Jove
Visualize
联系我们
JoVE
x logofacebook logolinkedin logoyoutube logo
关于 JoVE
概览领导团队博客JoVE 帮助中心
作者
出版流程编辑委员会范围与政策同行评审常见问题投稿
图书馆员
用户评价订阅访问资源图书馆顾问委员会常见问题
研究
JoVE JournalMethods CollectionsJoVE Encyclopedia of Experiments存档
教育
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab Manual教师资源中心教师网站
使用条款与条件
隐私政策
政策

相关概念视频

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...
Elastic Collisions: Introduction01:00

Elastic Collisions: Introduction

An elastic collision is one that conserves both internal kinetic energy and momentum. Internal kinetic energy is the sum of the kinetic energies of the objects in a system. Truly elastic collisions can only be achieved with subatomic particles, such as electrons striking nuclei. Macroscopic collisions can be very nearly, but not quite, elastic, as some kinetic energy is always converted into other forms of energy such as heat transfer due to friction and sound. An example of a nearly...
Elastic Collisions: Case Study01:15

Elastic Collisions: Case Study

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...
Impact01:30

Impact

Impact occurs when two bodies collide, leading to the application of impulsive forces between them. Analyzing impact mechanics involves considering two colliding particles moving along a line known as the line of impact, which passes through their centers and is perpendicular to the contact plane.
When particles with different initial velocities collide, they induce deformation by applying equal and opposite impulses. At the point of maximum deformation, the particles move together with...
Types of Impact01:30

Types of Impact

Impacts can be classified in various forms, primarily under two subgroups: central impact and oblique impact. A central impact occurs when two objects collide head-on, possessing opposite velocities aligned along the line of impact. Conversely, an oblique impact occurs when two objects collide at an angle, resulting in a modification of both direction and velocity.
The coefficient of restitution is a metric for understanding the dynamics of impacts. It quantifies the ratio of relative velocity...
Impact: Problem Solving01:26

Impact: Problem Solving

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...

您也可能阅读

相关文章

通过共同作者、期刊和引用图与本文相关的文章。

排序
Same author

Amplified crevicular leukocyte activity in aggressive periodontal disease.

Journal of dental research·2002
Same author

Some effects of non-surgical therapy on gingival inflammatory cell subsets in patients with early-onset periodontitis associated with Actinobacillus actinomycetemcomitans.

Journal of periodontology·2002
Same author

PMN responses following use of 2 biodegradable GTR membranes.

Journal of clinical periodontology·2001
Same author

Bacterial susceptibility to amoxicillin and potassium clavulanate in advanced periodontitis patients not responding to mechanical therapy.

Journal of clinical periodontology·2000
Same author

Some effects of non-surgical therapy on gingival inflammatory cell subsets in patients with adult and early-onset periodontitis.

Journal of periodontology·2000
Same author

Actinobacillus actinomycetemcomitans in destructive periodontal disease. Three-year follow-up results.

Journal of periodontology·2000

相关实验视频

Updated: Jul 6, 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

洪都拉斯:起源于尘埃颗粒之间的冲击.

D E Lange, J W Larimer

    Science (New York, N.Y.)
    |November 30, 1973
    PubMed
    概括

    石分析显示,早期太阳星云中的高速撞击可能形成了体. 这一发现支持了早期太阳系颗粒动力学和圆柱体形成的理论.

    科学领域:

    • * 星球科学 星球科学
    • * 宇宙化学 * 宇宙化学
    • * 天体物理学 * 天体物理学

    背景情况:

    • * 圆柱体是石的基本组成部分,为早期太阳系提供了洞察力.
    • * 圆柱体的形成机制,特别是它们所需的高温和速度,仍然是科学辩论的主题.
    • *以前的理论模型提出了高速颗粒碰撞作为可能的体形成途径.

    研究的目的:

    • * 为了研究圆柱体形成期间的物理条件和冲击速度.
    • * 提供观察证据支持冲击驱动的冠状管形成机制.
    • * 测试关于原行星星云中的粒速的理论预测.

    主要方法:

    • * 显微镜检查一个带条条的柱体,其中含有来自威石的磁性球体.
    • * 分析孔道内部的断裂模式和部分融化.
    • *根据观察到的物理效应计算撞击速度.

    主要成果:

    • * 纳瓦维石的一条带条的圆柱体包含一个嵌入的磁铁球体.
    • * 碎裂和部分化的证据表明发生了高能碰撞事件.
    • * 估计撞击速度范围从10^5到10^6厘米/秒.

    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

    Visually Based Characterization of the Incipient Particle Motion in Regular Substrates: From Laminar to Turbulent Conditions
    11:51

    Visually Based Characterization of the Incipient Particle Motion in Regular Substrates: From Laminar to Turbulent Conditions

    Published on: February 22, 2018

    相关实验视频

    Last Updated: Jul 6, 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

    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

    Visually Based Characterization of the Incipient Particle Motion in Regular Substrates: From Laminar to Turbulent Conditions
    11:51

    Visually Based Characterization of the Incipient Particle Motion in Regular Substrates: From Laminar to Turbulent Conditions

    Published on: February 22, 2018

    结论:

    • * 纳瓦维石体中观察到的特征支持了高速度撞击导致体形成的假设.
    • * 这一发现证实了卡梅伦和惠普尔关于早期太阳星云中的粒速的理论预测.
    • *撞击事件被证实是产生行星体的关键组成部分chondrules的可行机制.