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相关概念视频

Surface Tension01:24

Surface Tension

Surface tension is defined as the force per unit length (γ) acting along the surface of a liquid. It arises due to strong intermolecular forces of attraction. A molecule located inside the bulk of the liquid is surrounded by other molecules and experiences equal forces in all directions. However, a molecule at the surface experiences unbalanced forces because there are more neighboring molecules below than above. This creates a net inward force that pulls surface molecules toward the interior,...
Buoyancy01:12

Buoyancy

When an object is placed in a fluid, it either floats or sinks. All objects in a fluid experience a buoyant force. For example, a metal ball sinks, while a rubber ball floats. Similarly, a submarine can sink and float by adjusting its buoyancy.  The concept of buoyancy raises several interesting questions. For instance, where does this buoyant force come from? How much buoyant force is required to make an object sink or float? Do objects that sink get any support at all from the fluid? 
To get...
Surface Tension and Surface Energy01:16

Surface Tension and Surface Energy

When a paint brush is immersed in water, the bristles wave freely inside the water. When it is taken out, the bristles stick together. The reason behind this effect is surface tension.
Consider a beaker filled with liquid. The bulk molecules in the liquid experience equal attractive forces on all sides with the surrounding molecules. However, the surface molecules experience a net attractive force downward due to the bulk molecules. The surface of the liquid behaves like a stretched membrane,...
Surface Tension of Fluid01:22

Surface Tension of Fluid

Surface tension is a fundamental property of fluids, occurring at the boundary between a liquid and a gas or between two immiscible liquids. This phenomenon arises from the cohesive forces between molecules at the fluid's surface, creating an effect similar to a stretched elastic membrane. Inside each fluid, molecules are equally attracted in all directions by neighboring molecules, but surface molecules experience a net inward force, resulting in surface tension.
Surface tension varies with...
Tidal Forces01:06

Tidal Forces

The origin of Earth's ocean tides has been a subject of continuous investigation for over 2000 years. However, the work of Newton is considered to be the beginning of the proper understanding of the phenomenon. Ocean tides are the result of gravitational tidal forces. These same tidal forces are present in any astronomical body; they are responsible for the internal heat that creates the volcanic activity on Io, one of Jupiter's moons, and the breakup of stars that get too close to black holes.
Buoyancy and Stability for Submerged and Floating Bodies01:11

Buoyancy and Stability for Submerged and Floating Bodies

In fluid mechanics, buoyancy and stability are key concepts for understanding the behavior of submerged and floating bodies. When a stationary body is fully or partially submerged in a fluid, the fluid exerts a force on the body known as the buoyant force. This force acts vertically upward through a point called the center of buoyancy, which is the center of the displaced fluid volume. According to Archimedes' principle, the magnitude of the buoyant force is equal to the weight of the fluid...

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相关实验视频

Updated: Jul 11, 2026

Total Internal Reflection Absorption Spectroscopy (TIRAS) for the Detection of Solvated Electrons at a Plasma-liquid Interface
08:50

Total Internal Reflection Absorption Spectroscopy (TIRAS) for the Detection of Solvated Electrons at a Plasma-liquid Interface

Published on: January 24, 2018

特里顿:我们看到了表面吗?

D P Cruikshank, R H Brown, L P Giver

    Science (New York, N.Y.)
    |July 21, 1989
    PubMed
    概括

    新的望远镜数据揭示了海王星的卫星Triton上的甲冰和. 这表明,顿的大气层足够透明,太阳光可以到达它的表面,这可能揭示了表面的特征.

    科学领域:

    • 行星科学 行星科学
    • 天体生物学 天体生物学
    • 大气科学 大气科学

    背景情况:

    • 海王星的卫星特里顿拥有独特的大气和表面组成.
    • 了解Triton上挥发物质的物理状态是了解其环境的关键.

    研究的目的:

    • 为了评估在Triton上的甲和的数量和物理状态.
    • 为了确定Triton上的大气透明度和表面条件.

    主要方法:

    • 分析新的望远镜数据.
    • 甲和气挥发物的实验室测量.

    主要成果:

    • 甲冰存在于Triton的表面.
    • 特里顿的大气层足够透明,太阳光可以透到表面.
    • 存在于大气和凝结 (液体或固体) 状态,在表面或作为薄云.

    结论:

    • 特里顿的表面条件受到大气和凝结的挥发物的影响.
    • 特里顿大气层的透明度对表面过程和观测有影响.
    • 旅行者号航天器的成像预计将解决顿的表面特征.

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    Chemotactic Response of Marine Micro-Organisms to Micro-Scale Nutrient Layers
    22:38

    Chemotactic Response of Marine Micro-Organisms to Micro-Scale Nutrient Layers

    Published on: May 28, 2007

    相关实验视频

    Last Updated: Jul 11, 2026

    Total Internal Reflection Absorption Spectroscopy (TIRAS) for the Detection of Solvated Electrons at a Plasma-liquid Interface
    08:50

    Total Internal Reflection Absorption Spectroscopy (TIRAS) for the Detection of Solvated Electrons at a Plasma-liquid Interface

    Published on: January 24, 2018

    Treating Surfaces with a Cold Atmospheric Pressure Plasma using the COST-Jet
    06:36

    Treating Surfaces with a Cold Atmospheric Pressure Plasma using the COST-Jet

    Published on: November 2, 2020

    Chemotactic Response of Marine Micro-Organisms to Micro-Scale Nutrient Layers
    22:38

    Chemotactic Response of Marine Micro-Organisms to Micro-Scale Nutrient Layers

    Published on: May 28, 2007