12/29/2023 0 Comments Image face of mars![]() This graph shows altimeter results from Mars Global Surveyor of other volcanoes of Mars on the Tharsis Ridge. This graph shows altimeter results from Mars Global Surveyor of the size difference between the two hemispheres of Mars (northern vs southern). This graph shows altimeter results from Mars Global Surveyor of other volcanoes of Mars. This graph shows altimeter results from Mars Global Surveyor of the size of Olympus Mons. The sequence shows the water clouds moving across the face of Mars. This graph shows proof of the existence of clouds of water on Mars. The scale to the left shows that purple regions are the coldest, about -170 degrees F (140K), while the yellow areas are the warmest at about 17 degrees F (270K). This image shows temperature data from the surface of the planet. Red areas are the warmest at about 30 degrees F (270K). The purple regions are the coldest, about -200 degrees F (140K), while the This image illustrates the global magnetic field of Mars. This image illustrates the Martian magnetosphere & its interaction with the solar wind. This image illustrates surface magnetic fields of Mars. This image also illustrates the process of aero-braking. This image illustrates one way in which the magnetometer instrument studies the planet. This image shows a portion of the Labyrinthus Noctis region on Mars. This image shows a portion of the Nirgal Vallis region on Mars. This image shows a portion of the Schiaparelli region on Mars. (Courtesy Malin Space Science Systems - 153K) This is image shows flow ejecta of a crater on Icaria Planum. (Courtesy Malin Space Science Systems - 142K) (Courtesy Malin Space Science Systems )Ĭomplex floor deposits within the western Ganges Chasma. This is an image of the Medusae Fossae region. This is an image of West Tithonium Chasma, on the western edge of Valles Marineris. This is an image of layered terrain in the south polar region, and a potential Mars '98 landing site. Vallis, one of the Martian valley systems cutting throughĬratered plains in the Xanthe Terra region of Mars. Orbiter Camera during the 87th orbit around Mars of the This picture of a canyon on the Martian surface was obtained aįew minutes after 10 PM PST, January 8, 1998, by the Mars The outline of the next image is shown as a Viking Orbiter 1 frame 897A32, reproduced at a scale of 150 Steep slopes within the Valles Marineris. Seen in this view are a plateau and surrounding Shortly after the Mars Global Surveyor spacecraft began it'sĨ0th orbit. Of the Martian surface was obtained in the earlyĮvening of January 1, 1998, by the Mars Orbiter Camera ![]() The outline of the next image is shown as a white box. Mosaic of Viking Orbiter 1 frames 428A62,Ĥ28A63, and 428A65, reproduced at a scale of 80 meters/pixel The outlines of other images are shown as white boxes. Survey Mars Digital Image Mosaic, reproduced at a scale of 230 Viewing of this image in high resolution is recommended. Some of these regions are shown below at higher resolution. This is a labeled map showing regions imaged by Mars Global Surveyor early in the mission.
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