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The Payload and Operations of the Hera MissionOn 26 September 2022, NASA’s DART mission successfully impacted on Dimorphos, the secondary of the binary asteroid Didymos. DART released the Light Italian Cubesat for Imaging of Asteroids (LICIACube) two weeks before the impact, and LICIACube flew by the asteroids three minutes after the impact. On approach, DART took images of both asteroids, which, supported by additional imagery from LICIACube, characterized the pre-impact state of the Didymos system. DART changed the orbit of Dimorphos around Didymos, reducing its orbital period by 33 minutes.

DART will be followed by a detailed investigation of the Didymos system and the outcome of the impact by ESA’s Hera mission. Hera will be launched in October 2024 and arrive at Didymos in early 2027. The presentation will focus on the payload of the Hera mission and the operations at the asteroid system.

The main objectives of the Hera mission are to:
- Measure the mass of Dimorphos to accurately measure the momentum transfer efficiency of the DART impact.
- Characterise the change of the surface of Dimorphos by DART, including the properties (and existence!) of the DART crater, to improve our understanding of impact physics and to observe unweathered material, recently exposed at the surface.
- Determine the physical properties of Dimorphos, including its internal structure, to allow scaling of the impact to different types of asteroids.
- Measure the dynamical and physical state of the Didymos and Dimorphos system to constrain binary formation scenarios.

Hera is equipped with the following payload:

  1. Two Asteroid Framing Cameras (AFCs) for both science and navigation.
    There resolution is ~10-4 rad/pixel, or 40 cm/pixel for close observations from
    4 km. They will provide the target global properties as well as local
    geomorphology and will investigate the crater and impact site. They will also
    measure the mass of Dimorphos through the “wobble” motion of Didymos.

  2. The Planetary ALTimeter (PALT) will measure the distance to the target and shape and topography information complementary to that from AFC images.

  3. The Thermal InfraRed Imager (TIRI) will provide information about the thermal
    properties of the Didymos system and spectral information in the mid-infrared
    (6 bands from 7 – 14 µm).

  4. The Hyperscout-H hyperspectral imager will provide mineralogical information
    from 25 spectral bands between 665 and 975 nm.

  5. Milani, a 6 unit cubesat, will carry a visible to near-IR imaging spectrometer
    (ASPECT, 500 – 2500 nm) to derive mineralogical information on the
    composition of the asteroids, and a thermogravimeter (VISTA) to measure the
    abundance and constrain the composition of ambient dust particles.

  6. Juventas, a 6 unit cubesat, will carry a monostatic low-frequency radar
    (JuRa), and a gravimeter (GRASS) to derive interior and surface properties of
    the asteroids.

  7. The Radio Science experiment will measure the gravity field of the Didymos
    system. Measurements of the acceleration of the Hera spacecraft by the
    asteroid pair through the radio link between Earth and Hera will be used as
    well as the inter-satellite link between Hera and the two cubesats.


We will describe how the goals of Hera will be achieved with the different payload
elements.
Document ID
20230002154
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Michael Küppers
(European Space Astronomy Centre Madrid, Spain)
Patrick Michel ORCID
(Observatoire de la Côte d’Azur Nice, France)
Paul A. Abell
(Johnson Space Center Houston, Texas, United States)
Alan Fitzsimmons
(Queen's University Belfast Belfast, United Kingdom)
Simon F. Green
(The Open University Milton Keynes, United Kingdom)
Monica Lazzarin
(University of Padua Padova, Veneto, Italy)
Seiji Sugita
(University of Tokyo Tokyo, Japan)
Stephan Ulamec
(German Aerospace Center Cologne, Germany)
Ian Carnelli
(European Space Research and Technology Centre Noordwijk-Binnen, Netherlands)
Paolo Martino
(European Space Research and Technology Centre Noordwijk-Binnen, Netherlands)
Date Acquired
February 15, 2023
Subject Category
Instrumentation and Photography
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: 8th IAA Planetary Defense Conference
Location: Vienna
Country: AT
Start Date: April 3, 2023
End Date: April 7, 2023
Sponsors: GMV Innovating Solutions (Spain)
Funding Number(s)
WBS: 265759.04.01.03
CONTRACT_GRANT: EUH 2020 870377
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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