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In-Flight Operation of the Dawn Ion Propulsion System Through the Preparations for Escape From Vesta

机译:通过准备逃离Vesta的黎明离子推进系统在飞行中的操作

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The Dawn mission, part of NASA's Discovery Program, has as its goal the scientific exploration of the two most massive main-belt asteroids, 4 Vesta, and the dwarf planet 1 Ceres. The Dawn spacecraft was launched from the Cape Canaveral Air Force Station on September 27, 2007 on a Delta-II 792SH-9.5 rocket that placed the 1218-kg spacecraft into an Earth-escape trajectory. On-board the spacecraft is an ion propulsion system (IPS) developed at the Jet Propulsion Laboratory which will provide a total delta-V of approximately 11 km/s for the heliocentric transfer to Vesta, orbit capture at Vesta, transfer between Vesta science orbits, departure and escape from Vesta, heliocentric transfer to Ceres, orbit capture at Ceres, transfer between Ceres science orbits, and orbit maintenance maneuvers for all Vesta and Ceres science orbits. Full-power thrusting from December 2007 through October 2008 was used to successfully target a Mars gravity assist flyby in February 2009 that provided an additional delta-V of 2.6 km/s. Deterministic thrusting for the heliocentric transfer to Vesta resumed in June 2009 and concluded with orbit capture at Vesta on July 16, 2011. An additional 231 hours of IPS thrusting was used to enter the first Vesta science orbit, called Survey orbit, on August 3, 2011 at an altitude of about 2,735 km. The IPS was then used over the next year to transfer the spacecraft to the other science orbits: a high altitude mapping orbit (HAMO-1) in September 2011 at an altitude of approximately 673 km, a low altitude mapping orbit (LAMO) at approximately 210 km altitude, and a second high altitude mapping orbit (HAMO-2) at approximately 673 km altitude. To date the IPS has been operated for approximately 24,327 hours, consumed approximately 260 kg of xenon, and provided a delta-V of approximately 7 km/s. IPS performance characteristics are very close to the expected performance based on analysis and testing performed pre-launch. Thrusting for escape from Vesta and cruise to Ceres is planned to start in late July 2012 with a planned arrival date at Ceres in February 2015. This paper provides an overview of Dawn's mission objectives and the results of Dawn IPS mission operations through preparations for departure from Vesta.
机译:作为美国国家航空航天局(NASA)发现计划的一部分,“黎明”计划的目标是对两个最大的主带小行星小行星4 Vesta和矮行星1 Ceres进行科学探索。黎明号航天器于2007年9月27日从卡纳维拉尔角空军基地发射,并搭载Delta-II 792SH-9.5火箭,将1218千克重的航天器置于逃生轨道。航天器上装有由喷气推进实验室开发的离子推进系统(IPS),该系统将提供约11 km / s的总delta-V,用于向心星向Vesta的日心传输,在Vesta的轨道捕获,在Vesta科学轨道之间的传输,从Vesta起飞和逃逸,日心向Ceres的转移,Ceres的轨道捕获,Ceres科学轨道之间的转移以及所有Vesta和Ceres科学轨道的轨道维护演习。从2007年12月到2008年10月的全功率推力被成功地用于2009年2月的火星重力辅助飞越,提供了2.6 km / s的额外增量V值。确定性向天心向维斯塔转移的推力于2009年6月恢复,并于2011年7月16日在维斯塔捕获了轨道。8月3日,额外的231小时IPS推力被用于进入第一个维斯塔科学轨道,称为勘测轨道, 2011年海拔约2,735公里。然后在明年使用IPS将航天器转移到其他科学轨道:2011年9月在约673 km的高空测绘轨道(HAMO-1),在约673 km的低空测绘轨道(LAMO) 210公里的高度,以及第二个高海拔制图轨道(HAMO-2),其高度约为673公里。迄今为止,IPS已运行约24,327小时,消耗了约260千克氙,并提供了约7 km / s的ΔV。根据发布前进行的分析和测试,IPS性能特征非常接近预期性能。计划从2012年7月下旬开始推进从Vesta逃逸并巡航至Ceres,计划于2015年2月到达Ceres。本文通过准备出发的方式,概述了Dawn的任务目标和Dawn IPS任务的结果。维斯塔

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