Mars in 3D (2/6/2008)

This is a mosaic of Olympus Mons, the highest volcano on Mars, which towers 26 km above the surrounding plains. The image covers an area of approximately 600 000 sq km and is colour-coded according to height based on data from the Digital Terrain Model (DTM). The High Resolution Stereo Camera (HRSC) on board ESA’s Mars Express orbiter imaged the region over 18 orbits. This image is an ortho-image mosaic, where the projecting rays are perpendicular to the plane of projection. This corrects any deformations introduced by an imaging camera. Such an image can be fitted directly on to a map. From the observations, 16 HRSC orbit strips, with around 35 Gigabytes of data were used to generate a Digital Terrain Model (DTM) mosaic and an ortho-image mosaic. The DTM mosaic has a resolution of 150 m/pixel. The resolution of individual nadir images (taken by pointing the camera vertically down to the surface) is in the range of 12 to 40 m/pixel. Individual terrain models with a resolution of up to 50 m were derived for every HRSC image strip. The high-resolution DTMs and ortho-images are derived through a complex process. Matching surface features were used to 'stitch' the images strips together, and complex geometrical calculations were used to produce the 3D coordinates of all measured points in the area. Credits: ESA/ DLR/ FU Berlin (G. Neukum)

Mars is about to come into 3D focus as never before, thanks to the data from the Mars Express High Resolution Stereo Camera (HRSC). A new high-resolution Digital Terrain Model data set that is about to be released onto the Internet, will allow researchers to obtain new information about the Red Planet in 3D.

Digital Terrain Models (DTMs) allow scientists to ‘stand’ on planetary surfaces. Although ordinary images can give spectacular bird’s-eye views, they can only convey part of the picture. They miss out on the topography, or the vertical elevation of the surroundings. That’s where Mars Express comes in.

The HRSC was especially designed to provide this information and, after years of specialised data processing, the first comprehensive release of 3D data of a large part of the martian surface is now ready. “Understanding the topography of Mars is essential to understanding its geology,” says Prof. Gerhard Neukum, Freie Universität (FU) Berlin, Germany, Principal Investigator for the HRSC.

The DTM can instantly tell researchers the slope of hillsides or the height of cliffs, the altitude and slope of lava flows or desert plains. “This data is essential for understanding how water or lava flowed across Mars,” says Neukum.

It also helps planetary scientists to better interpret other data sets, for example the results of the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS). “Once we know where the surface is, we can correctly interpret the radar echoes we get from below it,” says former ESA scientist Angelo Rossi, a member of the HRSC team.

The Mars Express DTM is the most detailed topographic data set ever released for Mars. Its release has been made possible by processing individual image swaths taken by the HRSC as Mars Express sweeps through its orbit. The individual swaths are then put together into mosaics that cover large regions. The high-resolution images used have a resolution of 10 m/pixel. The DTM elevation data derived from these images is provided in pixels of up to 50 m, with a height accuracy of 10 m.

The orbit of Mars Express determines the resolution of its pictures. When it is closest to the surface, it can take the most detailed pictures. “As the mission continues, we are gradually filling in the gaps and collecting high-resolution data whenever possible,” says Neukum.

The team plans to add more data to the DTMs to extend the surface coverage as Mars Express continues its mission until at least 2009 and HRSC continues its unique scrutiny of the planet.

How was it done

Constructing a Digital Terrain Model requires a spacecraft to look at the same surface feature twice, each time from a different angle. Most attempts to do this in the past have required the spacecraft to target the same feature from two different orbital passes. The High Resolution Stereo Camera (HRSC) on Mars Express is the only experiment that can do it in one pass. To achieve its complementary views, HRSC has nine individual scan lines that point fore, aft and straight down. It therefore sees a feature coming, sees it directly underneath and watches it recede into the distance, providing all the different angles needed.

NASA’s Mars Global Surveyor carried a laser altimeter instrument (MOLA) that provided spot heights across the surface of Mars, but these were often separated by many kilometres. HRSC provides altitude data for every data point the camera sees. It is the first time that high-resolution images have been accompanied by high-resolution topography.

The work of deriving new high-resolution archivable DTMs is split between DLR and FU Berlin. The systematic orbit-by-orbit processing of the DTMs is done entirely at DLR’s Institute of Planetary Research, Berlin, which also runs the HRSC experiment for ESA‘s Mars Express on behalf of, and in cooperation with, the PI and his team at the Institute of Geological Sciences, FU Berlin.

Mosaics of certain features on Mars, such as the Olympus Mons volcano, are processed at FU Berlin using DTM data of individual strips and specialised software developed within the HRSC Co-Investigator Team.

The additional funding required for the special processing of the individual image swaths and for the creation of the mosaics was provided by the German space agency (DLR), to the DLR Institute for Planetary Research and the Institute for Geological Sciences of the FU Berlin. DTMs had been processed in the past for exclusively scientific and outreach purposes, but with additional resources now available, it is possible to release the DTM data in higher quality.

Note: This story has been adapted from a news release issued by ESA

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