Mars rovers survive the night through specific thermal and power management systems
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Scientific literature and technical documentation confirm that Mars rovers utilize specialized power systems, solar arrays, batteries, and thermal management strategies to survive extreme Martian temperature drops.
NASA's Mars Exploration Rover (MER) project involved delivering two mobile science laboratories (rovers) on the surface of Mars to remotely conduct geologic investigations, including characterization of a diversity of rocks and soils. The rovers were launched separately in 2003 and have been in operation on the surface of Mars since January 2004. The rovers underwent a comprehensive pre-launch environmental assurance program that included assembly/subsystem and system-level testing in the areas of dynamics, thermal, and electromagnetic (EMC), as well as venting/pressure, dust, radiation, and solid-particle (meteoroid, orbital debris) analyses. Due to the Martian diurnal cycles of extreme temperature swings, the susceptible hardware that were mounted outside of the thermal controlled zones also underwent thermal cycling qualification of their packaging designs and manufacturing processes. This paper summarizes the environmental assurance program for the MER project, with emphasis on the pre-launch thermal testing program for ensuring that the rover hardware would operate and survive the Mars surface temperature extremes. These test temperatures are compared with some of the Mars surface operational temperature measurements. Selected anomalies resulting from operating the rover hardware in the Mars extreme thermal environment are also presented.
Testing of the Mars Exploration Rovers to Survive the Extreme Thermal Environments | Published in Journal of Microelectronics and Electronic Packaging This website uses cookies We use cookies to enhance your experience and support COUNTER Metrics for transparent reporting of readership statistics. Cookie data is not sold to third parties or used for marketing purposes. Deny cookies Customize ≫ cookies Allow all cookies Skip to main content Journal of Microelectronics & Elect Pkg RSS Feed Enter the URL below into your favorite RSS reader. http://localhost:8583/feed × ISSN 1551-4897 General Vol.
4, Issue 4, 2007 October 01, 2007 EDT Testing of the Mars Exploration Rovers to Survive the Extreme Thermal Environments Kin F. Man , Alan R. Hoffman , Dynamics Testing EMC Testing Environmental Assurance Environmental Testing Extreme Thermal Environments Mars Environments Mars Exploration Rover Natural Space Thermal Testing Spacecraft Testing ccby-nc-nd-4.0 • https://doi.org/10.4071/1551-4897-4.4.145 Journal of Microelectronics & Elect Pkg Man, Kin F., and Alan R. Hoffman. 2007. “Testing of the Mars Exploration Rovers to Survive the Extreme Thermal Environments.” Journal of Microelectronics and Electronic Packaging 4 (4): 145–54. https://doi.org/10.4071/1551-4897-4.4.145 .
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The design goal for the rovers was 600 meters of travel; in fact, they have traveled jointly more than 50 kilometers. After scouting around its rim, Opportunity drove down the steep walls into an impact crater called Victoria, then succeeded with some difficulty in climbing back out to resume its route (Figure 10.15). Dust covering the rovers’ solar cells caused a drop in power, but when a seasonal dust storm blew away the dust, the rovers resumed full operation. In order to survive winter, the rovers were positioned on slopes to maximize solar heating and power generation. In 2006, Spirit lost power on one of its wheels, and subsequently became stuck in the sand, where it continued operation as a fixed ground station. Meanwhile, in 2008, Phoenix (a spacecraft “reborn” of spare parts from a previous Mars mission that had failed) landed near the edge of the north polar cap, at latitude 68°, and directly measured water ice in the soil. In 2011, NASA launched its largest (and most expensive) Mars mission since Viking (see Figure 10.1).
A computational tool for conceptual design and optimization of planetary rovers
The design process of a Mars rover is driven by multiple design constraints, namely overall mass, power consumption and volume (dimensions). Various systems, such as mobility, manipulation, handling, power, thermal, communication, navigation, avionics and science instruments, together make a complete rover vehicle and they should function collectively to perform a given task. Each of the subsystems can be thought of as modular building blocks that are integrated together to form a fully functional rover vehicle. When approaching the design of such a vehicle, the designer should take into account of cross design dependencies existent between different subsystems and technology limitations. Performing any particular task, would lead to many design possibilities. Choosing the final design from many feasible solutions is arguably a daunting task. In order to make this process simple and convenient, as well as to understand the design non-linearity existing in this solution space, the authors have employed a systems engineering approach to develop a tool comprising subsystem models.
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Power module
The power system modelled here is a photovoltaic system or solar arrays acting as the primary
power source. The solar arrays must generate a sufficient amount of power to satisfy subsystem
charging and battery recharging demands. Batteries supply energy during peak operations and
during periods when there is no sunlight . Batteries should also maintain the temperature of
rover systems during cold nights. Solar arrays consist of sola r cells that are available in
different technologies. They are responsible for converting solar energy in to electricity
through the photovoltaic effect. Here GaInP/GaAs/Ge triple junction cell technology with a
conversion efficiency of 26.8% is assumed. The solar arrays are assumed inclinable or tiltable
to suitable angles by means of actuators. This method enables the capability of tracking the
sun to maintain maximum solar radiation reaching the cells during the entire sol. Likewise, the
battery is assumed to be of Li-ion technology with an operational efficiency of 95%. Although
solar cells suggest a primary element of the solar array, it may not contribute significantly to
overall mass. The structure ( Marraystruct), cover glass, interconnects and substra te forms the
significant portion of the overall array mass. The relationships for determining power
subsystem mass is given as follows:
𝑀𝑀𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑎𝑎𝑎𝑎𝑒𝑒𝑡𝑡𝑐𝑐𝑡𝑡𝑒𝑒𝑡𝑡 = 6𝑚𝑚𝑐𝑐𝑒𝑒𝑒𝑒𝑒𝑒 ⋅ 𝐴𝐴𝑒𝑒𝑡𝑡 (8)
𝑀𝑀𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑎𝑎𝑒𝑒𝑡𝑡𝑡𝑡𝑎𝑎𝑐𝑐𝑡𝑡 = 0.0.82𝑀𝑀𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑎𝑎𝑎𝑎𝑒𝑒𝑡𝑡𝑐𝑐𝑡𝑡𝑒𝑒𝑡𝑡 (9)
𝑀𝑀𝑎𝑎𝑡𝑡𝑡𝑡 =
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INCAS BULLETIN, Volume 15, Issue 1/ 2023
A case to design a rover concept that should carry scientific payloads of 50 kg in mass is
considered to demonstrate the feasibility of the approach. Genetic Algorithm is chosen as the
optimization technique because of the large number of design v ariables and serving the
purpose of efficiently handling global optimization problems. GA works on the principle of
life evolution process based on the Darwinian principle. Goldberg first introduced it as a meta-
heuristic, numerical optimization technique [10]. In GA, a set of operations is performed on a
population of encoded solutions known as individuals or chromosomes. Each possible solution
is en coded as a set of genes. During each iteration (or generation), the individuals in the
population undergo selection, crossover, mutation and fitness evaluation operations. The
global search of design solutions followed in GA prevents convergence of solutions or trapped
in the local optima. Unlike other optimization methods, GA does not require gradients or
derivatives of the function to be minimized. Also it does not require initial guess values of the
design variables. Only the boundary values to the design space are needed. GA varies the
values of design variables over a number of generations until satisfying a set of criteria. In GA,
the fitness function represents the objective functions and constraints. A higher fitness
indicates better solution. In the fitness function, the constraints are handled such that
unfeasible solutions are penalized by a penalty factor. With each GA generation, the fitness of
the population is improved. The best solution selected is the individual with the best fitness at
the end of the last generation.
Mission requirements definition
The model requires mission level inputs from the user that informs the environment and
vehicle operational conditions on Mars. They help in understanding the soil type that is
described by Bekker’s friction and cohesion properties [11] . Also the terrain conditions are
specified to understand whether the rover should operate on slopes. Operational requirements
define the nominal and peak power consumption of systems. Battery recharge duration
available per sol is also specified. Temperature conditions to be maintained inside WEB should
be also provided.
Table 3 - Assumed operational requirements for one experimental cycle
Nominal Peak
Day power consumption per
exp. cycle
Communication (W) 30 255
Drilling (W) 45 80
Science (W) 21 21
Thermal control (W) 8 8
Night power consumption
per exp. cycle Thermal control (Whr) 96 540
Operational hours per exp.
Cycle
Communication (hrs) 1 1
Drilling (hrs) 1 1
Science (hrs) 1 1
Thermal control (hrs) 1 1
Battery recharge plan: [day 1, day 2,
..,day 12] (hrs)
[2, 2, 2, 1, 2, 1, 1, 2, 2, 2, 3,
3]
Temperature inside WEB (K) 293
Environmental conditions
The mission specifications are as follows: The rover is expected to operate at 20° latitude.
Areocentric longitude of Mars about Sun during landing is assumed to be 180°. The rover
should be capable of climbing and des cending slopes up to 35° and also safely traverse
Everything we examined (3)
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