ExploreNEOs III: Physical characterization of 65 low-deltaV NEOs
Michael Mueller, M. Delbo', J. L. Hora, D. E. Trilling, B., Bhattacharya, W. F. Bottke, S. Chesley, J. P. Emery, G. Fazio, A. W. Harris,, A. Mainzer, M. Mommert, B. Penprase, H. A. Smith, T. B. Spahr, J. A., Stansberry, C. A. Thomas

TL;DR
This study provides new size and albedo constraints for 65 low-deltaV near-Earth objects using thermal infrared data, aiding target selection for future space missions, including potential manned missions.
Contribution
It offers the first detailed physical characterization of 65 low-deltaV NEOs, expanding the dataset crucial for mission planning and understanding NEO compositions.
Findings
65 NEOs characterized in size and albedo
Identification of potential primitive, volatile-rich objects
Enhanced dataset for mission target selection
Abstract
Space missions to NEOs are being planned at all major space agencies, and recently a manned mission to an NEO was announced as a NASA goal. Efforts to find and select suitable targets (plus backup targets) are severely hampered by our lack of knowledge of the physical properties of dynamically favorable NEOs. In particular, current mission scenarios tend to favor primitive low-albedo objects. For the vast majority of NEOs the albedo is unknown. Here we report new constraints on the size and albedo of 65 NEOs with rendezvous deltaV < 7 km/s. Our results are based on thermal-IR flux data obtained in the framework of our ongoing (2009--2011) ExploreNEOs survey (Trilling et al. 2010) using NASA's "Warm Spitzer" space telescope. As of 2010 July 14, we have results for 293 objects in hand (including the 65 low-deltaV NEOs presented here); before the end of 2011 we expect to have measured…
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Taxonomy
TopicsComputational Physics and Python Applications · Gamma-ray bursts and supernovae · Particle accelerators and beam dynamics
