Observations of Phobos, Deimos, and bright stars with the Imager for Mars Pathfinder

Details Observations of Phobos, Deimos, and bright stars with the Imager for Mars Pathfinder Observations of Phobos, Deimos, and bright stars with the Imager for Mars Pathfinder

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999jgr...104.9055t&link_type=abstract

Journal of Geophysical Research, Volume 104, Issue E4, p. 9055-9068

Mathematics

Logic

8

Planetology: Solar System Objects: Martian Satellites, Planetology: Comets And Small Bodies: Surfaces And Interiors, Planetology: Solid Surface Planets: Atmospheres-Structure And Dynamics, Planetology: Solar System Objects: Mars

Scientific paper

The Imager for Mars Pathfinder (IMP) was used to observe several objects during the Martian night. The satellites, Phobos and Deimos, were observed on two occasions each, through the IMP geological filters covering the wavelength range 440 nm to 1 μm. The observations were converted to geometric albedo using triaxial ellipsoid models of the satellites and phase functions derived from Viking Orbiter images. The spectral slopes over the full wavelength range were 7.9(+/-0.5)% (100 nm)-1 and 9.6(+/-0.6)% (100 nm)-1, respectively, referenced to 600 nm. In the Deimos spectra, some evidence for decreased reddening toward the trailing hemisphere was found. The geometric albedoes of Phobos and Deimos were found to be 0.065 (+/-0.09) and 0.068 (+/-0.009), respectively, averaged over 440 and 600 nm, in good agreement with previous measurements. The nighttime optical depth was investigated using observations of stars. A mean value of 0.56 (+/-0.09) was determined from measurements at different airmass. A possible maximum in the optical depth near 0200 local time was found, which may result from condensation during the night. A measurement of the egress of Phobos from eclipse was made. Modeling of the light curve gave a scale height for the scatterers of 10-15 km. The exact time of the eclipse reappearance over the limb could be reconstructed from the measurements and was in reasonable accord with predictions, although a small modification to the predicted position of Phobos of 6.8 (+/-6.0) km would have produced better agreement.

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