Laying the groundwork for future exploration and scientific inquiry into the nature and origins of our solar system, the Dawn mission studied the dwarf planet Ceres and discovered a frozen world with bright concentrations of salts and minerals, and the presence of organic molecules in several locations on the surface. With its closest approach to Earth of 1.6 AU, Ceres is a prime candidate for in-situ robotic exploration beyond Mars, hosting potentially liquid water, cryovolcanism, and the building blocks for life. This paper discusses a mission proposal for the collection of samples from the surface of the dwarf planet Ceres and their subsequent return to Earth for laboratory analysis. A full Pre-Phase A study was conducted to define in-depth the mission concepts and objectives, assess the feasibility of such a mission, and develop a preliminary program proposal. Eighteen potential mission architectures were analysed, giving way to a mission design consisting of four main phases: an outbound trajectory of a main spacecraft carrying a lander, via Mars flyby to Ceres orbit and rendezvous; a surface exploration mission involving multiple hops of the sample-collecting lander, focused on salt-brine faculae of Occator crater and locations containing high concentrations of organics; sample return capsule launch from the surface with in-orbit docking to the main spacecraft; and the return to Earth with the ejection of the sample return capsule for re-entry and collection. This 11.5-year mission will utilize proven as well as new technologies, relying upon a pair of 240 mN gridded ion thrusters for the interplanetary trajectory, and the green propellant LMP-103s for powering the unique, controlled hops of the lander to multiple locations across the low-gravity environment of Ceres. Small, state-of-the-art sensors and instruments have been carefully chosen to maximize the scientific performance of the mission while keeping the mass at a minimum. Cost, performance, and risk assessments throughout multiple in-depth mock customer reviews showed the sample-return mission to be feasible for a limited mass of samples, provided that the timeline for mission development is properly coordinated with Ceres transfer windows. The complete mission proposal, including scientific goals and measurement instrumentation, preliminary spacecraft design, trajectory and mission design, results of the pre-Phase A feasibility assessment, program proposal, and mission concept review are all presented.

Ceres Lander Exploration and Sample Return Mission

Alessandro Billi
Membro del Collaboration Group
;
Oscar Caliman
Membro del Collaboration Group
;
Osama Eldeeb
Membro del Collaboration Group
;
Francesco Foti
Membro del Collaboration Group
;
Emanuele Luzzati
Membro del Collaboration Group
;
Francesco Salzo
Membro del Collaboration Group
;
Salvo Marcuccio
Secondo
Methodology
2022-01-01

Abstract

Laying the groundwork for future exploration and scientific inquiry into the nature and origins of our solar system, the Dawn mission studied the dwarf planet Ceres and discovered a frozen world with bright concentrations of salts and minerals, and the presence of organic molecules in several locations on the surface. With its closest approach to Earth of 1.6 AU, Ceres is a prime candidate for in-situ robotic exploration beyond Mars, hosting potentially liquid water, cryovolcanism, and the building blocks for life. This paper discusses a mission proposal for the collection of samples from the surface of the dwarf planet Ceres and their subsequent return to Earth for laboratory analysis. A full Pre-Phase A study was conducted to define in-depth the mission concepts and objectives, assess the feasibility of such a mission, and develop a preliminary program proposal. Eighteen potential mission architectures were analysed, giving way to a mission design consisting of four main phases: an outbound trajectory of a main spacecraft carrying a lander, via Mars flyby to Ceres orbit and rendezvous; a surface exploration mission involving multiple hops of the sample-collecting lander, focused on salt-brine faculae of Occator crater and locations containing high concentrations of organics; sample return capsule launch from the surface with in-orbit docking to the main spacecraft; and the return to Earth with the ejection of the sample return capsule for re-entry and collection. This 11.5-year mission will utilize proven as well as new technologies, relying upon a pair of 240 mN gridded ion thrusters for the interplanetary trajectory, and the green propellant LMP-103s for powering the unique, controlled hops of the lander to multiple locations across the low-gravity environment of Ceres. Small, state-of-the-art sensors and instruments have been carefully chosen to maximize the scientific performance of the mission while keeping the mass at a minimum. Cost, performance, and risk assessments throughout multiple in-depth mock customer reviews showed the sample-return mission to be feasible for a limited mass of samples, provided that the timeline for mission development is properly coordinated with Ceres transfer windows. The complete mission proposal, including scientific goals and measurement instrumentation, preliminary spacecraft design, trajectory and mission design, results of the pre-Phase A feasibility assessment, program proposal, and mission concept review are all presented.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11568/1151101
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