Mars Observer camera

The Mars Observer camera (MOC) is a three-component system (one narrow-angle and two wide-angle cameras) designed to take high spatial resolution pictures of the surface of Mars and to obtain lower spatial resolution, synoptic coverage of the planet's surface and atmosphere. The cameras are based on the “push broom” technique; that is, they do not take “frames” but rather build pictures, one line at a time, as the spacecraft moves around the planet in its orbit. MOC is primarily a telescope for taking extremely high resolution pictures of selected locations on Mars. Using the narrow-angle camera, areas ranging from 2.8 km × 2.8 km to 2.8 km × 25.2 km (depending on available internal digital buffer memory) can be photographed at about 1.4 m/pixel. Additionally, lower-resolution pictures (to a lowest resolution of about 11 m/pixel) can be acquired by pixel averaging; these images can be much longer, ranging up to 2.8 × 500 km at 11 m/pixel. High-resolution data will be used to study sediments and sedimentary processes, polar processes and deposits, volcanism, and other geologic/geomorphic processes. The MOC wide-angle cameras are capable of viewing Mars from horizon to horizon and are designed for low-resolution global and intermediate resolution regional studies. Low-resolution observations can be made every orbit, so that in a single 24-hour period a complete global picture of the planet can be assembled at a resolution of at least 7.5 km/pixel. Regional areas (covering hundreds of kilometers on a side) may be photographed at a resolution of better than 250 m/pixel at the nadir. Such images will be particularly useful in studying time-variable features such as lee clouds, the polar cap edge, and wind streaks, as well as acquiring stereoscopic coverage of areas of geological interest. The limb can be imaged at a vertical and along-track resolution of better than 1.5 km. Different color filters within the two wide-angle cameras permit color images of the surface and atmosphere to be made to distinguish between clouds and the ground and between clouds of different composition.

[1]  D. J. Milton,et al.  Geological framework of the south polar region of Mars. , 1972 .

[2]  R. Sharp Mars: Troughed terrain , 1973 .

[3]  James A. Cutts,et al.  Nature and origin of layered deposits of the Martian polar regions , 1973 .

[4]  M. Carr The volcanism of Mars , 1973 .

[5]  D. J. Milton Water and processes of degradation in the Martian landscape , 1973 .

[6]  B. White,et al.  Wind Tunnel Simulations of Light and Dark Streaks on Mars , 1974, Science.

[7]  Victor R. Baker,et al.  Paleohydraulic Interpretation of Quaternary Alluvium Near Golden, Colorado , 1974, Quaternary Research.

[8]  G. Hulme,et al.  The Interpretation of Lava Flow Morphology , 1974 .

[9]  Michael C. Malin,et al.  Channels on Mars , 1975 .

[10]  J. Pirraglia Martian Atmospheric Lee Waves , 1975 .

[11]  R. Greeley,et al.  Estimates of the wind speeds required for particle motion on Mars , 1976 .

[12]  Michael J. S. Belton,et al.  Cloud Patterns, Waves and Convection in the Venus Atmosphere , 1976 .

[13]  G. Briggs,et al.  Martian Dynamical Phenomena During June-November 1976: Viking Orbiter Imaging Results , 1977 .

[14]  Morphology of chasma walls, Mars , 1977 .

[15]  H. Masursky,et al.  Geology of the Valles Marineris: First analysis of imaging from the Viking 1 Orbiter Primary Mission , 1977 .

[16]  R. Greeley,et al.  Some Martian volcanic features as viewed from the Viking orbiters , 1977 .

[17]  R. Greeley,et al.  Martian impact craters and emplacement of ejecta by surface flow , 1977 .

[18]  J. McCauley,et al.  Geologic map of the Coprates Quadrangle of Mars , 1978 .

[19]  J. Veverka,et al.  Seasonal and secular variation of wind streaks on Mars - An analysis of Mariner 9 and Viking data , 1979 .

[20]  G. Briggs,et al.  Viking Orbiter imaging observations of dust in the Martian atmosphere , 1979 .

[21]  P. Mouginis-Mark Martian fluidized crater morphology: Variations with crater size, latitude, altitude, and target material , 1979 .

[22]  H. Kieffer,et al.  Thermal infrared properties of the Martian atmosphere: 3. Local dust clouds , 1979 .

[23]  J. Cutts,et al.  Evolution of Martian polar landscapes - Interplay of long-term variations in perennial ice cover and dust storm intensity , 1979 .

[24]  R. M. Henry,et al.  Frontal systems during passage of the Martian north polar hood over the Viking Lander 2 site prior to the first 1977 dust storm , 1979 .

[25]  J. Veverka,et al.  Frost streaks in the south polar cap of Mars , 1979 .

[26]  P. Gierasch,et al.  Spiral clouds on Mars - A new atmospheric phenomenon , 1979 .

[27]  J. Pollack,et al.  Properties and effects of dust particles suspended in the Martian atmosphere , 1979 .

[28]  Michael H. Carr,et al.  Formation of Martian flood features by release of water from confined aquifers , 1979 .

[29]  D. Pieri Martian valleys: morphology, distribution, age, and origin. , 1980, Science.

[30]  J. Burns,et al.  The astronomical theory of climatic change on Mars , 1980 .

[31]  J. L. Mitchell,et al.  Interaction of eddies and mean zonal flow on Jupiter as inferred from Voyager 1 and 2 images , 1981 .

[32]  J. Veverka,et al.  Classification of wind streaks on Mars , 1981 .

[33]  Yale Mintz,et al.  A Martian general circulation experiment with large topography , 1981 .

[34]  Victor R. Baker,et al.  Channels and valleys on Mars , 1983 .

[35]  P. Gierasch,et al.  Wind streaks on Mars: Meteorological control of occurence and mode of formation , 1981 .

[36]  Roger J. Yerdon,et al.  Global patterns in cloud forms on Mars , 1981 .

[37]  Verner E. Suomi,et al.  Cloud motions on Venus - Global structure and organization , 1981 .

[38]  S. Collins,et al.  Jovian winds from Voyager 2. I. Zonal mean circulation. , 1982 .

[39]  P. Christensen,et al.  Martian dust mantling and surface composition: Interpretation of thermophysical properties , 1982 .

[40]  Richard W. Zurek,et al.  Martian great dust storms: An update , 1982 .

[41]  C. Peterson A secondary origin for the central plateau of Hebes Chasma , 1982 .

[42]  Victor R. Baker,et al.  The Channels of Mars , 1982 .

[43]  P. Christensen Eolian intracrater deposits on Mars: Physical properties and global distribution , 1983 .

[44]  R. Kahn,et al.  The spatial and seasonal distribution of Martian clouds and some meteorological implications , 1984 .

[45]  G. Schubert,et al.  Zonal winds in the middle atmosphere of Venus from Pioneer Venus radio occultation data , 1984 .

[46]  R. Greeley,et al.  Martian crater dark streak lengths: explanation from wind tunnel experiments , 1984 .

[47]  P. Thomas,et al.  Martian intracrater splotches: Occurrence, morphology, and colors , 1984 .

[48]  P. Gierasch,et al.  Dust Devils on Mars , 1985, Science.

[49]  B. Jakosky The seasonal cycle of water on Mars , 1985 .

[50]  Ronald Greeley,et al.  Book Review: Wind as a geological process on earth, Mars, Venus and Titan. / CUP, 1985 (paperback edition 1987) , 1986 .

[51]  M. C. Malin,et al.  Design and development of the mars observer camera , 1991, Int. J. Imaging Syst. Technol..

[52]  MARS OBSERVER MISSION , 1992 .

[53]  G. Schubert,et al.  GENERAL CIRCULATION AND THE DYNAMICAL STATE OF THE VENUS ATMOSPHERE , 2022, Venus.