Modeling Impact Cratering on Titan
We model Titan’s crater size distribution considering Centaur objects as the main impactors and compare our results with updated observational crater counts, obtaining the surface age for each crater diameter. Presented by Natalia Rossignoli, Instituto de Astrof´ısica de La Plata, CCT La Plata - CONICET - UNLP.
Видео Modeling Impact Cratering on Titan канала Lunar and Planetary Institute
Видео Modeling Impact Cratering on Titan канала Lunar and Planetary Institute
Показать
Комментарии отсутствуют
Информация о видео
15 сентября 2020 г. 6:00:41
00:23:28
Другие видео канала
Observations of Small Solar System Objects with Ground- and space-Based ObservatoriesCompositional Remote Sensing of Planetary Surfaces with SpectroscopyPlanetary Radar: AreciboCold Case: Fractional Crystallization in Cryomagmatic SystemsNew HorizonsTo Be (a CK) or Not To Be (a CK)?: The Unusual Case of Northwest Africa 10588LPI Professional Development for Planetary Scientists: Managing Stress FatigueDragonfly: A Rotorcraft Lander at TitanLive from LPSCSouth Sevier High School Moon 101 PresentationHayabusa2 Returned Samples: Unique and Pristine Record of Solar System Materials from Asteroid RyuguOcean-Surface Exchange at the Icy Ocean Worlds:DecadalHaiku Contest PresentationThe Road to Mission Science: Seminars for students and early career researchersCarbonaceous Chondrites — Nebular/Accretion Processes and Secondary ProcessingGeologic Map of the Hokusai Quadrangle (H05) of MercuryEvaluating the Emplacement Mechanisms of Vredefort Impact Melt DikesThe Internal Happenings of Dwarf Planet HaumeaDragonfly