PIA00949: Magnetic Sources in the Crust of Mars
 Target Name:  Mars
 Is a satellite of:  Sol (our sun)
 Mission:  Mars Global Surveyor (MGS)
 Spacecraft:  Mars Global Surveyor Orbiter
 Instrument:  Magnetometer 
 Product Size:  715 x 572 pixels (w x h)
 Produced By:  Goddard Space Flight Center
 Producer ID:  MRPS84979
 Addition Date:  1997-10-13
 Primary Data Set:  MGS EDRs
 Full-Res TIFF:  PIA00949.tif (360.8 kB)
 Full-Res JPEG:  PIA00949.jpg (50.93 kB)

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Original Caption Released with Image:

This is a simple schematic representation of localized magnetic sources in the crust of Mars, buried beneath the surface, and revealed by observation of the magnetic field (blue) extending up to satellite altitude (about 120 kilometers). Most of our close passes to date - for which we have data - reveal the presence of one or more magnetic anomalies close to the path of the spacecraft. Since the sources must be close to the path of the satellite, we can only infer that the crust of Mars is strewn with similar magnetic anomalies, awaiting discovery. Where we can obtain enough data - that is to say, spaced more or less evenly in longitude with a spacing comparable to our periapsis altitude - we can construct a detailed image of the magnetic state of the Martian crust. We can then perhaps learn about the history of the now-extinct early Mars dynamo and the evolution of the surface of Mars.

The Jet Propulsion Laboratory's Mars Surveyor Operations Project operates the Mars Global Surveyor spacecraft with its industrial partner, Lockheed Martin Astronautics, from facilities in Pasadena, CA and Denver, CO. JPL is an operating division of California Institute of Technology (Caltech).

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