Dust Fans on the Seasonal Carbon Dioxide Polar Cap
NASA/JPL/University of Arizona
Dust Fans on the Seasonal Carbon Dioxide Polar Cap
PSP_003180_0945  Science Theme: Seasonal Processes
twitter  •  tumblr

WALLPAPER
800
1024
1152
1280
1440
1600
1920
2048
2560

HIFLYER
PDF (11 x 17)


During the long dark night of Martian winter at the South Pole, carbon dioxide in its solid form (also known as “dry ice”) accumulates and forms a seasonal polar cap.

As the sun comes up in the spring, the ice evaporates in a complex way. This observation shows dark dust being blown across the seasonal south polar cap. The dust comes from the surface beneath the ice: it either starts at spots bare of ice, or it’s possible that it’s lofted from below the ice in geyser-like plumes.

Local winds blow the dust from its source, forming a long fan. When the wind changes direction, a new fan is formed pointing in the new direction In this single image we can see that the wind has blown in a number of directions. This data will be used to study weather patterns near the South Pole.

Written by: Candy Hansen  (18 April 2007)
 
Acquisition date
01 April 2007

Local Mars time
20:08

Latitude (centered)
-85.405°

Longitude (East)
104.073°

Spacecraft altitude
245.4 km (152.5 miles)

Original image scale range
52.9 cm/pixel (with 2 x 2 binning) so objects ~159 cm across are resolved

Map projected scale
50 cm/pixel

Map projection
Polarstereographic

Emission angle
22.4°

Phase angle
61.9°

Solar incidence angle
80°, with the Sun about 10° above the horizon

Solar longitude
210.8°, Northern Autumn

For non-map projected images
North azimuth:  155°
Sub-solar azimuth:  36.2°
JPEG
Black and white
map projected  non-map

IRB color
map projected  non-map

Merged IRB
map projected

Merged RGB
map projected

RGB color
non-map projected

JP2
Black and white
map-projected   (624MB)

IRB color
map-projected   (331MB)

JP2 EXTRAS
Black and white
map-projected  (416MB)
non-map           (371MB)

IRB color
map projected  (174MB)
non-map           (260MB)

Merged IRB
map projected  (586MB)

Merged RGB
map-projected  (543MB)

RGB color
non map           (232MB)
ADDITIONAL INFORMATION
B&W label
Color label
Merged IRB label
Merged RGB label
EDR products
HiView

NB
IRB: infrared-red-blue
RGB: red-green-blue
About color products (PDF)

Black & white is 5 km across; enhanced color about 1 km
For scale, use JPEG/JP2 black & white map-projected images

USAGE POLICY
All of the images produced by HiRISE and accessible on this site are within the public domain: there are no restrictions on their usage by anyone in the public, including news or science organizations. We do ask for a credit line where possible:
NASA/JPL/University of Arizona

POSTSCRIPT
NASA’s Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, Calif., manages the Mars Reconnaissance Orbiter for NASA’s Science Mission Directorate, Washington. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona.