EGU21-3286, updated on 03 Mar 2021
https://doi.org/10.5194/egusphere-egu21-3286
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

VAPRE: Facilitating Planetary Probe Mission Design and Entry Site Selection

Alena Probst1, Linda Spilker1, Tom Spilker2, David H. Atkinson1, Olivier Mousis3, Mark Hofstadter1, and Amy Simon4
Alena Probst et al.
  • 1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, (alena.probst@jpl.nasa.gov)
  • 2Independent Consultant
  • 3Laboratoire d'Astrophysique de Marseille, CNES-CNRS-INSU, Aix-Marseille Université, Marseille, France
  • 4Goddard Space Flight Centre, NASA, Greenbelt, MD

In the pursuit of deciphering the formation of our solar system, the exploration of the compositional and dynamical structure of planetary atmospheres with entry probes plays a crucial role. A probe's measurements provide insight into an atmosphere's deeper composition and dynamical processes not accessible via remote sensing, providing key information on the origin and possible migration of planets during early formation phase. A planetary entry probe mission has been in discussion in several Planetary Science Decadal Surveys, one to Saturn has been identified as a mission of highest priority in the current one 2013-2022, and a mission to Uranus and/or Neptune carrying a probe is being considered as a Flagship mission in the next one spanning 2023-2032.

In the development of such missions, the probe approach and delivery trajectory is a critical element to mission success, including ring avoidance, and targeting of highly desirable regions in the atmosphere, while balancing other requirements such as providing an optimal communication geometry between the probe and the relay spacecraft while meeting the mission's science objectives. Due to the complexity of the problem, mission concept studies are usually limited to the investigation of a limited number of specific trajectories and probe delivery opportunities to a very small, pre-defined range of latitudes while leaving a huge trade space unexplored.

The tool VAPRE (Visualization of Atmospheric PRobe Entry conditions) has been developed to enable a fast and wide-range evaluation of entry conditions for planetary probes, spanning the complete range of latitudes for each of the three planets. VAPRE allows a rapid assessment of feasible entry sites by evaluating a large number of arrival trajectories based on their hyperbolic arrival velocities with respect to parameters such as the flight path angle and the relative entry velocity of the probe at the entry interface point. VAPRE facilitates the mission design process by combining the evaluation of technical feasibility and science value for the investigated scenarios to assess potential entry sites. VAPRE is developed in the framework of IPED (Impact of the Probe Entry zone on the trajectory and probe Design), which is a two- to three-year research study to investigate both the impact of interplanetary and approach trajectories on the feasible range of entry sites as well as on probe design, considering Saturn, Uranus, and Neptune as target bodies.

In this paper we fully demonstrate the functionalities of the VAPRE tool on a case scenario for a mission to the Ice Giants.

The presented research was supported by an appointment to the NASA Postdoctoral Program (NPP) at the Jet Propulsion Laboratory (JPL), California Institute of Technology, administered by Universities Space Research Association (USRA) under contract with National Aeronautics and Space Association (NASA). © 2020 All rights reserved.

How to cite: Probst, A., Spilker, L., Spilker, T., Atkinson, D. H., Mousis, O., Hofstadter, M., and Simon, A.: VAPRE: Facilitating Planetary Probe Mission Design and Entry Site Selection, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-3286, https://doi.org/10.5194/egusphere-egu21-3286, 2021.

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