低轨巨型星座构型设计与控制研究进展与展望

近年来低轨星座计划发展迅速,低轨巨型星座已成为全球争夺空间战略资源的\"新战场\".首先,概述了Telesat、OneWeb、Starlink等低轨巨型星座计划的发展现状,以及中国互联网星座计划的基本情况.在此基础上,分别从星座的任务需求、覆盖特性、摄动补偿和备份策略4个方面,综述了星座的构型设计方法及其特点.然后,根据卫...     

Current status of the BepiColombo/MMO spacecraft design

This paper shows the current baseline of the conceptual design of the BepiColombo/MMO (mercury magnetospheric orbiter) spacecraft, which is conducted by the ISAS Mercury Exploration Working Group. The MMO is a spinning spacecraft of 200 kg mass whose spin axis is nearly perpendicular to the Mercury orbital plane. The current status of the overall MMO system and subsystems such as thermal control, communication, power, etc. are described. The latest status of the development of critical technologies for the MMO and the outline of the international cooperation between ESA and ISAS are also presented.     

我国空间站安全与任务保证工作若干问题探讨

从我国空间站运营阶段对安全性、可靠性、维修性及质量保证(SRMQA)工作的需求出发,在系统分析国外载人航天安全与任务保证(SMA)工作体系的基础上,总结国际空间站安全性可靠性工作的先进经验,并针对我国空间站对航天员安全、寿命与可靠性要求更高的需求,从管理和技术应用两个方面,系统论述了我国空间站安全与任务保证应重点开展的安全性、寿命与可靠性等工作。     

一种面向服务的航电任务系统软件架构

OSGi(Open Service Gateway Initiative)标准是面向服务软件架构的典型架构,OSGi为面向服务插件开发提供了一种动态的、可部署的基础框架环境。QT是1991年奇趣科技开发的一个跨平台的C++图形用户界面应用程序框架,它提供给应用程序开发者建立艺术级的图形用户界面所需的所有功能。基于OSGi标准和QT提出并实现了一种面向服务的航电任务系统软件架构,介绍了OSGi标准以及QT,同时对QT实现OSGi中核心关键技术进行了分析,提供了一个航电任务系统的面向服务解决方案。     

CCSDS空间包在MOIMS领域中的应用

为了适应未来航天任务的发展,构建以服务为导向的、开放的、可重用的航天器任务操作系统,分析了CCSDS(Consultative Committee for Space Data Systems,空间数据系统咨询委员会)中MOIMS (Mission Operations and Information Management System,任务操作及信息管理系统)领域的任务操作服务框架的原理、层次结构及优点,对任务操作相关的通用服务、功能服务、COM(Common Object Model,通用对象模型)及MAL(Message Abstraction Layer,消息抽象层)对服务的抽象化描述方法进行了研究.MAL向任务操作相关的服务提供了通用的服务模型框架,所有服务均可用MAL消息格式进行规范化的描述,在此基础上建立了MAL消息格式与CCSDS空间包的映射关系,从而以CCSDS空间包为信息栽体实现了航天器与地面系统间的任务操作通信,可以作为以服务为导向的任务操作系统实际工程应用的参考.     

我国首次火星探测任务

我国首次火星探测任务于2016年立项实施。综合介绍了国际火星探测的历史和现状,我国首次火星探测任务的工程目标和科学目标、总体技术方案、关键技术难点、预期创新成果。我国首次火星探测任务将通过一次发射,实现火星环绕和着陆巡视,对火星开展全球性普查和局部的精细探测,推进火星地形地貌与地质构造、土壤特征与水冰分布、表明物质组成、大气电离层和气候环境、物理场与内部构造等方面的研究。实现火星探测任务目标,针对火星探测面临的各种特殊环境,需突破长期自主管理与控制等8类关键技术,取得的一系列创新成果,将为我国建立独立自主的深空探测基础工程体系,掌握深空探测基础共性技术,形成开展深空探测的基础工程能力。     

月球重力场模型误差对CE-5T1探测器定轨的影响

利用嫦娥五号再入返回飞行试验拓展任务期间获取的探测器(CE-5T1)实测数据,采用内符合方法比较了3种重力场模型的实测数据定轨结果,发现采用GRAIL(Gravity Recovery And Interior Laboratory,重力恢复与内部实验室)重力场模型进行定轨的结果最优。相比于之前的嫦娥系列探测器定轨常用的LP(Lunar Prospector,月球勘探者)重力场模型,采用GRAIL重力场模型定轨后测距数据的残差降低了1个量级。进一步采用不同重力场模型进行轨道外推,定量分析重力场模型对不同类型轨道的影响,结果表明,对于倾角为90°的环月极轨道,不同重力场模型的轨道外推结果差异较小;而对于倾角为20°和40°的环月轨道,不同重力场模型的外推星历的偏差均方根可达到2km,大于当前环月探测器的定轨精度。为此,建议在后续探月任务中使用GRAIL重力场模型进行轨道确定。     

H-reversal trajectory: A new mission application for high-performance solar sails

The aim of this paper is to quantify the performance of a flat solar sail to perform a double angular momentum reversal maneuver and produce a new class of two-dimensional, non-Keplerian orbits in the ecliptic plane. For a given pair of orbital parameters, the orbital period and the perihelion distance, it is possible to find the minimum solar sail characteristic acceleration required to fulfil a double angular momentum reversal trajectory. This problem is addressed using an optimal formulation and is solved through an indirect approach. The new trajectories are symmetrical with respect to the sun-perihelion line and exhibit a bean-like shape. Two main difficulties must be properly taken into account. On one side the sail is required to perform a rapid reorientation maneuver when it approaches the perihelion. Suitable simulations have shown that such a maneuver is feasible. In the second place the new trajectories require the use of high performance solar sails. For example, assuming an orbital period equal to 5 years, the required solar sail characteristic acceleration is greater than 3.4 mm/s². Such a value, although beyond the currently available sail performance, is comparable to what is required by the original concept of H-reversal maneuvers introduced by Vulpetti in 1996.     

软着月任务窗口与轨道设计方法研究

建立了一套应用于多约束条件下软着月任务的窗口计算以及轨道设计方法。针对经历发射 段、地月转移段、绕月段及动力下降段的月球探测器,综合考虑各个特征点的位置、光照、 测控等约束,结合轨道特性,采用着月点→近月点→入轨点→发射点倒推的方式,快速确 定探测器的发射窗口。在其中选择发射时刻后即可计算转移轨道的轨道根数初值,并搜索计 算精确轨道。该方法对于我国月球探测后期工程的发射窗口计算与轨道设计工作有较重要的 参考价值。
     

A possible flyby anomaly for Juno at Jupiter

In the last decades there have been an increasing interest in improving the accuracy of spacecraft navigation and trajectory data. In the course of this plan some anomalies have been found that cannot, in principle, be explained in the context of the most accurate orbital models including all known effects from classical dynamics and general relativity. Of particular interest for its puzzling nature, and the lack of any accepted explanation for the moment, is the flyby anomaly discovered in some spacecraft flybys of the Earth over the course of twenty years. This anomaly manifest itself as the impossibility of matching the pre and post-encounter Doppler tracking and ranging data within a single orbit but, on the contrary, a difference of a few mm/s in the asymptotic velocities is required to perform the fitting.Nevertheless, no dedicated missions have been carried out to elucidate the origin of this phenomenon with the objective either of revising our understanding of gravity or to improve the accuracy of spacecraft Doppler tracking by revealing a conventional origin.With the occasion of the Juno mission arrival at Jupiter and the close flybys of this planet, that are currently been performed, we have developed an orbital model suited to the time window close to the perijove. This model shows that an anomalous acceleration of a few mm/s² is also present in this case. The chance for overlooked conventional or possible unconventional explanations is discussed.