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TOPIC: Mars Reconnaissance orbiter


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HiRISE Images: 17 December 2008



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New images for 17 December 2008

Walpaper (ZIP):
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iPHONE 320x480
PSP 480x272


Scoured Crater Rim
Scoured Crater Rim (PSP_010369_2065)
Kasei Valles forms one of the largest outflow channel systems on Mars thought to be carved by enormous floods over a billion years ago.
North Polar Layered Deposits
North Polar Layered Deposits (PSP_010366_2590)
The swirling patterns of layers are mostly caused by erosion, exposing the horizontal layers on ridges and valleys.
Complex Crater in Arabia Terra
Complex Crater in Arabia Terra (PSP_010354_2165)
The crater is intersected by one of the putative shorelines of the hypothesised ancient northern ocean.
Cyane Fossae Pits
Cyane Fossae Pits (PSP_010345_2150)
Graben are found in many places on Earth, with some of the best-known examples in the canyon lands area of southern Utah.
Sedimentary Layers in Columbus Crater
Sedimentary Layers in Columbus Crater (PSP_010281_1510)
Layered sedimentary rocks are found on the crater walls and floor, and may have been deposited by water or by wind.
Terraced Fan in Aeolis Region
Terraced Fan in Aeolis Region (PSP_009729_1735)
This image shows the southwest region of a degraded craters floor, located near the equator.
Fretted Terrain Valley Traverse
Fretted Terrain Valley Traverse (PSP_009719_2230)
Fretted terrain is thought to involve movement of ice-rich material in its formation.
Small Crater on Arcuate Ridge West of Olympia Mensae
Small Crater on Arcuate Ridge West of Olympia Mensae (PSP_009717_2545)
It has been suggested that arcuate ridges were formed by ancient glaciers on Mars.
Mesa in Acidalia Region
Mesa in Acidalia Region (PSP_009709_2155)
This scene in the Acidalia Planitia contains a variety of features, the most prominent of which are two mesas (hills).


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NASA's Mars Reconnaissance Orbiter has completed its primary, two-year science phase. The spacecraft has found signs of a complex Martian history of climate change that produced a diversity of past watery environments.
The orbiter has returned 73 terabits of science data, more than all earlier Mars missions combined. The spacecraft will build on this record as it continues to examine Mars in unprecedented detail during its next two-year phase of science operations.

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Anaglyph images 
Multiple Levels of Gullies
Multiple Levels of Gullies (PSP_004085_1420)
Fractured Mounds in Elysium Planitia
Fractured Mounds in Elysium Planitia (PSP_003597_1765)
Swirls of Rock in Candor Chasma
Swirls of Rock in Candor Chasma (PSP_001984_1735)




Planetary Data System orbit ranges 930010399 of the primary science phase.

Bright Feature Showing Possible Layering
Bright Feature Showing Possible Layering (PSP_009300_1545)
Possible Clays in the Circum-Ganges Chasma Plains
Possible Clays in the Circum-Ganges Chasma Plains (PSP_009301_1720)
High-Latitude Exposure of North Polar Layered Deposits
High-Latitude Exposure of North Polar Layered Deposits (PSP_009301_2720)
Sample
Sample (PSP_009304_1495)
Sample
Sample (PSP_009304_1805)
Ridges in Olympus Mons Aureole
Ridges in Olympus Mons Aureole (PSP_009304_2015)
Rocky Terrain
Rocky Terrain (PSP_009304_2405)
Candidate Crater Cluster Formed between September 2003 and June 2008
Candidate Crater Cluster Formed between September 2003 and June 2008 (PSP_009305_1830)
Cerberus Fossae Graben and Streak
Cerberus Fossae Graben and Streak (PSP_009306_1875)
Western Portion and Ejecta of Corinto Crater
Western Portion and Ejecta of Corinto Crater (PSP_009307_1970)
Polar Layered Deposits Unconformity
Polar Layered Deposits Unconformity (PSP_009307_2630)
Phlegra Montes Thermophysical Boundary
Phlegra Montes Thermophysical Boundary (PSP_009308_2295)
High-Latitude Exposure of North Polar Layered Deposits
High-Latitude Exposure of North Polar Layered Deposits (PSP_009309_2725)
Central Structures of Large Crater in Arabia Terra
Central Structures of Large Crater in Arabia Terra (PSP_009310_2015)
Albedo-Temperature Boundary
Albedo-Temperature Boundary (PSP_009311_1735)
Crenulate Ridge
Crenulate Ridge (PSP_009312_2145)



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Public Presentation About Mars Orbiter's Images and Findings
Mars scientists will present dramatic images and key findings from NASA's Mars Reconnaissance Orbiter at a free evening program in Pasadena on Thursday, Dec. 4, celebrating completion of the mission's first two-year science phase.
The Mars Reconnaissance Orbiter has already collected more data than all other past and current Mars missions combined. Its findings point to a complex history of climate change on the Red Planet, both early in its history and in more recent times.
The orbiter has cameras examining Mars at scales from revealing details the size of a desk to providing daily weather observations of the entire planet. Other instruments map minerals on the surface, probe with radar beneath the surface and monitor the atmosphere.
The public program will being at 7 p.m. Dec. 4 in the von Karman Auditorium at NASA's Jet Propulsion Laboratory, 4800 Oak Grove Dr. , Pasadena.

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HiRISE Images: 26 November 2008



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New images for 26 November 2008

Walpaper (ZIP):
800x600 1024x768 1152x864 1280x960 1440x1080 1600x12001920x1440 2048x1536 2560x1920
iPHONE 320x480
PSP 480x272

Yardangs in South Amazonis
Yardangs in South Amazonis (PSP_010334_1760)
Yardangs typically form in dry, desert environments with strong prevailing winds that are unidirectional.
Volcanic Fissure Vent in Elysium Planitia
Volcanic Fissure Vent in Elysium Planitia (PSP_010269_1900)
The most prominent feature in this image is the discontinuous line of pits and troughs that cuts across its center.
Aeolian Features, Large and Small
Aeolian Features, Large and Small (PSP_010221_1420)
Dust devils form in many parts of Mars, but they are often particularly distinct on sand dunes.
Complex Terrain East of Holden Crater
Complex Terrain East of Holden Crater (PSP_010197_1540)
This fascinating distribution of materials and landforms comprises a spectacular landscape.
Hydraotes Chaos
Hydraotes Chaos (PSP_009709_1810)
The mesa located in the center of the image has elongated depressions that might be evidence of past fluvial activity.
Meander in Valley Network
Meander in Valley Network (PSP_009706_2125)
As a target for HiRISE. However, at HiRISE resolution the valley is visible throughout its course.
Student Image of the Week: Kasei Valles
Student Image of the Week: Kasei Valles (PSP_006005_2050)
This image was suggested by Kathleen Hartrum's middle school science club at Conestoga Middle School in Beaverton, Oregon.



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HiRISE Images: 19 November 2008



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New images for 19 November 2008

Walpaper (ZIP):
800x600 1024x768 1152x864 1280x960 1440x1080 1600x12001920x1440 2048x1536 2560x1920
iPHONE 320x480
PSP 480x272

Light-Toned Rocks in Terra Meridiani
Light-Toned Rocks in Terra Meridiani (PSP_010222_1815)
At the finest scale, the light sediments visible in this image are intricately textured.
Dunes in Abalos Undae
Dunes in Abalos Undae (PSP_010219_2785)
It is possible that the dunes are no longer migrating and the tiny ripples are the only active parts today.
Reading the Rock Record at Nili Fossae
Reading the Rock Record at Nili Fossae (PSP_010206_1975)
This image captures a record of changing environments on ancient Mars, as recorded in the rock record at Nili Fossae.
Stratigraphy of the North Polar Deposits
Stratigraphy of the North Polar Deposits (PSP_010198_2645)
This image is particularly interesting because it crosses complicated trough geometry, making the layers appear curved and exposing multiple stratigraphic levels.
Colorful Ancient Rocks Near Mawrth Vallis
Colourful Ancient Rocks Near Mawrth Vallis (PSP_010183_2035)
Polygonal fracture patterns (similar to a tiled floor) are visible on the surfaces of some of these rocks.
Barchan Dunes in Chasma Boreale
Barchan Dunes in Chasma Boreale (PSP_010169_2650)
Barchan dunes are also commonly found on Earth, and are crescent-shaped with a steep slip face bordered by horns oriented in the downwind direction.
Western Rim Region of Korolev Crater
Western Rim Region of Korolev Crater (PSP_007961_2530)
At highest resolution both bright and dark areas of the surface are covered by polygonal fracture patterns



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HiRISE Images: 12 November 2008



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