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関連する概念動画

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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関連する実験動画

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

火星の衝突で加工された岩石

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
まとめ

火星での衝突過程は岩石を断片化し,大気圏への入り口を生き残った小さな弾丸がある. これらの衝突は小さなクレーターを作り,火星の表面の進化と土壌の組成に影響を与えます.

科学分野:

  • 惑星科学は惑星科学である.
  • 地質学 地質学 地質学
  • インパクトクラテリング (インパクトクラテリング)

背景:

  • パスファインダーミッションは,火星着陸地点で様々な岩石の形状を観測した.
  • これらの形態学は,重要な表面改変プロセスを示唆しています.

研究 の 目的:

  • 火星表面の特徴の形成における衝突過程の役割を調査する.
  • 火星の土壌の進化に小規模なインパクターがもたらす潜在的貢献を決定する.

主な方法:

  • パスファインダー着陸地での岩石の断片化パターンの分析.
  • 火星に衝突するセンチメートルサイズの弾丸の大気圏入りシミュレーション.

主要な成果:

  • 衝突による岩石の損傷 (クレーター化,裂け方,断片化) が観察された.
  • シミュレーションにより,センチメートルのサイズの弾丸が火星の大気中を通過して生き残ったことが確認されています.
  • 衝突速度は数キロメートル/秒に達する.

結論:

  • 衝突過程は,火星の岩石破壊の重要な要因である.

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Emission Spectroscopic Boundary Layer Investigation during Ablative Material Testing in Plasmatron
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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

関連する実験動画

Last 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

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

  • 小さな衝突点 (センチメートルの大きさ) は,直径"メートル未満のクレーターを作り出します.
  • これらの小さなクレーターは,火星の表面と土壌の進行中の進化に貢献しています.