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THE MESSENGER SCIENCE PAYLOAD

机译:信使科学有效载荷

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The MESSENGER spacecraft will orbit Mercury and gather data for one Earth year with a miniaturized scientific payload. The MESSENGER project is in the integration and test phase in mid 2003. Seven assembled and calibrated instruments are mounted on the spacecraft. The Gamma-Ray and Neutron Spectrometer has a Gamma-Ray Spectrometer to measure atomic composition with a high-purity germanium detector and a Neutron Spectrometer that uses lithium-glass and boron-loaded plastic scintillators for sensing thermal, epithermal, and fast neutrons. The X-Ray Spectrometer measures Mercury surface elemental abundances by examining solar-flare-induced X-ray fluorescence lines. Three gas-filled proportional counters detect the X-ray fluorescence lines from the planet's surface, and a solid-state solar monitor measures the X-ray input to the planet. The Mercury Dual Imaging System (MDIS) has both wide-field and narrow-field cameras to map the surface of the planet. MDIS is also multi-spectral, with a 12-position filter wheel for the wide-field camera. The Mercury Atmospheric and Surface Composition Spectrometer measures both surface spectral reflectance in the visible and near infrared and exospheric emission lines in the ultraviolet and visible. The Mercury Laser Altimeter (MLA) determines the range to the planet with a resolution of 0.3 m. MLA will be combined with the radio-science investigation to map the gravitational field of the planet and determine the obliquity and physical libration amplitude. A magnetometer, mounted on a 3.6-m boom, will map the internal and external magnetic field. The Energetic Particle and Plasma Spectrometer will measure particles accelerated in the magnetosphere and the interactions of the magnetosphere with the solar wind. MDIS has its own pivot platform. All of the other instruments are fixed to the spacecraft. Pointing is accomplished by steering the entire spacecraft. All of the instruments are designed to deal with the extreme thermal environment at Mercury, where the sunward face of the spacecraft will reach temperatures above 350°C. MESSENGER will launch in May 2004 and begin orbital observations of Mercury in October 2009.
机译:Messenger SpaceCraft将用小型化的科学有效载荷来收集一个地球年的数据。 Messenger项目在2003年中期的集成和测试阶段。七个组装和校准的仪器安装在航天器上。伽马射线和中子光谱仪具有γ射线光谱仪,用于测量具有高纯度锗检测器的原子组合物和中子谱仪,用于使用锂 - 玻璃和硼负载的塑料闪烁体来传感热,换术和快速中子。 X射线光谱仪通过检查太阳耀斑诱导的X射线荧光线来测量汞表面元素丰富。三个气体填充的比例计数器检测来自行星表面的X射线荧光线,固态太阳能监视器测量输入到行星的X射线。汞双成像系统(MDIS)具有宽场和窄场相机来映射行星的表面。 MDIS也是多光谱的,具有12位滤光轮,用于宽野相机。汞气氛和表面成分光谱仪在紫外线中的可见和近红外线和极端发射线中测量表面光谱反射率和可见光。汞激光高度计(MLA)确定行星的范围,分辨率为0.3米。 MLA将与无线电科学调查相结合,以映射地球的引力场并确定倾斜和物理挽损的倾幅。磁力计安装在3.6米的吊杆上,将映射内部和外部磁场。能量粒子和等离子体光谱仪将测量磁层中加速的颗粒和磁层与太阳风的相互作用。 MDIS有自己的枢轴平台。所有其他仪器都固定在航天器上。指向通过转向整个航天器来实现。所有仪器都旨在处理汞的极端热环境,航天器的阳光面将达到350°C以上的温度。 Messenger将于2004年5月推出,并于2009年10月开始轨道观察汞。

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