Astrofísicas: Objetos cercanos a la Tierra

  • Publicación
    Regional Photometric Modeling of Asteroid (101955) Bennu
    We present a regional photometric analysis of asteroid (101955) Bennu, using image data from the MapCam color imager of the OSIRIS-REx Camera Suite (OCAMS)...
  • Publicación
    Spectral Rotational Characterization of the Didymos System prior to the DART Impact
    The smallest member of the Didymos binary near-Earth object system (Dimorphos) is the target of the DART/LICIACube mission, the first attempt to change the...
  • Publicación
    Spin-driven evolution of asteroids' top-shapes at fast and slow spins seen from (101955) Bennu and (162173) Ryugu
    Proximity observations by OSIRIS-REx and Hayabusa2 provided clues on the shape evolution processes of the target asteroids, (101955) Bennu and (162173) Ryugu...
  • Publicación
    Surface Heterogeneity, Physical, and Shape Model of Near-Earth Asteroid (52768) 1998 OR2
    On 2020 April 29, the near-Earth object (52768) 1998 OR2 experienced a close approach to Earth at a distance of 16.4 lunar distances (LD). 1998 OR2 is a...
  • Publicación
    The binary near-Earth Asteroid (175706) 1996 FG3 - An observational constraint on its orbital evolution
    Using our photometric observations taken between April 1996 and January 2013 and other published data, we derived properties of the binary near-Earth Asteroid...
  • Publicación
    The ESA Hera Mission: Detailed Characterization of the DART Impact Outcome and of the Binary Asteroid (65803) Didymos
    Hera is a planetary defense mission under development in the Space Safety and Security Program of the European Space Agency for launch in 2024 October. It will...
  • Publicación
    The Second International Asteroid Warning Network Timing Campaign: 2005 LW3
    The Earth close approach of near-Earth asteroid 2005 LW3 on 2022 November 23 represented a good opportunity for a second observing campaign to test the timing...
  • Publicación
    Visible spectroscopy of the Polana-Eulalia family complex: Spectral homogeneity
    The Polana-Eulalia family complex is located in the inner part of the asteroid belt, bounded by the ν6 and the 3:1 resonances, where we can find another three...