meetings - Space Flight Mechanics Committee
meetings - Space Flight Mechanics Committee
meetings - Space Flight Mechanics Committee
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Feb 12, 2013<br />
Puna Room C&D<br />
SESSION 12: SPECIAL SESSION: MARS SCIENCE LABORATORY (MSL) -- II<br />
Chair: Dr. Gerhard Kruizinga, Jet Propulsion Laboratory<br />
8:00 AAS Entry System Design and Performance Summary for the Mars Science<br />
13-422 Laboratory Mission<br />
Allen Chen, NASA / Caltech JPL<br />
While the Sky Crane portion of Mars Science Laboratory’s Entry, Descent, and Landing<br />
system draws well-deserved attention as the iconic image of the landing, the entry segment<br />
is at least an equally harrowing part of the journey where a multitude of opportunities for<br />
failure exist. Over 99% of the spacecraft’s kinetic energy is dissipated during entry; all<br />
before the use of the supersonic parachute or the descent engines. This paper provides an<br />
overview of the entry segment design and summarizes Curiosity’s as flown entry<br />
performance on the night of August 5th.<br />
8:20 AAS Mars Science Laboratory Entry, Descent, and Landing Trajectory and<br />
13-307 Atmosphere Reconstruction<br />
Chris Karlgaard, Analytical <strong>Mechanics</strong> Associates, Inc.; Mark Schoenenberger,<br />
NASA Langley Research Center; Prasad Kutty, NASA Langley Research Center;<br />
Jeremy Shidner, Analytical <strong>Mechanics</strong> Associates, Inc.<br />
On August 5th 2012, The Mars Science Laboratory (MSL) entry vehicle successfully<br />
entered Mars' atmosphere and landed the Curiosity rover on its surface. Onboard<br />
instrumentation was used to reconstruct the entry trajectory and measure information about<br />
the atmosphere encountered. The instrumentation includes IMU accelerations and angular<br />
rates; surface pressure measurements from the Mars Entry Atmospheric Data System<br />
experiment; radar altimeter data; and the vehicle aerodynamic database. These data sources<br />
are blended using a Kalman filter. This paper provides an overview of the approach and the<br />
details of the results of the reconstruction.<br />
8:40 AAS Mars Science Laboratory Entry, Descent, and Landing Flush Air Data System<br />
13-308 Atmosphere Reconstruction<br />
Rafael Lugo, North Carolina State University<br />
A method is presented that enables atmosphere reconstruction from flush air data pressure<br />
observations. An innovative technique that permits the inclusion of redundant data types<br />
through the use of Monte Carlo dispersions is used as the framework for the inclusion of the<br />
pressure observations. The method is applied to the entry, descent, and landing flight data<br />
from Mars Science Laboratory. In addition to extracting atmosphere properties, the<br />
inclusion of pressure data is shown to aid in the quantification of trajectory parameter<br />
uncertainties in the hypersonic flight regime by reducing the state estimate uncertainties<br />
recovered from the Monte Carlo technique.<br />
Page 50<br />
23 rd AAS / AIAA <strong>Space</strong> <strong>Flight</strong> <strong>Mechanics</strong> Meeting