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Resolving the Origin of Deimos: Combining Global and Local Composi-tional Analysis with the small-sat TASTE Mission

Dr. John Robert Brucato — Research Director
INAF – Arcetri Astrophysical Observatory
Missions Scientific

Schedule

Poster Wednesday, May 27, 2026 · 5:00 PM · Posters Area – Kiosk 1

Abstract

Understanding the formation of Phobos and Deimos is critical for decoding the history of Mars and the evolution of the outer Solar System. The scientific debate centers on two models: for-mation via a Martian giant impact or the capture of D-type asteroids. The TASTE – Terrain Analyzer and Sample Tester Explorer mission seeks to resolve the origin of Deimos by provid-ing essential, detailed knowledge. The high-level scientific objectives of TASTE are to deter-mine Deimos’s origin by combining global morphology and elemental composition from close orbit with local surface organic and mineralogical composition acquired via a lander.

TASTE will provide characterization, complementing the expected results of the JAXA MMX mission, which focuses on Phobos. The investigation strategy involves two distinct phases:
• Global Characterization (Orbiter): An hyperspectral camera and a miniaturized X-γ-ray spectrometer will characterize the surface’s elemental composition from a stable Quasi-Satellite Orbit. Additionally, radio science will acquire data on Deimos’ gravity field, providing constraints on its interior structure.
• Local Surface Analysis (Lander): The lander will descend to the surface. Once land-ed, the Surface Sample Analyser will perform detailed chemical analysis. This direct view and analysis is crucial for characterizing the local organic and mineralogical com-position, which holds the key to definitively linking Deimos to either the impact ejecta or carbonaceous chondrite parent bodies.
TASTE, currently in Phase B, uses a 16U CubeSat architecture to perform scientific investiga-tion in a deep-space, low-gravity environment. This talk will present the scientific objectives, the critical role of the mission’s data in the origin debate, and the required measurement syner-gy.

Acknowledgements: This work is funded by the Italian Space Agency (ASI) within the Alcor Program, as part of the development of the TASTE mission under contract n. 2024-45-I.0. The project is led by Italian consortia: INAF & POLIMI

Authors

  • John Brucato — Research Director / Programme Manager
    INAF – Arcetri Astrophysical Observatory, Florence Italy
  • Prof. Michèle Lavagna — Full Professor / System Engineer
    POLIMI – DAER, Milan Italy
  • Dr. Fabrizio Fiore — Research Director / Payload Manager
  • TASTE Team