Trepo - Selaus asiasanan mukaan "115"

Viitteet 1-4 / 4

    • Analysis of full microwave propagation and backpropagation for a complex asteroid analogue via single-point quasi-monostatic data 

      Sorsa, Liisa-Ida; Pursiainen, Sampsa; Eyraud, Christelle (2020)
      article
      Information carried by the full wave field is particularly important in applications involving wave propagation, backpropa- gation, and a sparse distribution of measurement points, such as in tomographic imaging of a small ...

    • Asteroid (16) Psyche's primordial shape: A possible Jacobi ellipsoid 

      Ferrais, M.; Vernazza, P.; Jorda, L.; Rambaux, N.; Hanuš, J.; Carry, B.; Marchis, F.; Marsset, M.; Viikinkoski, M.; Brož, M.; Fetick, R.; Drouard, A.; Fusco, T.; Birlan, M.; Podlewska-Gaca, E.; Jehin, E.; Bartczak, P.; Berthier, J.; Castillo-Rogez, J.; Cipriani, F.; Colas, F.; Dudziński, G.; Dumas, C.; Ğ Urech, J.; Kaasalainen, M.; Kryszczynska, A.; Lamy, P.; Le Coroller, H.; Marciniak, A.; Michalowski, T.; Michel, P.; Santana-Ros, T.; Tanga, P.; Vachier, F.; Vigan, A.; Witasse, O.; Yang, B. (29.06.2020)
      article
      <p>Context. Asteroid (16) Psyche is the largest M-type asteroid in the main belt and the target of the NASA Psyche mission. It is also the only asteroid of this size (D> 200 km) known to be metal rich. Although ...

    • Evidence for differentiation of the most primitive small bodies 

      Carry, B.; Vernazza, P.; Vachier, F.; Neveu, M.; Berthier, J.; Hanuš, J.; Ferrais, M.; Jorda, L.; Marsset, M.; Viikinkoski, M.; Bartczak, P.; Behrend, R.; Benkhaldoun, Z.; Birlan, M.; Castillo-Rogez, J.; Cipriani, F.; Colas, F.; Drouard, A.; Dudziński, G. P.; Desmars, J.; Dumas, C.; Ďurech, J.; Fetick, R.; Fusco, T.; Grice, J.; Jehin, E.; Kaasalainen, M.; Kryszczynska, A.; Lamy, P.; Marchis, F.; Marciniak, A.; Michalowski, T.; Michel, P.; Pajuelo, M.; Podlewska-Gaca, E.; Rambaux, N.; Santana-Ros, T.; Storrs, A.; Tanga, P.; Vigan, A.; Warner, B.; Wieczorek, M.; Witasse, O.; Yang, B. (17.06.2021)
      article
      <p>Context. Dynamical models of Solar System evolution have suggested that the so-called P- and D-type volatile-rich asteroids formed in the outer Solar System beyond Neptune's orbit and may be genetically related ...

    • VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis 

      Vernazza, P.; Ferrais, M.; Jorda, L.; Hanuš, J.; Carry, B.; Marsset, M.; Brož, M.; Fetick, R.; Viikinkoski, M.; Marchis, F.; Vachier, F.; Drouard, A.; Fusco, T.; Birlan, M.; Podlewska-Gaca, E.; Rambaux, N.; Neveu, M.; Bartczak, P.; Dudziński, G.; Jehin, E.; Beck, P.; Berthier, J.; Castillo-Rogez, J.; Cipriani, F.; Colas, F.; Dumas, C.; ǦUrech, J.; Grice, J.; Kaasalainen, M.; Kryszczynska, A.; Lamy, P.; Le Coroller, H.; Marciniak, A.; Michalowski, T.; Michel, P.; Santana-Ros, T.; Tanga, P.; Vigan, A.; Witasse, O.; Yang, B.; Antonini, P.; Audejean, M.; Aurard, P.; Behrend, R.; Benkhaldoun, Z.; Bosch, J. M.; Chapman, A.; Dalmon, L.; Fauvaud, S.; Hamanowa, Hiroko; Hamanowa, Hiromi; His, J.; Jones, A.; Kim, D. H.; Kim, M. J.; Krajewski, J.; Labrevoir, O.; Leroy, A.; Livet, F.; Molina, D.; Montaigut, R.; Oey, J.; Payre, N.; Reddy, V.; Sabin, P.; Sanchez, A. G.; Socha, L. (12.10.2021)
      article
      Until recently, the 3D shape, and therefore density (when combining the volume estimate with available mass estimates), and surface topography of the vast majority of the largest (D ≥ 100 km) main-belt asteroids have ...