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相关概念视频

Emission Spectra02:39

Emission Spectra

When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
Mass Spectrum: Interpretation01:24

Mass Spectrum: Interpretation

An unknown compound can be established by identifying the molecular ion peak in the mass spectrum. The molecular ion peak is often weak or absent due to the predominance of fragmentation in high-energy electron beams. In such cases, a soft-energy electron beam can be used to scan the spectrum to enhance the intensity of the molecular ion peak. Additionally, chemical ionization, field ionization, and desorption ionization spectra are used to obtain a relatively intense molecular ion peak.To...
Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

Atomic emission spectroscopy (AES) is an analytical technique used to determine the elemental composition of a sample by analyzing the light emitted from excited atoms. In AES, atoms in a sample are excited to higher energy levels by thermal energy from high-temperature sources, such as plasma, arcs, or sparks. When these excited atoms return to lower energy states, they emit light at specific wavelengths characteristic of each element. The resulting atomic emission spectrum, which consists of...
Atomic Emission Spectroscopy: Interference01:30

Atomic Emission Spectroscopy: Interference

In atomic emission spectroscopy (AES), high-temperature atomizers excite a broad range of elements and molecules that generate complex emissions from sources such as oxides, hydroxides, and flame combustion products in the flame or plasma. Several strategies can be employed to minimize spectral interferences caused by overlapping emission lines or bands. These include increasing instrument resolution, choosing alternative emission lines, optimally placing the detector in low-background regions,...
Atomic Emission Spectroscopy: Lab01:29

Atomic Emission Spectroscopy: Lab

AES is a powerful analytical technique, especially effective when used with plasma sources, producing abundant spectra in characteristic emission lines. The Inductively Coupled Plasma (ICP), in particular, yields superior quantitative analytical data due to its high stability, low noise, low background, and minimal interferences under optimal experimental conditions. However, newer air-operated microwave sources are emerging as promising alternatives that could be more cost-effective than...
Electronic Distance Measuring Instruments01:30

Electronic Distance Measuring Instruments

Electronic Distance Measuring Instruments (EDMs) are essential tools in modern surveying, offering precise distance measurements by emitting electromagnetic signals and calculating the time required for these signals to travel to a target and return. Two primary types of signals are used in EDMs — light waves and microwaves — each suited to specific environmental and distance requirements. Light-wave-based EDMs utilize either infrared or laser light, providing high accuracy over short distances...

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Updated: Jul 13, 2026

Electron Spin Resonance Micro-imaging of Live Species for Oxygen Mapping
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Electron Spin Resonance Micro-imaging of Live Species for Oxygen Mapping

Published on: August 26, 2010

在Eros附近:成像和光谱结果.

Veverka1, Robinson, Thomas

  • 1Space Sciences Building, Cornell University, Ithaca, NY 14853, USA. Department of Geological Sciences, Northwestern University, 309 Locy Hall, Evanston, IL 60208, USA. Applied Physics Laboratory, Johns Hopkins University, 1110 Johns Hopkins Road, L.

Science (New York, N.Y.)
|September 23, 2000
PubMed
概括

小行星Eros是一颗大而长长的天体,表现出一个充满坑的表面,有突出的线条和丰富的喷射块. 它的组成与普通的地铁相一致,表明了显著的内部多孔性.

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科学领域:

  • 接近地球的物体研究研究
  • 小行星地质学
  • 星球科学 星球科学

背景情况:

  • 小行星Eros是一颗长长的近地天体,尺寸为34x11x11公里.
  • 它的表面有大量的石坑,最大的可见石坑直径为5.5公里.

研究的目的:

  • 描述小行星Eros的地质特征和组成.
  • 了解Eros的表面过程和内部结构.

主要方法:

  • 分析表面形态,包括坑道,线条和喷射块.
  • 用光谱分析 (800-2500nm) 确定表面成分.
  • 密度测量 (2.67 +/- 0.1 g/cm3) 来推断内部的多孔性.

主要成果:

  • 埃罗斯的表面充满了小石坑 (小于1公里) 和突出的沟和山脊,可能是由于过去的碰撞.
  • 丰富的喷射块 (30-100米) 存在,与白色差异的变化与火山口墙壁的 regolith 运动有关.
  • 频谱数据与普通石组成一致,表明内部孔隙度为10-30%.

结论:

  • 埃罗斯的地质特征提供了对小行星表面演变和撞击过程的见解.
  • 推断的组成和多孔性表明,Eros是一个由普通的石材料形成的原始物体.