Crossmark

Spin orbit resonance cascade via core shell model: application to Mercury and Ganymede

Published Online: 2024-09-10

Published Print: 2024-10

Authors

Pinzari, Gabriella

Scoppola, Benedetto

Veglianti, Matteo
Funding

Funding for this research was provided by:

Ministero dell'Università e della Ricerca (E83C18000100006)

Agenzia Spaziale Italiana (E83C18000100006)

Università degli Studi di Roma Tor Vergata
License Information

Text and Data Mining valid from 2024-09-10

Version of Record valid from 2024-09-10
More Information

Article History

Received: 13 February 2024

Revised: 15 July 2024

Accepted: 19 July 2024

First Online: 10 September 2024

Declarations

:

: The authors declare no conflict of interest.

Document is current