Logotipo del repositorio
Comunidades
Todo Digital INTA
Iniciar sesión
¿Nuevo Usuario? Pulse aquí para registrarse ¿Has olvidado tu contraseña?
  1. Inicio
  2. Buscar por autor

Examinando por Autor "Mora Rueda, Marcos"

Seleccione resultados tecleando las primeras letras
Mostrando 1 - 1 de 1
  • Resultados por página
  • Opciones de ordenación
  • Cargando...
    Miniatura
    PublicaciónAcceso Abierto
    Boulder exhumation and segregation by impacts on rubble-pile asteroids
    (Elsevier, 2022-07-21) Ormö, Jens; Raducan, Sabina D.; Jutzi, Martin; Herreros, Isabel; Luther, Robert; Collins, Gareth S.; Wünnemann, Kai; Mora Rueda, Marcos; Hamann, C.; European Commission; Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737
    Small asteroids are often considered to be rubble-pile objects, and such asteroids may be the most likely type of Near Earth Objects (NEOs) to pose a threat to Earth. However, impact cratering on such bodies is complex and not yet understood. We perform three low-velocity (≈ 400 m/s) impact experiments in granular targets with and without projectile-size boulders. We conducted SPH simulations that closely reproduced the impact experiments. Our results suggest that cratering on heterogeneous targets displaces and ejects boulders, rather than fragmenting them, unless directly hit. We also see indications that as long as the energy required to disrupt the boulder is small compared to the kinetic energy of the impact, the disruption of boulders directly hit by the projectile may have minimal effect on the crater size. The presence of boulders within the target causes ejecta curtains with higher ejection angles compared to homogeneous targets. At the same time, there is a segregation of the fine ejecta from the boulders, resulting in boulders landing at larger distances than the surrounding fine grained material. However, boulders located in the target near the maximum extent of the expanding excavation cavity are merely exhumed and distributed radially around the crater rim, forming ring patterns similar to the ones observed on asteroids Itokawa, Ryugu and Bennu. Altogether, on rubble-pile asteroids this process will redistribute boulders and finer-grained material heterogeneously, both areally around the crater and vertically in the regolith. In the context of a kinetic impactor on a rubble-pile asteroid and the DART mission, our results indicate that the presence of boulders will reduce the momentum transfer compared to a homogeneous, fine-grained target.
footer.link.logos.derechosLogo Acceso abiertoLogo PublicacionesLogo Autores
Logo Sherpa/RomeoLogo DulcineaLogo Creative CommonsLogo RecolectaLogo Open AireLogo Hispana

Dspace - © 2024

  • Política de cookies
  • Política de privacidad
  • Aviso Legal
  • Accesibilidad
  • Sugerencias