2 (No Transcript) 3 (No Transcript) 4 Can the mission be extended another 10 years?
Do we have enough fuel on board?
Will the power subsystem survive another 10 years?
Do we have to change the orbit?
Can the critical units be preserved?
Communications Subsystem
Attitude and Orbit Control Subsystem
Data Management Subsystem
Thermal Subsystem
Will the mission scenario have to be modified?
How to preserve the Mission Teams?
How to maintain the overall system?
5 The Available Propellant
Bi-propellant Reaction Control System
2x4 Thrusters Main Engine
475.5 kg of propellant at launch
35.2 kg (24.3 kg oxidant, 10.9 kg fuel) today
1.5/1 usage ratio ? 28.7 kg available
Uncertainties due to
Bookkeeping (1)
Fuel trapped above membrane (4.6 kg)
Usage per year 2.7 kg
Estimates remaining fuel good for 4 to 10 years!
6 Preserving onboard Propellant
Reduce uncertainties by applying Thermal Propellant Gauging Method
Define momentum neutral guidance strategy
No wheel off-loadings needed
Impact on science
Avoid large gravity gradient torques
Control solar radiation pressure torques
Optimise wheel off-loading attitudes
50 propellant saving for WOL
No pointing constraints on instruments
Loss of accurate long term control of the ground track
7 Battery Status and Energy Management
3 Li-Ion batteries First use for complex mission profile
ABSL performing real time ground test
Degradation due to
Cycle Life ? DoD and cycling rate
Calendar Life ? SoC and temperature
A number of models used
BEAST Predicts electrical and thermal performance
LIFE Predicts ageing
Electric / Thermal model Predicts Voltages
8 Battery Models
Models provide good fit
Current degradation (18) can be deduced
But
No predictive ageing effects
Therefore
Engineering studies
9 Engineering Studies for Battery Degradation
Engineering studies based on extrapolations from qualification tests
Li-Ion batteries do not fail catastrophically
Engineering studies are reasonable
10 Maximum Survivable Eclipse Duration
Eclipse duration acceptable if
Batteries fully recharged before start of next eclipse
Enough power to cope with Safe Mode at end of eclipse
Eclipses will become shorter 1.5 hrs in 2005 to 0.5 hrs in 2015
Maximum DoD driven by Solar energy
11 Energy Management
Battery preservation
Maintain SoC
Maintain batteries at low temperatures
Only outside power limited seasons
Eclipse Reduction
Can be achieved by modifying the orbital period
Requires fuel
Could have an impact on quality of orbit for Science
Trade-off required
12 Earth Mars Communications Subsystem
2 x Dual band transponder, 2x LGA S-band, HGA X-band
2 x Travelling Wave Tube Amplifier
2x Waveguide Interface Unit
Status Nominal
Total ON/OFF cycles 2900 ? 1.24 per day
TWTA qualified for 20000 cycles ? not before 2020
DRIVE-OFF strategy tested and will be implemented during power permitting seasons
WIUs and RFDUs identical to Rosetta ? Life Time 12 years
Tests ongoing with additional ground stations to ensure downlink bandwidth
Agreements for provision of S-band bandwidth till 2008. X-band Safe Mode might have to be defined
13 MEX Lander Communications Subsystem
Designed for communications with Beagle-2, and cross-support with NASA landers
Ultra High Frequency Transponder, Proximity-1 protocol
MELACOM re-programmable to allow for future protocols
Communications tests with MERs successful
DC-DC converter life limiting unit, designed for 50kRAD total radiation dose
Further analysis required, yet initial engineering judgement by manufacturer is positive
14 Attitude and Orbit Control
Reaction Control Subsystem
414 N Main Engine - isolated
2x4 10 N Thrusters all manoeuvres can be done by 4 thrusters
2 Star Trackers, 30 deg angle between their optical axes Identical to Rosettas
Reaction Wheel Assembly 4 wheels in skewed configuration
2 Inertial Measurement Units each including a set of 3 gyroscopes
2 Solar Array Drive Mechanisms Mechanism and Electronics identical to Rosettas
2 Sun Acquisition Sensors Identical to Rosettas
15 Reaction Wheels and IMU
3 of the 4 Reaction wheels are sufficient for attitude control
A thruster control mode is available (Safe Hold Mode)
Reliability figures for the Reaction Wheels given w.r.t operations temperatures
MEX RWs operate below these temperatures
IMUs and Gyroscopes can be used in all combinations
IMU 2 being used to maintain balance in usage periodic swaps foreseen
16 IMU and Gyroscope Lifetime 17 Data Management Subsystem
Central Management Unit Identical to Rosettas
Remote Terminal Unit Identical to Rosettas
AOCSM Interface Unit Identical to Rosettas
Solid State Mass Memory Extrapolation of reliability figures shows 0.95 reliability at 12 years from launch, yet still providing at least half the memory capacity.
18 Thermal Subsystem
5 heaters controlled by instruments
9 heaters payload interface thermal control
4 heaters no longer used since arrival at Mars
6 heaters used for AOCS equipment
8 heaters used for CPS lines and platform equipment
Platform heater groups controlled by thermostats
Thermostats mechanical lifetime of 1 million cycle at 2-3A
19 Thermostat Fast Cycling
Oscillations at stable thermal conditions
Work-around implemented switch OFF affected circuit for 30 mins every 1.5 hour (leaving redundant circuit ON)
Nr of cycles a day from 1200-1500 to 300-500
20 Extension Feasibility
Technical feasibility for long operational scenarios demonstrated
Resulting mission scenarios will require adaptation of the science mission
Trade-off required
Structure required for preservation of the mission team
Maintenance and preservation of the overall system will be needed
21 Conclusions and Recommendations
Obtain a more accurate estimation of the amount of propellant left onboard
Investigate further the possibilities to optimise Reaction Wheel Off-loadings for minimum propellant consumption
Optimise the fuel/oxidant mixture ratio if manoeuvres are foreseen
Store the batteries at lowest possible temperature and State of Charge
Trade off pros and cons of modifying the orbit to decrease eclipse duration
Investigate ways to optimize heater power consumption
Obtain lifetime test and/or analysis data from manufacturers of the various critical units
Establish preliminary operational concepts and corresponding ground resource profiles that would allow actual implementation of the selected strategies
22 Conclusions and Recommendations 2
No show stoppers identified
Active strategies required to preserve resources and units
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