Drop Your Thesis 2018: 4.7 Seconds of Microgravity Conditions to Enable Future CubeSat Landings on Asteroids
- Paper number
IAC-18,E2,3-GTS.4,5,x44451
- Author
Mr. Elioenai Sitepu, United Kingdom, Cranfield University
- Coauthor
Dr. Joan Pau Sanchez Cuartielles, United Kingdom, Cranfield University
- Coauthor
Ms. Carole Le Blay, United Kingdom, Cranfield University, UK
- Coauthor
Mr. George Kersey, United Kingdom, Cranfield University, UK
- Coauthor
Mr. Stuart Ogborne, United Kingdom, Cranfield University, UK
- Coauthor
Mr. Daniyal Ahmad Durrani, United Kingdom, Cranfield University, UK
- Coauthor
Dr. Luca Zanotti Fragonara, United Kingdom, Cranfield University, UK
- Coauthor
Mr. Florian Gautier, United Kingdom, Cranfield University, UK
- Coauthor
Dr. Jennifer Kingston, United Kingdom, Cranfield University
- Year
2018
- Abstract
An increasing number of interplanetary missions are aiming at visiting asteroids and other small bodies, since these may provide clues to understand the formation and evolution of our Solar System. CubeSats allow a low-cost solution to land on these objects, as opposed to risking a much more expensive mothership. The weak gravitational field on these small bodies may also enable the possibility of simply dropping a CubeSat from afar (i.e. ballistic landing). However, ballistic landing of an unpowered spacecraft would only be feasible within certain asteroid locations, and only if sufficient energy can be dissipated at touchdown. If such conditions are not met, the spacecraft will rebound off the surface and escape the asteroid. The amount of dissipated energy is measured by means of the coefficient of restitution, which is defined as the ratio between the velocities after and before the impact. It is likely that the necessary coefficient of restitution may already occur naturally due to the energy loss expected through the deformation of the regolith layer during the touchdown. Indeed, previous low-velocity impact experiments in microgravity seem to indicate that this is exactly the case. However, data from past asteroid touchdowns, Hayabusa and Philae, indicate the contrary. \newline\ The paper describes an experiment designed by students from the Astronautics and Space Engineering MSc course at Cranfield University (Land3U Team), which aims to bridge the aforementioned disagreement between mission data and microgravity experiments. The experiment was proposed and awarded by ESA Education for ESA’s “Drop Your Thesis! 2018 campaign”. The experiment, will take place at the ZARM Drop Tower in Bremen next November 2018. With the constraint of 5 drops, the experiment will measure the coefficient of restitution during an available time window of 4.74 seconds of microgravity condition. The aim of this study is to understand the behaviour of CubeSat landing on asteroids with an additional objective of developing a damping mechanism that could increase the dissipated energy. A 3U CubeSat mock-up will be used to represent a future asteroid lander. In order to mimic the landing condition of actual missions, the mock-up will be given a velocity of 10-20cm/s with minimal tilting. This will be achieved by an automated release mechanism that will meet these requirements. An analogue of asteroid regolith will be selected to simulate its mechanical properties. This presentation will review the final design and the engineering challenges of the experiment.
- Abstract document
- Manuscript document
IAC-18,E2,3-GTS.4,5,x44451.pdf (🔒 authorized access only).
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