The NEOTωIST mission (Near-Earth Object Transfer of angular momentum spin test). (October 2016)

• Record Type: Journal Article
• Authors: Drube, Line; Harris, Alan W.; Engel, Kilian; Falke, Albert; Johann, Ulrich; Eggl, Siegfried; Cano, Juan L.; Ávila, Javier Martín; Schwartz, Stephen R.; Michel, Patrick
• Is Part Of: Acta astronautica. Volume 127(2016)
• Page Start: 103
• Page End: 111
• Publication Date: 2016-10
• Subjects: DSNR Detection Signal-to-Noise Ratio -- FoM Figure of Merit -- NEO Near-Earth Object -- NEOTωIST Near-Earth Object Transfer of angular momentum (=ω*I) Spin Test -- LPF Lisa Pathfinder Propulsion module; Near-Earth Objects -- Asteroids -- Impact hazard -- Asteroid deflection -- Planetary defense -- Kinetic impactor; Astronautics -- Periodicals; Outer space -- Exploration -- Periodicals; Astronautics; Periodicals; 629.405
• DOI: 10.1016/j.actaastro.2016.05.009
• Languages: English
• ISSNs: 0094-5765

Abstract

Abstract: We present a concept for a kinetic impactor demonstration mission, which intends to change the spin rate of a previously-visited asteroid, in this case 25143 Itokawa. The mission would determine the efficiency of momentum transfer during an impact, and help mature the technology required for a kinetic impactor mission, both of which are important precursors for a future space mission to deflect an asteroid by collisional means in an emergency situation. Most demonstration mission concepts to date are based on changing an asteroid's heliocentric orbit and require a reconnaissance spacecraft to measure the very small orbital perturbation due to the impact. Our concept is a low-cost alternative, requiring only a single launch. Taking Itokawa as an example, an estimate of the order of magnitude of the change in the spin period, δ P, with such a mission results in δ P of ~4 min (0.5%), which could be detectable by Earth-based observatories. Our preliminary study found that a mission concept in which an impactor produces a change in an asteroid's spin rate could provide valuable information for the assessment of the viability of the kinetic-impactor asteroid deflection concept. Furthermore, the data gained from the mission would be of great benefit for our understanding of the collisional evolution of asteroids and the physics behind crater and ejecta-cloud development.