Share
Satellites of the Outer Solar System: Exchange Processes Involving the Interiors
Grasset, O. ; Blanc, M. ; Coustenis, A. (Author)
·
Springer
· Paperback
Satellites of the Outer Solar System: Exchange Processes Involving the Interiors - Grasset, O. ; Blanc, M. ; Coustenis, A.
Choose the list to add your product or create one New List
✓ Product added successfully to the Wishlist.
Go to My Wishlists
Origin: U.S.A.
(Import costs included in the price)
It will be shipped from our warehouse between
Monday, July 29 and
Monday, August 05.
You will receive it anywhere in United Kingdom between 1 and 3 business days after shipment.
Synopsis "Satellites of the Outer Solar System: Exchange Processes Involving the Interiors"
Recent space missions to the outer solar system, Galileo (1996-2003) and Cassini-Huygens (2004-today), together with ground observations, have revealed that the moons of the outer solar system are enigmatic objects, introducing extraordinary challenges for geologists, astrobiologists, organic chemists, and planetologists. Chemical exchange exists through the different layers that form their interiors, and also from the interior to the surface. The most convincing evidence is certainly the discovery of water vapour and ice particles emerging from Enceladus's active south polar region. Evidence for exchange with a subsurface liquid ocean has also been provided by the inference of hydrated salts on the surfaces of Jupiter's moons, Europa and Ganymede, as well as the detection of sodium salts in particles originating in Enceladus's plumes. Aqueous exchange with the rocky core may also be possible, considering that 40Ar has been observed in the plumes of Enceladus during one flyby of Cassini and in the atmosphere of Titan. The ongoing CH4 replenishment in Titan's atmosphere is additional striking evidence of exchange processes within the moons.
