RESEARCH MASTER INTERNSHIP 2016-2017
Transcription
RESEARCH MASTER INTERNSHIP 2016-2017
RESEARCH MASTER INTERNSHIP 2016-2017 Space Systems for Planetary Applications/DEOS Location : Superviser : Naomi MURDOCH Tel. : E-mail. : Toulouse, France +33 5 61 33 87 03 [email protected] INTERNSHIP DESCRIPTION Domains : Planetary Science, Geophysics, Mechanics, Space Systems Title : Measuring the surface mechanical properties of an asteroid during landing In 2014, the European Space Agency’s (ESA’s) Rosetta spacecraft became the first mission to successfully deliver a lander to a comet’s surface. Though the Philae lander eventually came to rest, its anchoring harpoons failed to fire upon descent, and the lander proceeded to rebound twice over a duration of approximately 2 hours before reaching its final destination, roughly 1 km away from the intended landing site [1,2]. The understanding of surface-lander interactions is particularly important for current and future space missions that include lander components e.g., the MASCOT and the MINERVA rovers on-board JAXA's Hayabusa-2 mission [3], MASCOT2 and possibly AGEX on board ESA's AIM mission [4-6]. In addition, the surface – lander interactions can allow esimates to be made of the mechanical properties of the small body surface material [1]. Here at ISAE-SUPAERO we have developed a drop tower experiment (Fig 1) in order to study the problematic of landing on asteroids and comets in very low gravity conditions. In the experiment rig, reduced-gravity is simulated by releasing a free-falling projectile into a surface container with a downward acceleration less than that of Earth's gravity. The acceleration of the surface is controlled through the use of an Atwood machine, or a system of pulleys and counterweights. Accelerometers, placed on the surface container and inside the projectile, provide acceleration data, while high-speed cameras capture the collision and act as secondary data sources. For detailed information about the experiment see [7]. Figure 1: Images sequence depicting the initial release, free-fall, and collision phases for a 2.0 m drop test. The top row of images is from an AEE MagiCam SD100 camera that was mounted inside of the surface container, and the bottom row of images is still frames from the Ultima APX-RS Photron high-speed camera. See [3] for more details. The goal of this research project is to study the impact dynamics during low-velocity granular collision experiments, and to investigate how the asteroid mechanical surface properties can be determined from accelerometer data. The student will first develop a theoretical framework for determining the surface mechanical properties from accelerometer data. Then, laboratory experiments will be performed in 1g and in reduced-gravity using the ISAE-SUPAERO drop-tower to put this into practice. The influence of the projectile form and the surface material properties will also be investigated. The results will have a direct implication for the choice of instruments and the design of future asteroid landers. References [1] Biele, et al., « The landing(s) of Philae and inferences about comet surface mechanical properties” Science 349, aaa9816 (2015). [2] Ulamec, et al. « Rosetta Lander – Landing and operations on comet 67P/Churyumov–Gerasimenko » Acta Astronaut. 125, 80 (2016). [3] Tsuda et al., « System design of the Hayabusa 2 asteroid sample return mission to 1999 FJU3G », Acta Astronautica 91 (2013). [4] Michel et al., « Science case for the asteroid impact mission (AIM): A component of the asteroid impact and deflection assessment (AIDA) mission », Advances in Space Research 57, 12, (2016). [5] Ho et al., « A Mobile Asteroid Surface Scout for the AIDA Mission », EGU (2016). [6] Karatekin et al., « The Asteroid Geophysical Explorer (AGEX); A proposal to explore Didymos system using Cubesats», EGU (2016). [7] Sunday et al., « A novel facility for reduced-gravity testing: A setup for studying low-velocity collisions into granular surfaces » Review of Scientific Instruments 87, 084504 (2016). 10 % Theoretical Research Possibility to go on a Ph.D.: 30 % Applied Research o Yes 60% Experimental Research o No APPLICANT PROFILE Knowledge and required level: The candidate must be rigorous, autonomous and enjoy lab work and data analysis. A background in physics, mechanics or planetary science would be an advantage, as would previous experience with Matlab and laboratory experiments. Applications should be sent by e-mail to the supervisor.