Astronomy and Astrophysics – Astronomy
Scientific paper
May 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994metic..29..394h&link_type=abstract
Meteoritics, vol. 29, no. 3, p. 394-396
Astronomy and Astrophysics
Astronomy
39
Grain Size, Meteorites, Mineralogy, Regolith, Spectral Reflectance, Spectrum Analysis, Surface Properties, Vesta Asteroid, Albedo, Comparison, Estimates, Graphs (Charts), Spatial Distribution
Scientific paper
The grain-size distribution of the regolith of asteroid 4 Vesta has been estimated by comparing its reflectance spectra (0.3-2.6 microns) with those of HED meteorites. The finest grain-size separate (less than 25 micrometers) of a particular howardite has a reflectance spectrum most similar to Vesta's. In order to better simulate Vesta's surface mineralogy, reflectance spectra of those finest HED meteorite powders were linearly combined, and Vesta's spectrum was scaled for the best fit between them. Both the albedo and the shape of reflectance spectrum of Vesta were well reproduced by regional mixtures of the finest (less than 25 micrometers) powders of HED meteorites. The result suggests the heterogeneity of Vesta's surface and provides an estimate of the visible reflectance of Vesta that is close to its Infrared Astronomical Satellite (IRAS) albedo. Thus, this suggests that fine grains can be generated and retained by relatively small bodies (Vesta is approximately 500 km in diameter).
Hiroi Takahiro
Pieters Carlé M.
Takeda Hiroshi
No associations
LandOfFree
Grain size of the surface regolith of asteroid 4 Vesta estimated from its reflectance spectrum in comparison with HED meteorites 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 Grain size of the surface regolith of asteroid 4 Vesta estimated from its reflectance spectrum in comparison with HED meteorites, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Grain size of the surface regolith of asteroid 4 Vesta estimated from its reflectance spectrum in comparison with HED meteorites will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-887815