|
News
|
 |
|
7 May 2004
These images were taken by the High Resolution Stereo Camera (HRSC) on board ESA’s Mars Express of the Acheron Fossae region, an area of intensive tectonic (continental ‘plate’) activity in the past.
The images show traces of enormous stress and corresponding strain in the crust of the Red Planet. The HRSC was pointed twice at this interesting geological feature in the Acheron Fossae mountain range, during orbits 37 and 143.
 |
|
||
|
(2) Acheron Fossae horsts and grabens (black/white)
|
For practical use on the internet, the images have been reduced in their resolution – the data originally obtained from orbit at an altitude of 765 kilometres (orbit 37) and 1240 kilometres (orbit 143) have a resolution of 30 metres and 50 metres per pixel respectively.
|
|
||
|
(3) Acheron Fossae horsts and grabens in 3D
|
In Greek mythology, Acheron is the river entering the underworld, the Hades, and ‘fossa’ is the Latin word for trough.
Acheron Fossae marks the northern edge of the Tharsis plateau. It is part of a network of extensional fractures that radiates outward from their central focus in the Tharsis ‘bulge’, a huge area of regional uplift where intensive volcanic activity occurred.
These curved ‘faults’ were caused in the process of this uplift: cracks in the crust formed when the hot material rising from deep in the mantle of Mars pushed the overlying ‘elastic’ lithosphere (surface layers of rock) upward. When the distorting tensions became too strong, the brittle crust on top of the lithosphere broke along zones of weakness.
Images 1-3, from orbit 37, are dominated by these curved features, showing a highly fractured, faulted and deformed area in the central part of the Acheron Fossae.
In geological terms, this is called a ‘horst and graben’ system. When several parallel faults form, the block of crust between them drops down, forming a ‘graben’. At Acheron, an almost classical example of parallel fault-bounded grabens has formed, dissected by remnants of the pre-existing topographical heights, the ‘horsts’.
|
|
||
|
(4) Disrupted crater at Acheron Fossae, colour
|
They show how the rifting crosses the older impact crater with at least three alternating horsts and grabens.
The Acheron Fossae region can be compared to rift zones on Earth, where continental plates spread apart, as is known from the Kenyan Rift Valley in eastern Africa.
|
|
||
|
(5) Disrupted crater at Acheron Fossae in black/white
|
From the edge of a horst in Acheron Fossae to the bottom of a graben, the digital elevation data from the HRSC reveal height differences of more than 1700 metres.
The large graben in the centre of the image is about 15 kilometres wide.
|
|
||
|
(6) Disrupted crater at Acheron Fossae in 3D
|
Erosional processes later transported material from the outside the area into the crater and resurfaced its floor, erasing the tectonic features inside the crater. The depth of the crater from rim to bottom is 2000 metres.
|
The colour and black and white images show the view looking straight down from the spacecraft; north is to the right. The perspective view shows the same region including some adjacent areas to the south without vertical exaggeration. The 3D images require stereoscopic glasses to view.
For more information on Mars Express HRSC images, you might like to read our updated 'Frequently Asked Questions'.