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Here, we analyse the orbit of the recently discovered asteroid 2012 XE133 with H = 23.5 mag to conclude that it is a new Venus co-orbital currently following a transitional trajectory between Venus' Lagrangian points L5 and L3. The object could have been a 1:1 librator for several thousand years and it may leave"},"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":"1303.3705","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2013-03-15T08:39:37Z","cross_cats_sorted":[],"title_canon_sha256":"68efed6b965e188c51d1c18896a9bf81d8e6145770155b5637d4dd8f832d744a","abstract_canon_sha256":"7622f753e9bf3962a40ea6d013b28188b7e532f966672248138eede89c70210c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:24:52.347873Z","signature_b64":"WaCW86s4Rbavj9lDedaXCJv9/YOeTyTtlelvopD65qFhBM5qoQ+pSRlbu7pIsEjeKQMQxnPLuYZQjOGcwR83Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8b736dffe72886ccda3eb97e1ebb56b3e5ab9e0a1cfafeb0430733ada7c2a6f0","last_reissued_at":"2026-05-18T03:24:52.347361Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:24:52.347361Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Asteroid 2012 XE133: a transient companion to Venus","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"C. de la Fuente Marcos, R. de la Fuente Marcos","submitted_at":"2013-03-15T08:39:37Z","abstract_excerpt":"Apart from Mercury that has no known co-orbital companions, Venus remains as the inner planet that hosts the smallest number of known co-orbitals (two): (322756) 2001 CK32 and 2002 VE68. Both objects have absolute magnitudes 18 < H < 21 and were identified as Venus co-orbitals in 2004. Here, we analyse the orbit of the recently discovered asteroid 2012 XE133 with H = 23.5 mag to conclude that it is a new Venus co-orbital currently following a transitional trajectory between Venus' Lagrangian points L5 and L3. 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