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関連する概念動画

¹H NMR of Labile Protons: Deuterium (²H) Substitution00:48

¹H NMR of Labile Protons: Deuterium (²H) Substitution

This lesson illustrates the role of deuterium substitution in simplifying the NMR spectrum of compounds comprising labile protons. One method employed is the use of deuterium. Amongst the three isotopes of hydrogen, deuterium (2H) has a nucleus composed of one proton and one neutron. When the D2O solvent is added to a pure dry ethanol solution, its labile proton is substituted with deuterium.
¹³C NMR: Distortionless Enhancement by Polarization Transfer (DEPT)01:20

¹³C NMR: Distortionless Enhancement by Polarization Transfer (DEPT)

When proton-coupled carbon-13 spectra are simplified by a broadband proton decoupling technique, structural information about the coupled protons is lost. Distortionless enhancement by polarization transfer (DEPT) is a technique that provides information on the number of hydrogens attached to each carbon in a molecule. While the DEPT experiment utilizes complex pulse sequences, the pulse delay and flip angle are specifically manipulated. The resulting signals have different phases depending on...
¹H NMR of Conformationally Flexible Molecules: Variable-Temperature NMR01:15

¹H NMR of Conformationally Flexible Molecules: Variable-Temperature NMR

The axial and equatorial protons in cyclohexane can be distinguished by performing a variable-temperature NMR experiment. In this process, except for one proton, the remaining eleven protons are replaced by deuterium. The deuterium substitution avoids the possible peak splitting caused by the spin-spin coupling between the adjacent protons. The remaining proton flips between the axial and equatorial positions.
Hybridization of Atomic Orbitals I03:24

Hybridization of Atomic Orbitals I

The mathematical expression known as the wave function, ψ, contains information about each orbital and the wavelike properties of electrons in an isolated atom. When atoms are bound together in a molecule, the wave functions combine to produce new mathematical descriptions that have different shapes. This process of combining the wave functions for atomic orbitals is called hybridization and is mathematically accomplished by the linear combination of atomic orbitals. The new orbitals that...
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...
Chemical Shift: Internal References and Solvent Effects01:17

Chemical Shift: Internal References and Solvent Effects

In an NMR sample, precise measurement of the absolute absorption frequencies of nuclei is difficult. A standard internal reference compound is added, and the frequency difference between the reference signal and sample signals is measured.
The internal reference compound generally used in NMR spectroscopy is tetramethylsilane (TMS). TMS is preferred because it is chemically inert, soluble in NMR solvents, and easily removable. Also, the highly shielded methyl protons in TMS yield an intense...

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関連する実験動画

Updated: Jul 12, 2026

Methane Hydrate Crystallization on Sessile Water Droplets
08:46

Methane Hydrate Crystallization on Sessile Water Droplets

Published on: May 26, 2021

土星で観測された脱塩メタン.

U Fink, H P Larson

    Science (New York, N.Y.)
    |July 28, 1978
    PubMed
    まとめ

    研究者らは土星の大気中にデュテリアスメタン (CH3D) を検出し,デュテリアムと水素の比率が木星に匹敵することを明らかにした. この発見は,初期の太陽系の組成に関する洞察を提供します.

    科学分野:

    • 惑星科学は惑星科学である.
    • スペクトル顕微鏡検査です.
    • 大気化学 大気化学

    背景:

    • 脱硫メタン (CH3D) は,惑星の大気の研究における重要なトレーサーである.
    • 以前の研究では,太陽系の様々な天体でデュテリウムと水素の比率を確立しました.

    研究 の 目的:

    • 土星の大気中のCH(3) Dの豊富さを決定するために.
    • 土星のデウテリウムと水素の比率を計算する.
    • 土星のデウテリウムの豊富さを他の太陽系天体と比較するために.

    主な方法:

    • フーリエ変換スペクトロメーターを用いた土星の5ミクロンスペクトルの観測.
    • CH(3) D. のV(2) 帯の吸収特性の分析

    主要な成果:

    • CH(3) Dの豊富さは,2.6 +/- 0.8cm-amagat.で測定されました.
    • 平均光譜線形成レベル温度は175 +/- 30Kと決定されました.
    • 土星の大気中のデウテリウムと水素の比率は約2×10−5であることが判明した.

    結論:

    さらに関連する動画

    Measuring Dissolved Methane in Aquatic Ecosystems Using An Optical Spectroscopy Gas Analyzer
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    Measuring Dissolved Methane in Aquatic Ecosystems Using An Optical Spectroscopy Gas Analyzer

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    Supercritical Nitrogen Processing for the Purification of Reactive Porous Materials
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    Supercritical Nitrogen Processing for the Purification of Reactive Porous Materials

    Published on: May 15, 2015

    関連する実験動画

    Last Updated: Jul 12, 2026

    Methane Hydrate Crystallization on Sessile Water Droplets
    08:46

    Methane Hydrate Crystallization on Sessile Water Droplets

    Published on: May 26, 2021

    Measuring Dissolved Methane in Aquatic Ecosystems Using An Optical Spectroscopy Gas Analyzer
    05:00

    Measuring Dissolved Methane in Aquatic Ecosystems Using An Optical Spectroscopy Gas Analyzer

    Published on: July 26, 2024

    Supercritical Nitrogen Processing for the Purification of Reactive Porous Materials
    09:05

    Supercritical Nitrogen Processing for the Purification of Reactive Porous Materials

    Published on: May 15, 2015

  • 土星の大気温は,5ミクロンの窓で,大気圏の奥深くから発する熱放射線を示唆しています.
  • 土星のデウテリウムと水素の比率は,木星と同等だが,地球より低い.
  • この比率は,初期の太陽系の原始的なデウテリウムと水素の比率を表しているのかもしれない.