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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.

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Microcracking Study of Carbon Fiber Composite Materials for Starshade Petals

We have conducted materials tests of representative carbon composite materials for starshade petals. The principal goal of these tests is to assess whether the level of microcracking of the materials as the petals are stowed or deployed (or even as they are handled during assembly) is likely to cause a problem with meeting the tight dimensional tolerances required for starlight suppression. Cracking can cause unexpected deformation, and the cracks can act as reservoirs for gases. It may also lead to roughening of the optical edge whose sharpness minimizes undesirable scattering of light. We use mechanical tests, microscopy, acoustic tomography and small‐angle x‐ray scattering to characterize the microcracking. These tests have found no large cracks (>100 microns) at bending strains up to 0.005, the strain at which audible popping occurred. The stress‐strain curves did not display any anomalies until a precipitous drop in stress at a strain of ~0.012 due to the formation of a transverse crack. Analysis of SAXS data is on‐going which will quantify microcrack distributions at the sub‐micron level. We find no large cracks (>100 microns) at the design strain tolerance for non‐critical structural elements (0.005); analysis is on‐going to quantify nanoscale cracking at the strains of critical structural elements (0.0005).

36 MATERIALS SCIENCE↗

Starshade Rendezvous Probe

The Starshade Rendezvous Probe Mission (https://smd-prod.s3.amazonaws.com/science-red/s3fs-public/atoms/files/Starshade2.pdf ) [1] will be the first space-based, high-contrast imaging mission with the potential to detect and characterize Earth-like planets in the habitable zone (HZ) around sunlike stars while at the same time exploring entire planetary systems about our nearest neighbors. Over the last two decades, astronomers have discovered and cataloged thousands of planets around other stars. Nevertheless, we have yet to find a planetary system like our own or to characterize discovered small planets to determine if they are similar to Earth. The next step in exploration is to image full planetary systems, including their HZs, and to obtain planetary spectra with enough sensitivity to determine if a planet is Earth-like. A space-based direct imaging mission to ultimately find and characterize other Earth-like planets is a long-term priority for space astrophysics [2, 3].

Seager, Sara↗