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関連する概念動画

Torque Free Motion01:15

Torque Free Motion

751
The torque-free motion refers to the movement of a rigid body in space when no external torques are acting upon it. This type of motion can be observed in environments where there are no external forces or frictions, like in outer space. For example, a rotation of Mars in space is a torque-free motion. Mars is an axisymmetric object, meaning it has an axis of symmetry along which it rotates, designated as the z-axis. The rotating frame of reference is defined such that the center of mass of...
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Variation of Atmospheric Pressure01:18

Variation of Atmospheric Pressure

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Change in atmospheric pressure with height is particularly interesting. The decrease in atmospheric pressure with increasing altitude is due to the decreasing gravitational force per unit area as we move away from the surface of the earth.
Assuming the air temperature is constant at a given altitude and that the ideal gas law of thermodynamics describes the atmosphere to a good approximation, one can find the variation of atmospheric pressure with height.
Let p(y) be the atmospheric pressure at...
3.8K
Escape Velocities of Gases01:19

Escape Velocities of Gases

1.3K
To escape the Earth's gravity, an object near the top of the atmosphere at an altitude of 100 km must travel away from Earth at 11.1 km/s. This speed is called the escape velocity. The temperature at which gas molecules attain the rms speed, which is equal to the escape velocity, can be estimated by using the equation for the average kinetic energy of the gas molecules. According to the kinetic theory of gas, the average kinetic energy of the gas molecules is proportional to its...
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Adiabatic Processes for an Ideal Gas01:18

Adiabatic Processes for an Ideal Gas

3.9K
When an ideal gas is compressed adiabatically, that is, without adding heat, work is done on it, and its temperature increases. In an adiabatic expansion, the gas does work, and its temperature drops. Adiabatic compressions actually occur in the cylinders of a car, where the compressions of the gas-air mixture take place so quickly that there is no time for the mixture to exchange heat with its environment. Nevertheless, because work is done on the mixture during the compression, its...
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General External Flow Characteristics01:26

General External Flow Characteristics

480
The study of external flow is essential for creating structures and objects that interact efficiently and safely with moving fluids, such as air or water. When a body is immersed in a flowing fluid, it experiences two primary forces: drag, which opposes motion along the flow direction, and lift, which acts perpendicular to the flow. The shape, size, and orientation of the object influence these forces.Streamlined and Blunt Bodies in External FlowObjects in fluid flow are classified as...
480
Acceleration due to Gravity on Other Planets01:24

Acceleration due to Gravity on Other Planets

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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...
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関連する実験動画

Updated: Jan 2, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 15, 2013

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火星の上層大気圏の地球循環

M Benna1,2, S W Bougher3, Y Lee4,2

  • 1Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA. mehdi.benna@nasa.gov.

Science (New York, N.Y.)
|December 14, 2019
PubMed
まとめ

火星

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Scattering And Absorption of Light in Planetary Regoliths
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Exploring the Effects of Atmospheric Forcings on Evaporation: Experimental Integration of the Atmospheric Boundary Layer and Shallow Subsurface
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Exploring the Effects of Atmospheric Forcings on Evaporation: Experimental Integration of the Atmospheric Boundary Layer and Shallow Subsurface

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関連する実験動画

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Scattering And Absorption of Light in Planetary Regoliths
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科学分野:

  • 惑星科学
  • 大気科学
  • 航空学

背景:

  • 火星の熱層は 大気中の揮発性物質が 宇宙に流出する際の 重要なインターフェースとして機能します
  • 地球の循環は太陽エネルギーによって導かれ 熱圏の構造とダイナミクスを支配します

研究 の 目的:

  • 火星熱圏内の地球循環パターンをマップする
  • 火星の大気動力学への太陽エネルギー再分配の影響を理解するために

主な方法:

  • 火星大気と揮発性進化 (MAVEN) 宇宙船からのデータを使用した.
  • 火星熱圏の ニュートラル風のパターンを測定した

主要な成果:

  • 地球の熱圏と比較して 単純で持続的な循環パターンを明らかにしました
  • 風のパターンと火星の地形との強い相関を観測した.
  • 循環に影響を与える重要な要因として,オーログラフィック重力波を特定した.

結論:

  • 火星の熱循環は 地球より複雑で季節的に安定しています
  • トポグラフィは重力波を通して大気動態を形作る上で重要な役割を果たします
  • MAVENのデータは火星の大気逃亡の過程について 前例のない洞察を提供します