Hubble reveals potential titanium oxide deposits at Aristarchus and Schroter's Valley Rille

This view of the lunar impact crater Aristarchus and adjacent features (Herodotus crater, Schroter's Valley rille) illustrates the ultraviolet and visible wavelength characteristics of this geologically diverse region of the Moon. The two inset images illustrate one preliminary approach for isolating differences due to such effects as composition, soil maturity, mixing, and impact ejecta emplacement. The colour composite in the lower right focuses on the 26-mile-diameter (42-kilometer-diameter) Aristarchus impact crater, and employs ultraviolet- to visible-color-ratio information to accentuate differences that are potentially diagnostic of ilmenite- (i.e, titanium oxide) bearing materials as well as pyroclastic glasses.

Credit:

NASA, ESA and J. Garvin (NASA/GSFC)

About the Image

NASA press release
Id:opo0529b
Type:Collage
Release date:19 October 2005, 19:00
Size:3000 x 2400 px

About the Object

Name:Moon
Type:Solar System : Planet : Satellite : Feature : Surface
Category:Solar System

Image Formats

r.titleLarge JPEG
878.7 KB
r.titleScreensize JPEG
232.9 KB

Colours & filters

BandWavelengthTelescope
Ultraviolet
Mid-UV
250 nm Hubble Space Telescope
ACS
Ultraviolet
Near-UV
344 nm Hubble Space Telescope
ACS
Optical
V
502 nm Hubble Space Telescope
ACS
Optical
R
658 nm Hubble Space Telescope
ACS

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