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The best-fit orientation of the asteroid's spin axis is determined to be $\\lambda =237.7^\\circ$ and $\\beta=-83.8^{\\circ}$ considering the observation uncertainties, and its rotation period is $\\sim$ 3.5935 h . Using the derived shape model, we adopt the so-called advanced thermophysical model (ATPM) to fit three published sets of mid-infrared observations of 1996 FG3 \\citep{Wolters2011,Walsh2012}, so as to evaluate its surface properties."},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1401.5357","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2014-01-21T15:58:32Z","cross_cats_sorted":[],"title_canon_sha256":"3810f4f83478765a844a3db33be2a03261ebc985e5ed0fd1fe75adce404704eb","abstract_canon_sha256":"9ab73301721151bd704fac9d9a85baaa0a124d7c8c448a20e23a1444af022a5d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:55:19.221219Z","signature_b64":"dhQbOu+m9nPNRfvMt37lAvqt8pNCS4Wox+LcrX4frtzssodmaBfkhzEHOcFUyu+5Gb9kO3cvYcXFtVOMw0/qAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e6e4c2d27288e64ad77bf20a0ae36a73860e53064d3fcb480c0f10ba85d8e6ff","last_reissued_at":"2026-05-18T02:55:19.220694Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:55:19.220694Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Shape, Thermal and Surface Properties determination of a Candidate Spacecraft Target Asteroid (175706) 1996 FG3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Jianghui Ji, LiangLiang Yu, Su Wang","submitted_at":"2014-01-21T15:58:32Z","abstract_excerpt":"In this paper, a 3D convex shape model of (175706) 1996 FG3, which consists of 2040 triangle facets and 1022 vertices, is derived from the known lightcurves. 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