ESAESA ScienceMars Express
   
Europe goes to Mars
About Mars Express
About Mars
Meet the team
Multimedia
VideoTalkMars Express imagesMars Express videosHRSC videosAnimation in 11 languagesDownload wallpapersDownload screensavers3D Flash 'model'Make a model
Services
Comments Bookmark and Share
 
 
 
 
News
 
printer friendly page
Nicholson Crater on Mars
 
Perspective view of Nicholson Crater central peak - looking west
 
15 July 2005
These images, taken by the High Resolution Stereo Camera (HRSC) on board ESA’s Mars Express spacecraft, show Nicholson Crater, located at the southern edge of Amazonis Planitia on Mars.
 
 
Nicholson Crater
Map showing Nicholson Crater in context
The HRSC obtained these images during orbit 1104 with a ground resolution of approximately 15.3 metres per pixel. The scenes show the region around Nicholson Crater, at approximately 0.0° South and 195.5° East.

Nicholson Crater, measuring approximately 100 kilometres wide, is located at the southern edge of Amazonis Planitia, north-west of a region called Medusae Fossae.
 
 
Colour nadir view of Nicholson Crater
Located in the centre of this crater is a raised feature, about 55 kilometres long and 37 kilometres wide, which extends to a maximum height of roughly 3.5 kilometres above the floor of the crater.

At present, it is still unclear how this central feature was shaped and what kind of processes led to its formation. It is thought that the remnant hill could be composed of material from underground or was built as a result of atmospheric deposition.
 
 
Black and white nadir view of Nicholson Crater
The tall feature in the centre of this hill is the central peak of the crater, which forms when the surface material ‘rebounds’ after being compressed during the formation of an impact crater.

However, it is clear that this feature has been heavily sculpted after its creation, by the action of wind or even water.
 
 

Colour 3D perspective view of central peak - looking north-west
 
 
Close-up perspective view - looking north-west
 
 
The colour images were processed using the HRSC nadir (vertical view) and three colour channels. The perspective views were calculated from the digital terrain model derived from the stereo channels.
 
 
3D anaglyph view of Nicholson Crater
The 3D anaglyph images were created from the nadir channel and one of the stereo channels. Stereoscopic glasses are needed to view the 3D images Image resolution has been decreased for use on the internet.

For more information on Mars Express HRSC images, you might like to read our updated 'Frequently Asked Questions'.
 
 

 


Mars Express image browser
Recent images
Sulphate deposits in Juventae Chasma‘Butterfly’ impact crater in Hesperia PlanumFly over the Chasma Boreale at Martian north poleThe Biblis Patera volcanoWater ice in crater at Martian north poleCoprates Chasma and Coprates CatenaAncient floods on Mars: Iani Chaos and Ares VallisCrater Holden and Uzboi VallisTithonium Chasma up closeThe mesas of Aureum ChaosThe Medusa Fossae formation on Mars‘Hourglass’ shaped craters filled with traces of glacier
More information
High Resolution Stereo CameraBehind the lens...
 
 
 
   Copyright 2000 - 2010 © European Space Agency. All rights reserved.