Completed
Sintering timescales (Myr) Comparisons with resurfacing rates can constrain surface properties
Class Central Classrooms beta
YouTube videos curated by Class Central.
Classroom Contents
Radiation Processing of Dust, Asteroids and Moons - What Does It Do and What Can It Tell Us?
Automatically move to the next video in the Classroom when playback concludes
- 1 Intro
- 2 Organizers
- 3 Webinar Format
- 4 Today's Speaker
- 5 Stars interact with planetary materials
- 6 Definitions: ·lonizing Radiation: lons, electrons, and photons containing energy above the target ionization threshold
- 7 Radiation Chemistry & Space Weathering 101
- 8 Saturnian Magnetosphere Evironm
- 9 Electron environment at Mimas
- 10 The PacMan Anomalies
- 11 MeV Electron Energy Losses in H2O
- 12 Sintering of regolith grains
- 13 Radiation induced diffusion
- 14 Molecular Dynamics Simulation of Elect Excitation in Water Ice
- 15 Estimates of spherical grain sintering rat
- 16 ROUGH Approximations of Resurfacing
- 17 Sintering timescales (Myr) Comparisons with resurfacing rates can constrain surface properties
- 18 Determining the Origins of Phobos and Demos
- 19 Solar wind sputtering of small bod.
- 20 Sputtering and secondary ion detection
- 21 Monte Carlo Simulations
- 22 Sputtering Experiment
- 23 SIMS: Experimental Yields Secondary ion yields for lunar soil exposed to keV energy ions
- 24 Relative Secondary lon Yield
- 25 Simulated lon Trajectories and Densit
- 26 Small body classification
- 27 PRISM Mission so to Phobos and Deimos
- 28 Formation of pre-biotic molecules in spa
- 29 Chiral-specific reactions caused by sp polarized electrons
- 30 Spin-polarized LEE Damage of Chiral Molec
- 31 Argonne National Laboratory
- 32 Amino Acid Damage: Chirality and Magnetization
- 33 XPS Characterization of Deposited Film
- 34 Cross-section statistical testing
