Posts Tagged ‘JPL’

The following pictures and details were posted on NASA’s website.


These images show a very young lunar crater on the side of the moon that faces away from Earth, as viewed by NASA’s Moon Mineralogy Mapper on the Indian Space Research Organization’s Chandrayaan-1 spacecraft. On the left is an image showing brightness at shorter infrared wavelengths. On the right, the distribution of water-rich minerals (light blue) is shown around a small crater. Both water- and hydroxyl-rich materials were found to be associated with material ejected from the crater.

Credits: ISRO/NASA/JPL-Caltech/USGS/Brown Univ.




This image of the moon is from NASA’s Moon Mineralogy Mapper on the Indian Space Research Organization’s Chandrayaan-1 mission. It is a three-color composite of reflected near-infrared radiation from the sun, and illustrates the extent to which different materials are mapped across the side of the moon that faces Earth.
Small amounts of water and hydroxyl (blue) were detected on the surface of the moon at various locations. This image illustrates their distribution at high latitudes toward the poles.
Blue shows the signature of water and hydroxyl molecules as seen by a highly diagnostic absorption of infrared light with a wavelength of three micrometers. Green shows the brightness of the surface as measured by reflected infrared radiation from the sun with a wavelength of 2.4 micrometers, and red shows an iron-bearing mineral called pyroxene, detected by absorption of 2.0-micrometer infrared light.

Image credit: ISRO/NASA/JPL-Caltech/Brown Univ./USGS



These graphs show detailed measurements of light as a function of color or wavelength. The data, called spectra, are used to identify minerals and molecules. On the left are spectra of lunar rocks, minerals and soil returned to Earth by NASA’s Apollo missions, taken in the visible to shorter-wavelength infrared range. The blue bar shows where a dip in the light is expected due to the presence of water and hydroxyl molecules. To the left are model spectra for pure water (H2O) and hydroxyl (OH-).

Image credit: ISRO/NASA/JPL-Caltech/Brown Univ.



These images from NASA’s Moon Mineralogy Mapper on the Indian Space Research Organization’s Chandrayaan-1 spacecraft show data for the hemisphere of the moon that faces Earth. The image on the left shows albedo, or the sunlight reflected from the surface of the moon. The image on the right shows where infrared light is absorbed in the characteristic manner that indicates the presence of water and hydroxyl molecules. That image shows that signature most strongly at the cool, high latitudes near the poles. The blue arrow indicates Goldschmidt crater, a large feldspar-rich region with a higher water and hydroxyl signature.

Image credit: ISRO/NASA/JPL-Caltech/Brown Univ.



Many small, fresh craters bear signatures of water and hydroxyl, which are detected as absorptions of infrared light in the range of 3 micrometers by NASA’s Moon Mineralogy Mapper. Figure A, on the left, shows feldspar-rich terrain on the side of the moon facing away from Earth. The arrows point to the location of small, fresh craters. Figure B, on the right, indicates the reflectance as a function of wavelength for craters in Figure A. The water and hydroxyl signature in these regions is seen as a characteristic dip in reflectance in the infrared light near the 3-micrometer range, a region noted with a light-blue band. The dashed line shows background soil that doesn’t contain significant water or hydroxyl.

Image credit: ISRO/NASA/JPL-Caltech/Brown Univ.