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関連する概念動画

States of Water01:23

States of Water

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...
Global Climate Change01:50

Global Climate Change

Throughout its ~4.5 billion year history, the Earth has experienced periods of warming and cooling. However, the current drastic increase in global temperatures is well outside of the Earth’s cyclic norms, and evidence for human-caused global climate change is compelling. Paleoclimatology, the study of ancient climate conditions, provides ample evidence for human-caused global climate change by comparing recent conditions with those in the past.
Conditions on Early Earth02:06

Conditions on Early Earth

Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
Conditions on Early Earth02:06

Conditions on Early Earth

Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
Radiation: Applications01:17

Radiation: Applications

The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
Masonry in Cold and Hot Weather Conditions01:21

Masonry in Cold and Hot Weather Conditions

In cold weather, masonry construction requires specific precautions to ensure mortar does not freeze before curing, as this can significantly weaken its strength and watertightness. Mortar temperature should be maintained between 60°F and 80°F to support proper hydration and curing. Below 40°F, mortar water must be heated, but should not exceed 120°F as high temperatures can reduce mortar's compressive and bond strength.
Other key practices include keeping masonry units and sand dry and...

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関連する実験動画

Updated: Jun 24, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
06:04

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 16, 2013

初期の火星:どのくらい暖かく,どれくらい湿ったか?

S W Squyres1, J F Kasting

  • 1Center for Radiophysics and Space Research, Cornell University, Ithaca, NY 14853, USA.

Science (New York, N.Y.)
|August 5, 1994
PubMed
まとめ

初期の火星は,降水だけでなく,地熱の熱とインパクトによる液体の水を持っていたかもしれません. メタンのような温室効果ガスの温和な温暖化は,地表水の流れを支えたかもしれない.

科学分野:

  • 惑星科学は惑星科学である.
  • 気候科学 気候科学
  • 地質学 地質学 地質学

背景:

  • 初期の火星は河川の侵食を示し,より暖かく湿った気候を示唆しています.
  • 純粋な二酸化炭素 (CO2) と水 (H2O) の大気は,凍結に近い温度には不十分である.
  • 以前のモデルでは,火星の初期に継続的に液体の水が存在していたことを説明するのに苦労しました.

研究 の 目的:

  • 初期の火星の気候温暖化のための代替メカニズムを調査する.
  • 液体の水を可能にするために,地熱と衝撃熱の役割を調査する.
  • 火星の温暖化に微量ガスによる潜在的貢献を評価する.

主な方法:

  • 火星の初期の大気条件の熱力学モデリング.
  • 地熱活動や衝撃イベントを含む熱源の分析.
  • メタン (CH4),アンモニア (NH3),二酸化硫黄 (SO2) から生じる温室効果ガスの影響の評価.

主要な成果:

  • 地熱と衝撃の熱によって駆動される水熱コンベクションは,水層の充填と地下水の浸出のための実行可能なメカニズムです.
  • 微量ガス (CH4,NH3,SO2) を補足した低圧CO2大気は,必要な温暖化をもたらすことができる.

さらに関連する動画

Manufacturing Simple and Inexpensive Soil Surface Temperature and Gravimetric Water Content Sensors
08:49

Manufacturing Simple and Inexpensive Soil Surface Temperature and Gravimetric Water Content Sensors

Published on: December 21, 2019

Simulation of Early Earth Hydrothermal Chimneys in a Thermal Gradient Environment
06:29

Simulation of Early Earth Hydrothermal Chimneys in a Thermal Gradient Environment

Published on: February 27, 2021

関連する実験動画

Last Updated: Jun 24, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
06:04

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 16, 2013

Manufacturing Simple and Inexpensive Soil Surface Temperature and Gravimetric Water Content Sensors
08:49

Manufacturing Simple and Inexpensive Soil Surface Temperature and Gravimetric Water Content Sensors

Published on: December 21, 2019

Simulation of Early Earth Hydrothermal Chimneys in a Thermal Gradient Environment
06:29

Simulation of Early Earth Hydrothermal Chimneys in a Thermal Gradient Environment

Published on: February 27, 2021

  • エピソード的な高傾きイベントは,局所的な地表温暖化に寄与している可能性があります.
  • 結論:

    • 初期の火星の液体の水は,降水量だけに依存していないかもしれない.
    • 地熱熱と地熱の影響は,地表水の維持に重要な役割を果たした可能性がある.
    • 温室効果ガスの痕跡と軌道の変化は,一時的な地表水の合理的な説明を提供します.