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関連する概念動画

Simple Harmonic Motion and Uniform Circular Motion01:42

Simple Harmonic Motion and Uniform Circular Motion

While simple harmonic motion and uniform circular motion may be two separate concepts, they correlate and interlink with each other. Simple harmonic motion is an oscillatory motion in a system where the net force can be described by Hooke's law, while uniform circular motion is the motion of an object in a circular path at constant speed.
There is an easy way to produce simple harmonic motion by using uniform circular motion. For instance, consider a ball attached to a uniformly rotating...
Gravitation01:16

Gravitation

In the years before Newton, a general belief prevailed that different laws governed objects in the sky than objects on Earth. When Kepler wrote down the three laws of planetary motion, explaining in detail the geometrical properties of the planetary orbits around the Sun, there was no immediate idea to discern their connection with more fundamental laws. It was Isaac Newton who, in 1665–66, figured out the connection between planetary motion, the motion of the moon around the Earth, and the...
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...
Energy of a Satellite in a Circular Orbit01:11

Energy of a Satellite in a Circular Orbit

Thousands of artificial satellites orbit the Earth every day at various distances from the Earth. Satellites that orbit the Earth below an altitude of 1,600 km are considered to be orbiting in low-Earth orbit (LEO). Research satellites and Earth observation satellites are usually placed in LEO, and mostly orbit the Earth in elliptical orbits. Navigation satellites are placed in medium-Earth orbit (MEO), ranging from 2,000 km to 36,000 km from the surface of the Earth. Meanwhile, communication...
Tidal Forces01:06

Tidal Forces

The origin of Earth's ocean tides has been a subject of continuous investigation for over 2000 years. However, the work of Newton is considered to be the beginning of the proper understanding of the phenomenon. Ocean tides are the result of gravitational tidal forces. These same tidal forces are present in any astronomical body; they are responsible for the internal heat that creates the volcanic activity on Io, one of Jupiter's moons, and the breakup of stars that get too close to black holes.
Cause and Effect01:53

Cause and Effect

While variables are sometimes correlated because one does cause the other, it could also be that some other factor, a confounding variable, is actually causing the systematic movement in our variables of interest. For instance, as sales in ice cream increase, so does the overall rate of crime. Is it possible that indulging in your favorite flavor of ice cream could send you on a crime spree? Or, after committing crime do you think you might decide to treat yourself to a cone?

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関連する実験動画

Updated: Jul 12, 2026

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
06:14

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

月面に人為的な衝突による地震データ.

G Latham, M Ewing, J Dorman

    Science (New York, N.Y.)
    |November 6, 1970
    PubMed
    まとめ

    アポロ12号の地震データは,月の表面を明らかにした.

    科学分野:

    • 地震学 地震学とは
    • 月科学 月科学 月科学
    • 地質物理学 地質物理学とは地質物理学です.

    背景:

    • アポロ12号の宇宙飛行士たちは,月面に地震観測ステーションを設置した.
    • 地震データは,月の衝撃や自然発生の地震を記録しています.

    研究 の 目的:

    • 月面衝突による地震の反響を分析するために.
    • アポロ12号の着陸地点付近の月面のメアの地震特性を理解するために,アポロ12号の着陸地点付近の月面メアの地震特性を理解するために,アポロ12号の着陸地点付近の月面メアの地震特性を理解するために,アポロ12号の着陸地点付近の月面メアの地震特性を理解するために,アポロ12号の着陸地点付近の月面メアの地震特性を理解するために,アポロ12号の着陸地点付近の月面メアの地震特性を理解するために.
    • 月の浅い地下構造を調査するために.

    主な方法:

    • 月面衝突による地震波の拡散の分析.
    • 地震信号の解釈は,反響や自然現象を含む.
    • 地震速度のモデリングと波の吸収.

    主要な成果:

    • 月面衝突で異常な長さの反響が記録された.
    • 月の海の地震速度は深さとともに上昇し,20kmで5~6km/sまで上昇する.
    • 月面の海に観測された非常に低い地震波吸収.

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    Last Updated: Jul 12, 2026

    Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
    06:14

    Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

    Published on: July 30, 2020

    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

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  • 外部20kmでは主要な地殻マントルの境界線が検出されなかった.
  • 表面波の散乱は,月面波の異質性を示唆している.
  • 結論:

    • 月面地震の反響は,表面波の分散と散乱によって引き起こされる可能性が高い.
    • 月の外側の20kmは異質で,明確な地殻-マントルの境界がない.
    • 地震データは,月の内部構造と組成についての洞察を提供します.