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Mars Images Show Topography Of Red Planet

Date:
February 18, 2008
Source:
European Space Agency
Summary:
Mars is about to come into 3D focus as never before, thanks to the data from the Mars Express High Resolution Stereo Camera. A new high-resolution Digital Terrain Model data set that has just been released onto the Internet, will allow researchers to obtain new information about the Red Planet in 3D.
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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 has just been 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.

Production details

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.

More images are available at: http://www.esa.int/esa-mmg/mmg.pl?mission=Mars+Express&keyword=+--%3E+Keyword&idf=+--%3E+ID&Ic=on&subm3=GO


Story Source:

Materials provided by European Space Agency. Note: Content may be edited for style and length.


Cite This Page:

European Space Agency. "Mars Images Show Topography Of Red Planet." ScienceDaily. ScienceDaily, 18 February 2008. <www.sciencedaily.com/releases/2008/02/080205111718.htm>.
European Space Agency. (2008, February 18). Mars Images Show Topography Of Red Planet. ScienceDaily. Retrieved March 28, 2024 from www.sciencedaily.com/releases/2008/02/080205111718.htm
European Space Agency. "Mars Images Show Topography Of Red Planet." ScienceDaily. www.sciencedaily.com/releases/2008/02/080205111718.htm (accessed March 28, 2024).

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