PIA14852: Mercury's High-Potassium Diet
Target Name: Mercury
Is a satellite of: Sol (our sun)
Mission: MESSENGER
Spacecraft: MESSENGER
Instrument: Gamma-Ray and Neutron Spectrometer (GRNS)
Product Size: 5333 x 3000 pixels (width x height)
Produced By: Johns Hopkins University/APL
Full-Res TIFF: PIA14852.tif (48 MB)
Full-Res JPEG: PIA14852.jpg (646.7 kB)

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Original Caption Released with Image:

The abundance of potassium (K) and thorium (Th) on the surface of Mercury as measured by the MESSENGER Gamma-Ray Spectrometer. These values are compared to similar measurements of the K and Th content of Venus, Earth, the Moon, and Mars. Because K is a volatile element and Th a refractory one, this ratio is a sensitive measure of thermal processes that fractionate elements by volatility. For example, the ratio for the Moon (360) is much lower than that for Earth (3000), reflecting volatile loss during the Moon's formation by a giant impact. The ratio for Mercury is comparable to that of the other terrestrial planets, indicating that Mercury is not highly depleted in volatile elements, ruling out some models for its formation and early history. This finding is supported by the identification of sulfur on the surface by the MESSENGER X-Ray Spectrometer.

Date Presented: September 29, 2011, at a NASA Press Briefing
Instrument: Gamma Ray Spectrometer (GRS)

These images are from MESSENGER, a NASA Discovery mission to conduct the first orbital study of the innermost planet, Mercury. For information regarding the use of images, see the MESSENGER image use policy.

Image Credit:
Courtesy AAAS/Science

Image Addition Date:
2011-09-29