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Mercury's Sodium Tail
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Mercury's Sodium Tail
Release Date: January 30, 2008
Topics: MASCS, Mercury Flyby 1, NASA Press Conference 1/30/2008



This plot shows the intensity of emission of light associated with sodium atoms in the vicinity of Mercury. The observations were made with the Ultraviolet and Visible Spectrometer (UVVS) section of the Mercury Atmospheric and Surface Composition Spectrometer (MASCS). The intensity (up to 40 kiloRayleighs) indicates the relative abundance of material, in this case sodium atoms, along the observational line of sight back to the spacecraft. While sodium from Mercury has been observed with Earth-based telescopes, this is the highest-spatial-resolution image ever made. The geometry and observing circumstances have to be disentangled to infer the true spatial distribution, but the observations do confirm a north-south asymmetry that has previously been observed in ground-based sodium images.

The sodium emission is at 589 nm (in the visible part of the spectrum and the same wavelength, or color, as in sodium lamps and street lights on Earth). Because sodium atoms have intense emission, they are easy to detect, and this makes sodium a good tracer for other volatile elements in Mercury’s exosphere.

Credit: NASA/University of Colorado/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington


For information regarding the use of MESSENGER images, see the image use policy.


   

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