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相关概念视频

Phase Transitions: Sublimation and Deposition02:33

Phase Transitions: Sublimation and Deposition

18.4K
Some solids can transition directly into the gaseous state, bypassing the liquid state, via a process known as sublimation. At room temperature and standard pressure, a piece of dry ice (solid CO2) sublimes, appearing to gradually disappear without ever forming any liquid. Snow and ice sublimate at temperatures below the melting point of water, a slow process that may be accelerated by winds and the reduced atmospheric pressures at high altitudes. When solid iodine is warmed, the solid sublimes...
18.4K
Sublimation01:03

Sublimation

1.0K
Sublimation is the direct transformation of a solid to a gaseous state. For instance, at standard pressure and room temperature, solid carbon dioxide sublimes to gaseous carbon dioxide. The phase diagram depicts the conditions required for sublimation. This process occurs at the solid-gas phase boundary and is not observed above the triple point of the substance. The reverse of sublimation is called deposition, where a gaseous substance condenses directly into a solid. Sublimation and...
1.0K
States of Water01:23

States of Water

54.3K
Water exists in any one of the three classical states: solid (ice), liquid (water), and gas (steam or water vapor). The state of water depends on i) the intermolecular forces that draw molecules together and ii) the kinetic energy that leads to movements that pull them apart.
Water freezes when the intermolecular forces are greater than the kinetic energy. Unlike most other substances, water is less dense in its solid state than in its liquid state. This is because each water molecule can form...
54.3K
Phase Transitions: Vaporization and Condensation02:39

Phase Transitions: Vaporization and Condensation

19.1K
The physical form of a substance changes on changing its temperature. For example, raising the temperature of a liquid causes the liquid to vaporize (convert into vapor). The process is called vaporization—a surface phenomenon. Vaporization occurs when the thermal motion of the molecules overcome the intermolecular forces, and the molecules (at the surface) escape into the gaseous state. When a liquid vaporizes in a closed container, gas molecules cannot escape. As these gas phase...
19.1K
Phase Transitions: Melting and Freezing02:39

Phase Transitions: Melting and Freezing

13.4K
Heating a crystalline solid increases the average energy of its atoms, molecules, or ions, and the solid gets hotter. At some point, the added energy becomes large enough to partially overcome the forces holding the molecules or ions of the solid in their fixed positions, and the solid begins the process of transitioning to the liquid state or melting. At this point, the temperature of the solid stops rising, despite the continual input of heat, and it remains constant until all of the solid is...
13.4K
Acceleration due to Gravity on Other Planets01:24

Acceleration due to Gravity on Other Planets

4.4K
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...
4.4K

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相关实验视频

Updated: Oct 10, 2025

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

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在冥王星上的Sputnik Planitia中以升华驱动的对流

Adrien Morison1, Stéphane Labrosse2, Gaël Choblet3

  • 1Physics and Astronomy, University of Exeter, Exeter, UK.

Nature
|December 16, 2021
PubMed
概括

化驱动的对流解释了Sputnik Planitia在冥王星上的多边形表面模式. 这个过程需要较低的基底热流或较高的粘度对比度在冰层内.

科学领域:

  • 星球科学
  • 地质学
  • 表面过程

背景情况:

  • 冥王星上的Sputnik Planitia具有独特的多边形表面图案.
  • 以往涉及固态对流的模型未能复制观察到的平面多边形和窄槽的地形.

研究的目的:

  • 调查表面化在Sputnik Planitia的冰盆内推动对流的作用.
  • 为了使对流模型与观察到的表面形态相协调.

主要方法:

  • 在冥王星的Sputnik Planitia中对流过程的数值建模.
  • 对不同基底热量流和冰粘度对比对表面图案的影响的分析.

主要成果:

  • 化驱动的对流成功地重现了观察到的多边形结构.
  • 该模型表明基底热量比以前接受的值低 (~0.3 mW m-2).
  • 另外,通常接受的热流量 (2-3 mW m−2) 可以维持这些模式,具有显著更高的粘度对比度 (~3,000).

结论:

  • 表面升华是推动对流和塑造Sputnik Planitia表面的一个关键机制.
  • 这些发现表明我们对冥王星冰中的热流和物质特性有了更好的理解.

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