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WARNING: This section is long and very image intensive (135 scenes)

SECTION 19

PLANETARY REMOTE SENSING

Remote Sensing Techniques


Imaging remote sensing as applied to Earth goes back to the middle of the last century, when the first photos were taken from balloons. As applied to the rest of the solar system, one must look to the first observations (documented by sketches) made by Galileo in 1610 when he turned a telescope to the heavens and caught a glimpse of the surface complexities exhibited on our nearest neighbor, the Moon, and then later confirmed the Copernican Revolution with his discoveries of moons, or orbiting satellites, around Jupiter. Since then, first with telescopes and, after the opening of the Space Age, with orbiting spacecraft, flyby, probe, and lander missions to the Moon and the planets, most of the same instruments that survey the electromagnetic spectrum interacting with the Earth have been the principal tools used in exploring our planetary associates and beyond - searching well into outer space to look at stars and other members of the Universe. This is evident from this list of remote sensing methods depending on EM spectral measurements that have provided exceptional information about planetary surfaces, atmospheres, and, indirectly, interiors: *

METHOD EM SPECTRUM INFORMATION INTERPRETATION MISSION
Gamma-Ray Spectroscopy Gamma rays Gamma spectrum K, U, Th Abundances Apollo 15, 16: Venera
X-ray Fluorescence spectrometry X-rays Characteristic Wavelengths Surface mineral/ chemical comp. Apollo; Viking Landers
Ultraviolet Spectrometry UV Spectrum of Reflected sunlight Atmospheric Composition: H,He,CO2 Mariner; Pioneer; voyager
Photometry UV, Visible Albedo Nature of Surface; Composition Earth Telescopes; Pioneer
Multispectral Imagers UV, Visible, IR Spectral & Spatial Surface Features; Composition On most missions
Reflectance Spectrometers Visible, IR Spectral intensities of reflected solar radiation Surface Chemistry; mineralogy; processes Telescopes; Apollo
Laser Altimeter Visible Time delay between emitted & reflected pulses Surface Relief Apollo 15,16,17
Polarimeter Visible Surface Polarization Surface Texture; Composition Pioneer; Voyager
Infrared Radiometer (includes scanners) Infrared Thermal radiant intensities Surface & atmospheric temperatures; compos. Apollo; Mariner; Viking; Voyager
Microwave Radiometer Microwave Passive microwave emission Atmosphere/Surface temperatures; structure Mariner; Pioneer Venus
Bistatic Radar Microwave Surface reflection profiles Surface Heights; roughness Apollo 14,15,16; Viking
Imaging Radar Microwave Reflections from swath Topography & roughness Magellan; Earth systems
Lunar Sounder Radar Multifrequency Doppler Shifts Surface Profiling & imaging; conductivity Apollo 17
S-Band Transponder Radio Doppler shift single frequency Gravity data Apollo
Radio Occultation Radio Frequency & intensity change Atmospheric density & pressure Flybys  & Orbiters

* Adapted from Billy P. Glass, Introduction to Planetary Geology, 1982, Cambridge University, Press

This list is incomplete but is still highly representative. The Command and Service Module (CSM) on the Apollo lunar missions carried a complement of other instruments including alpha-particle spectrometers, mass spectrometers, magnetometers, far UV spectrometers, scintillometers, and others designed to make geochemical and geophysical measurements. The astronauts also deployed on-surface instruments for specific studies; among these were seismometers, magnetometers, gravimeters, solar wind gauges, cosmic ray detectors, heat flow probes, and laser ranging retroreflectors. However, in retrospect, sensors that produce images, especially photographs and the like, have provided the most direct and readily interpretible sets of data, and will continue to be a mainstay of future missions.


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Code 935, Goddard Space Flight Center, NASA
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Updated: 1999.03.15.