TITANSLAKES

"Titan's Lakes: Croll-Milankovitch, Seasonal and Hydrologic Cycles"

Coordinatore	WEIZMANN INSTITUTE OF SCIENCE    more  Organization address address: HERZL STREET 234 city: REHOVOT postcode: 7610001 contact info Titolo: Ms. Nome: Gabi Cognome: Bernstein Email: send email Telefono: +972 8 934 4026 Fax: +972 8 934 4165
Nazionalità Coordinatore	Israel [IL]
Totale costo	100˙000 €
EC contributo	100˙000 €
Programma	FP7-PEOPLE Specific programme "People" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
Code Call	FP7-PEOPLE-2012-CIG
Funding Scheme	MC-CIG
Anno di inizio	2012
Periodo (anno-mese-giorno)	2012-08-01   -   2016-07-31

 Partecipanti

#	participant	country	role	EC contrib. [€]
1	WEIZMANN INSTITUTE OF SCIENCE  Organization address address: HERZL STREET 234 city: REHOVOT postcode: 7610001 contact info Titolo: Ms. Nome: Gabi Cognome: Bernstein Email: send email Telefono: +972 8 934 4026 Fax: +972 8 934 4165	IL (REHOVOT)	coordinator	100˙000.00

Mappa

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 Obiettivo del progetto (Objective)

'A set of liquid hydrocarbon lakes and lake basins has been discovered in Titan's high latitudes. The lakes exhibit a dramatic hemispheric asymmetry; significant area fractions of the northern high latitudes are covered by lakes, while the same southern latitudes are largely devoid of such features. We consider the hypothesis and its consequences that in addition to known seasonal changes, the observed difference in lake distribution may be caused by an asymmetry in the seasons owing to the orbit. Due to Saturn's eccentricity, the instantaneous solar insolation received at Titan is asymmetric. The asymmetry drives a hemispheric difference in evaporation minus precipitation, and hence, in the accumulation of lakes on Titan's northern and southern surfaces. The effect is modulated by, and reverses with, dynamical variations in the orbit. In this picture, much like in Earth's climate and glacial cycles, the resulting vigorous hydrologic cycle has a period of tens of thousands of years. We seek to answer the following fundamental questions:

1. To what extent do Titan's varying orbital parameters control the long-term volatile transport and surface reservoirs? 2. How do Titan's lakes and seas respond to seasonal forcing? 3. What is the relative role of subsurface transport of methane and ethane? 4. What constraints and general properties may be derived in order to better understand Titan's overall climatologic and hydrologic evolution?'