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関連する概念動画

Atomic Structure01:33

Atomic Structure

All matter is composed of atoms, the smallest individual units of elements. Each atom is made up of three subatomic particles: protons, neutrons, and electrons. Together, these three particles account for the mass and the charge of an atom.The History of Atomic TheoryThe first person to propose that everything on Earth is made up of tiny particles was the Greek philosopher Democritus, around 450 B.C. He used the term atomos, Greek for “indivisible,” from which the modern term “atom” is derived.
Conditions on Early Earth02:06

Conditions on Early Earth

Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
Subatomic Particles03:37

Subatomic Particles

Dalton was only partially correct about the particles that make up matter. All matter is composed of atoms, and atoms are composed of three smaller subatomic particles: protons, neutrons, and electrons. These three particles account for the mass and the charge of an atom.
Constant Volume Calorimetry02:41

Constant Volume Calorimetry

Calorimeters are useful to determine the heat released or absorbed by a chemical reaction. Coffee cup calorimeters are designed to operate at constant (atmospheric) pressure and are convenient to measure heat flow (or enthalpy change) accompanying processes that occur in solution at constant pressure. A different type of calorimeter that operates at constant volume, colloquially known as a bomb calorimeter, is used to measure the energy produced by reactions that yield large amounts of heat and...
Conditions on Early Earth02:06

Conditions on Early Earth

Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
Atomic Structure01:17

Atomic Structure

The Greek philosopher Democritus proposed that everything on Earth is made up of tiny particles called atomos, Greek for "indivisible," from which the modern term "atom" is derived. In the 19th century, John Dalton proposed the atomic theory that is still largely correct today. He put forth five postulates to explain how atoms made up the world around us. (1) All matter is composed of infinitely small particles or atoms. (2) All atoms of a given element are identical to one another and (3) are...

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関連する実験動画

Updated: Jul 9, 2026

A Method for Studying the Temperature Dependence of Dynamic Fracture and Fragmentation
09:12

A Method for Studying the Temperature Dependence of Dynamic Fracture and Fragmentation

Published on: June 28, 2015

天体物理学:天文学者は最初の炭素爆弾を発見した.

R Irion

    Science (New York, N.Y.)
    |September 6, 2007
    PubMed
    まとめ
    この要約は機械生成です。

    超密度の高い恒星の炭素燃料による熱核爆発.

    さらに関連する動画

    Preparation and Reactivity of Gasless Nanostructured Energetic Materials
    09:50

    Preparation and Reactivity of Gasless Nanostructured Energetic Materials

    Published on: April 2, 2015

    Blast Quantification Using Hopkinson Pressure Bars
    09:41

    Blast Quantification Using Hopkinson Pressure Bars

    Published on: July 5, 2016

    関連する実験動画

    Last Updated: Jul 9, 2026

    A Method for Studying the Temperature Dependence of Dynamic Fracture and Fragmentation
    09:12

    A Method for Studying the Temperature Dependence of Dynamic Fracture and Fragmentation

    Published on: June 28, 2015

    Preparation and Reactivity of Gasless Nanostructured Energetic Materials
    09:50

    Preparation and Reactivity of Gasless Nanostructured Energetic Materials

    Published on: April 2, 2015

    Blast Quantification Using Hopkinson Pressure Bars
    09:41

    Blast Quantification Using Hopkinson Pressure Bars

    Published on: July 5, 2016

    科学分野:

    • 天体物理学 天体物理学
    • 恒星の進化について

    背景:

    • 恒星の熱核爆発は,通常,水素またはヘリウムを含む.
    • 星の燃焼を理解することは,天体物理学の鍵です.

    研究 の 目的:

    • 炭素のみの熱核恒星爆発の潜在的な発見を報告するために.
    • 星のモデルへの影響を調査する.

    主な方法:

    • 宇宙爆発の観測. 宇宙爆発の観測.
    • 爆発の元素組成の分析.

    主要な成果:

    • 超密度の高い星の表面で3時間の熱核爆発.
    • この爆発は,炭素のみによって引き起こされたようです.

    結論:

    • このイベントは,炭素のみによって駆動された最初の観測された宇宙爆発かもしれません.
    • 確認は,恒星の燃焼と炭素爆発のモデルの修正につながる可能性があります.