Abstract

We present the results of two sets of experiments that investigate laser-based metal-to-rock attachment techniques. Asteroids and comets have low surface gravity which pose a challenge to landers with moving parts. Such parts can generate torques and forces which may tip the lander over or launch it into deep space. Thus, if a lander on a small body is to have moving parts, the spacecraft must be equipped with an anchoring mechanism. To this end, we sought to use a laser to melt and bind a piece of metal mimicking a part of a spacecraft to a rock mimicking the surface of a typical asteroid. In the first set of experiments, extra material was not fed in during the processing. The second set were performed using a standard wire feeder used in laser welding, which added metal to the experiment during processing. During the first experiments, we discovered that a traditional weld, where two melt pools mix and solidify to form a strong bond, was not possible—the melt pools would not mix, and when they did, the resulting weld was extremely brittle. The second set of experiments resulted in a physico-mechanical bond, where a hole was drilled with a laser, and a wire was melted and fed into the hole. These latter experiments were successful in forming bonds as strong as 115 N. Such an attachment mechanism can also be used to maneuver small boulders on asteroid surfaces, to redirect small, monolithic asteroids, or in space-debris removal.

Highlights

  • IntroductionLanding (and staying anchored) on a small body such as an asteroid or comet is a challenge due to the micro-gravity environment

  • Landing on a small body such as an asteroid or comet is a challenge due to the micro-gravity environment

  • We discovered that a traditional weld, where two melt pools mix and solidify to form a strong bond, was not possible—the melt pools would not mix, and when they did, the resulting weld was extremely brittle

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Summary

Introduction

Landing (and staying anchored) on a small body such as an asteroid or comet is a challenge due to the micro-gravity environment. The 100-kg Philae lander, part of ESA’s Rosetta mission, sought to tackle this challenge with a diverse suite of landing equipment: harpoons, thrusters, and screws. The thruster and harpoon failed to fire and the screws proved insufficient to hold the spacecraft down on their own, leading to a multiple-contact landing [1]. JAXA’s Hayabusa mission had an alternative approach: three landers (1–10 kg in mass) were deployed from the main spacecraft, which had no landing gear at all, and were, instead, designed to bounce along the surface of asteroid (162173) Ryugu and these proved successful [2]. A summary of other anchoring techniques currently existing or in development is given in Zacny et al 2013 [3]

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