Mars MGS MOLA - MEX HRSC Blended Shaded Relief 200m v2
This is a shaded relief of the original DEM described next. This data product, now at version 2, is a blend of digital elevation model (DEM) data derived from the Mars Orbiter Laser Altimeter (MOLA), an instrument aboard NASA’s Mars Global Surveyor spacecraft (MGS), and the High-Resolution Stereo Camera (HRSC), an instrument aboard the European Space Agency’s (ESA) Mars Express spacecraft (MEX). This was created in support of thermal modelling studies and product creation for Mars (Fergason, Laura and Hare, 2017; Laura & Fergason, 2016).
MOLA fired infrared laser pulses downward 10 times per second and measured the time it took for the reflected pulses to return from the surface. The image used for the MOLA base of this map represents more than 600 million measurements gathered between 1999 and 2001. The average accuracy of each point is originally ~100 meters in horizontal position and the total elevation uncertainty is at least ±3 m. MOLA produced global topographic coverage with a spatial resolution of about 300 x 1000 m at the equator, and better near the poles.
HRSC, the only dedicated stereo camera orbiting Mars, is a multi-sensor push broom instrument comprising 9 CCD line sensors mounted in parallel for simultaneous high-resolution stereo, multicolor and multi-phase imaging by delivering 9 superimposed image swaths. The HRSC design permits stereo imaging with triple to quintuple panchromatic along-track stereo including a nadir-directed, forward and aft-looking (+/-18.91), and 2 inner (+/-12.81) stereo line sensors. The along-track acquisition of stereo imagery avoids changes in atmospheric and illumination conditions. The sub-pixel accuracy of the three-dimensional point determination allows the derivation of DEMs with a grid size of up to 50 m and a height accuracy of a single pixel with up to 10 m. Pixel resolution for this DEM is 200 meters per pixel (m).
Mission and Instrument Information:
Mars Global Surveyor was the first successful U.S. mission launched to Mars since the Viking mission in 1976 (Albee et al., 2001). MGS launched on November 7, 1996 atop a three-stage Delta II launch vehicle from launch pad 17A at Cape Canaveral Air Station, FL. The thirdstage Star 48B solid rocket later propelled the spacecraft out of Earth orbit and on its way to Mars. After a 20-year absence at the planet, MGS ushered in a new era of Mars exploration with its five science investigations (NASA JPL, 2010).
MGS arrived at Mars in September, 1997 and has contributed a multitude of findings, including signs of past, persistent water such as an ancient delta and currently active water features in the gullies of canyon walls. After nearly a decade of discovery, MGS went silent in November, 2006 (NASA JPL, 2010).
The MOLA created the most accurate global topographic map of any planet in the solar system, giving scientists elevation maps precise to within about 30 centimeters (1 foot) in the vertical dimension. Data from the laser altimeter identified pathways for the flow of past water and the locations, sizes, and volumes of watersheds. The instrument detected the heights of clouds and identified dynamic features in the atmosphere, such as gravity waves (NASA JPL, 2010).
The MOLA showed seasonal changes in the height of the Martian surface (such as snow depth) that represented the first direct global measurement of the amount and distribution of condensed carbon dioxide. In June 2001, part of the laser reached the end of its life, but a sensor continued to detect changes in surface brightness in the near infrared part of the spectrum. These data provided evidence of cloud coverage and atmospheric variations (NASA JPL, 2010).
The ESA launched Mars Express on June 2, 2003. At this time of year the positions of the two planets made for the shortest possible route, a condition that occurs once every 26 months. The spacecraft began its six-month journey from the Baikonur launch site in Kazakhstan on board a Russian Soyuz/Fregat launcher. Data collected by the orbiter instruments is transmitted to an ESA ground station at New Norcia near Perth, Australia, at a rate of up to 230 kbps. Between 0.5 and 5 Gbits of scientific data is transmitted from the spacecraft to Earth every day (ESA, 2010).
The HRSC is imaging the entire planet in full color, 3D and with a resolution of about 10 meters. Selected areas will be imaged at 2-meter resolution. One of the camera's greatest strengths will be the unprecedented pointing accuracy achieved by combining images at the two different resolutions. Another will be the 3D imaging which will reveal the topography of Mars in full color (ESA, 2010).
Albee, A. L., et al. (2001). Overview of the Mars Global Surveyor mission. Journal of Geophysical Research, 106(E10), 23291–23316. https://doi.org/10.1029/2000JE001306
European Space Agency (ESA) (2010). Mars Express. Mars Express Orbiter Instruments. https://www.esa.int/Science_Exploration/Space_Science/Mars_Express/Mars_Express_instruments
Fergason, R.L., Laura, J.R., Hare, T.M. (2017). THEMIS-Derived Thermal Inertia on Mars: Improved and Flexible Algorithm. Paper presented at 48th Lunar and Planetary Science Conference, Houston, TX. https://www.hou.usra.edu/meetings/lpsc2017/pdf/1563.pdf
Fergason, R. L., P. R. Christensen, and H. H. Kieffer (2006). High-resolution thermal inertia derived from the Thermal Emission Imaging System (THEMIS): Thermal model and applications. Journal of Geophysics Research, 111(E12). https://doi.org/10.1029/2006JE002735
Laura, J., and Fergason, R.L. (2016). Modeling martian thermal inertia in a distributed memory high performance computing environment. Paper presented at Big Data, 2016 IEEE International Conference on Big Data, Washington, DC. https://doi.org/10.1016/j.pss.2006.12.003
National Aeronautics and Space Administration (NASA) Jet Propulsion Laboratory (JPL) (2010). Mars Global Surveyor. https://mars.nasa.gov/mgs/overview/
Neukum, G., Jaumann, R., and the HRSC Co-Investigator and Experiment Team (2004). HRSC: The High Resolution Stereo Camera of Mars Express. In Wilson, A. (Ed.), Mars Express: The scientific payload (pp. 17-35). Noordwijk, The Netherlands: ESA. https://www.esa.int/esapub/sp/sp1240/sp1240web.pdf
Neumann, G. A., Smith, D.E., and Zuber, M. T. (2003). Two Mars years of clouds detected by the Mars Orbiter Laser Altimeter. Journal of Geophysics Research, 108(E4), 5023. https://doi.org/10.1029/2002JE001849
Smith, D.E., et al. (2001). Mars Orbiter Laser Altimeter—Experiment summary after the first year of global mapping of Mars. Journal of Geophysical Research, 106(E10), 23689–23722. https://doi.org/10.1029/2000JE001364
Fergason, R.L, Hare, T.M., Laura, J., 2017, HRSC and MOLA Blended Digital Elevation Model at 200m, Astrogeology PDS Annex, U.S. Geological Survey, http://bit.ly/HRSC_MOLA_Blend_v0
- USGS Astrogeology Science Center
- USGS Astrogeology Science Center
- DLR, NASA, Goddard Space Flight Center
- Added to Astropedia
- 28 September 2017
- 5 November 2019
This shaded relief (hillshade) is just a visual representation for the original DEM.
- Geospatial Data Presentation Form
- Shaded-Relief Map, Remote-sensing Data, Grey Scale
- HRSC and MOLA Blend
- Online Linkage
- Native Data Set Environment
- ISIS v3, GDAL, ESRI Arcinfo
- Supplemental Information
- http://sci.esa.int/mars-express/42328-hrsc-high-level-data-products-available/, https://www.esa.int/Our_Activities/Space_Science/Mars_Express/The_mission
- Topography, Image Processing, Remote Sensing, Photogrammetry
- Mars Express, Mars Global Surveyor
- HRSC, MOLA
Contact and Distribution
- Access Constraints
- Please cite authors
- Use Constraints
Data Status and Quality
- Time Period of Content Begin
- 1 October 2015
- Time Period of Content End
- 1 September 2017
- Currentness Reference
- Publication date
- In Work
- Update Frequency
- As needed
- Logical Consistency Report
- There are areas where the blending of the HRSC on top of MOLA did not always work well. Care should be taken when using for scientific analysis. The average accuracy of each point is originally ~100 meters in horizontal position and ~1 meter in radius (Neumann and others, 2001). However, the total elevation uncertainty is at least ±3 m due to the global error in the areoid (±1.8 meters) and regional uncertainties in its shape (G.A. Neumann, written commun., 2002). The MOLA data were initially referenced to an internally consistent inertial coordinate system, derived from tracking of the MGS spacecraft. These values include the orientation of the north pole of Mars (including the effects of precession), the rotation rate of Mars, and a value for W0 of 176.630°, where W0 is the angle along the equator to the east, between the 0° meridian and the equator’s intersection with the celestial equator at the standard epoch J2000.0 (Seidelmann and others, 2002). This value of W0 was chosen in order to place the 0° meridian through the center of the small (~500 m) crater Airy-0, within the crater Airy. Longitude increases to the east and latitude is planetocentric as allowed by IAU/IAG standards and in accordance with current NASA and USGS standards.
- Completeness Report
This was completed using HRSC DEMs released 2017 or earlier (through HRSC DEM h7500_0000.da4.tif). The HRSC Team is re-working all HRSC DEMs and this product will eventually be superseded.
Two HRSC DEMs were removed due to larger than normal height differences (h0938_0000 and h0927_0000). Several DEMS (~10 in total), were slightly crop to help create a more consistent edge blend into MOLA.
HRSC DEMs used in this product now covers 44% of Mars.
- Process Date
- 24 September 2017
- Process Description
This is a hillshade of the original blended DEM. Hillshade exxageration is about 2X using gdaldem.
This blend was accomplished by taking the full-res (463m/p) MOLA DEM and blending the high-res HRSC DEMs (~50m/p) into it. The HRSC DEMs required a re-projection from their original Sinusoidal projection into Simple Cylindrical. A cell-size of 200m/p was chosen as a compromise between up-sampling the MOLA and down-sampling the HRSC DEMs. Both up-sampling (MOLA) and down-sampling (HRSC) used a bilinear interpolation. Blending distance across the HRSC edge (into MOLA) was 5km (100 pixels) to ensure a smooth transition.
- Horizontal Positional Accuracy Value
- Horizontal Positional Accuracy Report
- Accurate to Control Net
- Entity and Attribute Detailed Description
- shaded relief representation of original topography
- PDS Status
- PDS 3 Like
- Source PDS Archive
- Mars Express
- Source Originator
- Planetary Data System
- Source Title
- High Resolution Stereo Camera (HRSC) and Mars Orbiter Laser Altimeter (MOLA)
- Source Online Linkage
- http://pds-geosciences.wustl.edu/missions/mgs/mola.html , http://pds-geosciences.wustl.edu/missions/mgs/index.htm , http://pds-geosciences.wustl.edu/missions/mars_express/hrsc.htm , http://pds-geosciences.wustl.edu/missions/mars_express/default.htm
- Type of Source Media
- Minimum Latitude
- Maximum Latitude
- Minimum Longitude
- Maximum Longitude
- Direct Spatial Reference Method
- Object Type
- Lines (pixels)
- Samples (pixels)
- Bit Type
- Quad Name
- Radius A
- Radius C
- Pixel Resolution (meters/pixel)
- Scale (pixels/degree)
- Horizontal Coordinate System Units
- Map Projection Name
- Simple Cylindrical
- Latitude Type
- Longitude Direction
- Positive East
- Longitude Domain
- -180 to 180