The MSI will provide information on both physical geology and on mineralogical composition, by measuring the spectrum of reflected sunlight. This instrument will be able to resolve features smaller than 10 meters in size. This means it could also detect satellites, minor objects such as moons, orbiting Eros. In addition, the MSI will serve as one of the tools to provide information necessary to calculate the density of Eros, by providing imagery that will be used to estimate the asteroid's volume. Other information needed for this computation is the mass of Eros, which will be determined from the orbital period (from the radio science experiment), attitude data from the star camera, and altitude data from the Laser Rangefinder.
![[Picture of the MSI]](MSI2.gif)
Lesson Plans on Remote
Sensing
Lesson Plans on the
Electromagnetic Spectrum
MSI
Overview on NEAR Web
Server
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Contact Steve Bowser (slbowser@umd5.umd.edu)
or Joy Maloney (jmaloney@umd5.umd.edu) for further information. |