Regression of Martian North Polar Cap: 1990-1997 Hubble Space Telescope Observations

Details Regression of Martian North Polar Cap: 1990-1997 Hubble Space Telescope Observations Regression of Martian North Polar Cap: 1990-1997 Hubble Space Telescope Observations

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998icar..136..175c&link_type=abstract

Icarus, Volume 136, Issue 2, pp. 175-191.

Physics

Optics

16

Scientific paper

Hubble Space Telescope imaging of Mars from December 13, 1990, through April 17, 1997, has resulted in the synoptic monitoring of parts of four consecutive martian north polar cap regressional cycles spanning L_s = 335.65 deg to L_s = 144.56 deg. The 1990-1993 observations were obtained with the Wide Field Planetary Camera 1 (WFPC1) instrument while subsequent observations from 1994 to 1997 were obtained with the improved optics of the Wide Field Planetary Camera 2 (WFPC2). Mars observations were obtained from the ultraviolet (218 nm) to the near-infrared (1042 nm), which has allowed us to constrain the effects of clouds and dust particulates on cap edge measurements. HST observations of the polar cap regressions after L_s = 0 deg are fairly consistent from year to year with some variations possible before L_s = 0 deg. The 1991 observations at L_s = 35.25 deg and L_s = 59.88 deg in the longitude range 270 deg-280 deg possibly support a standstill in cap retreat at a latitude 70 degN. The standstill in cap retreat reported in previous years at a latitude 67 degN was not observed in 1992-1997. Comparison with previous ground-based and spacecraft observations suggests that interannual variations may be significant; they may be due to interannual atmospheric changes such as global dust storm activity. Lambert albedos of the north polar cap in red and violet bandpasses are similar to those reported before.

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