GLOBAL IMAGING OF MARS BY HUBBLE-SPACE-TELESCOPE DURING THE 1995 OPPOSITION

Hubble space telescope (HST) imaging of Mars near the 1995 opposition resulted in excellent synoptic-scale images of the planet during the s pring season in the northern hemisphere. Because this season coincides with the aphelion position of Mars in its orbit, it is therefore the most difficult for ground based observation because of the relatively small angular size of Mars. This is the first sequence of images fully utilizing the capability of the new Planetary Camera to produce globa l synoptic images of the planet. The images reveal bright, discrete cl ouds associated with topographic features superimposed on a zonal band of condensate clouds between latitudes -10 degrees and 30 degrees; th e maximum violet optical depth of the cloud band is about 0.3. In a fe w instances, the appearance of clouds beyond the morning terminator ca n be used to infer cloud heights of roughly 8 km. A large, dark albedo feature in the Cerberus region, observed for many years by ground-bas ed observers, has almost disappeared in the 1995 HST images. Other asp ects of Mars, such as the north polar cap, appear much as they did dur ing previous oppositions. Although cloudy regions were observed by spa cecraft during this season, the HST images uniquely reveal the global extent of significant optical depth clouds.