{"paper":{"title":"Orbit and Bulk Density of the OSIRIS-REx Target Asteroid (101955) Bennu","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Andrea Milani, Benjamin Rozitis, Dante S. Lauretta, Davide Farnocchia, David Vokrouhlicky, Ellen S. Howell, Federica Spoto, Jean-Luc Margot, Joshua P. Emery, Lance A. M. Benner, Michael C. Nolan, Michael W. Busch, Patrick A. Taylor, Paul W. Chodas, Steven R. Chesley, William F. Bottke","submitted_at":"2014-02-23T02:48:49Z","abstract_excerpt":"The target asteroid of the OSIRIS-REx asteroid sample return mission, (101955) Bennu (formerly 1999 RQ$_{36}$), is a half-kilometer near-Earth asteroid with an extraordinarily well constrained orbit. An extensive data set of optical astrometry from 1999--2013 and high-quality radar delay measurements to Bennu in 1999, 2005, and 2011 reveal the action of the Yarkovsky effect, with a mean semimajor axis drift rate $da/dt = (-19.0 \\pm 0.1)\\times 10^{-4}$ au/Myr or $284\\pm 1.5\\;\\rm{m/yr}$. The accuracy of this result depends critically on the fidelity of the observational and dynamical model. As a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1402.5573","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}