Matches in SemOpenAlex for { <https://semopenalex.org/work/W9281483> ?p ?o ?g. }
Showing items 1 to 71 of
71
with 100 items per page.
- W9281483 startingPage "61" @default.
- W9281483 abstract "Asynchronous binary asteroids have been found to be abundant among fast-spinning near-Earth asteroids (NEAs) smaller than 2 km in diameter; Pravec et al. (2005, Icarus, submitted) derived that 15 +/4 % of NEAs in the size range 0.3 to 2 km are binary with the secondary-to-primary mean diameter ratio >=0.18. The early results from the surveys of the Vesta family and the Hungaria group (Ryan et al., 2004, Planet. Space Sci. 42, 1093; 2004, Bull. Amer. Astron. Society 36, 1181; Warner et al., 2005, IAU Circ. 8511) suggest that the population extends beyond the region of terrestrial planets, but with characteristics shifted to larger sizes and longer periods; the four known binaries in the Vesta family/Hungaria group are 3 to 6 km large and they have primary rotation periods in a range of 3 to ~4 h, i.e., on the tail of the distribution of primary rotation periods of NEAs. The comparison suggests that formation and evolution mechanisms of asynchronous NEA and main-belt binaries may be similar and are related to their fast spins and rubble-pile structure. None of the current theories of their formation of evolution, however, explains the observed properties of both NEA and main-belt asynchronous binaries in full. We have established a collaborative observational program, called Photometric Survey for Asynchronous Binary Asteroids to discover and describe asynchronous binaries over a range of heliocentric distances from NEAs through Mars-crossers to inner main-belt asteroids. One new binary Amor asteroid, 2005 AB has been found during the first few months of the survey operation (Reddy et al., 2005, IAU Circ. 8483), and we have obtained follow-up data for two other binary systems. I outline the motivations, the technique, and the strategy of the Survey." @default.
- W9281483 created "2016-06-24" @default.
- W9281483 creator A5037076052 @default.
- W9281483 date "2005-05-01" @default.
- W9281483 modified "2023-09-26" @default.
- W9281483 title "Photometric Survey for Asynchronous Binary Asteroids" @default.
- W9281483 cites W1661810726 @default.
- W9281483 cites W2006728351 @default.
- W9281483 cites W2035542287 @default.
- W9281483 cites W2064106185 @default.
- W9281483 cites W2075404505 @default.
- W9281483 cites W2116003137 @default.
- W9281483 cites W2118596075 @default.
- W9281483 cites W2137144885 @default.
- W9281483 cites W2139359797 @default.
- W9281483 cites W3045929403 @default.
- W9281483 hasPublicationYear "2005" @default.
- W9281483 type Work @default.
- W9281483 sameAs 9281483 @default.
- W9281483 citedByCount "2" @default.
- W9281483 crossrefType "journal-article" @default.
- W9281483 hasAuthorship W9281483A5037076052 @default.
- W9281483 hasConcept C121332964 @default.
- W9281483 hasConcept C127313418 @default.
- W9281483 hasConcept C1276947 @default.
- W9281483 hasConcept C144024400 @default.
- W9281483 hasConcept C149923435 @default.
- W9281483 hasConcept C2908647359 @default.
- W9281483 hasConcept C44870925 @default.
- W9281483 hasConcept C51244244 @default.
- W9281483 hasConcept C58142911 @default.
- W9281483 hasConcept C87355193 @default.
- W9281483 hasConceptScore W9281483C121332964 @default.
- W9281483 hasConceptScore W9281483C127313418 @default.
- W9281483 hasConceptScore W9281483C1276947 @default.
- W9281483 hasConceptScore W9281483C144024400 @default.
- W9281483 hasConceptScore W9281483C149923435 @default.
- W9281483 hasConceptScore W9281483C2908647359 @default.
- W9281483 hasConceptScore W9281483C44870925 @default.
- W9281483 hasConceptScore W9281483C51244244 @default.
- W9281483 hasConceptScore W9281483C58142911 @default.
- W9281483 hasConceptScore W9281483C87355193 @default.
- W9281483 hasLocation W92814831 @default.
- W9281483 hasOpenAccess W9281483 @default.
- W9281483 hasPrimaryLocation W92814831 @default.
- W9281483 hasRelatedWork W1615946943 @default.
- W9281483 hasRelatedWork W1667456944 @default.
- W9281483 hasRelatedWork W1969018290 @default.
- W9281483 hasRelatedWork W1978569623 @default.
- W9281483 hasRelatedWork W2059988943 @default.
- W9281483 hasRelatedWork W2060416392 @default.
- W9281483 hasRelatedWork W2089104496 @default.
- W9281483 hasRelatedWork W2536388523 @default.
- W9281483 hasRelatedWork W2609006042 @default.
- W9281483 hasRelatedWork W2754711580 @default.
- W9281483 hasRelatedWork W2779485105 @default.
- W9281483 hasRelatedWork W2911820169 @default.
- W9281483 hasRelatedWork W2951716568 @default.
- W9281483 hasRelatedWork W2979919192 @default.
- W9281483 hasRelatedWork W3041855551 @default.
- W9281483 hasRelatedWork W3084866254 @default.
- W9281483 hasRelatedWork W3105782835 @default.
- W9281483 hasRelatedWork W3147631179 @default.
- W9281483 hasRelatedWork W633941908 @default.
- W9281483 hasRelatedWork W2905355221 @default.
- W9281483 hasVolume "24" @default.
- W9281483 isParatext "false" @default.
- W9281483 isRetracted "false" @default.
- W9281483 magId "9281483" @default.
- W9281483 workType "article" @default.