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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...
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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...
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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

10.5K

冥王星のスプートニク・プラニティアにおける亜熱流動

Adrien Morison1, Stéphane Labrosse2, Gaël Choblet3

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

Nature
|December 16, 2021
PubMed
まとめ

スプートニク・プランティアの多角形の表面パターンを説明します このプロセスは,より低い基礎熱流または窒素氷層内のより高い粘度コントラストを必要とします.

科学分野:

  • 惑星科学
  • 地理学
  • 表面処理

背景:

  • 冥王星のスプートニク・プラニティアには 独特の多角形の表面パターンがあります
  • 固体コンベクションを含む以前のモデルは,平らな多角形と狭い谷の観測された地形を再現できませんでした.

研究 の 目的:

  • スプートニク・プランティアの窒素の氷の盆地内のコンベクションを駆動する表面の亜熱化の役割を調査する.
  • 観測された表面形態とコンベクションのモデルを調和させる.

主な方法:

  • 冥王星のスプートニク・プラニティア内のコンベクションプロセスの数値モデリング.
  • 基礎熱流の変化と氷の粘度コントラストの表面パターンへの影響の分析.

主要な成果:

  • サブリメーション駆動コンベクションは,観察された多角構造を成功裏に再現します.
  • このモデルは,以前に受け入れられた値よりも低い基礎熱流 (~0.3 mW m−2) を示しています.
  • また,一般的に受け入れられている熱流量 (2-3 mW m−2) は,これらのパターンを著しく高い粘度コントラスト (~3,000) で維持できます.

結論:

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Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
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Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas

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Thermocapillary Convection Space Experiment on the SJ-10 Recoverable Satellite
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Last Updated: Oct 10, 2025

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  • スプートニク・プランティアの表面を形作る 重要なメカニズムです
  • この発見は,冥王星の窒素氷の熱流と物質特性の理解を修正することを示唆しています.