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
‘Butterfly’ impact crater in Hesperia Planum
 
Colour view of 'butterfly'-shaped crater at Hesperia Planum
 
4 January 2006
These images, taken by the High Resolution Stereo Camera (HRSC) on board ESA’s Mars Express spacecraft, show a large elliptical impact crater in the Hesperia Planum region of Mars.
 
 
Map showing 'butterfly' crater in context
The HRSC obtained these images during orbit 368 with a ground resolution of approximately 16.7 metres per pixel. The scenes show the region of Hesperia Planum, at approximately 35.3° South and 118.7° East.

A large elliptical impact crater is visible within the scene, measuring approximately 24.4 km long, 11.2 km wide and reaching a maximum depth of approximately 650 metres below the surrounding plains.
 
 
Black and white nadir view of Hesperia Planum
Ejecta from this impact can be seen extending away from the crater, including two prominent lobes of material north-west and south-east of the crater.

The large circular feature, partly cut off by the border of the image, has a diameter of roughly 45 km.

This appears to be an impact crater that was subsequently resurfaced by lava flows, preserving the outline of the underlying crater. The curving features visible in the north of the image, known as ‘wrinkle ridges’, are caused by compressional tectonics.
 
 
Close-up perspective view of 'butterfly' crater - looking north
While the majority of impact craters are relatively circular, the elliptical shape of this impact crater suggests a very low impact angle (less than 10 degrees).

The long axis of the impact crater is viewed as the impacting direction of the projectile. Similar elliptical craters are observed elsewhere on Mars, as well as on our Moon.

The colour scenes have been derived from the three HRSC-colour channels and the nadir channel. The perspective views have been calculated from the digital terrain model derived from the stereo channels.
 
 
3D anaglyph view of Hesperia Planum
The 3D anaglyph image was calculated from the nadir and one stereo channel. 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'.
 
 

Perspective view of 'butterfly' crater - looking north
 
 
 


Mars Express image browser
Recent images
Sulphate deposits in Juventae ChasmaFly over the Chasma Boreale at Martian north poleThe Biblis Patera volcanoWater ice in crater at Martian north poleNicholson Crater on MarsCoprates 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.