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相关概念视频

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.
Nuclear Stability03:18

Nuclear Stability

Protons and neutrons, collectively called nucleons, are packed together tightly in a nucleus. With a radius of about 10−15 meters, a nucleus is quite small compared to the radius of the entire atom, which is about 10−10 meters. Nuclei are extremely dense compared to bulk matter, averaging 1.8 × 1014 grams per cubic centimeter. If the earth’s density were equal to the average nuclear density, the earth’s radius would be only about 200 meters.
To hold positively charged protons together in the...
Radioactive Decay and Radiometric Dating02:48

Radioactive Decay and Radiometric Dating

Radioactivity is a spontaneous disintegration of an unstable nuclide and is a random process, as all the nuclei in the sample do not decay simultaneously. The number of disintegrations per unit time is called the activity (A), which is directly proportional to the number of nuclei in the sample. The decay constant (λ) is an average probability of decay per nucleus in unit time.
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 Nuclei: Larmor Precession Frequency01:11

Atomic Nuclei: Larmor Precession Frequency

The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession, and the angular frequency...
Escape Velocities of Gases01:19

Escape Velocities of Gases

To escape the Earth's gravity, an object near the top of the atmosphere at an altitude of 100 km must travel away from Earth at 11.1 km/s. This speed is called the escape velocity. The temperature at which gas molecules attain the rms speed, which is equal to the escape velocity, can be estimated by using the equation for the average kinetic energy of the gas molecules. According to the kinetic theory of gas, the average kinetic energy of the gas molecules is proportional to its temperature.

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相关实验视频

Updated: Jun 24, 2026

Experimental Protocol to Investigate Particle Aerosolization of a Product Under Abrasion and Under Environmental Weathering
07:47

Experimental Protocol to Investigate Particle Aerosolization of a Product Under Abrasion and Under Environmental Weathering

Published on: September 16, 2016

月球岩石的气体保留和宇宙射线暴露年龄 15555

F A Podosek, J C Huneke, G J Wasserburg

    Science (New York, N.Y.)
    |January 28, 1972
    PubMed
    概括

    在Mare Imbrium中的月球玄武岩15555表明,最后一次岩流发生在33亿年前. 进一步的分析表明,它的年龄略微较小,为3220亿年,而宇宙射线暴露的年龄为9000万年.

    科学领域:

    • 月球地质学 月球地质学
    • 地质时间学 (Geochronology)
    • 太空化学 太空化学

    背景情况:

    • 海 (Mare Imbrium) 是一个大型的月球海,以其玄武岩平原而闻名.
    • 哈德利里尔 (Hadley Rille) 是Mare Imbrium内的一个突出的曲的里尔,提供了对月球火山历史的见解.
    • 月球玄武岩15555为放射测年提供了一个样本,以确定火山事件的时间线.

    研究的目的:

    • 为了确定Mare Imbrium的Hadley Rille地区最后一次岩流的年龄.
    • 为了确定月球玄武岩的结晶年龄15555.5.
    • 为了计算月球样本的宇宙射线暴露年龄.

    主要方法:

    • 阿贡-40/阿贡-39 (40Ar/39Ar) 地质时间学实验是在月球玄武岩15555.5的石质分离物和整个岩石样本上进行的.
    • 使用放射测年法测量同位素比率.
    • 对宇宙射线的暴露年龄是通过分析斯帕洛基因-38与的比率来确定的.

    主要成果:

    • 在40Ar/39Ar的实验中,我们得出了最后一次岩流的年龄为3.31±0.03亿年.
    • 对整个岩石样本的分析表明,放射性-40的损失很大,导致低平原年龄为3.22 ± 0.03亿年.

    更多相关视频

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
    07:54

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas

    Published on: April 3, 2018

    Separation of Uranium and Thorium for 230Th-U Dating of Submarine Hydrothermal Sulfides
    08:43

    Separation of Uranium and Thorium for 230Th-U Dating of Submarine Hydrothermal Sulfides

    Published on: May 20, 2019

    相关实验视频

    Last Updated: Jun 24, 2026

    Experimental Protocol to Investigate Particle Aerosolization of a Product Under Abrasion and Under Environmental Weathering
    07:47

    Experimental Protocol to Investigate Particle Aerosolization of a Product Under Abrasion and Under Environmental Weathering

    Published on: September 16, 2016

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
    07:54

    Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas

    Published on: April 3, 2018

    Separation of Uranium and Thorium for 230Th-U Dating of Submarine Hydrothermal Sulfides
    08:43

    Separation of Uranium and Thorium for 230Th-U Dating of Submarine Hydrothermal Sulfides

    Published on: May 20, 2019

  • 据计算,宇宙射线暴露的年龄为90±1000万年.
  • 结论:

    • 月球玄武岩的年代是15555年,为哈德利·里尔地区的火山活动提供了精确的年龄.
    • 石质和整个岩石样本之间的年龄差异凸显了样本准备和月球基岩中潜在的气扩散的重要性.
    • 确定的宇宙射线暴露年龄为我们提供了关于样品在月球表面暴露的时间的见解.