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https://hdl.handle.net/10316/4391
Title: | The population of Near Earth Asteroids in coorbital motion with Venus | Authors: | Morais, M. H. M. Morbidelli, A. |
Keywords: | Asteroids, dynamics; Resonances | Issue Date: | 2006 | Citation: | Icarus. 185:1 (2006) 29-38 | Abstract: | We estimate the size and orbital distributions of Near Earth Asteroids (NEAs) that are expected to be in the 1:1 mean motion resonance with Venus in a steady state scenario. We predict that the number of such objects with absolute magnitudes H<18 and H<22 is 0.14±0.03 and 3.5±0.7, respectively. We also map the distribution in the sky of these Venus coorbital NEAs and we see that these objects, as the Earth coorbital NEAs studied in a previous paper, are more likely to be found by NEAs search programs that do not simply observe around opposition and that scan large areas of the sky. | URI: | https://hdl.handle.net/10316/4391 | DOI: | 10.1006/icar.2002.6937 | Rights: | openAccess |
Appears in Collections: | FCTUC Física - Artigos em Revistas Internacionais |
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file98152bb0bad44604b2daaa66630924c4.pdf | 876.24 kB | Adobe PDF | View/Open |
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