis, F.
A1 Kidger, M.
A1 Anguita, Francisco
A1 Llorca Ballester, J.
A1 Ruiz Pérez, Javier
AB Vulcanism was rst detected on Io in 1978 byVoyager 1. Since then it has been recognisedthat Io is the most volcanically active bodyin the Solar System. Although the initialvolcanic activity observed was in the form ofSO2 geysers and sulphur lakes, the Galileomission has detected temperatures as highas 1800K on the surface, far in excess ofthe temperatures that can be explained bysulphur-driven activity. Galileo observa-tions suggest that silicate vulcanism is theprincipal driver of activity, even though thetemperatures measured are even in excessof those measured in terrestrial silicate vul-canism, but the relationship between silicateand sulphur-driven activity is not well un-derstood. We propose a project to monitorlow-temperature vulcanism on Io systemat-ically, using CanariCam on the GTC. Thisproject will allow a better understanding ofthe mechanisms of sulphur-driven vulcanism,and the relative importance of silicate andsulphur-driven activity.
PB Instituto de Astronomia de la UNAM. Universidad Nacional Autónoma de México
SN 1405-2059
YR 2005
FD 2005
LK https://hdl.handle.net/20.500.14352/50168
UL https://hdl.handle.net/20.500.14352/50168
LA eng
DS Docta Complutense
RD 2 may 2024