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Rosetta enters hibernation
Institution:1. European Space Operation Centre/European Space Agency, R. Bosch Strasse 5, 64298 Darmstadt, Germany;2. Vega Space Gmbh, c/o ESOC, Europaplatz 5, 64293 Darmstadt, Germany;1. Department of Mechanical Engineering, Faculty of Engineering, Malayer University, Malayer, Iran;2. Laser Materials Processing Research Center, Malayer University, Malayer, Iran;3. Department of Mechanical Engineering, Urmia University, Urmia, Iran;4. School of Mech. & Maun. Eng., Dublin City University, Dublin, Ireland;5. Institute of Synthetic Biology, Shenzhen Institute of Advanced Technology, Chinese Academy of Science, Shenzhen 518005, China;1. School of Automation Science and Electrical Engineering, Beihang University, Beijing, 100191, PR China;2. Engineering Technology Department, Old Dominion University, Norfolk, VA, 23529, USA;1. Institute of Geophysics, China Earthquake Administration, Beijing 100000, China;2. Institute of Earthquake Forecasting, China Earthquake Administration, Beijing 100000, China
Abstract:The International Rosetta Mission was launched on 2nd March 2004 on its 10 years journey to comet 67P/Churyumov–Gerasimenko. Rosetta will reach the comet in 2014, orbit it for about 1.5 years down to distances of a few kilometres and deliver the Lander Philae onto its surface.Following the fly-by of Asteroid (21-)Lutetia in 2010, Rosetta continued its travel towards the planned comet encounter in 2014. In this phase Rosetta became the solar-powered spacecraft that reached the largest Sun distances in history of spaceflight, up to an aphelion at 5.3 AU in October 2012. At distances above 4.5 AU the spacecraft's solar generator power is not sufficient to keep all spacecraft systems active. Therefore in June 2011 the spacecraft was spun up to provide gyroscopic stabilisation, and most of its on-board units, including those used for attitude control and communications, were switched off. Over this “hibernation” phase of about 2.5 years the spacecraft will keep a minimum of autonomy active to ensure maintenance of safe thermal conditions.After Lutetia fly-by, flight controllers had to tackle two anomalies that had significant impacts on the mission operations. A leak in the reaction control subsystem was confirmed and led to the re-definition of the operational strategy to perform the comet rendezvous manoeuvres planned for 2011 and 2014. Anomalous jumps detected in the estimated friction torque of two of the four reaction wheels used for attitude control forced the rapid adoption of measures to slow down the wheels degradation. This included in-flight re-lubrication activities and changes in the wheels operational speed regime.Once the troubleshooting of the two anomalies was completed, and the related operational scenarios were implemented, the first large (790 m/s) comet rendezvous manoeuvre was executed, split into several long burns in January and February 2011. The second burn was unexpectedly interrupted due to the anomalous behaviour of two thrusters, causing attitude off-pointing. Flight controllers modified the thrusters operation parameters in the on-board software and managed to re-start the sequence of burns and successfully complete the manoeuvre. After the manoeuvre, preparation for the critical spin-up and hibernation entry activities, planned for June 2011, began.This paper presents the activities carried out on Rosetta in the final year before hibernation entry. The major anomalies and the related troubleshooting and workaround solutions are detailed. Lessons learned from the operation of the first spacecraft operating with solar power at Jupiter-like distances from the Sun are presented and discussed.
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