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SUMMARY:Synchrotron radiation X-ray tomographic microscopy\, noble gas mas
 s spectroscopy\, infrared and Raman microscopy correlated study of the Ito
 kawa asteroid particles returned by the Hayabusa space probe
DTSTART;VALUE=DATE-TIME:20160706T050000Z
DTEND;VALUE=DATE-TIME:20160706T053000Z
DTSTAMP;VALUE=DATE-TIME:20260513T224733Z
UID:indico-contribution-1277@indico.inp.nsk.su
DESCRIPTION:Speakers: Sergey Pavlov (German Aerospace Center)\nThe analysi
 s of ateroid’s surface grains allows to match remote observations and mo
 deling of its history and current properties with laboratory experiments. 
 Mass spectrometry and electron microscopy of the dust enables detailed stu
 dy of the history of asteroidal regolith and compare the results with theo
 retical considerations of the evolution of rubble piles in the inner solar
  system. A correlated study including consequential Raman and infrared mic
 rospectroscopy\, synchrotron radiation X-ray tomographic microscopy (SRXTM
 ) and noble gas mass spectroscopy has been implemented for the determinati
 on of cosmic-ray exposure ages and trapped Xe content in a few particles r
 eturned by the JAXA’s Hayabusa space probe from the near-Earth asteroid 
 25143 Itokawa\, the first successful sample return mission to an asteroid.
  New data support the uniformly short exposure to cosmic rays of the Itoka
 wa regolith of \n\nhttps://indico.inp.nsk.su/event/3/contributions/1277/
LOCATION:Budker INP Parallel session Hall
URL:https://indico.inp.nsk.su/event/3/contributions/1277/
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