Stellar Occultation Observations of Saturn's North-Polar Temperature Structure

Details Stellar Occultation Observations of Saturn's North-Polar Temperature Structure Stellar Occultation Observations of Saturn's North-Polar Temperature Structure

1997-12-09

arxiv.org/abs/astro-ph/9712122v1

Icarus 132 (1998) 298

Astronomy and Astrophysics

Astrophysics

27 pages, 8 figures, Icarus in print

Scientific paper

10.1006/icar.1998.5901

We have observed a stellar occultation of GSC5249-01240 by Saturn's north polar region on November 20, 1995 from NASA's Infrared Telescope Facility (IRTF). This is the first recorded occultation by the polar region of a giant planet. The occulted region extends 88 km in vertical height and 660 km in horizontal length, over a region from 82.5 to 85 degrees in planetocentric latitude and from 20 to 30 degrees in planetocentric longitude. Based on isothermal model fits to the light curve, we find an equivalent temperature of 130 \pm 10 K at a pressure level of 1.6 \pm 0.1 \mubar, which corresponds to a half-light latitude of 83.2 \pm 0.2 degrees and longitude of 24.1 \pm 0.5 degrees. Using numerical inversion procedures, we have retrieved the temperature profile of the occulted region, which suggests an increase in temperature (with radius) of 14.5 K between 6 and 10 \mubar. We also find temperature fluctuations of 1 to 5 K along the path probed by the occultation; if the observed temperature gradients of these fluctuations apply to the vertical direction only, then this region is super-adiabatic. More likely these thermal gradients are due to a combination of diffractive scintillations and horizontal temperature variations. Given that isothermal model fits and numerical inversions cannot separate individual contributions to observed temperature fluctuations, such as from vertical variations, horizontal variations, and scintillations, this occultation requires a further study.

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