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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...
Types of Collisions - II01:19

Types of Collisions - II

When two or more objects collide with each other, they can stick together to form one single composite object (after collision). The total mass of the object after the collision is the sum of the masses of the original objects, and it moves with a velocity dictated by the conservation of momentum. Although the system's total momentum remains constant, the kinetic energy decreases, and thus such a collision is an inelastic collision. Most of the collisions between objects in daily life are...
Rocket Propulsion in Gravitational Field - I01:20

Rocket Propulsion in Gravitational Field - I

Rockets range in size from small fireworks that ordinary people use to the enormous Saturn V that once propelled massive payloads toward the Moon. The propulsion of all rockets, jet engines, deflating balloons, and even squids and octopuses are explained by the same physical principle: Newton's third law of motion. The matter is forcefully ejected from a system, producing an equal and opposite reaction on what remains.
The motion of a rocket in space changes its velocity (and hence its...
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...
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...
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...

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相关实验视频

Updated: Jul 21, 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

火星上碰撞加工的岩石在火星上发生碰撞.

Horz1, Cintala, Rochelle

  • 1NASA Johnson Space Center, Houston, TX 77058, USA. Lockheed Martin, 2400 NASA Road 1, Houston, TX 77058, USA.

Science (New York, N.Y.)
|September 25, 1999
PubMed
概括

火星上的碰撞过程破碎了巨石,小弹子在进入大气中幸存下来. 这些撞击造成了小石坑,影响了火星表面的演变和土壤组成.

科学领域:

  • 行星科学 行星科学
  • 地质地质地质地质地质地
  • 冲击石坑的形成

背景情况:

  • 路径探测器任务在火星着陆地点观察到各种巨石形态.
  • 这些形态学表明了显著的表面修饰过程.

研究的目的:

  • 调查碰撞过程在塑造火星表面特征中的作用.
  • 确定小冲击物对火星土壤演变的潜在贡献.

主要方法:

  • 在Pathfinder着陆地点对岩石碎片化模式的分析.
  • 对于触及火星的厘米大小的弹药进入大气层的模拟.

主要成果:

  • 观察到因碰撞而造成的巨石损伤 (坑道,裂,碎片).
  • 模拟证实了几厘米大小的弹子在火星大气层中幸存下来.
  • 撞击速度达到每秒几公里.

结论:

  • 碰撞过程是火星巨石破坏的一个重要因素.
  • 小撞击物 (厘米大小) 会产生直径小于1米的石坑.
  • 这些小石坑有助于火星表面和土壤的不断演变.

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Scattering And Absorption of Light in Planetary Regoliths

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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

Emission Spectroscopic Boundary Layer Investigation during Ablative Material Testing in Plasmatron
09:41

Emission Spectroscopic Boundary Layer Investigation during Ablative Material Testing in Plasmatron

Published on: June 9, 2016

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019