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Radar detection of phobos.

S J Ostro, R F Jurgens, D K Yeomans

    Science (New York, N.Y.)
    |March 24, 1989
    PubMed
    Summary
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    Radar studies reveal Phobos

    Area of Science:

    • Planetary Science
    • Radar Astronomy
    • Small Body Characterization

    Background:

    • Phobos, Mars' largest moon, is a key target for understanding small solar system bodies.
    • Previous studies on Phobos' surface properties have been limited.
    • Radar observations offer a unique method to probe subsurface characteristics.

    Purpose of the Study:

    • To investigate the surface properties of Phobos using radar echoes.
    • To determine the physical characteristics of Phobos' regolith.
    • To compare Phobos' radar signature with other small solar system objects.

    Main Methods:

    • Analysis of radar echoes from Phobos at a 3.5-cm wavelength.
    • Measurement of Phobos' radar albedo, polarization ratio, and echo spectral shape.

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  • Comparison of Phobos' radar signature with data from asteroids and the Moon.
  • Main Results:

    • Phobos exhibits a smoother surface than the Moon at centimeter-to-decimeter scales.
    • The mean bulk density of Phobos' uppermost regolith is approximately 2.0 g cm(-3).
    • Phobos' radar signature is distinct from Earth-approaching objects but similar to large C-class asteroids.

    Conclusions:

    • Phobos' surface and shallow subsurface share characteristics with mainbelt asteroids.
    • Radar data suggests Phobos may have a different origin or evolutionary path than previously assumed.
    • Further radar studies can refine our understanding of Phobos' composition and history.