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At least 721 records · Page 40

Infrared instrumentation in space exploration.

IR spectrometers, radiometers, horizon sensors, rotating-prism planet-seekers and detector cooling using solid cryogens, for use in high altitude rockets and Earth satellites

ROCKET INSTRUMENTATION↗

Optimized silicon solar cells for space exploration power systems

A program is described aimed at designing and fabricating improved silicon solar cells for a range of missions extending from 0.1 to 15 astronomical units (Mercury to Jupiter). For missions lying inside Earth radius (Mercury, Venus) the major cell property required was very low series resistance, allowing high curve fill factor to be maintained at the higher intensities. For the Mercury mission, the temperature of the cell had to be kept low. This was achieved by reflecting more of the incident sunlight by use of large area front contacts. For the outer missions (Mars, the Asteroid belts and Jupiter) the formation of a Schottky barrier at the back contact had to be avoided (by use of a P+ layer under the back contact) and the excess leakage current of the PN junction had to be reduced. Optimum grid patterns were also derived and used for these missions.

Iles, P. A.↗

Robots in space exploration

A brief outline of NASA's current robotics program is presented. Efforts are being concentrated on a roving surface vehicle for Mars exploration. This vehicle will integrate manipulative, locomotive, and visual functions and will feature an electromechanical manipulator, stereo TV cameras, a laser rangefinder, a minicomputer, and a remote off-line computer. The program hinges on the iterative development of complex scenarios describing the robot's mission and the interrelationships among its various subsystems.

Dobrotin, B. M.↗

Space exploration and the history of solar-system volatiles

The thermochemical history of volatile substances in all solar-system planets, satellites, and planetoids is discussed extensively. The volatiles are viewed as an interface between the abiotic and biotic worlds and as a key to the history of bodies of the solar system. A flowsheet of processes and states is exhibited. Differences in bulk volatiles distribution between the planetary bodies and between the interior, surface, and atmosphere of each body are considered, as well as sinks for volatiles in degassing. The volatiles-rich Jovian and Saturnian satellites, the effect of large-planet magnetosphere sweeps on nearby satellites, volatiles of asteroids and comets, and the crucial importance of seismic, gravity, and libration data are treated. A research program encompassing analysis of the elemental and isotopic composition of rare gas in atmospheres, assay of volatiles-containing phases in regoliths, and examination of present or past atmospheric escape/accretion processes is recommended.

Fanale, F. P.↗