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Impulse01:13

Impulse

16.0K
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...
16.0K
Elastic Collisions: Case Study01:15

Elastic Collisions: Case Study

17.1K
Elastic collision of a system demands conservation of both momentum and kinetic energy. To solve problems involving one-dimensional elastic collisions between two objects, the equations for conservation of momentum and conservation of internal kinetic energy can be used. For the two objects, the sum of momentum before the collision equals the total momentum after the collision. An elastic collision conserves internal kinetic energy, and so the sum of kinetic energies before the collision equals...
17.1K
Acceleration due to Gravity on Other Planets01:24

Acceleration due to Gravity on Other Planets

3.4K
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...
3.4K
Escape Velocity01:26

Escape Velocity

5.6K
The escape velocity of an object is defined as the minimum initial velocity that it requires to escape the surface of another object to which it is gravitationally bound and never to return. For example, what would be the minimum velocity at which a satellite should be launched from the Earth's surface such that it just escapes the Earth's gravitational field?
To calculate the escape velocity, it is assumed that no energy is lost to any frictional forces. In practice, a satellite...
5.6K
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

2.2K
No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
2.2K
Impact: Problem Solving01:26

Impact: Problem Solving

619
In an experiment conducted during a Mars mission, a rover propels a projectile with an initial velocity, and the projectile rebounds after colliding with the Martian surface. To ascertain the maximum height attained by the projectile after this collision, the known restitution coefficient and acceleration due to gravity are employed.
By designating the launch point as the origin and utilizing kinematic equations, the vertical component of the projectile's velocity at the point of impact is...
619

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関連する実験動画

Updated: May 5, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
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Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Published on: June 5, 2014

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ヒット・アンド・ラン惑星衝突.

Erik Asphaug1, Craig B Agnor, Quentin Williams

  • 1Earth Sciences Department, Institute for Geophysics and Planetary Physics, 1156 High St, University of California, Santa Cruz, California 95064, USA.

Nature
|January 13, 2006
PubMed
まとめ
この要約は機械生成です。

陸上の惑星形成の際に発生する巨大衝突は,地球に惑星が形成されるのを引き起こす可能性があります.

さらに関連する動画

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

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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

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関連する実験動画

Last Updated: May 5, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
09:44

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Published on: June 5, 2014

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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

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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

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科学分野:

  • 惑星科学は惑星科学である.
  • 天体物理学 天体物理学
  • 地質学 地質学 地質学

背景:

  • 地球上の惑星の形成は,巨大な衝突で終わったと考えられています.
  • 何百もの惑星の胚が衝突し,惑星,月,小惑星が形成されました.

研究 の 目的:

  • 単なる合併以上の惑星の衝突の結果を調査する.
  • 惑星形成における新しい衝突ダイナミクスの影響を理解する.

主な方法:

  • 惑星の胚衝突のシミュレーション.
  • 変形と断片化を含む衝突結果の分析.

主要な成果:

  • 衝突する惑星は必ずしも合体することはなく,より小さな惑星は逃れることができる.
  • 衝突の結果には,変形,スピンアップ,減圧,そして断片化が含まれます.
  • ヒット・アンド・ランの衝突は,様々な残骸を生成します.

結論:

  • ヒット・アンド・ランの衝突は,惑星形成の重要な要因である.
  • これらの衝突残骸は小惑星の形成と隕石の起源に関連しています.