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Science 14 July 1967:
Vol. 157. no. 3785, pp. 193 - 195
DOI: 10.1126/science.157.3785.193
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Articles

Bistatic-Radar Detection of Lunar Scattering Centers with Lunar Orbiter I

G. L. Tyler 1, V. R. Eshleman 1, G. Fjeldbo 1, H. T. Howard 1, and A. M. Peterson 1

1 Center for Radar Astronomy, Stanford University, Stanford, California 94305

Continuous-wave signals transmitted from Lunar Orbiter I have been received on Earth after they have been reflected from the surface of the moon. The frequency spectrum of the reflected signals is used to locate discrete, heterogeneous, scattering centers on the lunar surface. The scattering centers are probably distinguished from the surrounding terrain by a higher surface reflectivity. Continuous-wave bistatic radar could provide an important new method for the study and mapping of planetary surfaces.


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Radar Astronomy: Rotation rates of Venus and Mercury and density of the atmosphere of Mars are recent radar discoveries.
V. R. Eshleman (1967)
Science 158, 585-597
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