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Mars Exploration Program
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Dr. Bill Boynton
August 24, 2004
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NASA/JPL-Caltech
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A new map of Mars' gravity made with three NASA spacecraft is the most detailed to date, providing a revealing glimpse into the hidden interior of the Red Planet. Satellites always orbit a planet's...
Mars Gravity Map
This image shows two small tributaries, just east of where they join Shalbatana Vallis.
Shalbatana Vallis
This is a Mars Odyssey visible color image of an unnamed crater in western Arcadia Planitia (near 39 degrees N, 179 degrees E). The crater shows a number of interesting internal and external featur...
Western Arcadia Planitia
The dune field in this polar region crater looks like a stubby arrow pointing the way west. This unnamed crater is located in Planum Chronium.
Unnamed crater is located in Planum Chronium.
This view of an area about 140 kilometers (about 90 miles) wide in the Meridiani Planum region of Mars shows the region around NASA's Mars Exploration Rover Opportunity.
Orbital View of Opportunity's Region
How do you converse with a robot nearly one hundred million miles away? In this video, Odyssey team members describe communications with the 2001 Mars Odyssey spacecraft using the antennas of the D...
Challenges of Getting to Mars: Telecommunications
This image is near the southern edge of a low, broad volcanic feature called Syrtis Major.
Syrtis Major
Mars is experiencing large regional dust storms over its northern hemisphere during the past week.
The Martian Dust Storm of June 2018
Fans and ribbons of dark sand dunes creep across the floor of Bunge Crater in response to winds blowing from the direction at the top of the picture.
Mars Odyssey All Stars: Bunge Crater Dunes
Seen shortly after local Martian sunrise, clouds gather in the summit pit, or caldera, of Pavonis Mons, a giant volcano on Mars, in this image from the Thermal Emission Imaging System (THEMIS) on N...
Morning Clouds Atop Martian Mountain
This false-color map shows the area within Gale Crater on Mars, where NASA's Curiosity rover landed on Aug. 5, 2012 PDT (Aug. 6, 2012 EDT) and the location where Curiosity collected its first drill...
Location of John Klein Drill Site
This image shows the context for orbital observations of exposed rocks that had been buried an estimated 5 kilometers (3 miles) deep on Mars.
Nature's Drilling Exposes Deeply Buried Minerals
Color coding in this map of a far-northern site on Mars indicates the change in nighttime ground-surface temperature between summer and fall. This site, like most of high-latitude Mars, has water i...
Depth-to-Ice Map of an Arctic Site on Mars
This image from NASA's Mars Odyssey shows ice-rich clouds over the summit of Arsia Mons.
Ice-Rich Clouds - False Color
This movie shows three views of the Martian moon Phobos as viewed in visible light by NASA's 2001 Mars Odyssey orbiter. The apparent motion is due to movement by Odyssey's infrared camera, Thermal ...
Odyssey's Three Views of Phobos in Visible Light
This computer-generated view based on multiple orbital observations shows Mars' Gale crater as if seen from an aircraft north of the crater.
Oblique view of Gale Crater from the North (Unannotated)
Just as on Earth, volcanism and tectonism are found together on Mars. Here is an example: the ridges and fractures of Claritas Fossae are affecting or perhaps hosting the volcanic flows of Solis Pl...
Volcanism & Tectonism
On the southwest edge of the immense volcanic region of Tharsis, lava from its giant volcanoes flowed down to meet the old cratered landscape of Terra Sirenum.
Terra Sirenum
Artist’s concept of Comet Siding Spring approaching Mars, shown with NASA’s orbiters preparing to make science observations of this unique encounter.
NASA's Mars Orbiters Maneuvers as Comet Siding Spring Approaching Mars
This computer-generated view based on multiple orbital observations shows Mars' Gale crater as if seen from an aircraft north of the crater.
Oblique view of Gale Crater from the North
This image superimposes Gamma-Ray Spectrometer data from NASA's Mars Odyssey orbiter onto topographic data from the laser altimeter on NASA's Mars Global Surveyor.
Potassium Concentrations on Mars
This mosaic of day and night infrared THEMIS images shows landslides flowed over 100 kilometers (62 miles) across the floor of Melas Chasma.
mosaic of day and night infrared THEMIS
The channels in this VIS image are part of Tyrrhena Fossae on the northern flank of Tyrrhenus Mons.
Tyrrhena Fossae
Large fractures have formed 'steps' in this region of Tempe Terra.
Tempe Terra
Interact with this 3D model of Mars Odyssey.
Mars Odyssey Orbiter, 3D Model
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