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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...
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Related Experiment Video

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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Hit-and-run planetary collisions.

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
Summary
This summary is machine-generated.

Giant impacts during terrestrial planet formation can result in

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Area of Science:

  • Planetary Science
  • Astrophysics
  • Geology

Background:

  • Terrestrial planet formation is thought to have concluded with giant impacts.
  • Hundreds of planetary embryos collided, forming planets, the Moon, and asteroids.

Purpose of the Study:

  • To investigate the outcomes of planetary collisions beyond simple merging.
  • To understand the implications of novel collision dynamics for planet formation.

Main Methods:

  • Simulations of planetary embryo collisions.
  • Analysis of collision outcomes, including deformation and fragmentation.

Main Results:

  • Colliding planets do not always merge; smaller planets can escape.
  • Collision outcomes include deformation, spin-up, depressurization, and fragmentation.
  • Hit-and-run collisions produce diverse remnants.

Conclusions:

  • Hit-and-run collisions are a significant factor in planet formation.
  • These collision remnants are relevant to asteroid formation and meteorite origins.