Preliminary reconstruction of martian atmospheric structure from Phoenix entry measurements Paul...
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![Page 1: Preliminary reconstruction of martian atmospheric structure from Phoenix entry measurements Paul Withers and David Catling Abstract P54B-08.](https://reader035.fdocuments.us/reader035/viewer/2022062401/5a4d1aef7f8b9ab05997d141/html5/thumbnails/1.jpg)
Preliminary reconstruction of martian atmospheric structure
from Phoenix entry measurements
Paul Withers and David Catling([email protected])
Abstract P54B-08Friday 2009.12.18 17:20-17:30
Fall AGU Meeting 2009San Francisco, CA
![Page 2: Preliminary reconstruction of martian atmospheric structure from Phoenix entry measurements Paul Withers and David Catling Abstract P54B-08.](https://reader035.fdocuments.us/reader035/viewer/2022062401/5a4d1aef7f8b9ab05997d141/html5/thumbnails/2.jpg)
Phoenix atmospheric entry• 25 May 2008• Landing site at
– 68.2N, 234.3E– -4.1 km (MOLA)
• Ls=77, LST ~16:30• Ballistic entry with
many similarities to Pathfinder and MER
• Accelerometers and gyroscopes on board
JPL figure
![Page 3: Preliminary reconstruction of martian atmospheric structure from Phoenix entry measurements Paul Withers and David Catling Abstract P54B-08.](https://reader035.fdocuments.us/reader035/viewer/2022062401/5a4d1aef7f8b9ab05997d141/html5/thumbnails/3.jpg)
Smoothed axial accelerations
WARNING – Currently archived PDS data contain small, but significant, errorPlease ask for details
![Page 4: Preliminary reconstruction of martian atmospheric structure from Phoenix entry measurements Paul Withers and David Catling Abstract P54B-08.](https://reader035.fdocuments.us/reader035/viewer/2022062401/5a4d1aef7f8b9ab05997d141/html5/thumbnails/4.jpg)
Trajectory reconstruction• Attitude found directly
using gyroscopes, angle of attack is well behaved
• Parachute deployment at 13.5 km and 391 m/s (Mach 1.7)
• First ground contact at 1.10 +/- 1.49 km above ground level and 6.1 +/- 3.6 m/s
Reconstruction process essentially same as used for Spirit and Opportunity, with exception of gyroscope data
![Page 5: Preliminary reconstruction of martian atmospheric structure from Phoenix entry measurements Paul Withers and David Catling Abstract P54B-08.](https://reader035.fdocuments.us/reader035/viewer/2022062401/5a4d1aef7f8b9ab05997d141/html5/thumbnails/5.jpg)
Atmosphere reconstruction
Reconstruction process essentially same as used for Spirit and Opportunity, but with updated aerodynamics and known attitude
Static stability indicates thatatmosphere is generally stable,especially around 70 km
![Page 6: Preliminary reconstruction of martian atmospheric structure from Phoenix entry measurements Paul Withers and David Catling Abstract P54B-08.](https://reader035.fdocuments.us/reader035/viewer/2022062401/5a4d1aef7f8b9ab05997d141/html5/thumbnails/6.jpg)
Comparison to data/models
MCS profile provided by David Kass, LMD profile from online Mars Climate DatabaseLow dust and high dust engineering models published by Tamppari et al. (2008)
Agreement with MCS profile is generally good
Both observed T(p) in middle atmosphere differ significantly from LMD prediction
Tamppari low dust model is very similar to Phoenix profile below 60 km
![Page 7: Preliminary reconstruction of martian atmospheric structure from Phoenix entry measurements Paul Withers and David Catling Abstract P54B-08.](https://reader035.fdocuments.us/reader035/viewer/2022062401/5a4d1aef7f8b9ab05997d141/html5/thumbnails/7.jpg)
Archiving status
• Data processing has stabilized and hopefully no further revisions are needed
• Ancilliary files produced and everything formatted for PDS
• Data processing documentation written• Currently inspecting dataset for any
problems, hoping to deliver to PDS in early 2010
![Page 8: Preliminary reconstruction of martian atmospheric structure from Phoenix entry measurements Paul Withers and David Catling Abstract P54B-08.](https://reader035.fdocuments.us/reader035/viewer/2022062401/5a4d1aef7f8b9ab05997d141/html5/thumbnails/8.jpg)
Conclusions• Trajectory and atmospheric structure from Phoenix entry
reconstructed successfully• Trajectory appears consistent with previous engineering
reconstructions and independent checks• Large temperature gradients in middle atmosphere• Atmosphere is stable• Atmospheric profile is broadly consistent with near-
simultaneous MCS observations• Engineering atmospheric model (low dust case) was very
accurate• LMD model was accurate in lower, but not middle, atmosphere
![Page 9: Preliminary reconstruction of martian atmospheric structure from Phoenix entry measurements Paul Withers and David Catling Abstract P54B-08.](https://reader035.fdocuments.us/reader035/viewer/2022062401/5a4d1aef7f8b9ab05997d141/html5/thumbnails/9.jpg)
Backup
![Page 10: Preliminary reconstruction of martian atmospheric structure from Phoenix entry measurements Paul Withers and David Catling Abstract P54B-08.](https://reader035.fdocuments.us/reader035/viewer/2022062401/5a4d1aef7f8b9ab05997d141/html5/thumbnails/10.jpg)
Problem with current PDS archive
• Basic data products at PDS are:– Vector accelerations and angular velocities in a specific spacecraft-
fixed frame
• Data reached Earth in instrument frame, were later transformed into a spacecraft frame for archiving
• A preliminary version of transformation matrix was used here, corresponding to the spacecraft as designed, not as built
• Actual matrix differs slightly in third decimal place, which is actually important
• Straight-forward to correct archived data by multiplying by another matrix
• PDS Atmosphere Node is working on erratum notice