As noted above, one of the more challenging mission requirements is the ability to both charge and discharge the battery at very low temperatures (-30oC) using moderately aggressive rates (i.e., C/5 rates based on the nameplate capacity of 25Ah). In addition to having to support the power and energy requirements under these conditions, there was some concern that lithium plating on the anode could occur during the low temperature charging which may lead to performance degradation.8 Furthermore, there was some concern that the low temperature capability of the battery could be compromised by being subjected to long, high temperature operation, making end of mission requirements difficult to meet.
To address these concerns, a comprehensive performance test program was under-taken, which included the following: (i) determining the impact of high temperature exposure, (ii) simulating the launch pad storage conditions, (iii) continuously cycling between the temperature extremes (+30oC, +20oC, -25oC, and -30oC) with periodic diagnostic capacity and impedance characterization at +30oC, -25oC and -30oC, (iv) low temperature charge and discharge characterization (-25oC to -40oC), and (v) accelerated mission relevant testing, consisting of 60% DOD cycling over a wide temperature range.
In summary, the InSight Li-Ion chemistry with an ester-containing low temperature electrolyte delivered improved performance compared to the compared to the heritage NCO-based chemistry which has been used on previous rover and lander missions to Mars, including: (i) >15% higher capacity and energy at ambient temperature, (ii) superior low temperature performance (-25oC and below), and (iii) improved resilience to high temperature exposure. Furthermore, the battery chemistry was demonstrated to be very resilient to continuous operation at -30oC, with no indirect evidence of lithium plating occurring or noticeable performance degradation observed. Thus far, the flight batteries have completed over 100 Sols of operation of the surface of Mars and have displayed excellent performance and health characteristics.
ACKNOWLEDGEMENT
The work described here was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration (NASA) and supported by the Mars InSight Mission.
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