European component of the AIDA mission: science investigation of a binary system

Bibcode
2018EPSC...12..620M
Michel, P.; Küppers, Michael; Biele, Jens; Campo Bagatin, Adriano; Carry, Benoît; Charnoz, Sébastien; Fitzsimmons, Alan; Green, Simon; Hérique, Alain; Jutzi, Martin; Karatekin, Ozgur; de Leon, J.; Murdoch, Naomi; Pravec, Petr; Sierks, Holger; Tortora, Paolo; Tsiganis, Kleomenis; Vincent, Jean-Baptiste; Wünnemmann, Kai; Carnelli, Ian
Referencia bibliográfica

European Planetary Science Congress 2018, held 16-21 September 2018 at TU Berlin, Berlin, Germany, id.EPSC2018-620

Fecha de publicación:
9
2018
Número de autores
20
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
Hera provides a robust and cost-effective means to perform a planetary defense validation test with a solid balance between risk and innovation. In the frame of the AIDA collaboration, Hera contributes to a truly international planetary defense initiative. It will bring completely new knowledge and insights on asteroid science that will be of great benefit to those seeking a deeper understanding of the processes underlying solar system formation.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    ROSALIA: ROman Sky Analyst for Low surface brightness Imaging & Astronomy
    Diffuse emission in the outskirts of galaxies, such as stellar tidal streams, galaxy stellar halos and intracluster light, provides important constraints on the structure and evolution of the Universe. However, such low surface brightness diffuse emission can be up to thousands of times dimmer (>29 AB mag/[square arcseconds]) than the sky
    Laine, Seppo et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024AAS...24412902L
    Número de citas
    0
  • Sin árbitro
    A Systematic Search for and Characterization of White Dwarf Binaries Across the H-R Diagram
    White dwarfs (WDs) are the endpoint of evolution for 97% of stars. Most of these stars are in multiple systems, and a significant fraction of those are compact enough to exchange mass, altering the structures and subsequent evolution of both stars. The physical mechanisms that facilitate these mass exchanges include common envelope evolution, Roche
    Anguiano, Borja et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024AAS...24410807A
    Número de citas
    0
  • Sin árbitro
    The molecular gas perspective on the growth and death of H emitters in the Spiderweb protocluster at Alpha z=2.16
    Galaxy clusters at low redshift are dominated by massive quiescent galaxies hosting stellar populations 10 Gyrs old, indicating that they were formed in the early universe when clusters were still in the process of being assembled (i.e., protoclusters). The rapid growth of galaxies within protoclusters is driven by the efficient transformation of
    Martinez, J. M. P.

    Fecha de publicación:

    3
    2024
    Bibcode
    2024aecc.conf...12M
    Número de citas
    0