Volatiles in interplanetary dust particles:  a review.
The paper presents a review of the volatiles found within interplanetary dust particles.  These particles have been shown to represent primitive material from early in the solar system's formation and also may contain records of stellar processes.  The organogenic elements (i.e., H, C, N, O, and S) are among the most abundant elements in our solar system, and their abundances, distributions, and isotopic compositions in early solar system materials permit workers to better understand the processes operating early in the evolutionary history of solar system materials.  Interplanetary dust particles have a range of elemental compositions, but generally they have been shown to be similar to carbonaceous chondrites, the solar photosphere, Comet Halley's chondritic cores, and matrix materials of chondritic chondrites.  Recovery and analysis of interplanetary dust particles have opened new opportunities for analysis of primitive materials, although interplanetary dust particles represent major challenges to the analyst because of their small size.
Gibson
E K
EK
Planetary Science Branch, NASA Johnson Space Center, Houston, Texas.
D000535:Aluminum / Q000032:analysis; D002244:Carbon / Q000032:analysis / Q000737:chemistry*; D004391:Dust / Q000032:analysis*; D005118:Extraterrestrial Environment; D006859:Hydrogen / Q000032:analysis; D008855:Microscopy, Electron, Scanning; D018543:Minor Planets; D009584:Nitrogen / Q000032:analysis; D010100:Oxygen / Q000032:analysis; D016082:Solar System; D018531:Spacecraft / Q000295:instrumentation; D013455:Sulfur / Q000032:analysis
D004391:Dust; D013455:Sulfur; D002244:Carbon; D006859:Hydrogen; D000535:Aluminum; D009584:Nitrogen; D010100:Oxygen