Laboratory amorphous carbon: A possible analog of cometary dust

Details Laboratory amorphous carbon: A possible analog of cometary dust Laboratory amorphous carbon: A possible analog of cometary dust

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987esasp.278..677b&link_type=abstract

In ESA, Proceedings of the International Symposium on the Diversity and Similarity of Comets p 677-679 (SEE N88-21884 14-91)

Physics

Amorphous Materials, Carbon, Granular Materials, Halley'S Comet, Visible Spectrum, Hydrogenation, Particle Mass, Space Environment Simulation

Scientific paper

Spacecraft and ground based observations of Halley's comet in the near IR have revealed an emission band around 3.4 μm. Laboratory samples of hydrogenated amorphous carbon grains (HAC) (diameter ≅ 80 Å) have shown a similar feature at 3.4 μm. In this paper the authors discuss the possibility that the band can be attributed to small HAC particles.

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