Dynamic water loss of antigorite by impact process

· by · in ,

Toshimori Sekine, Tomoaki Kimura, Takamichi Kobayashi, Tsutomu Mashimo

Icarus, available online 25 November 2014

PDF LINK

Related posts (automatically generated):

  1. Water delivery to the Moon by asteroidal and cometary impacts
  2. The delivery of water by impacts from planetary accretion to presentOPEN ACCESS 
  3. Water Delivery and Giant Impacts in the ‘Grand Tack’ Scenario
  4. Chemostratigraphy of the Sudbury impact basin fill: volatile metal loss and post-impact evolution of a submarine impact basin
  5. A solar wind-derived water reservoir on the Moon hosted by impact glass beadsOPEN ACCESS 
  6. Oxygen isotopic evidence for accretion of Earth’s water before a high-energy Moon-forming giant impactOPEN ACCESS 
  7. Variations in the amount of water ice on Ceres’ surface suggest a seasonal water cycleOPEN ACCESS 
  8. The Dynamic Formation Process of the CB Chondrite Gujba
  9. Incorporation of water into olivine during nebular condensation: Insights from density functional theory and thermodynamics, and implications for phyllosilicate formation and terrestrial water inventory
  10. In-situ visualization of dynamic fracture and fragmentation of an L-type ordinary chondrite by combined synchrotron X-ray radiography and microtomography
Tags: , ,