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関連する概念動画

Kinetic Molecular Theory and Gas Laws Explain Properties of Gas Molecules02:34

Kinetic Molecular Theory and Gas Laws Explain Properties of Gas Molecules

The test of the kinetic molecular theory (KMT) and its postulates is its ability to explain and describe the behavior of a gas. The various gas laws (Boyle’s, Charles’s, Gay-Lussac’s, Avogadro’s, and Dalton’s laws) can be derived from the assumptions of the KMT, which have led chemists to believe that the assumptions of the theory accurately represent the properties of gas molecules.
Basic Postulates of Kinetic Molecular Theory: Particle Size, Energy, and Collision02:43

Basic Postulates of Kinetic Molecular Theory: Particle Size, Energy, and Collision

The ideal-gas equation, which is empirical, describes the behavior of gases by establishing relationships between their macroscopic properties. For example, Charles’ law states that volume and temperature are directly related. Gases, therefore, expand when heated at constant pressure. Although gas laws explain how the macroscopic properties change relative to one another, it does not explain the rationale behind it.
Physical Principles Governing Gas Exchange01:16

Physical Principles Governing Gas Exchange

Gas behavior plays a vital role in understanding bodily processes such as external and internal respiration. External respiration involves the diffusion of oxygen into the blood and carbon dioxide out of it in the lungs. In contrast, internal respiration happens in body tissues, where these gases move in opposite directions.
Gas Laws Governing Respiration
The behavior of gases is guided by Dalton's Law of partial pressures and Henry's Law.
Dalton's Law asserts that the total pressure exerted by...
Gas Solubility01:31

Gas Solubility

Gas solubility in liquids forms liquid-gas solutions, such as soft drinks, where carbon dioxide is dissolved in water, and the ocean, where the solubility of oxygen and carbon dioxide supports marine life. The ability of oceans to dissolve gases impacts weather conditions in the troposphere.However, gas-liquid interactions vary. For instance, hydrogen chloride gas is highly soluble in water, while oxygen's solubility is much lower. Because these solutions are non-ideal, Raoult’s law, which...
Real Gases: Effects of Intermolecular Forces and Molecular Volume Deriving Van der Waals Equation04:01

Real Gases: Effects of Intermolecular Forces and Molecular Volume Deriving Van der Waals Equation

Thus far, the ideal gas law, PV = nRT, has been applied to a variety of different types of problems, ranging from reaction stoichiometry and empirical and molecular formula problems to determining the density and molar mass of a gas. However, the behavior of a gas is often non-ideal, meaning that the observed relationships between its pressure, volume, and temperature are not accurately described by the gas laws.
Gas Exchange and Transport01:20

Gas Exchange and Transport

Gas exchange, the intake of molecular oxygen (O2) from the environment and the outflow of carbon dioxide (CO2) into the environment, is necessary for cellular function. Gas exchange during respiration occurs largely via the movement of gas molecules along pressure gradients. Gas travels from areas of higher partial pressure to areas of lower partial pressure. In mammals, gas exchange occurs in the alveoli of the lungs, which are adjacent to capillaries and share a membrane with them.

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関連する実験動画

Updated: Jul 12, 2026

Cryogenic Liquid Jets for High Repetition Rate Discovery Science
08:34

Cryogenic Liquid Jets for High Repetition Rate Discovery Science

Published on: May 9, 2020

恒星形成に関連するガスジェット.

W J Welch, S N Vogel, R L Plambeck

    Science (New York, N.Y.)
    |June 21, 1985
    PubMed
    まとめ

    若い恒星の天体は,強力で集中したジェットと風を発射し,周囲のガスに影響を与え,化学的変化を引き起こします. この流出段階は恒星に共通しており,蓄積の終わりを示している可能性があります.

    科学分野:

    • 天体物理学 天体物理学
    • 恒星の進化について
    • アストロケミストリー アストロケミストリー

    背景:

    • 若い恒星物体 (YSO) は,エネルギーに満ちたコリマートアウトフロー (ジェット/風) を生み出します.
    • これらの流出は,周囲の恒星間ガスと塵と相互作用する.
    • 観測シグネチャーには,分子放射 (例えば,一酸化炭素) とマザーが含まれます.

    研究 の 目的:

    • 若い恒星物体の周辺で起こる物理的,化学的プロセスを調査する.
    • 恒星の進化と恒星間介質におけるアウトフローの役割を理解する.
    • ショックフロントに関連した化学的多量変化を分析する.

    主な方法:

    • 分子線観測 (例えば,一酸化炭素) を利用した観測天文学.
    • ウォーターマザー放射の検出.
    • ヘルビック・ハロ・オブジェクトの識別と分析.

    主要な成果:

    • YSO.O.の近くで,渦巻くスイープアップガスを観測した.
    • 検出された水マザー放出と Herbig-Haro オブジェクトは,アウトフローに参加しています.
    • 衝撃現象に関連した重要な化学物質の豊富さの変動が記録されています.

    さらに関連する動画

    Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer
    07:24

    Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer

    Published on: February 19, 2018

    関連する実験動画

    Last Updated: Jul 12, 2026

    Cryogenic Liquid Jets for High Repetition Rate Discovery Science
    08:34

    Cryogenic Liquid Jets for High Repetition Rate Discovery Science

    Published on: May 9, 2020

    Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer
    07:24

    Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer

    Published on: February 19, 2018

    結論:

    • 恒星の流出は,YSOの光度範囲にわたる一般的な現象です.
    • これらの流出は,周囲の恒星間媒体の化学構造に大きく影響する.
    • 流出段階は,おそらく,恒星の蓄積の遅い段階の重要な段階を表しています.