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関連する概念動画

Impulse01:13

Impulse

According to Newton’s second law of motion, the rate of change of the momentum of an object is the net external force acting on it. The total change in momentum between two timepoints thus depends on both the external force acting on it and the time over which it acts. Describing this mathematically, the total change of an object’s motion is proportional to the force vector and the time over which it is applied. This product is called impulse.
Additionally, it can be shown that the total...
Conservation of Angular Momentum: Application01:18

Conservation of Angular Momentum: Application

A system's total angular momentum remains constant if the net external torque acting on the system is zero. Examples of such systems include a freely spinning bicycle tire that slows over time due to torque arising from friction, or the slowing of Earth's rotation over millions of years due to frictional forces exerted on tidal deformations. However in the absence of a net external torque, the angular momentum remains conserved. The conservation of angular momentum principle requires a change...
Gravity between Spherical Bodies01:27

Gravity between Spherical Bodies

Newton's law of gravitation describes the gravitational force between any two point masses. However, for extended spherical objects like the Earth, the Moon, and other planets, the law holds with an assumption that masses of spherical objects are concentrated at their respective centers.
This assumption can be proved easily by showing that the expression for gravitational potential energy between a hollow sphere of mass (M) and a point mass (m) is the same as it would be for a pair of extended...
Detection of Black Holes01:10

Detection of Black Holes

Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

An object absorbing an electromagnetic wave would experience a force in the direction of propagation of the wave. This force occurs because electromagnetic waves contain and transport momentum. The force accounts for the wave's radiation pressure exerted on the object. Maxwell's prediction was confirmed in 1903 by Nichols and Hull by precisely measuring radiation pressures with a torsion balance. The measuring instrument had mirrors suspended from a fiber kept inside a glass container. Nichols...
Coriolis Force01:23

Coriolis Force

An accelerating particle experiences a force equal to the mass multiplied by the acceleration in an inertial frame of reference. Consider a particle in a non-inertial frame of reference, such as a sliding ball on a rotating table. The acceleration of the ball in this rotating reference frame is different than in the intertial frame, which modifies its equation of motion. The fictitious forces acting additionally on a rotating frame of reference alter Newton's Second Law expression. Centripetal...

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関連する実験動画

Updated: Jun 24, 2026

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

月面で観測された隕石嵐.

F K Duennebier, Y Nakamura, G V Latham

    Science (New York, N.Y.)
    |June 4, 1976
    PubMed
    まとめ

    月面の地震計は,より強い隕石の衝突を検知し,月が密集した隕石雲に遭遇したことを示した. 1975年6月のイベントには,幅約0.1天文単位,質量が10^14グラムまでの雲が含まれる.

    科学分野:

    • 月面地震学 月面地震学
    • 隕石の衝撃に関する研究
    • 太陽系動態 太陽系動態

    背景:

    • 月面ミッションからの地震データは,地表の活動に関する洞察を提供します.
    • 隕石の衝突を理解することは,惑星科学と宇宙探査にとって極めて重要です.

    研究 の 目的:

    • 月面に隕石が衝突した証拠を探すために地震データを分析する.
    • 観測された隕石との遭遇の性質と規模を特徴づけるため.

    主な方法:

    • 月面の地震計で記録された地震データの分析.
    • 地震信号の解釈により,衝撃事件とその特徴を特定する.

    主要な成果:

    • 隕石の衝突活動が増加したいくつかの短い期間を検知した.
    • 1975年6月に有意な隕石雲との遭遇を特定した.
    • 1975年6月の雲の特徴:直径0.1AU,質量は10^1310^14グラムでした.

    結論:

    • 月は,密集した隕石雲との遭遇を経験しています.
    • 地震モニタリングは,月の衝突イベントの検出と研究に有効です.

    さらに関連する動画

    Simultaneous Measurement of Turbulence and Particle Kinematics Using Flow Imaging Techniques
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    Simultaneous Measurement of Turbulence and Particle Kinematics Using Flow Imaging Techniques

    Published on: March 12, 2019

    Scattering And Absorption of Light in Planetary Regoliths
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    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    関連する実験動画

    Last Updated: Jun 24, 2026

    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

    Simultaneous Measurement of Turbulence and Particle Kinematics Using Flow Imaging Techniques
    10:53

    Simultaneous Measurement of Turbulence and Particle Kinematics Using Flow Imaging Techniques

    Published on: March 12, 2019

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

  • これらの発見は,太陽系の小さな天体の分布と行動を理解するのに役立ちます.