Mars
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Mars Express' High Resolution Stereo Camera (HRSC) has provided snapshots of the Aeolis Mensae region on the Red Planet. The region, imaged on 26 and 29 March 2007, during Mars Express orbit number 4136 and 4247, is located at approximately 6° South and 145° East. Deep valleys are incised into the highlands in the northern part of the scene showing linear features on the floor of the valley. Similar linear features are also seen in the lower part of the picture but the morphology is different from the region in the upper part in that there are no incisions. Also, the area is far less cratered and hence the erosion must be of a relatively recent origin. Scientists have reason to believe that the valleys might primarily originate from tectonic activity, possibly also modelled locally by subsequent fluid or mass wasting activity. This perspective view was obtained from a Digital Terrain Model derived from the HRSC stereo channels. Credits: ESA/DLR/FU Berlin (G. Neukum)
 
 
Tectonic signatures at Aeolis Mensae
Mars Express' High Resolution Stereo Camera (HRSC) has provided snapshots of the Aeolis Mensae region on the Red Planet. The region, imaged on 26 and 29 March 2007, during Mars Express orbit number 4136 and 4247, is located at approximately 6° South and 145° East. Deep valleys are incised into the highlands in the northern part of the scene showing linear features on the floor of the valley. This perspective view was obtained from a Digital Terrain Model derived from the HRSC stereo channels. Credits: ESA/DLR/FU Berlin (G. Neukum)
 
 
Tectonic signatures at Aeolis Mensae
This image provides another perspective view of the Deuteronilus Mensae region on Mars taken by the High-Resolution Stereo Camera (HRSC) onboard ESA's Mars Express with a ground resolution of approximately 29 metres per pixel. The dark depression visible at the top-left of the image measures 2 000 metres in depth and 110 kilometres in diameter, north to south. Deeply incised valleys of a depth ranging from 800 to 1200 metres are clearly identifiable in the north - eastern part of the scene. It is believed that those valleys may have originated from intense flooding by melted water ice. The water then froze rather quickly and flowed down the slopes of the depression like a glacier. The view has been calculated from the digital terrain model derived from the stereo channels. Credits: ESA/DLR/FU Berlin (G. Neukum)
 
 
Deuteronilus Mensae on Mars
This image shows a perspective view of the Deuteronilus Mensae region on Mars. It was taken on 14 March 2005 by the High-Resolution Stereo Camera (HRSC) onboard ESA's Mars Express with a ground resolution of approximately 29 metres per pixel. It is believed that the valleys visible in the image may have originated from intense flooding by melted water ice. The water then froze rather quickly and flowed down the slopes of the depression like a glacier. The view has been calculated from the digital terrain model derived from the stereo channels. Credits: ESA/DLR/FU Berlin (G. Neukum)
 
 
Deuteronilus Mensae on Mars
This image shows the Deuteronilus Mensae region on Mars, an area primarily characterized by glacial features. It was taken on 14 March 2005 (orbit number 1483) by the High Resolution Stereo Camera (HRSC) onboard ESA's Mars Express with a ground resolution of approximately 29 metres per pixel. The area is located on the northern edge of Arabia Terra and borders the southern high- and northern lowlands, at approximately 39° North and 23° East. The scene has been derived from the three HRSC colour channels and the nadir channel. Credits: ESA/DLR/FU Berlin (G. Neukum)
 
 
Deuteronilus Mensae on Mars
Atmospheric structures can be seen in this image of Mars taken by the OSIRIS narrow-angle camera at 19:28 CET on 24 February 2007 from a distance of about 240 000 km. The image was produced through a special combination of the green and red colour filters, emphasising the brightness difference. This image processing step enhances the structures in the atmosphere, either dust or clouds. Credits: ESA © 2007 MPS for OSIRIS Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA
 
 
Rosetta OSIRIS image of Mars
Atmospheric structures can be seen in this image of Mars taken by the OSIRIS narrow-angle camera at 19:28 CET on 24 February 2007 from a distance of about 240 000 km. The image was produced through a special combination of the green and red colour filters, emphasising the brightness difference. This image processing step enhances the structures in the atmosphere, either dust or clouds. Credits: ESA © 2007 MPS for OSIRIS Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA
 
 
Rosetta OSIRIS image of Mars
This ultraviolet image of Mars was taken on 24 February 2007 with the OSIRIS wide-angle camera through the 'OH' colour filter, intended for the indirect detection of water when observing comet 67/P Churyumov-Gerasimenko. Clouds are visible at the North polar cap of Mars and at the morning 'limb' (border or outermost edge of a celestial body). A high-altitude cloud is also visible and shown in the inset. Credits: ESA © 2007 MPS for OSIRIS Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA
 
 
Rosetta OSIRIS image of Mars
The first true-colour image generated using the OSIRIS orange (red), green and blue colour filers. The image was acquired on 24 February at 19:28 CET from a distance of about 240 000 km; image resolution is about 5 km/pixel. Credits: ESA © 2007 MPS for OSIRIS Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA
 
 
Rosetta OSIRIS image of Mars
This image composite is based on near-infrared, green and near-ultra-violet colour information obtained by the OSIRIS Narrow Angle Camera. At the southern part of the planet, the southern spring polar cap is clearly seen. At this time of the Martian year, a large fraction of Mars' atmosphere is evaporating from the southern polar cap and will migrate to the northern polar cap during nothern winter. Over most of the Martian disk one can see large cloud systems. The image was acquired on 24 February at 19:28 CET from a distance of about 240 000 km; image resolution is about 5 km/pixel. Credits: ESA © 2007 MPS for OSIRIS Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA
 
 
Rosetta OSIRIS image of Mars
An orange (red), green and near-UV colour filter composite image of Mars; the UV channel (the blue color) has been enhanced. The enhanced UV signal clearly shows the presence of the cloud system covering most of the Martian disk. The image was acquired on 24 February at 19:28 CET from a distance of about 240 000 km; image resolution is about 5 km/pixel. Credits: ESA © 2007 MPS for OSIRIS Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA
 
 
Rosetta OSIRIS image of Mars
Stunning image taken by the CIVA imaging instrument on Rosetta's Philae lander just 4 minutes before closest approach at a distance of some 1000 km from Mars. A portion of the spacecraft and one of its solar arrays are visible in nice detail. Beneath, an area close to the Syrtis region is visible on the planet’s disk. Credits: CIVA / Philae / ESA Rosetta
 
 
Stunning view of Rosetta skimming past Mars
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