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A new approach on the long term dynamics of neo's under Yarkorsky effect
Cita
Peláez Álvarez, Jesús 
ORCID: https://orcid.org/0000-0001-9755-1674, Urrutxua, Hodei, Bombardelli, Claudio ORCID: https://orcid.org/0000-0002-9181-1487 and Pérez Grande, María Isabel ORCID: https://orcid.org/0000-0002-7145-2835
(2011).
A new approach on the long term dynamics of neo's under Yarkorsky effect.
En: "2011 AAS/AIAA Astrodynamics Specialist Conference, Girdwood, Alaska", 31/07/2011 - 04/08/2011, Girdwood, Alaska. pp. 561-577.
ORCID: https://orcid.org/0000-0001-9755-1674, Urrutxua, Hodei, Bombardelli, Claudio ORCID: https://orcid.org/0000-0002-9181-1487 and Pérez Grande, María Isabel ORCID: https://orcid.org/0000-0002-7145-2835
(2011).
A new approach on the long term dynamics of neo's under Yarkorsky effect.
En: "2011 AAS/AIAA Astrodynamics Specialist Conference, Girdwood, Alaska", 31/07/2011 - 04/08/2011, Girdwood, Alaska. pp. 561-577.
Descripción
| Título: | A new approach on the long term dynamics of neo's under Yarkorsky effect |
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| Autor/es: |
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| Tipo de Documento: | Ponencia en Congreso o Jornada (Artículo) |
| Título del Evento: | 2011 AAS/AIAA Astrodynamics Specialist Conference, Girdwood, Alaska |
| Fechas del Evento: | 31/07/2011 - 04/08/2011 |
| Lugar del Evento: | Girdwood, Alaska |
| Título del Libro: | AAS/AIAA Astrodynamics Specialist Conference July 31 ‐ August 4, 2011 Girdwood, Alaska |
| Fecha: | 2011 |
| Materias: | |
| ODS: | |
| Escuela: | E.T.S.I. Aeronáuticos (UPM) [antigua denominación] |
| Departamento: | Motopropulsión y Termofluidodinámica [hasta 2014] |
| Licencias Creative Commons: | Reconocimiento - Sin obra derivada - No comercial |
Resumen
To calculate the force associated with the Yarkovsky effect the temperature distribution on the surface of the asteroid should be determined; it depends on the asteroid orbit, size and shape, spin axis orientation and period, mass, density of surface layers, albedo, thermal conductivity, capacity and IR emissivity of the material. The uncertainty of many of these parameters invites to develop simplified methods to calculate the influence of the Yarkovsky effect on long term dynamics of asteroids. In this paper we present one of this method based in a special perturbation procedure developed in our group.
Más información
| ID de Registro: | 12629 |
|---|---|
| Identificador DC: | https://oa.upm.es/12629/ |
| Identificador OAI: | oai:oa.upm.es:12629 |
| Depositado por: | Memoria Investigacion |
| Depositado el: | 27 Feb 2013 09:06 |
| Ultima Modificación: | 27 Feb 2024 11:14 |
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