• Non ci sono risultati.

D. Turrini, ISSI Team “Vesta, the key to the origins of the Solar System”, and EChO

N/A
N/A
Protected

Academic year: 2022

Condividi "D. Turrini, ISSI Team “Vesta, the key to the origins of the Solar System”, and EChO"

Copied!
2
0
0

Testo completo

(1)

Mem. S.A.It. Vol. 87, 216

SAIt 2016 c Memorie

della

The formation of giant planets and its e ects on protoplanetary disks: the case of Jupiter and the

Jovian Early Bombardment

D. Turrini, ISSI Team “Vesta, the key to the origins of the Solar System”, and EChO

“Planetary Formation” working group

INAF-IAPS, Istituto di Astrofisica e Planetologia Spaziali, Area di Ricerca di Tor Vergata, via Fosso del Cavaliere 100, 00133, Rome, Italy

Abstract.

The formation of giant planets is accompanied by a short but intense primordial bombardment (Safronov 1969; Weidenschilling 1975, 2001; Turrini, Magni & Coradini 2011): the prototype for this class of events is the Jovian Early Bombardment (JEB) caused by the formation of Jupiter in the Solar System (Turrini, Magni & Coradini 2011; Turrini, Coradini & Magni 2012). The JEB affected the collisional evolution of the minor bodies in the inner Solar System by inflicting mass loss to planetesimals (Turrini, Coradini & Magni 2012; Turrini 2014; Turrini & Svetsov 2014) due to cratering erosion and, at the same time, delivering water and volatile materials to the asteroid belt (Turrini & Svetsov 2014). The JEB also resulted in a significant number of collisions between Jupiter and planetesimals formed over a wide orbital range, delivering volatile and refractory materials to the giant planet and its circumplanetary disk (Turrini, Nelson

& Barbieri 2015). In this talk I’ll discuss how the study of the effects of the JEB on Vesta can be used to constrain the early evolution of the Solar System (Turrini 2014; Turrini & Svetsov 2014) and how these constraints can, in turn, provide insight on the composition of Jupiter and of its satellites. Finally, I’ll discuss the implications of the JEB model for extrasolar planets (Turrini, Nelson & Barbieri 2015).

References

Safronov, V. S. 1969, Evolution of the protoplanetary cloud and formation of the earth and plan- ets. Translated from Russian in 1972. Keter Publishing House, 212 p.

Turrini D., Magni G., Coradini A. 2011, MNRAS, 413, 2439 Turrini D., Coradini A., Magni G. 2012, ApJ, 750, 8

Turrini D. 2014, Planet. Space Sci., 103, 82 Turrini D., Svetsov V. 2014, Life, 4, 4

Turrini D., Nelson R., Barbieri M. 2015, Experimental Astronomy, 40, 501

(2)

Turrini D. et al.: The formation of Jupiter and the Jovian Early Bombardment 217 Weidenschilling S. 1975, Icarus, 26, 361

Weidenschilling S., et al. 2001, Earth, Planets, and Space, 53, 1093

Riferimenti

Documenti correlati

Sotto l'effetto della corrente di luci- datura l'elettrolita, durante il proce- dimento di lucidatura, forma sulla superficie dei pezzi il cosiddetto film di lucidatura, uno

an American employed by a Japanese branch office of the American company, the abuse of the right to dismiss theory was recognized as an aspect of Japan’s distinctive

The main goals of pharmacological therapy in HCM include control of symptoms and exercise lim- itation, abolition or reduction of dynamic intraventricular gradi- ents, treatment of

Le scelte degli autori dei testi analizzati sono diverse: alcuni (per esempio Eyal Sivan in Uno specialista) usano materiale d’archivio co- me fotografie e filmati, altri invece

What type of catheter is most effective at preventing catheter-related infections, including catheter-related bloodstream infection (CR-BSI), e.g., number of lumens, tunnelled

CAMBIO DEI CATETERI Cateteri venosi periferici Come metodo per prevenire la flebite e le infezione associate al catetere e’ stato proposto il cambio programmato dei

To answer this question, we generated a large number of RSA key pairs from 22 software libraries (both open- source and closed-source) and 16 different cryptographic smartcards from

Con i LEDs ora a disposizione, la luce bianca che può essere generata ha una efficienza luminosa massima di 30 lm/W (lumen/Watt).In figura 1.5 è riportato uno spettro