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21.01.2011
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The geometrical relationships between Mars, Phobos, and Mars Express at the time of the sequence.
Copyright ESA/DLR/FU Berlin (G. Neukum). |
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This image has been photometrically enhanced to illuminate darker areas. Resolution: 3.9 meters per pixel.
Image: Copyright ESA/DLR/FU Berlin (G. Neukum). |
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The HRSC-camera recorded images of Phobos on 9 January 2011 at a distance of 100 km with a resolution of 8.1 m/pixel. Due to the stereo viewing geometry during the flyby a small part of the moon's edge is only visible for the right eye resulting in odd 3D-perception in this area. This part has been slightly adjusted for better viewing. Also, for the left eye at the left edge of the image four small data gaps have been interpolated.
Image: Copyright ESA/DLR/FU Berlin (G. Neukum). |
','./preleases/492/medres/492-20110120-8974-Anaglyph-03-PhobosFlyby.jpg','3D Image<br>(red-cyan anaglyph) <br> [#492 Phobos Flyby Special Release (Orbit 8974)]'))
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Superimposed on the HRSC-nadir image are 7 SRC-images with a resolution of about 3 m/pixel. The Super Resolution Channel images show more details of the surface of Phobos.
Image: Copyright ESA/DLR/FU Berlin (G. Neukum). |
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Sequence of 5 HRSC-channels, orbit 8974: (left to right) stereo S1 (4.1 m/pixel), photometric P1 (8.1 m/pixel), nadir ND (3.9 m/pixel), photometric p2 (8.2 m/pixel), stereo S2 (4.3 m/pixel).
Image: Copyright ESA/DLR/FU Berlin (G. Neukum). |
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Image of Phobos with a resolution of 8.2 m/pixel in orbit 8974. The ellipses marked the previously planned (red) and currently considered (blue) landing sites for the Russian Phobos-Grunt mission.
Image: Copyright ESA/DLR/FU Berlin (G. Neukum). |
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The High Resolution Stereo Camera (HRSC) experiment on the ESA Mars Express Mission is led by the Principal Investigator (PI) Prof. Dr. Gerhard Neukum who also designed the camera technically. The science team of the experiment consists of 40 Co-Investigators from 33 institutions and 10 nations. The camera was developed at the German Aerospace Center (DLR) under the leadership of the PI G. Neukum and built in cooperation with industrial partners (EADS Astrium, Lewicki Microelectronic GmbH and Jena-Optronik GmbH). The experiment on Mars Express is operated by the DLR Institute of Planetary Research, through ESA/ESOC. The systematic processing of the HRSC image data is carried out at DLR. The scenes shown here were created by the PI-group at the Institute for Geological Sciences of the Freie Universitaet Berlin in cooperation with the German Aerospace Center (DLR), Institute of Planetary Research, Berlin.
Further information:
- Univ.-Prof. Dr. Gerhard Neukum
Freie Universitaet Berlin
Fachbereich Geowissenschaften
Fachrichtung Planetologie und Fernerkundung
Mobile: +49 171-7647177
Telefon: +49 30 838 70579; +49 30 838 70575 (Sekr.)
Email: gneukum@zedat.fu-berlin.de - Prof.Dr. Ralf Jaumann
Deutsches Zentrum für Luft- und Raumfahrt (DLR)
Institut für Planetenforschung, Planetengeologie
Tel.: +49 30 67055-400
Fax: +49 30 67055-402
Email: ralf.jaumann@dlr.de - Dr. Olivier Witasse
ESA Mars Express project scientist
ESTEC, The Netherlands
Email: owitasse@rssd.esa.int
Download
hochaufgelöste Bilddaten / high resolution image data
| Geometrical Relationship: |
| Sequence: |
| Planned landing site of the Russian Phobos-Grunt mission: |
| Stereo-1 channel image of Phobos: |
| SRC-Images: |
| 3D Image (red-cyan anaglyph): |
© Copyright: ESA/DLR/FU Berlin (G. Neukum)
