Jove
Visualize
联系我们
JoVE
x logofacebook logolinkedin logoyoutube logo
关于 JoVE
概览领导团队博客JoVE 帮助中心
作者
出版流程编辑委员会范围与政策同行评审常见问题投稿
图书馆员
用户评价订阅访问资源图书馆顾问委员会常见问题
研究
JoVE JournalMethods CollectionsJoVE Encyclopedia of Experiments存档
教育
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab Manual教师资源中心教师网站
使用条款与条件
隐私政策
政策

相关概念视频

Classifying Matter by Composition03:35

Classifying Matter by Composition

Matter: Pure Substances and Mixtures
According to its composition, the matter can be classified into two broad categories — pure substances and mixtures. 
A pure substance is a form of matter that has a constant composition throughout with uniform properties. For example, any sample of sucrose has the same composition and same physical properties, such as melting point, color, and sweetness, regardless of the source from which it is isolated. 
A mixture is composed of two or more types of...
The Soil Ecosystem02:23

The Soil Ecosystem

Plants obtain inorganic minerals and water from the soil, which acts as a natural medium for land plants. The composition and quality of soil depend not only on the chemical constituents but also on the presence of living organisms. In general, soils contain three major components:
What is Matter?01:13

What is Matter?

The substance of the universe—from a grain of sand to a star—is called matter. Scientists define matter as anything that occupies space and has mass. An object’s mass and its weight are related concepts, but not quite the same. An object’s mass is the amount of matter contained in the object and is the same whether that object is on Earth or in the zero-gravity environment of outer space. An object’s weight, on the other hand, is its mass as affected by the pull of gravity. Where gravity...
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.
What are Biogeochemical Cycles?00:54

What are Biogeochemical Cycles?

The most common elements in organic molecules, carbon, hydrogen, oxygen, nitrogen, sulfur, and phosphorus, are only available in the ecosystem in limited amounts. Therefore, these nutrients must be recycled through both biotic and abiotic components of the ecosystem, in processes generally called biogeochemical cycles.

您也可能阅读

相关文章

通过共同作者、期刊和引用图与本文相关的文章。

排序
Same author

Projecting Climate Dependent Coastal Flood Risk With a Hybrid Statistical Dynamical Model.

Earth's future·2022
Same author

Multiple host shifts by the emerging honeybee parasite, Varroa jacobsoni.

Molecular ecology·2015
Same author

A novel strain of sacbrood virus of interest to world apiculture.

Journal of invertebrate pathology·2014
Same author

Periodontal disease part I: types, etiology, and epidemiology.

Canadian family physician Medecin de famille canadien·2011
Same author

Laparoscopy in General Surgery: The pros and cons of endoscopic surgery.

Canadian family physician Medecin de famille canadien·2011
Same author

Medical aspects of renal insufficiency in urologic practice.

The Medical clinics of North America·2010

相关实验视频

Updated: Jul 12, 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 15, 2013

地球的组成 地球的组成

D L Anderson

    Science (New York, N.Y.)
    |January 20, 1989
    PubMed
    概括

    新的太阳组成估计揭示了更高的铁和水平,影响了宇宙丰度模型. 这表明,太阳系内部的天体具有更密集,化学分区的地幔组成.

    科学领域:

    • 行星科学 行星科学
    • 太空化学 太空化学
    • 地质物理学 地质物理学

    背景情况:

    • 以前的宇宙丰富度和星云组成模型依赖于体值.
    • 太阳组成估计已经更新了新的测量.

    研究的目的:

    • 根据新的太阳组成数据,修订宇宙丰度模型.
    • 推断行星地幔的化学组成和结构.

    主要方法:

    • 对新的太阳能组成估计的分析.
    • 将新的估计值与氏体值进行比较.
    • 地质物理数据的解释.

    主要成果:

    • 新的太阳能组成显示Fe和Ca相对于Mg,Al和Si的丰富.
    • 铁/和/的原子比率比合体值高30-40%.
    • 隐含的地幔组成包括~15%的FeO和更多的CaMgSi2O6 (二氧化).

    结论:

    • 需要修订宇宙丰度和星云组成.
    • 地质物理数据支持密集,富含FeO的下层地幔和富含二氧化的过渡区域.

    更多相关视频

    Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions
    11:50

    Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions

    Published on: June 13, 2015

    Combined Size and Density Fractionation of Soils for Investigations of Organo-Mineral Interactions
    08:38

    Combined Size and Density Fractionation of Soils for Investigations of Organo-Mineral Interactions

    Published on: February 15, 2019

    相关实验视频

    Last Updated: Jul 12, 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 15, 2013

    Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions
    11:50

    Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions

    Published on: June 13, 2015

    Combined Size and Density Fractionation of Soils for Investigations of Organo-Mineral Interactions
    08:38

    Combined Size and Density Fractionation of Soils for Investigations of Organo-Mineral Interactions

    Published on: February 15, 2019

  • 结果有利于化学区分的地幔,其FeO含量与太阳系内部天体的典型含量有关.