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IR Spectroscopy: Molecular Vibration Overview01:24

IR Spectroscopy: Molecular Vibration Overview

When Infrared (IR) radiation passes through a covalently bonded molecule, the bonds transition from lower to higher vibrational levels. The fundamental vibrational motions that result in infrared absorption can be classified as stretching or bending vibrations.
Stretching vibrations are vibrational motions that occur along the bond line, changing the bond length or distance between two bonded atoms. They are further distinguished as symmetric or asymmetric. In symmetric stretching, the...
IR Spectrum01:19

IR Spectrum

When infrared (IR) radiation passes through a molecule, the bonds stretch or bend by absorbing the radiation. This absorption creates the molecule's absorption spectrum, which is the plot of its percentage transmittance versus wavenumber.
Transmittance is defined as the ratio of the radiant power passing through a sample to that from the radiation's source. Multiplying the transmittance by 100 gives the percent transmittance (%T), which varies between 100% (no absorption) and 0% (complete...
Diffusion on Chromatography Columns01:07

Diffusion on Chromatography Columns

In column chromatography, when an analyte is introduced as a narrow band at the top of the column, the solutes begin to separate and broaden, developing a Gaussian profile. This broadening occurs due to various factors, such as longitudinal diffusion.
Longitudinal diffusion occurs when the solute molecules in the mobile phase diffuse from the more concentrated center of the chromatographic band to the more dilute regions on either side, both towards and against the flow direction. This...
IR Absorption Frequency: Delocalization01:04

IR Absorption Frequency: Delocalization

Electron delocalization refers to the distribution of electrons across multiple atoms within a molecule rather than being confined to a single atom or bond. This phenomenon is common in systems with conjugated bonds—structures where alternating single and double bonds allow π-electrons to move freely across the network. The movement of electrons stabilizes the molecule and can affect various chemical properties, including vibrational frequencies observed in IR spectroscopy.
In IR spectroscopy,...
UV–Vis Spectroscopy: Molecular Electronic Transitions01:16

UV–Vis Spectroscopy: Molecular Electronic Transitions

In Ultraviolet–Visible (UV–Vis) spectroscopy, the absorption of electromagnetic radiation is used to probe the electronic structure of molecules. This technique provides insights into molecular electronic transitions, particularly the movement of electrons between different molecular orbitals. Radiation is absorbed if the energy of the electromagnetic radiation passing through the molecule is precisely equal to the energy difference between the excited and ground states. During this process,...
IR Spectroscopy: Hooke's Law Approximation of Molecular Vibration01:16

IR Spectroscopy: Hooke's Law Approximation of Molecular Vibration

A covalently bonded heteronuclear diatomic molecule can be modeled as two vibrating masses connected by a spring. The vibrational frequency of the bond can be expressed using an equation derived from Hooke's law, which describes how the force applied to stretch or compress a spring is proportional to the displacement of the spring. In this case, the atoms behave like masses, and the bond acts like a spring.
According to Hooke's law, the vibrational frequency is directly proportional to the...

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Updated: Jul 12, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

赤色の長方形の分子分散星間帯域媒体は,赤色の長方形に示されています.

P J Sarre, J R Miles, S M Scarrott

    Science (New York, N.Y.)
    |August 4, 1995
    PubMed
    まとめ

    研究者らは,赤直角星雲の未確認放射帯の分子キャリアを特定した. これらの分子はまた,拡散した恒星間吸収帯を生成し,ガス相分子の形で存在することを示しています.

    科学分野:

    • 天体物理学 天体物理学
    • スペクトロスコーピーは,スペクトロスコーピーを用います.
    • アストロケミストリー アストロケミストリー

    背景:

    • 赤い長方形は,未確認の放射帯を持つユニークな二角形の星雲です.
    • 星間空間では分散型星間波帯 (DIB) が観測されているが,その媒体はほとんど不明である.

    研究 の 目的:

    • 赤四角星雲の未確認放射帯の性質を調査する.
    • これらの放射帯が,既知の分散型星間吸収帯とのキャリアを共有しているかどうかを判断する.

    主な方法:

    • 赤直角星雲の高解像度光学スペクトルスコピー. 赤直角星雲.
    • 中央恒星HD 44179.9からの距離の関数として放射帯の波長と幅の分析.
    • 赤直角帯の性質を,既知の拡散星間吸収帯と比較する.

    主要な成果:

    • 赤い長方形の観測された放射帯は,中央の星からの距離が大きくなるにつれて,ピーク波長と幅の減少を示しています.
    • これらの帯は,既知の拡散星間吸収帯 (例えば,5797,580,6614) と一致する値に収束する.
    • 同じ分子種が,赤方形の放射帯と,特定の星間吸収帯の両方に責任がある.

    さらに関連する動画

    In Situ Monitoring of Diffusion of Guest Molecules in Porous Media Using Electron Paramagnetic Resonance Imaging
    06:34

    In Situ Monitoring of Diffusion of Guest Molecules in Porous Media Using Electron Paramagnetic Resonance Imaging

    Published on: September 2, 2016

    Spatial Separation of Molecular Conformers and Clusters
    10:37

    Spatial Separation of Molecular Conformers and Clusters

    Published on: January 9, 2014

    関連する実験動画

    Last Updated: Jul 12, 2026

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    In Situ Monitoring of Diffusion of Guest Molecules in Porous Media Using Electron Paramagnetic Resonance Imaging
    06:34

    In Situ Monitoring of Diffusion of Guest Molecules in Porous Media Using Electron Paramagnetic Resonance Imaging

    Published on: September 2, 2016

    Spatial Separation of Molecular Conformers and Clusters
    10:37

    Spatial Separation of Molecular Conformers and Clusters

    Published on: January 9, 2014

    結論:

    • これらの未確認の赤方形の放射帯の媒体は,ガス相分子である.
    • これらの分子はまた,星間放射を星間化学と結びつける,特定の拡散した星間吸収帯に責任があります.