22 January 2016Time: 2:30pm
Venue: GO Jones Room 610
Series: Astronomy Unit Seminars
Speaker: Benoît Noyelles
Host: Carl Murray
Abstract: This talk will present a study that I published last year , explaining how Mercury got trapped into its current rotation state, i.e. the 3:2 spin-orbit resonance. I will show how a realistic tidal model, in which the dissipation depends on the tidal frequency, affects the results and prompted us to revisit the literature. As a consequence, the current rotational state should have established very swiftly, within a few tens of Gyr. I will also show how observing the current rotation of Mercury gives us clues on its interior, and will make the parallel with the synchronous icy satellites.
1: Noyelles B., Frouard J., Makarov V.V. & Efroimsky M., 2014, Spin-orbit evolution of Mercury revisited, Icarus, 241, 26-44