The Future of Stardust Science
A. J. Westphal, J. C. Bridges, D. E. Brownlee, A. L. Butterworth, B., T. De Gregorio, G. Dominguez, G. J. Flynn, Z. Gainsforth, H. A. Ishii, D., Joswiak, L. R. Nittler, R. C. Ogliore, R. Palma, R. O. Pepin, T. Stephan, M., E. Zolensky

TL;DR
This paper discusses the significance of Kuiper Belt objects as preserved remnants of early Solar System materials, highlights the contributions of the Stardust mission in sampling these objects, and outlines future scientific objectives to enhance our understanding of planetary formation.
Contribution
It introduces nine high-priority scientific objectives for future Stardust analyses to address unresolved questions in planetary science.
Findings
Stardust samples have led to over 142 publications and unexpected discoveries.
Kuiper Belt objects are key to understanding Solar System formation.
Samples from Stardust include the first solid interstellar medium particles.
Abstract
Recent observations indicate that >99% of the small bodies in the Solar System reside in its outer reaches --- in the Kuiper Belt and Oort Cloud. Kuiper Belt bodies are probably the best preserved representatives of the icy planetesimals that dominated the bulk of the solid mass in the early Solar System. They likely contain preserved materials inherited from the protosolar cloud, held in cryogenic storage since the formation of the Solar System. Despite their importance, they are relatively underrepresented in our extraterrestrial sample collections by many orders of magnitude (10 by mass) as compared with the asteroids, represented by meteorites, which are composed of materials that have generally been strongly altered by thermal and aqueous processes. We have only begun to scratch the surface in understanding Kuiper Belt objects, but it is already clear that the very…
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