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Updated: May 4, 2026

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
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Radiation analysis for manned missions to the Jupiter system
G De Angelis1, M S Clowdsley, J E Nealy
1Old Dominion University, Norfolk, VA 23508, USA. g.deangelis@larc.nasa.gov
Summary
Manned missions to Jupiter
Area of Science:
- Space exploration
- Planetary science
- Astrophysics
Background:
- Human exploration beyond Mars is a key objective.
- The Jovian system, particularly Callisto, presents unique challenges and opportunities for human missions.
- Previous studies have not fully analyzed the complexities of manned missions to Jovian moons.
Purpose of the Study:
- To analyze the feasibility of manned missions to Jupiter's moon Callisto.
- To evaluate mission trajectories, propulsion systems, and radiation exposure.
- To assess the viability of surface exploration on Callisto.
Main Methods:
- Mission analysis encompassing interplanetary cruise, Jupiter orbital insertion, and surface exploration.
- Trajectory design using various propulsion systems, with durations of 2-5 years.
- Radiation dose assessment using HZETRN code for hadrons and a custom code for electrons/photons, considering surface backscattering.
Main Results:
- Interplanetary cruise durations range from two to five years.
- Detailed analysis of Jupiter orbital insertion, including radiation belt traversal.
- Surface composition modeling of Callisto based on GALILEO data.
Conclusions:
- Manned missions to Callisto are feasible with careful planning of propulsion and trajectory.
- Radiation exposure during transit and orbital insertion requires mitigation strategies.
- Further research into Callisto's surface and radiation environment is crucial for mission success.
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