On 29th September 2022, the airborne observatory SOFIA flew its final science flight, concluding nearly 12 years of successful science operations. While the Astro2020 review has enabled the possibility of a NASA far-IR probe mission, such a platform - if realized instead of the alternative X-ray option - would likely not observe at best until the early-2030s. Therefore, for at least the next decade, the wavelength regime between ~30-300 µm has become inaccessible to the international community, aside from an assortment of upcoming and planned balloon-borne missions. This regime encompasses a range of key astrophysical observables across multiple spatial scales - from local star-forming cores, to molecular cloud complexes, to entire galaxies. As demonstrated by SOFIA observations, these include tracers of star formation & feedback, strong gas cooling lines, and diagnostics of dense ISM morphology, dynamics & polarization. The launch of JWST has opened new possibilities in the near- and mid-IR universe; however, the lack of complementary access to the far-IR will hamper our understanding of key concepts. In this paper, we will overview some of SOFIA’s science highlights, and present a number of major science cases for continuing far-IR observations. We will outline ongoing efforts to reprocess and preserve SOFIA’s scientific and technical archive. Finally, we will discuss how SOFIA’s scientific legacy was enabled by particular instrumentation & platform capabilities, establish where and how these capabilities can be improved upon, and place these in the context of future airborne and spaceborne far-IR mission proposals and concepts.
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