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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 Spectrum01:23

Mass Spectrum

A mass spectrum is the graphical representation of the relative abundance of the charged fragments in an analyte plotted against their mass-to-charge ratio (m/z). The plot's x-axis represents the ratio of the mass of the charged fragment to the number of charges it carries. The y axis of the plot represents the relative abundance of each charged species. The relative abundance is calculated from the signal intensity of each charged species recorded at the detector. The most intense signal (the...
IR Frequency Region: Fingerprint Region01:03

IR Frequency Region: Fingerprint Region

IR spectra are divided into two main regions: the diagnostic region and the fingerprint region. The diagnostic region of the spectrum lies above 1500 cm−1. The absorptions resulting from single-bond vibrations of the N–H, C–H, and O–H stretch at higher wavenumbers and appear on the left side of the spectrum. The stretching absorptions of the C≡C and C≡N occur between 2100–2300 cm−1. In contrast, those arising from stretching absorptions of the C=O, C=N, and C=C occur between 1600–1850 cm−1.
The...
Flame Photometry: Overview01:02

Flame Photometry: Overview

Flame photometry, also known as flame emission spectrometry, is a technique used for the qualitative and quantitative analysis of elements present in a sample using a flame as the source of excitation energy. The concept of flame photometry was realized in the early 1860s by Kirchhoff and Bunsen, who discovered that specific elements emit characteristic radiation when excited in flames. The first instrument developed for this purpose was used to measure sodium (Na) in plant ash using a Bunsen...
Flame Photometry: Lab01:16

Flame Photometry: Lab

In a flame photometer, when a solution like potassium chloride is aspirated into the flame, the solvent evaporates, leaving behind dehydrated salt. This salt dissociates into free gaseous atoms in their ground state. Some of these atoms absorb energy from the flame, leading to their excitation. The excited atoms return to the ground state, emitting photons at characteristic wavelengths. Because only electronic transitions are involved, the resulting emission lines are very narrow. The intensity...
Torque Free Motion01:15

Torque Free Motion

The torque-free motion refers to the movement of a rigid body in space when no external torques are acting upon it. This type of motion can be observed in environments where there are no external forces or frictions, like in outer space. For example, a rotation of Mars in space is a torque-free motion. Mars is an axisymmetric object, meaning it has an axis of symmetry along which it rotates, designated as the z-axis. The rotating frame of reference is defined such that the center of mass of...

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相关实验视频

Updated: Jul 13, 2026

Pore-scale Imaging and Characterization of Hydrocarbon Reservoir Rock Wettability at Subsurface Conditions Using X-ray Microtomography
12:18

Pore-scale Imaging and Characterization of Hydrocarbon Reservoir Rock Wettability at Subsurface Conditions Using X-ray Microtomography

Published on: October 21, 2018

由OMEGA/Mars Express观测所揭示的火星表面的多样性

Jean-Pierre Bibring1, Yves Langevin, Aline Gendrin

  • 1Institut d'Astrophysique Spatiale (IAS), Bâtiment 121, 91405 Orsay Campus, France. bibring@ias.u-psud.fr

Science (New York, N.Y.)
|February 19, 2005
PubMed
概括

矿物学观测中心,l

更多相关视频

Scattering And Absorption of Light in Planetary Regoliths
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Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
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Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

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相关实验视频

Last Updated: Jul 13, 2026

Pore-scale Imaging and Characterization of Hydrocarbon Reservoir Rock Wettability at Subsurface Conditions Using X-ray Microtomography
12:18

Pore-scale Imaging and Characterization of Hydrocarbon Reservoir Rock Wettability at Subsurface Conditions Using X-ray Microtomography

Published on: October 21, 2018

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
06:48

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Published on: May 10, 2020

科学领域:

  • 行星科学 行星科学
  • 矿物学是什么?矿物学是什么?
  • 地质地质地质地质地质地

背景情况:

  • 火星表面的组成对于理解它的地质演变至关重要.
  • 之前的任务提供了有限的高分辨率矿物学数据.

研究的目的:

  • 用可见近红外高光谱反射图像绘制火星表面矿物质的地图.
  • 通过详细的表面组成分析,了解火星的演变.

主要方法:

  • 在火星快速任务中使用矿物学,水,冰,活动观测仪 (OMEGA) 仪器.
  • 在0.3至5公里分辨率获得超光谱反射率图像.
  • 分析任务前9个月的数据.

主要成果:

  • 在北方和南方的火星地上识别和绘制了马菲克含铁的酸盐.
  • 检测到局部度的水合酸盐和硫酸盐.
  • 观测到北极多年树冠上的水冰组成和南极树冠上的二氧化碳冰层.
  • 在分析区域中没有发现碳酸盐的证据.

结论:

  • 火星表现出多样化和复杂的表面矿物学.
  • 这些发现为地球的地质历史和演变提供了关键的见解.
  • 欧米茄的数据揭示了极地帽之间明显的组成差异.