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関連する概念動画

Infrared (IR) Spectroscopy: Overview01:09

Infrared (IR) Spectroscopy: Overview

6.8K
When electromagnetic radiation passes through a material, atoms or molecules transition from a lower to a higher energy state by absorbing radiation corresponding to the energy difference between the two states. The absorption of infrared (IR) radiation causes transitions between vibrational energy levels in a molecule. Therefore, IR spectroscopy is a useful analytical tool for determining the molecular structure of molecules.
Different compounds display unique properties due to their...
6.8K
IR Spectrum01:19

IR Spectrum

3.3K
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%...
3.3K
IR Spectroscopy: Molecular Vibration Overview01:24

IR Spectroscopy: Molecular Vibration Overview

5.8K
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...
5.8K
IR Spectrometers01:25

IR Spectrometers

3.1K
There are two main infrared (IR) spectrophotometers: dispersive IR spectrometers and Fourier transform infrared (FTIR) spectrometers. In a dispersive IR spectrometer, a beam of infrared radiation produced by a hot wire is divided into two parallel equal-intensity beams using mirrors. One beam passes through the sample, while another is a reference beam. The beams then move through the monochromator, which separates the radiations into a continuous spectrum of different frequencies. The...
3.1K
IR Absorption Frequency: Delocalization01:04

IR Absorption Frequency: Delocalization

1.7K
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...
1.7K
IR Frequency Region: Fingerprint Region01:03

IR Frequency Region: Fingerprint Region

2.1K
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...
2.1K

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関連する実験動画

Updated: May 5, 2026

Diffuse Reflectance Infrared Spectroscopic Identification of Dispersant/Particle Bonding Mechanisms in Functional Inks
10:31

Diffuse Reflectance Infrared Spectroscopic Identification of Dispersant/Particle Bonding Mechanisms in Functional Inks

Published on: May 8, 2015

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銀河中心地域の赤外線拡散型星間波帯は,銀河の中心地域にある.

T R Geballe1, F Najarro, D F Figer

  • 1Gemini Observatory, 670 N. A'ohoku Place, Hilo, Hawaii 96720, USA. tgeballe@gemini.edu

Nature
|November 4, 2011
PubMed
まとめ

研究者らは,銀河の中心で13の新しい分散星間帯 (DIB) を発見した. これらの宇宙吸収特性は,おそらく炭素ベースの分子であり,以前に観測されたDIBよりも厳しい環境で現れる.

科学分野:

  • 天文学 天文学
  • 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.

背景:

  • 拡散星間帯 (DIB) は,星間物質による星間スペクトルで観測される吸収特性です.
  • 500以上のDIBが知られているが,主に可視波長と近赤外線波長で発生する.
  • DIBsの媒体は,多原子炭素を含む分子であると疑われるが,いずれも決定的に特定されていない.

研究 の 目的:

  • より長い赤外線波長 (1.5-1.8マイクロメートル) で新しいDIBを探し,特徴づけます.
  • 新しく発見されたDIBの起源と環境を調査する.
  • 銀河中心のDIB特性を他の拡散雲の特性と比較するために.

主な方法:

  • 高解像度スペクトロスコープによる,銀河の中心に向かって,高度に絶滅している恒星の観測.
  • 1.5-1.8マイクロメートルの波長区間のスペクトルの分析.
  • DIB強度と星間絶滅値の比較.

主要な成果:

  • 1.5-1.8マイクロメートルの範囲で13の新しい分散型恒星間帯を発見した.
  • これらのDIBは,主に銀河の中心に向かって観測され,この地域からの起源を示唆しています.

さらに関連する動画

Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies
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Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies

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Photoelectron Imaging of Anions Illustrated by 310 Nm Detachment of F&#8722;
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Photoelectron Imaging of Anions Illustrated by 310 Nm Detachment of F−

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関連する実験動画

Last Updated: May 5, 2026

Diffuse Reflectance Infrared Spectroscopic Identification of Dispersant/Particle Bonding Mechanisms in Functional Inks
10:31

Diffuse Reflectance Infrared Spectroscopic Identification of Dispersant/Particle Bonding Mechanisms in Functional Inks

Published on: May 8, 2015

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Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies
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Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies

Published on: December 18, 2015

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Photoelectron Imaging of Anions Illustrated by 310 Nm Detachment of F&#8722;
06:53

Photoelectron Imaging of Anions Illustrated by 310 Nm Detachment of F−

Published on: July 27, 2018

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  • これらのDIBの相対的な強さは,以前に知られているDIBに類似して,星間絶滅と相関しています.
  • 結論:

    • 銀河の中心には,これまで知られていなかった星間波帯が広がっており,温暖で厳しい環境から発生しています.
    • これらの新しいDIBsのキャリアは,既知のDIBsのキャリアに似ており,おそらく多原子炭素分子である可能性があります.
    • DIBの強さは,特定の環境に関係なく,一般的には拡散した恒星間物質の量に比例します.