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The SAMLER-KI (Semi-autonomous Micro Rover for Lunar Exploration using Artificial Intelligence) project aims to open up further potential for future lunar micro rover missions. The focus is on the conceptual design of a micro rover with a higher level of autonomy and the ability to survive the lunar night. Achieving this capability requires a sophisticated thermal design to endure the harsh lunar environment and maintain acceptable temperatures not only during the extreme cold of the lunar night but also while addressing the power demands of autonomous exploration activities during daytime operations. Simultaneously, the structural design must withstand the vibration loads experienced during rocket launch. The design process is challenged by the conflicting requirements between the structural and thermal subsystems, further compounded by the mission’s mass requirement of 20 kg. An initial rover design has been developed in alignment with these requirements and the overall mission scenario. This paper presents a structural and thermal assessment of the preliminary rover design concept under mission-relevant load conditions. The analyses identify critical design weaknesses, including major parasitic thermal pathways and structurally vulnerable components. Although the current design does not yet meet the imposed requirements, the findings provide essential insights into critical areas that show potential for improvement. These results are expected to guide future iterations towards achieving a feasible and robust thermal and structural design.
Innovative solar system exploration missions require ever larger velocity increments and thus ever more demanding propulsion capabilities. Using for those high-energy missions the state-of-the-art technique of chemical propulsion in combination with (eventually multiple) gravity assist maneuvers results in long, complicated, and inflexible mission profiles. Low-thrust propulsions systems can significantly enhance or even enable those high-energy missions, since they utilize the propellant more efficiently - like electric propulsion systems - or do not consume any propellant at all - like solar sails, that utilize solely the freely available solar radiation pressure for propulsion. Consequently, low-thrust propulsion systems permit significantly larger velocity increments and/or larger payload ratios and/or smaller launch vehicles, while at the same time allowing direct trajectories with reduced flight times, simpler mission profiles, and extended launch windows. One of the most important tasks during the feasibility analysis and the preliminary design of a deep space mission is the design and the optimization of the interplanetary transfer trajectory. Searching trajectories for low-thrust spacecraft, that are optimal with respect to transfer time or propellant consumption, is usually a difficult and time-consuming task that involves a lot of experience and expert knowledge, since the convergence behavior of traditional optimizers, that are based on numerical optimal control methods, depends strongly on an adequate initial guess, which is often hard to find. Even if the optimizer converges to an "optimal" trajectory, this trajectory is typically close to the initial guess that is rarely close to the (unknown) global optimum. Within this work, trajectory optimization problems are attacked from the perspective of artificial intelligence and machine learning, which is quite different from that of optimal control theory. Inspired by natural archetypes, a smart method for spacecraft trajectory optimization - that fuses artificial neural networks and evolutionary algorithms to evolutionary neurocontrollers - is developed. Before the novel method is employed for the trajectory optimization and mission analysis of some exemplary deep space missions, its convergence behavior is evaluated and the quality of the obtained solutions is assessed. It is demonstrated, by re-calculating trajectories for several existing low-thrust problems, that this novel method can be applied successfully for near-globally optimal spacecraft steering. Since evolutionary neurocontrollers explore the trajectory search space more exhaustively than a human expert can do by using traditional optimal control methods, they are able to find spacecraft steering strategies that generate better trajectories, which are closer to the global optimum. Using evolutionary neurocontrollers, low-thrust trajectories can be optimized without an initial guess and without the permanent attendance of an expert in astrodynamics and optimal control theory. Their field of application may be extended to a variety of optimal control problems.
Our objective function value for the given mission is J = 1.2 with a secondary performance index T = 1,271 d. To find the optimal sequence of flyby bodies to solve the given problem, we have used an adapted version of InTrance [1-3]. Because InTrance is a purely global trajectory optimization program based on Artificial Neural Networks (ANN) and Evolutionary Algorithms (EA), its local optimization capabilities are rather poor. Therefore, its accuracy is typically limited to a final distance ΔR of about 10 5 km and a final relative velocity ΔV of about 100 m/s (to the respective target asteroid). Nevertheless, for single leg optimization it is possible to optimize with the accuracy requirements needed to solve the given problem. For trajectory integration, we have used a maximal integration error of 10 -10 . We have used the following stepwise approach: 1. We let InTrance find a promising rendezvous candidate out of 27 manually target asteroids 2. The first rendezvous to the determined target asteroid was optimized to fulfill the given accuracy requirements of 1,000 km in distance and 1 m/s relative velocity. 3. The steps 1 and 2 were again carried out for another target asteroid. 4. A flyby to the first found body was optimized and another rendezvous to another candidate out of the list of remaining targets. The transfer with the shortest flight time was chosen. 5. The steps 3 and 4 were repeated until no more rendezvous or flybys could be achieved. We are absolutely aware of the fact that this approach can by principle not yield a globally optimal trajectory as the key to success is the generation of a promising sequence of rendezvous and flybys, but further adaptation of our tools to the given problem was not possible in the given time.
The paper at hand evaluates the necessity of depicting topographic features like boulders on the lunar environment in thermal analyses for a size of up to 6.5 m in diameter. The question regarding the thermal influence becomes relevant when analysing a technical system within the lunar environment. This influence on the thermal behaviour of a test object is investigated in sensitivity studies. It is shown that the local surroundings can significantly alter a system’s net heat flux and can lead to overheating or critically cooling down instead of theoretically surviving when not considering local topographic features. Especially for small and lightweight systems ≤20 kg, like micro rovers, the effect of the surrounding on the system’s temperature becomes critical due to the low thermal capacity. Thus, it is a substantial aspect to be accounted for during the design phase as well as in mission operation.
The issue of the hazard to Earth from NEOs has received increased attention recently in the U.S. because of congressional interest in the topic. This resulted in a study by the National Academies' National Research Council. That study was released in January. The SpaceGuard survey was aimed at finding 90% of the NEOs greater than 1 km in diameter. The next generation of surveys, the George E. Brown Survey, should be targeted at finding 90% of the smaller ones (diameter ¿ 140m is specified in congressional legislation). Current estimates indicate that a reasonable number of small NEOs will be discovered with rather short warning times before impact. This means that we should have a plan for mitigation of the hazard. A wide variety of physical characteristics of NEOs is relevant to mitigation in likely scenarios. However, certain characteristics are particularly relevant to mitigation. This talk will address the conclusions of the NRC study regarding characterization of and missions to NEOs.
The present work assesses the ability of existing potential-methodologies to accurately estimate the induced drag of highly non-planar lifting systems. Based on a phenomenological study, the impact of wake modeling on the induced drag characteristics is exemplarily evaluated for a rectangular-shaped biplane and a box wing configuration. This includes the influence on associated key design parameters like the height-to-span ratio and the longitudinal staggering. Representing the classical analysis case, the effect of variation of the freestream projected height-to-span ratio with the angle of attack is investigated for fixed geometric properties. For any non-zero staggering, non-linear wing-wake interactions, introduced by the rolled-up and force-free wake shape, are revealed to have noticeable influence on the estimation for the box wing configuration. In contrast to the biplane, the entire substitution of the force-free wake is not feasible. An accurate estimation involving higher angles of attack is found to be generally problematic.
Obstacle encounter probability dependent local path planner for UAV operation in urban environments
(2024)
Unmanned aerial vehicles (UAVs) are well-suited for various short-distance missions in urban environments. However, the path planner of such UAV is constantly challenged with the choice between avoiding obstacles horizontally or vertically. If the path planner relies on sensor information only, i.e. the path planner is a local planner, usually predefined manoeuvres or preferences are used to find a possible way. However, this method is stiff and inflexible. This work proposes a probabilistic decision-maker to set the control parameters of a classic local path planner during a flight mission. The decision-maker defines whether performing horizontal or vertical avoidance is preferable based on the probability of encountering a given number of obstacles. Here, the decision-maker considers predictions of possible future avoidance manoeuvres. It also defines an ideal flight altitude based on the probability of encountering obstacles. This work analyses the building height of all European capital cities and the probability of encountering obstacles at different altitudes to feed the decision-maker. We tested the feasibility of the proposed decision-maker with the 3DVFH*, a commonly used local path planner, in multiple simulations. The proposed probabilistic decision-maker allows the local path planner to reach the goal point significantly more often than the standard version of the 3DVFH*.