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1.INTRODUCTIONCurrently, the so-called Old Space projects, in which only individual assemblies are manufactured, are the state of the art for optical applications in space. The Fraunhofer IOF develops and manufactures high performance optics for Earth oberservation and interplanetary research like the DESIS telescope and spectrometer, which is oberserving vegetation health or water quality from the ISS since 2018 [8]. Another example for instruments built by the Fraunhofer IOF is the receiver telescope for the Ganymede Laser Altimeter as part of ESA’s JUICE mission to explore Jupiter’s Icy Moons. For these systems, a high level of risk mitigation is required. This means, that only well-known processes with a high technological readiness level comes into consideration. Especially for mechanical development regarding light weighting, the design is limited by conventional manufacturing processes like CNC milling. On the other hand, the area of New Space will launch hundreds of nano satellites [9] (e.g. for laser communication or daily Earth observation [10]) in the next few years. For these satellites, advanced light-weighted and very stiff telescopes (to be more independent from the selection of the launcher) are more important than before and thus, modern technologies like topology optimization and additive manufacturing becoming more and more interesting. These technologies allow for optimal and load-balanced material distribution and can thus increase the specific stiffness of the assembly. Further benefit is be generated by saving manufacturing time and material costs. 2.OPTICAL AND MECHANICAL DESIGNThe telescope used as a benchmark for the optimization follows the principle of a three-mirror-anastigmat (TMA) with a focal length of 175 mm and an F/4 aperture. Such telescopes are typically used in small Earth-observing satellites [11,12]. The TMA relies on three rotationally symmetric aspheric mirrors arranged on a common optical axis. In order to simplify the alignment of the system, two of those mirrors (M1 and M3) will be arranged on a common substrate [13] (see Figure 3). The mechanical design of the telescope is based on conventional methods for light-weighting. Thus, a ribbed housing and a cross drilled mirror substrate are used. The mass is about 2 kg and the external dimensions are 210 mm x 130 mm x 110 mm. In addition to the housing, which serves both as a mechanical structure and as a straylight baffle, the mirror substrate M1M3 and the mirror M2 of the telescope consists of bipods as well, which compensate interface errors and thermal gradients. 3.OPTIMIZATIONTo reduce the mass of the components as far as possible and to make the best possible use of the design freedoms given by the additive manufacturing process, two different optimizations are used. The optimization of the lightweight structure for the M1M3 mirror module is briefly described. The focus is on the topology optimization of the housing. 3.1Mirrors light-weighted by foam structuresThe mirror is filled inside with a stochastic Voronoi foam [14]. The density distribution of the foam is based on static load cases, resulting in a smaller cell size next to the interfaces for mounting at the housing. In addition to the front side, on which the functional areas are located, the backside has a closed surface as well, and thus, a high bending stiffness is generated (see Figure 5). The mass could be reduced to 44 % compared to the massive component and is thus slightly below the conventional light-weighted design, which was produced by cross-drilling. In addition, the stiffness can be increased, resulting in a significant increase for the specific stiffness. Table 1:Mass and eigenfrequencies of the optimized mirror substrate
Due to the high eigenfrequencies, which are above the typical incitation frequencies, the substrate is insensitive to random vibration. 3.2Topology optimization of the housingFor the housing, a topology optimization is used. A defined envelope curve is required for the optimization, in which the material can be manipulated by the optimization algorithm. The envelope has to provide the interfaces to the other components and the straylight baffle, as shown in Figure 6. The most critical load case for this type of mechanical structure is typically random vibration. Since topology optimizations based on random analyses are currently not possible and at the same time the combination of two time-intensive simulations is not reasonable, substitute loads have to be generated. The generation of these substitute loads is similar to a primary notching process, because only the force reaction at the boundary conditions and not the interface forces can be determined in a random analysis. Because the stresses caused by random vibration depend not only on the excitation, damping, and eigenfrequencies, but also on mass and stiffness, the Young’s modulus and density of the envelope are reduced to produce resilient loads. Therefore, the Young’s modulus and the density are multiplied by the expected lightweight factor ϕ. This model is now used to perform random analyses for the x-, y-, and z-directions and the forces reactions at the boundary conditions can be determined. In the next step, the model is accelerated with a quasi-static load (QSL) in x, y, and z and the results are scaled until the same forces occur at the boundary conditions. For the scaled QSL, the interface forces can be simulated and used for topology optimization. A fine and uniform mesh is used for the topology optimization. By a linear element order, the number of nodes can be reduced. The increased stiffness of the elements obtained is accepted for the optimization. In the recalculation of the result, a quadratic element order is then used. With an element size of 1.5 mm, the model consists of approx. 1.5 million elements. The interfaces and the stray light baffle must remain after the optimization and are therefore excluded from the design region. The following objectives are used for the optimization:
The used quasi-static-loads (QSL) were determined in the previous section. With an increase of the 7th mode under freefree conditions, the result has only six rigid-body modes and thus, a coherent body is obtained. Increasing the 1st mode with iso-static mounting reduces the sensitivity to random vibration. The minimum structure size should be at least twice the element size to avoid hourglass effects. 3.3Smoothing and regenerationAfter optimization, the result must be prepared for additive manufacturing, otherwise the non-continuous removal of elements would result in a very rough surface and there might not be enough material at the interfaces for a subsequent CNC milling process. Three steps are necessary: 3.4Results of topology optimized housingAfter smoothing the model, simulations can be performed with the optimized housing to validate the results. The results of the topology optimization are compared again to the massive envelope model and the conventional ripped housing. Compared to the massive envelope, the mass was reduced to 32 % and thus, the specified lightweight factor of 30 % was well met and is below the mass of the ribbed housing. The difference is more significant for the eigenfrequencies. Thus, the topology-optimized housing is 20 % more stiffly than the ribbed one. In summary, the specific stiffness could also be increased significantly. Table 2:Mass and eigenfrequencies of the optimized housing
The eigenfrequencies were determined under free-free conditions to evaluate the stiffness independent of boundary conditions. The 1st mode shows a global deformation of the housing in each case (see Figure 11). 4.ADDITIVE MANUFACTURING AND FURTHER PROCESS CHAINThe mirror and housing are additively manufactured using a selective laser melting (SLM) system as described in [7] and [14]. The parts can be further processed using the established manufacturing chain after removing the support structure. For the housing, this can be only CNC milling and diamond turning of the interfaces. For the mirror substrate, the complete process chain for high performance optics including plating with electroless nickel, shape correction, various polishing processes, and a high-reflective coating is required. The processes work almost independently of whether the component has been produced conventionally with CNC milling or using additive manufacturing. The process chain is shown in Figure 12. 5.TESTINGIn order to validate the FE simulations, especially for such a complex structure, vibration tests are carried out to determine the eigenfrequencies and to verify the load capacity. The test-setup is shown in Figure 13. 5.1Low-level sine searchFor the low-level sine search, the TMA was accelerated in the frequency range 5-2000 Hz with a sine-incitation of 0.5 g. The acceleration sensors show a significant increase of the response acceleration, when reaching the eigenfrequencies due to resonances. The comparison with the simulated harmonic analyses shows that only small deviations below 8 % occur between test and simulation of the eigenfrequency. For most modes, the deviation is much smaller. 5.2Random vibrationTo verify the loading capacity of the TMA, a random vibration test is performed with a broadband excitation in the x-, y-, and z-directions. A low-level sine test is performed before and after each random load case in order to determine the eigenfrequencies of the TMA. A change in the eigenfrequencies would indicate damage to the assembly. The change in the dominant eigenfrequencies (high effective masses in the translatory directions) are less than 1 %. It can therefore be assumed that the TMA is not damaged by the random vibration test. Table 3:Changes in the dominant eigenfrequencies due to random vibration testing
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