Composition of the Martian dust as derived by infrared spectroscopy from Mariner 9

Details Composition of the Martian dust as derived by infrared spectroscopy from Mariner 9 Composition of the Martian dust as derived by infrared spectroscopy from Mariner 9

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jgr....80.4925a&link_type=abstract

Journal of Geophysical Research, vol. 80, Dec. 10, 1975, p. 4925-4931.

Statistics

Computation

6

Dust Storms, Infrared Spectroscopy, Mars (Planet), Spectral Reflectance, Absorption Cross Sections, Brightness Temperature, Feldspars, Mariner 9 Space Probe, Mica, Optical Properties, Particle Size Distribution, Scattering Cross Sections, Silicates

Scientific paper

The Martian dust spectra obtained by the infrared interferometer spectrometer (Iris) experiment on Mariner 9 have been compared with modeling computations for various minerals and rocks. The model used was based upon a recently developed theory of absorption and scattering by particulate materials. The results indicate that the composition of Martian dust is biased toward silicate structures which involve a high degree of silicate oxygen sharing. A feldspar-rich dust of approximately 1-micron particle size appears to be the best candidate, although sheet-structure silicates cannot be ruled out.

Affiliated with

Also associated with

No associations

Rating

Composition of the Martian dust as derived by infrared spectroscopy from Mariner 9 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Composition of the Martian dust as derived by infrared spectroscopy from Mariner 9, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Composition of the Martian dust as derived by infrared spectroscopy from Mariner 9 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1578322