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Rocket Propulsion in Gravitational Field - II01:03

Rocket Propulsion in Gravitational Field - II

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A rocket's velocity in the presence of a gravitational field is decreased by the amount of force exerted by Earth's gravitational field, which opposes the motion of the rocket. If we consider thrust, that is, the force exerted on a rocket by the exhaust gases, then a rocket's thrust is greater in outer space than in the atmosphere or on a launch pad. In fact, gases are easier to expel in a vacuum.
A rocket's acceleration depends on three major factors, consistent with the...
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Acceleration due to Gravity on Other Planets01:24

Acceleration due to Gravity on Other Planets

4.0K
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...
4.0K
Rocket Propulsion in Gravitational Field - I01:20

Rocket Propulsion in Gravitational Field - I

2.7K
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...
2.7K
Doppler Effect - II01:05

Doppler Effect - II

3.3K
The Doppler effect has several practical, real-world applications. For instance, meteorologists use Doppler radars to interpret weather events based on the Doppler effect. Typically, a transmitter emits radio waves at a specific frequency toward the sky from a weather station. The radio waves bounce off the clouds and precipitation and travel back to the weather station. The radio frequency of the waves reflected back to the station appears to decrease if the clouds or precipitation are moving...
3.3K
Circular Orbits and Critical Velocity for Satellites01:16

Circular Orbits and Critical Velocity for Satellites

2.8K
The Moon orbits around the Earth. In turn, the Earth (and other planets) orbit the Sun. The space directly above our atmosphere is filled with artificial satellites in orbit. One can examine the circular orbit, the simplest kind of orbit, to understand the relationship between the speed and the period of planets and satellites with respect to their positions and the bodies that they orbit.
Nicolaus Copernicus (1473-1543) first suggested that the Earth and all other planets orbit the Sun in...
2.8K
Doppler Effect - I00:56

Doppler Effect - I

3.5K
The Doppler effect and Doppler shift were named after the Austrian physicist and mathematician Christian Johann Doppler in 1842, who conducted experiments with both moving sources and moving observers. Consider an observer standing on a street corner, observing an ambulance with a siren sound passing by at a constant speed. The observer experiences two characteristic changes in the sound of the siren. Initially, the sound increases in loudness as the ambulance approaches and decreases in...
3.5K

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Updated: May 25, 2025

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

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雅尔科夫斯基和YORP效果模拟在3200 Phaethon上进行.

Hiroki Senshu1, Hirotomo Noda2,3, Fumi Yoshida1,4

  • 1Planetary Exploration Research Center, Chiba Institute of Technology, 2-17-1 Tsudanuma, Narashino, Chiba 275-0016, Japan.

Philosophical transactions. Series A, Mathematical, physical, and engineering sciences
|February 27, 2025
PubMed
概括

小行星3200法顿

关键词:
菲顿 (Phaethon) 是一个神灵.约尔普 (YORP) 是一个约尔普.亚科夫斯基 (Yarkovsky) 是一个著名的作家.数字模拟的数字模拟.热建模 热建模 热建模

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Scattering And Absorption of Light in Planetary Regoliths
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Last Updated: May 25, 2025

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

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Scattering And Absorption of Light in Planetary Regoliths
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Scattering And Absorption of Light in Planetary Regoliths

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科学领域:

  • * 星球科学 星球科学
  • * 太阳系动力学

背景情况:

  • *小行星3200 Phaethon是双子座流星雨的母体.
  • * 费顿表现出一个极其奇特的轨道与一个小的周日点距离.

研究的目的:

  • *以数值研究小行星3200 Phaethon的热行为.
  • *精确评估热辐射对法的轨道和旋转运动的影响.

主要方法:

  • * 数值建模一个轨道周期的热变化.
  • *分析旋转轴与太阳相对方向的影响.

主要成果:

  • *热效应对轨道和旋转运动的变化信号在周日点附近.
  • *对于热诱导的动量而言,正规表达式不适用于法伊.
  • * 轨道平均热效应与观测和先前估计一致.

结论:

  • * 费顿独特的轨道特征导致复杂的热效应.
  • *这项研究提升了我们对小物体非引力作用的理解.