Descrizione del progetto
Uno studio intende scoprire come la materia organica ha forgiato l’evoluzione dei mondi ghiacciati
Una ricerca ipotizza che le molecole organiche pesanti costituiscano gran parte dei corpi del sistema solare esterno, quali lune ghiacciate, comete e oggetti transnettuniani. Finora, non si è tenuto affatto conto della presenza di materia organica carboniosa, ossia un componente della materia organica a bassa densità. Il progetto PROMISES, finanziato dall’UE, intende esaminare l’interazione tra la materia organica carboniosa, il ghiaccio e le rocce, un tassello importante per comprendere l’evoluzione dei mondi oceanici e valutarne il potenziale di ospitare forme di vita. Per effettuare la sintesi del materiale, i ricercatori utilizzeranno un dispositivo ad alta pressione denominato cella a incudine di diamante. Inoltre, si dedicheranno alla creazione di nuovi modelli per studiare le reazioni chimiche e le proprietà termochimiche delle molecole organiche pesanti interagenti.
Obiettivo
There is growing evidence that heavy organic molecules are a major component of the outer solar system bodies such as icy moons, comets, and Trans-Neptunian Objects (TNOs). Density profiles inferred from measurements of space missions require a low-density component in the core of the largest objects such as Ganymede and Titan. These observations suggest that a previously overlooked low-density component, identified as carbonaceous organic matter (COM), is one of the three main components, in addition to ice and rocks, building planetary bodies that formed beyond the ice line. However, there is a dearth of laboratory experiments and numerical simulations exploring the interaction of the heavy organic molecules constituting the COM with both the ice component (mainly H2O ices) and the rocky component (hydrated silicates, oxides and sulphides) at pressures relevant to icy moons. Observations from space missions also demonstrated that most icy moons are differentiated into a refractory core and an outer hydrosphere that includes a liquid layer (deep ocean), thus the name of ocean worlds. This raises the questions of the emergence of life at the ocean/core interface and of the habitability of ocean worlds. How does the presence of COM affect the thermal and chemical evolution of ocean worlds? The interaction between COM, ice and rocks is therefore essential for understanding the evolution of ocean worlds and for assessing their habitability potential. First, this project conducts laboratory experiments using diamond anvil cells (DAC) coupled with in situ Raman spectroscopy, a combination that is best suited for this kind of investigation. Second, it develops a thermochemical evolution model that can handle the chemical reactions and the thermo-chemical properties of the three components. Third, it applies the results to the evolution of ocean worlds in our solar system and beyond.
Campo scientifico
Parole chiave
Programma(i)
- HORIZON.1.1 - European Research Council (ERC) Main Programme
Argomento(i)
Meccanismo di finanziamento
ERC - Support for frontier research (ERC)Istituzione ospitante
44000 Nantes
Francia