Detection of lambda = 2 CM emission from minor planet 704 Interamnia

Astronomy and Astrophysics – Astronomy

Scientific paper

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Asteroids, Microwave Emission, Planetary Radiation, Superhigh Frequencies, Brightness Temperature, Centimeter Waves, Continuous Spectra, Gray Scale, Radiant Flux Density, Asteroids, Interamnia, Emissions, Centimeter Waves, Flux, Density, Dust, Temperature, Size, Diameter, Surface, Composition, Depth, Comparisons, Radio Methods, Earth-Based Observations, U Asteroids, Spectra, Eunomia, S Asteroids, Physical Properties, Astronomy

Scientific paper

Results are presented from a study of the 2 cm natural radio emissions from the class U asteroid 704 Interamnia. The study was performed with the NRAO VLA using 26 antennas in a compact hybrid configuration with base lengths from 0.1-2.2 km. The IF scans were centered at 14.97 GHz and 14.92 GHz. A brightness temperature plot is provided for 2 AU distance, assuming a 338 km diam for the asteroid. The scans revealed a surface dust layer at least 3 cm thick. Comparisons with spectra of 15 Eunomia, another rapidly rotating minor planet with a similar diameter reveals that this second object also has a surface dust layer a few centimeters thick.

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