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