Europlanet Science Congress 2020
Virtual meeting
21 September – 9 October 2020
Europlanet Science Congress 2020
Virtual meeting
21 September – 9 October 2020
EPSC Abstracts
Vol.14, EPSC2020-1064, 2020
https://doi.org/10.5194/epsc2020-1064
Europlanet Science Congress 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Potential Flyby Targets for the ESA Hera Mission

Alan Fitzsimmons1, Michael Khan2, Michael Küppers3, Patrick Michel4, and Petr Pravec5
Alan Fitzsimmons et al.
  • 1Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast, UK
  • 2ESA/ESOC, European Space Operations Center, Darmstadt, Germany
  • 3ESA/ESAC, Operations Department, European Space Astronomy Center, Villanueva de la Canada (Madrid), Spain
  • 4Universite Côte d'Azur, Observatoire de la Côte d'Azur, Centre National de la Recherche Scientifique, Laboratoire Lagrange, Nice, France
  • 5Astronomical Institute, Academy of Sciences of the Czech Republic, Ondrejov, Czech Republic

The Hera mission is the planetary defence mission approved under the ESA Space Safety Programme. Together with the NASA DART mission, it is the first Asteroid Deflection Demonstration. DART will impact Dimorphos, the natural satellite of Near Earth Asteroid Didymos, in 2022. Using the kinetic impactor technology, it will demonstrate the ability to change the trajectory of a small asteroid. Hera will launch in 2024 and arrive in the Didymos system at the end of 2026. Its primary goals are to accurately measure the mass of Dimorphos and to characterise the crater and effect of the DART impact on this small asteroid.

Hera will spend over 2 years matching orbits with Didymos, travelling through near-Earth space and the inner main-belt. This potentially allows Hera to perform an additional asteroid flyby enroute to Didymos.  For such a flyby, a number of factors need to be considered for target selection. Primary factors are the accuracy of the orbit of the asteroid, and distance from the nominal trajectory. Resolution of geomorphology requires a minimum number of spatial resolution elements at the desired flyby distance.  Previous observations on the form of lightcurves, colours or spectra are important for flyby science planning. Finally, a dynamical class of asteroid may be targeted for specific science priorities.

Analysis of the nominal trajectory shows approximately 100 asteroids passing the nominal position of Hera within 0.02 au. Ten of these potential targets are Near-Earth Asteroids, the rest being Mars-crossers and main-belt asteroids. We will present our current knowledge on these targets, and highlight the highest priority targets for further observation in the next 2-3 years. Although ground-based reconnaissance has started on some targets, further observations are required to support the flyby planning process.

Figure 1. Osculating orbital elements of asteroids passing close to Hera on its nominal trajectory to the Didymos system, without any additional trajectory adjustment. Red dots indicate a current flyby distance d < 0.01 au, blue circles indicate a current flyby distance 0.01 au < d < 0.02 au. The solid line indicates a perihelion distance of 1.3 au, asteroids to the left of this line are Near-Earth Asteroids.

How to cite: Fitzsimmons, A., Khan, M., Küppers, M., Michel, P., and Pravec, P.: Potential Flyby Targets for the ESA Hera Mission, Europlanet Science Congress 2020, online, 21 September–9 Oct 2020, EPSC2020-1064, https://doi.org/10.5194/epsc2020-1064, 2020

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