May 5 – 9, 2025
STELLENBOSCH, CAPE TOWN, SOUTH AFRICA
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A Gravity Tractor Mission Concept to a Binary Asteroid

May 8, 2025, 9:05 AM
8m
STELLENBOSCH, CAPE TOWN, SOUTH AFRICA

STELLENBOSCH, CAPE TOWN, SOUTH AFRICA

Protea Hotel by Marriott® Stellenbosch
Oral. Deflection / Disruption Modeling & Testing Session 6: Deflection / Disruption Modeling & Testing

Speaker

Ronald-Louis Ballouz (Johns Hopkins University Applied Physics Laboratory)

Description

Keywords: Gravity Tractor, Slow-pull Mitigation Technique, Binary Asteroids, Mission Concepts

There are a number of possible mitigation strategies that have been identified in the event a hazardous asteroid is discovered. NASA’s DART mission recently demonstrated the kinetic impactor technique [1]. The gravity tractor (GT) is attractive as the next technology for demonstration since other techniques may be prohibited by cost and legality [2]. A GT demonstration mission would align with NASA’s goal to "[d]evelop preliminary mission designs for future NEO deflection mission campaigns” [3]. Here, we present the design of a mission that would demonstrate a GT by changing the orbit of the secondary in an asteroid binary system.

The GT concept for deflecting asteroids involves bringing a spacecraft near an asteroid and controlling the spacecraft so that the asteroid’s orbit is altered by the spacecraft’s gravity [4]. This slow-pull mitigation strategy can achieve greater precision in an asteroid’s post-deflection orbit than impulsive mitigation techniques. GT also has the benefits of being agnostic to the material properties of the asteroid and not requiring contact between the spacecraft and asteroid. A GT may be used as the “primary” mitigation technique for hazardous asteroids that are found sufficiently far in advance of their Earth impact dates, or as a “secondary” mitigation technique applied after a “primary” impulsive technique to ensure the avoidance of gravitational keyholes. Inspired by the success of the DART mission, we are studying whether GTs will be more easily tested in a binary asteroid system in the same way that kinetic impactors are: a small velocity change on the order of what would be necessary in a real emergency is more easily detected and measured on an asteroid satellite's orbit than it is on a single asteroid’s heliocentric orbit [5].

We report on the preliminary design of a GT demonstration mission to a binary asteroid system. We identify three main goals that a GT mission to a binary asteroid should achieve: (1) guide and navigate the spacecraft to the vicinity of the secondary and precisely control its relative position (within a few body radii), (2) measure the change in the secondary’s orbit due to the GT, and (3) demonstrate long-duration tractoring operations in close proximity to the asteroid. We present mission requirements needed to achieve these mission goals. These requirements are used to define a concept of operations for a binary asteroid system “characterization phase” and “tractor phase,” which would lead to a measurable deflection of the secondary within a 12-month timeframe for asteroid proximity operations. We present the mission design, baseline payload, and spacecraft design that would meet these investigation requirements. In sum, this report outlines a demonstration mission of a GT at reasonable cost that will accomplish NASA’s goal of demonstrating a slow-pull asteroid deflection technique.

References

[1] Chabot, N., et al. (2024). Planet. Sci. J. 5 49

[2] Abell, P. and Frazier (2021). Planetary Defense Missions: Rapid Mission Architecture Study. Planetary Science Decadal Survey: Mission Concept Study Report.

[3] NASA Planetary Defense Strategy and Action Plan (2023). NASA. https://go.nasa.gov/3UO2mmt

[4] Lu, E. T. and Love, S. G. (2005). Nature, 438, 177–178.

[5] Merrill, C., et al., this conference.

Author

Ronald-Louis Ballouz (Johns Hopkins University Applied Physics Laboratory)

Co-authors

Andrew Rivkin Colby Merrill Rylie Bull (JHU/APL) Olivier Barnouin (Johns Hopkins Applied Physics Laboratory) Noble Hatten (Johns Hopkins Applied Physics Laboratory) Justin Atchison (The Johns Hopkins University Applied Physics Laboratory) Brent Barbee (NASA/GSFC/UMD) Nancy Chabot (Johns Hopkins University Applied Physics Lab) Andrew F Cheng (Johns Hopkins University Applied Physics Laboratory) R. Terik Daly (Johns Hopkins Applied Physics Laboratory) Carolyn M. Ernst (Johns Hopkins University Applied Physics Laboratory) Zachary Fletcher (Johns Hopkins University Applied Physics Laboratory) Dawn M. Graninger (Johns Hopkins University Applied Physics Laboratory) Ed Lu Prof. Derek Richardson (University of Maryland, College Park) Angela Stickle (Johns Hopkins Applied Physics Laboratory)

Presentation materials