Carbonaceous micrometeorites from Antarctica

• Published in: Meteoritics & Planetary Science
• Main Authors: ENGRAND, CÉCILE, MAURETTE, MICHEL
• Format: Article in Journal/Newspaper
• Language: English
• Published: Wiley 1998
• Subjects: Antarc*; Antarctic; Antarctica; Greenland
• Online Access: http://dx.doi.org/10.1111/j.1945-5100.1998.tb01665.x; https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fj.1945-5100.1998.tb01665.x; https://onlinelibrary.wiley.com/doi/pdf/10.1111/j.1945-5100.1998.tb01665.x

Abstract— Over 100 000 large interplanetary dust particles in the 50–500 μm size range have been recovered in clean conditions from ∼600 tons of Antarctic melt ice water as both unmelted and partially melted/dehydrated micrometeorites and cosmic spherules. Flux measurements in both the Greenland and Antarctica ice sheets indicate that the micrometeorites deliver to the Earth's surface ∼2000× more extraterrestrial material than brought by meteorites. Mineralogical and chemical studies of Antarctic micrometeorites indicate that they are only related to the relatively rare CM and CR carbonaceous chondrite groups, being mostly chondritic carbonaceous objects composed of highly unequilibrated assemblages of anhydrous and hydrous minerals. However, there are also marked differences between these two families of solar system objects, including higher C/O ratios and a very marked depletion of chondrules in micrometeorite matter; hence, they are “chondrites‐without‐chondrules.” Thus, the parent meteoroids of micrometeorites represent a dominant and new population of solar system objects, probably formed in the outer solar system and delivered to the inner solar system by the most appropriate vehicles, comets. One of the major purposes of this paper is to discuss applications of micrometeorite studies that have been previously presented to exobiologists but deal with the synthesis of prebiotic molecules on the early Earth, and more recently, with the early history of the solar system.