Jove
Visualize
お問い合わせ
JoVE
x logofacebook logolinkedin logoyoutube logo
JoVEについて
概要リーダーシップブログJoVEヘルプセンター
著者向け
出版プロセス編集委員会範囲と方針査読よくある質問投稿
図書館員向け
推薦の声購読アクセスリソース図書館諮問委員会よくある質問
研究
JoVE JournalMethods CollectionsJoVE Encyclopedia of Experimentsアーカイブ
教育
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab Manual教員リソースセンター教員サイト
利用規約
プライバシーポリシー
ポリシー

関連する概念動画

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...
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.
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...
Measuring Acceleration Due to Gravity01:12

Measuring Acceleration Due to Gravity

Consider a coffee mug hanging on a hook in a pantry. If the mug gets knocked, it oscillates back and forth like a pendulum until the oscillations die out.
A simple pendulum can be described as a point mass and a string. Meanwhile, a physical pendulum is any object whose oscillations are similar to a simple pendulum, but cannot be modeled as a point mass on a string because its mass is distributed over a larger area. The behavior of a physical pendulum can be modeled using the principles of...
Acceleration due to Gravity on Other Planets01:24

Acceleration due to Gravity on Other Planets

The gravitational acceleration of an object near the Earth's surface is called the acceleration due to gravity. It can be measured by conducting simple experiments on Earth. However, such an experiment is impossible to conduct on the surface of other planets.
Astronomical observations are thus used to measure the acceleration due to gravity on other planets. This can be determined by observing the effect of a planet's gravity on objects close to it. The crucial factor that helps in this...
Variation in Acceleration due to Gravity near the Earth's Surface01:20

Variation in Acceleration due to Gravity near the Earth's Surface

An object's apparent weight is its weight measured by a spring balance at its location. It is different from its true weight, the force with which the Earth pulls it, because of the Earth's rotation. Mathematically, an object's apparent weight equals its true weight minus the centripetal force that keeps it in a circular motion along with the Earth's surface every 24 hours.
The difference between the true and apparent weights is proportional to the square of the Earth's angular speed. Since the...

こちらも読む

関連記事

共著者、ジャーナル、引用グラフによってこの研究に関連する記事。

並び替え
Same author

Poststroke subgranular and rostral subventricular zone proliferation in a mouse model of neonatal stroke.

Journal of neuroscience research·2009
Same author

Neurogenesis and neuronal commitment following ischemia in a new mouse model for neonatal stroke.

Brain research·2008
Same author

The language problem.

Science (New York, N.Y.)·1981
Same author

Dynamical astronomy.

Science (New York, N.Y.)·1979
Same author

Pluto's Neighbor.

Science (New York, N.Y.)·1978
Same author

Archeoastronomy.

Science (New York, N.Y.)·1978

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

月の潮加速は,レーザー射程測定から決定される.

O Calame, J D Mulholland

    Science (New York, N.Y.)
    |March 3, 1978
    PubMed
    まとめ

    科学者たちは,月の世俗的な加速を測定するために,1969年から1976年の月のレーザーレンジングデータを分析しました. この研究では,潮摩擦効果と一致する,世紀の平方あたり -24.6 弧秒の加速が決定されました.

    科学分野:

    • * 天文学と天体物理学
    • * 地質物理学と地測量学
    • * 天体力学とは

    背景:

    • *月の軌道運動は,地球の潮摩擦の影響を受け,世俗的な加速を引き起こします.
    • * 過去の研究では,この加速を推定しましたが,正確な測定は,地球・月系システムの動態を理解するために不可欠です.

    研究 の 目的:

    • *月のレーザーレンジングデータを用いて,月の平均経度における異常な世俗的加速を決定する.
    • * この加速に対する潮摩擦の影響を評価する.
    • * 重力定数の変動から潮効果を分離する可能性を調査する.

    主な方法:

    • * 1969年から1976年までの月のレーザーレンジング (LLR) 測定の分析.
    • * 加速を導き出すために,様々な観測モデルとデータセットを適用する.
    • * 原子時間スケールと従来の推定値との比較による測定値の比較.

    主要な成果:

    • * 決定された世俗的加速度は, -24.6 ± 1.6 弧秒/世紀平方です.
    • *この値は,既定の従来の値と,他の方法による最近の発見とよく一致しています.
    • *月の平均距離の変化率を測定する試みは,観測期間が不十分であったため,有意な結果が得られませんでした.

    さらに関連する動画

    Measuring and Mapping Patterns of Soil Erosion and Deposition Related to Soil Carbonate Concentrations Under Agricultural Management
    08:09

    Measuring and Mapping Patterns of Soil Erosion and Deposition Related to Soil Carbonate Concentrations Under Agricultural Management

    Published on: September 12, 2017

    Measurements of Waves in a Wind-wave Tank Under Steady and Time-varying Wind Forcing
    08:54

    Measurements of Waves in a Wind-wave Tank Under Steady and Time-varying Wind Forcing

    Published on: February 13, 2018

    関連する実験動画

    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

    Measuring and Mapping Patterns of Soil Erosion and Deposition Related to Soil Carbonate Concentrations Under Agricultural Management
    08:09

    Measuring and Mapping Patterns of Soil Erosion and Deposition Related to Soil Carbonate Concentrations Under Agricultural Management

    Published on: September 12, 2017

    Measurements of Waves in a Wind-wave Tank Under Steady and Time-varying Wind Forcing
    08:54

    Measurements of Waves in a Wind-wave Tank Under Steady and Time-varying Wind Forcing

    Published on: February 13, 2018

    結論:

    • *この研究は,主に潮摩擦に起因する月の異常な世俗的な加速を確認しています.
    • * LLRデータは,月の軌道パラメータの推定を精製するための堅実な方法を提供します.
    • * 重力定数などの基本定数における潜在的な変動を調査するには,より長い観測基準線が必要である.