The University of Arizona

HiRISE Team Begins Releasing a Flood of Mars Images Over the Internet

By Lori Stiles, November 22, 2006

Russell crater -- This view of Russell crater is among the HiRISE views of Mars being released today. Russell crater sand dunes are carved by gullies that possibly form when carbon dioxide or water frost in the dunes is heated by sunlight, triggering avalanches of flowing sand. (Photo: NASA/JPL/University of Arizona)
Russell crater -- This view of Russell crater is among the HiRISE views of Mars being released today. Russell crater sand dunes are carved by gullies that possibly form when carbon dioxide or water frost in the dunes is heated by sunlight, triggering avalanches of flowing sand. (Photo: NASA/JPL/University of Arizona)

The University of Arizona-based team that operates the high-resolution camera on NASA's Mars Reconnaissance Orbiter, in conjunction with NASA, is releasing the first of what will be a non-stop flood of incredibly detailed Mars images taken during the spacecraft's two-year primary science mission.

The High Resolution Science Imaging Experiment (HiRISE) camera took almost 100 images during the first two weeks of its main science mission, which began Nov. 7.

"There's no Earth analog for some places we see, while other places look remarkably like Earth," said Professor Alfred S. McEwen of UA's Lunar and Planetary Laboratory, HiRISE principal investigator. "The details we're seeing are just fantastic."

The HiRISE team is posting about 15 of the new large images on the HiRISE Website http://hiroc.lpl.arizona.edu today. Last week, they added more than a dozen new Mars images, as well as reprocessed images, taken from low orbit during test imaging in early October. The team plans to release the latest HiRISE images on their Website every Wednesday.

The views released today show seemingly endless fields of sand dunes, including some carved by gullies that possibly form when carbon dioxide or water frost in the dunes is heated by sunlight, triggering avalanches of flowing sand. Other HiRISE images show layered arid terrains that resemble landscapes protected as national parks on our own planet, and a fossil delta inside a crater that once held a lake. HiRISE images resolve meter-sized blocks within the delta channel that may be blocks of sand and gravel carried along as the channels eroded.

HiRISE images also capture numerous impact craters, including Endurance crater that NASA's Opportunity rover explored for ten months of its now nearly 3-year mission. Details visible in the HiRISE image of Opportunity's landing site show the parachute lying on the Martian surface, Opportunity's heat shield at a different location, and the lander itself on the floor of the small impact crater where the airbag came to a stop.

Other images show layered polar terrains that likely record Martian climate changes, and also polygon-patterned northern plains regions that are among candidate landing sites for the Phoenix Lander spacecraft in 2008.

"You see stuff at this level of detail and you want to see more," said Candy Hansen of the Jet Propulsion Laboratory, a HiRISE co-investigator who has helped lead imaging operations at the HiRISE Operations Center (HiROC) during the first weeks of the science mission this month.

"These images are at a geologist's scale," Hansen said. "A geologist could hike the terrain seen in the width of one of our images, six kilometers, in a day. These images bring the planet down to scales that match our own human level of experience, and that's a big help with interpretation."

The HiRISE camera takes images of 3.5-mile-wide (6 kilometer) swaths as the orbiter flies at about 7,800 mph between 155 and 196 miles (250 to 316 km) above the planet. The camera resolves geologic features as small as 40 inches across.

"It's been a constant race to look at all these images while we're planning our future targets," McEwen said. "But it's important to examine the data so we can learn how to use the best possible settings, and make decisions about which targets we'll need to get in stereo or color."

HiRISE began a new imaging cycle last week (Nov. 19) and begins another next week (Dec. 3). Over the next couple of weeks, the camera is targeting "all the easy-to-find hardware on Mars," McEwen said. That includes NASA's rover Spirit, the Viking 1 and Viking 2 landers, and Mars Pathfinder.

McEwen has been working a 12-hour day, seven days a week this month. The rest of the team has been clocking major overtime, too.

"We're trying not to get people too burned out, but we have to keep up. We're going to get about a hundred new images every two weeks without a break," McEwen said. "The spacecraft doesn't take Thanksgiving or Christmas off."

Information about the Mars Reconnaissance Orbiter is online at http:// www.nasa.gov/mro. The mission is managed by NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology, Pasadena, for the NASA Science Mission Directorate, Washington. Lockheed Martin Space Systems, Denver, is the prime contractor and built the spacecraft. The High Resolution Imaging Science Experiment is operated by the University of Arizona. Ball Aerospace and Technology Corp., Boulder, Colo., built the HiRISE instrument.

IMAGES AND CAPTIONS:

  • Russell Crater
    Hundreds of enigmatic small troughs are seen to carve into the slopes of these dark sand dunes lying within Russell Crater on Mars. These features were previously identified as gullies in images from the Mars Orbiter Camera on Mars Global Surveyor, but the higher resolution HiRISE image brings out many new details and mysteries. The troughs extend from near the top of the dunes to their bases, indicating that some fluid material carved into the sand. The troughs commonly begin as smaller tributaries joined together, suggesting several sources of fluid. Distinct dark spots are located near where the troughs seem to originate. Several troughs appear to begin at alcoves. Several of these troughs have sinuous middle reaches whereas others are straighter. Further down slope, some trough edges appear elevated above the surrounding terrain, particularly in the lower reaches. The troughs seem to terminate abruptly, with no deposition of material, unlike at the bases of some other gullies on Mars that are not on dunes. One hypothesis for the origin of these troughs, which has been previously been proposed by the MOC team, is that CO2 (or maybe H2O) frost is deposited on the dunes in shadows or at night. Some frost may also be incorporated into the internal parts of the dunes due to natural avalanching. When the frost is eventually heated by sunlight, rapid sublimation triggers an avalanche of fluidized displaced sand, forming a gully. HiRISE will continue to target small trough features such as these and may return to search for any changes over time. (Photo: NASA/JPL/University of Arizona)
  • Delta in Eberswalde Crater
    This HiRISE image covers a portion of a delta that partially fills Eberswalde crater in Margaritifer Sinus. The delta was first recognized and mapped using MOC images that revealed various features whose presence required sustained flow and deposition into a lake that once occupied the crater. The HiRISE image resolves meter-scale features that record the migration of channels and delta distributaries as the delta grew over time. Differences in grain-size of sediments within the environments on the delta enable differential erosion of the deposits. As a result, coarser channel deposits are slightly more resistant and stand in relief relative to finer-grained over-bank and more easily eroded distal delta deposits. Close examination of the relict channel deposits confirms the presence of some meter-size blocks that were likely too coarse to have been transported by water flowing within the channels. These blocks may be formed of the sand and gravel that more likely moved along the channels that was lithified and eroded. Numerous meter-scale polygonal structures are common on many surfaces, but mostly those associated with more quiescent depositional environments removed from the channels. The polygons could be the result of deposition of fine-grained sediments that were either exposed and desiccated (dried out), rich in clays that shrunk when the water was removed, turned into rock and then fractured and eroded, or some combination of these processes. (Photo: NASA/JPL/University of Arizona)
  • Mars Exploration Rover Landing Site at Meridiani Planum
    Area a
    Area b
    Area c
    This HiRISE image shows the landing site of the Mars Exploration Rover Opportunity. The prominent impact crater on the right-hand side of the image is "Endurance crater" where Opportunity spent about ten months of its now nearly three-year mission. (Photo: NASA/JPL/University of Arizona)
    The bright irregularly-shaped feature in area "a" of the image is Opportunity's parachute, now lying on the martian surface. Near the parachute is the cone-shaped "backshell" that helped protect Opportunity's lander during its seven-month journey to Mars. Dark surface material may have been disturbed when the backshell touched down, exposing the lighter-toned materials seen next to the backshell. (Photo: NASA/JPL/University of Arizona)
    Area "B" of the image shows the impact point and the broken remnants of Opportunity's heat shield. The heat shield protected the vehicle during its fiery descent through the martian atmosphere, and then was released from the spacecraft during the final stages of the descent, breaking into two pieces when it hit the martian surface. Also visible is the small crater formed at the heat shield's impact point. Opportunity visited the heat shield during its drive southward from Endurance crater. (Photo: NASA/JPL/University of Arizona)
    Area "C" of the image shows "Eagle crater", the small martian impact crater where Opportunity's airbag-cushioned lander came to rest. The lander is still clearly visible on the floor of the crater. Opportunity spent about 60 martian days exploring rock outcrops and soils in Eagle crater before setting off to explore more of Meridiani Planum. (Photo: NASA/JPL/University of Arizona)

Contacts

Alfred S. McEwen, UA
Principal Investigator, HiRISE
520-621-4573
mcewen@lpl.arizona.edu


http://hiroc.lpl.arizona.edu/images/
http://marsprogram.jpl.nasa.gov/mro