TY - JOUR
T1 - Ceres Lander Exploration and Sample Return Mission
AU - Hubert, David
AU - Billi, Alessandro
AU - Cepeda, Oscar
AU - Eldeeb, Osama
AU - Foti, Francesco
AU - Luzzati, Emanuele
AU - Salzo, Francesco Paolo
AU - Tracchegiani, Fabrizio
AU - Marcuccio, Salvo
N1 - Publisher Copyright:
Copyright © 2022 by the International Astronautical Federation (IAF). All rights reserved.
PY - 2022
Y1 - 2022
N2 - 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.
AB - 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.
KW - Ceres
KW - Concept
KW - Dwarf Planet
KW - Interplanetary
KW - Mission Proposal
KW - Pre-Phase A
KW - Sample Return
UR - https://www.scopus.com/pages/publications/85167602031
M3 - Conference article
AN - SCOPUS:85167602031
SN - 0074-1795
VL - 2022-September
JO - Proceedings of the International Astronautical Congress, IAC
JF - Proceedings of the International Astronautical Congress, IAC
T2 - 73rd International Astronautical Congress, IAC 2022
Y2 - 18 September 2022 through 22 September 2022
ER -