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Transcript of Slide: 1 The first Moscow Solar System Symposium (1M-S3) >> Phobos Digital Terrain Model (DTM)and...
Slide: 1
The first Moscow Solar System Symposium (1M-S3) >>
Phobos Digital Terrain Model (DTM)Phobos Digital Terrain Model (DTM) and and Coordinate Refinement for Phobos-Grunt Mission Coordinate Refinement for Phobos-Grunt Mission
Support Support
K. Willner1, J.Oberst1,2, X. Shi3, H. Hoffmann2
1) Technische Universität Berlin, Department of Geodesy and Geoinformation Sciences, Berlin, Germany
2) German Aerospace Center (DLR), Institute of Planetary Research, Berlin-Adlershof, Germany3) Shanghai Astronomical Observatory, Chinese Academy of Sciences
The first Moscow Solar System Symposium (1M-S3) >> Slide: 2
March 2010 flybys – HRSC / SRC imagesMarch 2010 flybys – HRSC / SRC images
SRC image 7982 Nadir image 7982SRC image 7937
Stereo 2 image 7926
SRC image 7926 Nadir image 7926
The first Moscow Solar System Symposium (1M-S3) >> Slide: 3
Flyby Data Flyby Data
• Orbits 7915,7926, 7937: Nadir, Stereo and Photometry channels
• Area covered reaches from Western rim of Stickney to approx. 230° West and from North Pole to Equator
Orbit Flyby distance
ND / S1 / S2
Resolution
P1 / P2 Resolut
ion
7915 110 km 4 m/pixel
9 m/pixel
*7926 287 km 11
m/pixel24
m/pixel*
7937 476 km 19 m/pixel
39 m/pixel
Color channel resolutions
7948 663 km 29 m/pixel7959 850 km 34 m/pixel (8 x
binning)
* used for DTM reconstruction
The first Moscow Solar System Symposium (1M-S3) >> Slide: 4
Image coverage Image coverage
March 2010 flybys
• Observation geometry was similar for all flybys
• Similar coverage and light conditions for all flybys
• Proposed landing site area of Phobos Grunt is covered and illuminated
Nadir channel image orbit 7926
The first Moscow Solar System Symposium (1M-S3) >> Slide: 5
Landing Site DTMLanding Site DTM
Result of DTM reconstruction – 100 m/pixel lateral resolution, relative point accuracy +/- 10m
Control network published in EPSL serves as reference
Landing site location as described in Basilevsky & Shingareva, 2010
The first Moscow Solar System Symposium (1M-S3) >> Slide: 6
Perspective ViewPerspective View
N
The first Moscow Solar System Symposium (1M-S3) >> Slide: 7
Properties of the Landing AreaProperties of the Landing Area
• 2 x 2 degree grid shows gentle slopes within the landing area
• Almost flat terrain at landing site 1
• Small slope at proposed landing site 2
• Small number of craters in both proposed landing sites
12
Approx. Landing SitesBasilevsky & Shingareva, 2010
N
The first Moscow Solar System Symposium (1M-S3) >> Slide: 8
Effective Surface AccelerationEffective Surface Acceleration
Shi, X. et al., 2010
The first Moscow Solar System Symposium (1M-S3) >> Slide: 9
Effective Surface Acceleration - 2Effective Surface Acceleration - 2
Shi, X. et al., 2010
The first Moscow Solar System Symposium (1M-S3) >> Slide: 10
Coordinates of the Suggested Landing Coordinates of the Suggested Landing SitesSites
Landing Site
Longitude
Latitude
1 217.7°W 15.5°N2 212.0°W 21.5°N
Coordinates refer to the coordinate frame defined by the control network (Willner et al., 2010)
Coordinates have an accuracy of +/- 0.1°
Coordinates refer to the coordinate frame defined by the control network (Willner et al., 2010)
Coordinates have an accuracy of +/- 0.1°
The first Moscow Solar System Symposium (1M-S3) >> Slide: 11
OutlookOutlook
• Add further data and improve accuracy of DTM
• Image mosaic update (currently done)
• Map update
• Registration of color channel images to DTM
• Interpretation of multispectral images
The first Moscow Solar System Symposium (1M-S3) >> Slide: 12
Other Phobos ActivitiesOther Phobos Activities
ISSI Workshop Series:
Phobos and Deimos – After Mars Express,
Before Phobos Grunt
First Workshop, March 2010, next: April 2011.
http://www.issibern.ch/teams/phobosdeimos/
Planned: Publication of a „Phobos Book“
WorkshopTeam:
Jürgen Oberst (Coord.)Alexander T. BasilevskyVeronique DehantThomas C. DuxburyRobert A. JacobsonMartin PätzoldCarle M. PietersKira B. ShingarevaPeter C. ThomasWilliam ThuillotAlexander V. Zakharov
The first Moscow Solar System Symposium (1M-S3) >> Slide: 13
GETEMME, GETEMME, a Mission to Explore the Martian Satellites and the a Mission to Explore the Martian Satellites and the Fundamentals of Solar System PhysicsFundamentals of Solar System Physics
• A proposal for an ESA Cosmic Vision M-Class Mission for launch in 2022 or 2020
• Rendezvous with Deimos and Phobos, deploy Laser reflectors
• Monitor precise range from the spacecraft to Deimos, Phobos and Earth for 1 Mars year for studies of satellite dynamics and fundamental physics
• Comprehensive remote sensing of Deimos and Phobos
Proposal Team:
Jürgen Oberst, Valery Lainey, Christophe Le Poncin-Lafitte (Coordinators); Stephan Ulamec, Jens Biele, Harald Hoffmann, Konrad Willner,Veronique Dehant, Pascal Rosenblatt, Alexander V. Zakharov; > 100 proposal supporters