基于氢化镁的核电/核热双模共质空间核动力技术

针对未来空间任务对能源和动力日益提高的需求,提出了基于氢化镁的核电核热双模共质空间核动力技术。该技术以一种储氢密度高、热稳定性较好,能够以常温常压储存的氢化镁作为工质,通过核能加热后氢化镁分解成为核热推进可用的高压氢气和电推进可用的单质镁,并结合高效动态热电转换系统,形成大功率核电源、大功率超高比冲核电推进、高比冲氢气核热推进以及大推力镁核热推进多种工作模式。基于氢化镁的多模共质空间核动力技术解决了低温推进剂、气态工质在空间应用时的存储安全性和存储密度低的问题,其具备的多种工作模式能够针对不同任务需求提供相应的能源或者动力输出,提高核动力飞行器任务能力。     

核热推进反应堆燃料元件发展概述

深空探测作为我国航天领域未来的重要任务之一,需要性能更高的推进系统提供动力。核热推进系统具有高比冲、大推力、长运行寿命、可重复启动等优点,可为未来深空探测任务提供可靠的动力支撑。经过了60多年的发展,核热推进固态堆芯燃料元件被研制出了多种类型,如六棱柱石墨基燃料元件、扭曲条带燃料元件、六棱柱金属陶瓷燃料元件、球形包覆颗粒燃料元件、MITEE型燃料元件、SLHC型燃料元件、Grooved Ring型燃料元件等。总结归纳了核热推进固态堆芯燃料元件的发展状况,提出了发展核热推进固态堆芯燃料元件的关键技术,可为我国核热推进系统燃料元件的研制提供借鉴。     

Novel extraterrestrial processing for space propulsion

The concept of space processing of chemicals, in general, and propellants, in particular, is explored quantitatively. The theoretical parametric calculations are supplemented by a bench scale experiment. It is seen that for several candidate space mission scenarios (recommended by several committees for the near-term future, i.e. 1990–2000 A.D.), space processing of both space resources and Earth-carried resources can make decisive differences in the mission success for a given payload. To fix ideas and to demonstrate trends, the specific case of water splitting to extract oxygen, discard (or use without storage) the resulting hydrogen, and burn Earth-carried non-cryogenic liquid fuel(s) in a simple rocket motor, designed for periodic thrusting, is treated in some detail. Experimental hardware is assembled and demonstrated to perform adequately, besides showing compactness of the space-packaged “capsule” module that is self-contained.Building upon previous studies (Ash et al., IAF-82-210, 1982), the concept of in situ propellant production (ISPP) is reexamined in light of more recent energy and materials technologies. Missions to comets and Mars Sample Return are mentioned as candidate scenarios. The mission duration, reliability-repairability of hardware, resource availability in low Earth orbit (LEO), and the thrust requirements are considered in turn. It is seen that space storage of hydrogen for extended durations (5–10 years) involves problems that require detailed studies, besides involving many presently unanswered issues. A study of the energy option in LEO and in deep space is developed in simple terms. The different solar, radioisotope, and nuclear power sources are mentioned. Storage and handling of raw and processed chemicals are considered.Applications of state-of-the-art technologies are explored using a concept of incremental small steps; this approach would decrease risk and cost yet lead toward fully autonomous energy -processing hardware for future missions. Operations in microgravity and large structure behavior are also mentioned. The paper ends with a brief summary of available options, influences of possible future technologies and breakthroughs, and an examination in light of possible future (beyond 2000 A.D.) missions.     

High performance nuclear thermal propulsion system for near term exploration missions to 100 A.U. and beyond

A new compact ultra light nuclear reactor engine design termed MITEE (MIniature Reac Tor EnginE) is described. MITEE heats hydrogen propellant to 3000 K, achieving a specific impulse of 1000 seconds and a thrust-to-weight of 10. Total engine mass is 200 kg, including reactor, pump, auxiliaries and a 30% contingency. MITEE enables many types of new and unique missions to the outer solar system not possible with chemical engines. Examples include missions to 100 A.U. in less than 10 years, flybys of Pluto in 5 years, sample return from Pluto and the moons of the outer planets, unlimited ramjet flight in planetary atmospheres, etc. Much of the necessary technology for MITEE already exists as a result of previous nuclear rocket development programs. With some additional development, initial MITEE missions could begin in only 6 years.     

Deployment history and design considerations for space reactor power systems

The history of the deployment of nuclear reactors in Earth orbits is reviewed with emphases on lessons learned and the operation and safety experiences. The former Soviet Union's “BUK” power systems, with SiGe thermoelectric conversion and fast neutron energy spectrum reactors, powered a total of 31 Radar Ocean Reconnaissance Satellites (RORSATs) from 1970 to 1988 in 260 km orbit. Two of the former Soviet Union's TOPAZ reactors, with in-core thermionic conversion and epithermal neutron energy spectrum, powered two Cosmos missions launched in 1987 in ～800 km orbit. The US’ SNAP-10A system, with SiGe energy conversion and a thermal neutron energy spectrum reactor, was launched in 1965 in 1300 km orbit. The three reactor systems used liquid NaK-78 coolant, stainless steel structure and highly enriched uranium fuel (90–96 wt%) and operated at a reactor exit temperature of 833–973 K. The BUK reactors used U-Mo fuel rods, TOPAZ used UO₂ fuel rods and four ZrH moderator disks, and the SNAP-10A used moderated U-ZrH fuel rods. These low power space reactor systems were designed for short missions (～0.5 kW_e and ～1 year for SNAP-10A, <3.0 kW_e and <6 months for BUK, and ～5.5 kW_e and up to 1 year for TOPAZ). The deactivated BUK reactors at the end of mission, which varied in duration from a few hours to ～4.5 months, were boosted into ～800 km storage orbit with a decay life of more than 600 year. The ejection of the last 16 BUK reactor fuel cores caused significant contamination of Earth orbits with NaK droplets that varied in sizes from a few microns to 5 cm. Power systems to enhance or enable future interplanetary exploration, in-situ resources utilization on Mars and the Moon, and civilian missions in 1000–3000 km orbits would generate significantly more power of 10's to 100's kW_e for 5–10 years, or even longer. A number of design options to enhance the operation reliability and safety of these high power space reactor power systems are presented and discussed.     

Rationale and systems architecture for a near-term human lunar return

Early human missions to the Moon have landed on six different sites on the lunar surface. These have all been in the low-latitude regions of the near side of the Moon. Early missions were designed primarily to assure crew safety rather than for scientific value. While the later missions added increasingly more challenging science, they remained restricted to near-side, low-latitude sites. Since the 1970s, we have learned considerably more about lunar planetology and resources. A return within the next five to ten years can greatly stimulate future human space exploration activities. We can learn much more about the distribution of lunar resources, especially about hydrogen, hydrated minerals, and water ice because they appear to be abundant near the lunar poles. The presence of hydrogen opens the possibility of industrial use of lunar resources to provide fuel for space transportation throughout the solar system.This paper discusses the rationale for near-term return of human crews to the Moon, and the advantages to be gained by selecting the Moon as the next target for human missions beyond low-Earth orbit. It describes a systems architecture for early missions, including transportation and habitation aspects. Specifically, we describe a primary transportation architecture that emphasizes existing Earth-to-orbit transportation systems, using expendable launch vehicles for cargo delivery and the Space Shuttle and its derivatives for human transportation. Transfer nodes should be located at the International Space Station (ISS) and at the Earth-Moon L1 (libration point).Each of the major systems is described, and the requisite technology readiness is assessed. These systems include Earth-to-orbit transportation, lunar transfer, lunar descent and landing, surface habitation and mobility, and return to Earth. With optimum reliance on currently existing space systems and a technology readiness assessment, we estimate the minimum development time required and perform order-of-magnitude cost estimates of a near-term human lunar mission.     

核热推进载人火星探测方案设计

针对载人火星探测任务,结合我国现有技术基础,提出我国载人火星探测方案,重点研究载人火星探测任务推进系统的设计。首先,综合考虑载人深空探测任务的约束,采用Pork-Chop图设计了适用于不同任务场景的转移轨迹;然后,参考我国空间站技术,基于核热推进系统设计了我国载人火星探测任务的飞船;最后,对核热推进系统的发动机台数和推力进行了优化,得到了适用于不同任务场景的最优推进系统组合方案。本文所研究内容为我国未来载人火星探测任务提供了有益参考。     

核热推进地面试验技术研究

核热推进具有比冲高、推力大等特点,在载人深空探测和星际货运任务上具有广阔应用前景。核热推进技术的研发需要进行大量地面试验。首先回顾了美国与俄罗斯的核热推进地面试验技术的发展,对地面试验技术进行分类总结。然后基于一种小型核火箭方案,研究了燃料元件非核试验、燃料元件辐照考验试验和带核整机地面试验等关键地面试验技术,并提出了初步试验方案。最后对我国核热推进地面试验的发展提出了一些建议。     

利用气动减速的国外深空探测器热控设计特点分析

气动减速技术能在耗费较少燃料的情况下,使探测器顺利进入预定环绕轨道.面向气动减速技术的深空探测器迎风面需要承受较高的气动热负荷与气动力,使得迎风面热控材料的耐热与耐冲击能力成为探测器设计的关键.文章对国外相关应用实例进行了调研和综述,并在此基础上总结了此类深空探测器热控系统的设计特点,可为气动减速技术在我国深空探测任务...     

Radiation engineering analysis of shielding materials to assess their ability to protect astronauts in deep space from energetic particle radiation

An analysis is performed on four typical materials (aluminum, liquid hydrogen, polyethylene, and water) to assess their impact on the length of time an astronaut can stay in deep space and not exceed a design basis radiation exposure of 150 mSv. A large number of heavy lift launches of pure shielding mass are needed to enable long duration, deep space missions to keep astronauts at or below the exposure value with shielding provided by the vehicle. Therefore, vehicle mass using the assumptions in the paper cannot be the sole shielding mechanism for long duration, deep space missions. As an example, to enable the Mars Design Reference Mission 5.0 with a 400 day transit to and from Mars, not including the 500 day stay on the surface, a minimum of 24 heavy lift launches of polyethylene at 89,375 lbm (40.54 tonnes) each are needed for the 1977 galactic cosmic ray environment. With the assumptions used in this paper, a single heavy lift launch of water or polyethylene can protect astronauts for a 130 day mission before exceeding the exposure value. Liquid hydrogen can only protect the astronauts for 160 days. Even a single launch of pure shielding material cannot protect an astronaut in deep space for more than 180 days using the assumptions adopted in the analysis. It is shown that liquid hydrogen is not the best shielding material for the same mass as polyethylene for missions that last longer than 225 days.     

Research on hypersonic aircraft using pre-cooled turbojet engines

Systems analysis of a Mach 5 class hypersonic aircraft is performed. The aircraft can fly across the Pacific Ocean in 2 h. A multidisciplinary optimization program for aerodynamics, structure, propulsion, and trajectory is used in the analysis. The result of each element model is improved using higher accuracy analysis tools. The aerodynamic performance of the hypersonic aircraft is examined through hypersonic wind tunnel tests. A thermal management system based on the data of the wind tunnel tests is proposed. A pre-cooled turbojet engine is adopted as the propulsion system for the hypersonic aircraft. The engine can be operated continuously from take-off to Mach 5. This engine uses a pre-cooling cycle using cryogenic liquid hydrogen. The high temperature inlet air of hypersonic flight would be cooled by the same liquid hydrogen used as fuel. The engine is tested under sea level static conditions. The engine is installed on a flight test vehicle. Both liquid hydrogen fuel and gaseous hydrogen fuel are supplied to the engine from a tank and cylinders installed within the vehicle. The designed operation of major components of the engine is confirmed. A large amount of liquid hydrogen is supplied to the pre-cooler in order to make its performance sufficient for Mach 5 flight. Thus, fuel rich combustion is adopted at the afterburner. The experiments are carried out under the conditions that the engine is mounted upon an experimental airframe with both set up either horizontally or vertically. As a result, the operating procedure of the pre-cooled turbojet engine is demonstrated.     

The hydrogen value chain: applying the automotive role model of the hydrogen economy in the aerospace sector to increase performance and reduce costs

Hydrogen will assume a key role in Europe's effort to adopt its energy dependent society to satisfy its needs without releasing vast amounts of greenhouse gases. The paradigm shift is so paramount that one speaks of the “Hydrogen Economy”, as the energy in this new and ecological type of economy is to be distributed by hydrogen. However, H₂ is not a primary energy source but rather an energy carrier, a means of storing, transporting and distributing energy, which has to be generated by other means.Various H₂ storage methods are possible; however industries' favourite is the storage of gaseous hydrogen in high pressure tanks. The biggest promoter of this storage methodology is the automotive industry, which is currently preparing for the generation change from the fossil fuel internal combustion engines to hydrogen based fuel cells. The current roadmaps foresee a market roll-out by 2015, when the hydrogen supply infrastructure is expected to have reached a critical mass. The hydrogen economy is about to take off as being demonstrated by various national mobility strategies, which foresee several millions of electric cars driving on the road in 2020.Fuel cell cars are only one type of “electric car”, battery electric as well as hybrid cars – all featuring electric drive trains – are the others. Which type of technology is chosen for a specific application depends primarily on the involved energy storage and power requirements. These considerations are very similar to the ones in the aerospace sector, which had introduced the fuel cell already in the 1960s. The automotive sector followed only recently, but has succeeded in moving forward the technology to a level, where the aerospace sector is starting considering to spin-in terrestrial hydrogen technologies into its technology portfolio. Target areas are again high power/high energy applications like aviation, manned spaceflight and exploration missions, as well as future generation high power telecommunication satellites. Similar trends can be expected in the future for RADAR Earth Observation satellites and space infrastructure concepts of great scale.This paper examines current activities along the hydrogen value chain, both in the terrestrial and the aerospace sector. A general assessment of the synergy potential is complemented by a thorough analysis of specific applications serving as role models like a lunar manned base or pressurised rover, an aircraft APU or a high power telecommunications satellite. Potential performance improvements and cost savings serve as key performance indicators in these comparisons and trade-offs.     

用进化算法求解轨道转移的时间-能量优化问题

随着航天任务需求的多样化，对航天器轨道转移问题不但提出了最省燃料的要求，而且提出了最小时间的要求，这篇文章用进化算法解决了这一组合优化问题，仿真结果证明了算法的有效性。     

Ozone concentrations and ultraviolet fluxes on Earth-like planets around other stars

Coupled radiative-convective/photochemical modeling was performed for Earth-like planets orbiting different types of stars (the Sun as a G2V, an F2V, and a K2V star). O(2) concentrations between 1 and 10(-5) times the present atmospheric level (PAL) were simulated. The results were used to calculate visible/near-IR and thermal-IR spectra, along with surface UV fluxes and relative dose rates for erythema and DNA damage. For the spectral resolution and sensitivity currently planned for the first generation of terrestrial planet detection and characterization missions, we find that O(2) should be observable remotely in the visible for atmospheres containing at least 10(-2) PAL of O(2). O(3) should be visible in the thermal-IR for atmospheres containing at least 10(-3) PAL of O(2). CH(4) is not expected to be observable in 1 PAL O(2) atmospheres like that of modern Earth, but it might be observable at thermal-IR wavelengths in "mid-Proterozoic-type" atmospheres containing approximately 10(-1) PAL of O(2). Thus, the simultaneous detection of both O(3) and CH(4) - considered to be a reliable indication of life - is within the realm of possibility. High-O(2) planets orbiting K2V and F2V stars are both better protected from surface UV radiation than is modern Earth. For the F2V case the high intrinsic UV luminosity of the star is more than offset by the much thicker ozone layer. At O(2) levels below approximately 10(-2) PAL, planets around all three types of stars are subject to high surface UV fluxes, with the F2V planet exhibiting the most biologically dangerous radiation environment. Thus, while advanced life is theoretically possible on high-O(2) planets around F stars, it is not obvious that it would evolve as it did on Earth.     

核热火箭发动机系统循环方案分析与设计

核热火箭发动机是未来实现载人火星探测的首选动力方案,其具备高比冲、大推力和长工作寿命等优点。我国在此方面研究较少,亟需开展核热推进技术理论及方法的研究。核热火箭发动机系统循环分析与设计是关键问题之一,对推进系统总体设计有重要意义。分析了3种可用于核热火箭发动机系统循环的方案特点,基于闭式膨胀循环设计了比冲为910 s ...     

Comparison of advanced propulsion systems in cislunar space

Chemical engines fueled by LOX/aluminium powder, oxygen-fueled ion engines, solid core nuclear reactor engines and nuclear light bulb engines are analysed for transportation purposes in cislunar space. The markets envisaged are the nuclear waste disposal on the lunar surface and/or support of SPS construction in GEO. It is shown that the most fuel efficient permanent space transportation system is not necessarily the most economical choice due to high hardware cost.     

A Canadian high-energy neutron spectrometry system for measurements in space

Bubble Technology Industries Inc. (BTI), with the support of the Canadian Space Agency, has finished the construction of the Canadian High-Energy Neutron Spectrometry System (CHENSS). This spectrometer is intended to measure the high energy neutron spectrum (approximately 1-100 MeV) encountered in spacecraft in low earth orbit. CHENSS is designed to fly aboard a US space shuttle and its scientific results should facilitate the prediction of neutron dose to astronauts in space from readings of different types of radiation dosimeters that are being used in various missions.     

碳纤维复合材料贮箱内压和低温承载行为研究

碳纤维增强聚合物复合材料具有轻质高强的优异特性,是液氢液氧燃料贮箱的理想材料。然而液氢液氧燃料贮箱在服役时要承受极低温度载荷,复合材料贮箱箱体的低温结构可靠性尚未可知。开展了碳纤维/环氧复合材料缠绕贮箱结构在温度和内压载荷下的变形及损伤研究,分别进行了常温/低温抗渗漏测试,结合应变测量、声发射监测、氦质谱检漏等方法分别研究了内压以及低温工况对复合材料贮箱的应变分布及损伤泄漏状态影响机制。研究结果表明,封头与圆筒区域交界处易产生应变集中,低温载荷导致复合材料局部小幅度基体损伤及纤维/基体界面脱粘,但并未影响贮箱箱体承压性能和气密性。本研究可为未来大型航天器减质设计提供参考。     

甲烷-乙烷混合推进剂深度过冷技术的实验研究

针对甲烷采用液氮过冷可能发生甲烷冰堵风险,提出了在甲烷中添加乙烷,制备凝固温度更低的甲烷-乙烷混合推进剂的新方案,搭建实验系统测试了甲烷-乙烷凝固温度变化规律。研究发现,随着甲烷含量提高,混合推进剂凝固温度先降低后升高。当甲烷、乙烷比例为0.71∶0.29时,混合推进剂达到最低凝固温度,约73.0 K。当采用常压饱和液氮对混合推进剂过冷时,控制甲烷含量在0.52~0.81间可避免推进剂冻结。相较于常压饱和甲烷,防冻结区的混合推进剂密度提高了24.0%~38.4%,液相存在温区增大至35.7 K~40.5 K。此外,甲烷-乙烷混合推进剂具有理论比冲高、再生冷却性能佳、结焦与积碳小等优势。所提出的甲烷-乙烷混合推进剂在火星探测等任务中具有可观的应用前景。     

伴随卫星的燃料-时间优化回收

伴随卫星回收是伴星应用中的一项主要技术。航天任务需求对伴星回收问题不仅提出了最省燃料要求，而且提出了最小时间要求。本文设计了一条稳定的燃料-时间优化回收轨道。从相对运动的Hill方程出发，给出伴星回收问题描述，阐述回收轨道设计思想及稳定回收条件，提出一种有效的螺旋式回收策略，探讨参数确定方法，并对回收轨道的特点和稳定性进行分析，最后研究了燃料消耗量与回收时间及初始相位的关系。仿真结果表明，利用螺旋回收策略，可以保证伴随卫星快速、稳定回收，且能在燃料消耗量与回收时间之间寻求最佳折衷。