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

Gravimetry: Inorganic And Organic Precipitating Agents00:49

Gravimetry: Inorganic And Organic Precipitating Agents

In gravimetry, the precipitant is chosen carefully to obtain a pure solid that can be easily filtered. Common inorganic precipitants can be used to determine several cations and anions. In some cases, the formation of the same precipitate can be used to determine the cation and the anion. For example, the reaction of barium and chromate ions to give barium chromate is used to determine both barium and chromate. However, precipitates such as hydroxides, oxalates, and metal ammonium phosphates...
Minerals01:26

Minerals

Minerals are essential nutrients that the human body needs in small amounts to work properly. They play a vital role in many bodily functions, such as building strong bones and transmitting nerve impulses. Some minerals are needed for hormone production or to maintain a normal heartbeat. Major minerals include calcium, phosphorus, potassium, sulfur, sodium, chlorine, and magnesium, while trace minerals include iron, manganese, copper, iodine, zinc, cobalt, fluoride, and selenium.
Types of Building Stone01:30

Types of Building Stone

Building stones, essential materials for construction, are extracted from natural rock deposits and processed into specific forms and dimensions suitable for various building applications. These stones are broadly classified into three types based on their geological formation: igneous, sedimentary, and metamorphic.
Igneous rocks are formed from the solidification of magma or lava. An example is granite, known for its durability and resistance to weathering, making it ideal for parts of...
Quarrying of Stone01:15

Quarrying of Stone

Quarrying is the process of extracting stone from a quarry, where specialized techniques are employed to remove large blocks of stone safely and efficiently. This process can involve controlled explosions or more precision-oriented methods such as cutting and drilling.
One common method involves using a diamond belt saw to cut large blocks from the quarry face. These blocks can be about 50 feet long and 12 feet high. After the initial vertical cut, drilling is performed at the base of the block.
Stone Masonry01:29

Stone Masonry

Stone masonry is a construction technique that uses individual stones to build structures and can be categorized into two main types: rubble and ashlar. Rubble masonry uses uneven, naturally shaped stones such as river rocks or fragments from quarries. This method often requires the mason to select and possibly shape each stone to fit the designated space, ensuring a proper build, even with irregular stone sizes and shapes. Ashlar masonry, on the other hand, employs uniformly cut stones that...
Aggregates Classification01:29

Aggregates Classification

Aggregate classification is generally based on its size, petrographic characteristics, weight, and source. Size classification ranges from coarse to fine aggregates, defined by the size of the particles. Coarse aggregates are particles that do not pass through ASTM sieve No. 4, and aggregates that pass through the sieve are fine aggregates.
Petrographic classification groups aggregates based on common mineralogical characteristics. Some of the common mineral groups found in aggregates are...

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

Constraints on the martian crust away from the InSight landing site.

Nature communications·2022
Same author

Alteration history of Séítah formation rocks inferred by PIXL x-ray fluorescence, x-ray diffraction, and multispectral imaging on Mars.

Science advances·2022
Same author

Compositionally and density stratified igneous terrain in Jezero crater, Mars.

Science advances·2022
Same author

Upper mantle structure of Mars from InSight seismic data.

Science (New York, N.Y.)·2021
Same author

Thickness and structure of the martian crust from InSight seismic data.

Science (New York, N.Y.)·2021
Same author

The SuperCam Instrument Suite on the NASA Mars 2020 Rover: Body Unit and Combined System Tests.

Space science reviews·2020
Same journal

Keep the Hubble and James Webb Space Telescopes alive - the science is worth the price tag.

Nature·2026
Same journal

Say hello to hard helium.

Nature·2026
Same journal

How to avoid dementia - what the science really says.

Nature·2026
Same journal

Save Hubble: the race to preserve the space telescope kicks off.

Nature·2026
Same journal

How long can humans live? All evidence points to a maximum of 125 years.

Nature·2026
Same journal

Listen to Gen Z when it comes to AI in education.

Nature·2026
查看所有相关文章

相关实验视频

Updated: May 14, 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

小行星和安德西特.

Richard Arculus1, Ian H Campbell, Scott M McLennan

  • 1Research School of Earth Sciences, Australian National University, Canberra, Australian Capital Territory 0200, Australia. Ross.Taylor@anu.edu.au

Nature
|May 30, 2009
PubMed
概括
此摘要是机器生成的。

这项研究挑战了某些石代表小行星上形成石地的新方法的说法. 分析表明,关于石生成的现有理论仍然有效.

更多相关视频

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
09:44

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Published on: June 5, 2014

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

相关实验视频

Last Updated: May 14, 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

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
09:44

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Published on: June 5, 2014

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

科学领域:

  • 行星科学 行星科学
  • 地质化学 地质化学

背景情况:

  • 在俯冲区的陆地石产量是众所周知的.
  • 最近的一项研究提出了一种新的机制,用于在小行星上产生石地,使用石GRA 06128和GRA 06129.

研究的目的:

  • 评估一项关于在小行星上产生石地的新模式的说法.
  • 分析石GRA 06128和GRA 06129.的组成数据.

主要方法:

  • 分析稀土元素 (REE) 和其他光电爱好者元素数据.
  • 流星组成与行星地形成现有模型的比较.

主要成果:

  • 构成数据,特别是REEs的构成数据,不支持拟议的石生成的新机制.
  • 研究的石的组成与已知的石形成过程一致.

结论:

  • 关于在小行星上产生石的新方式的说法没有得到提供的数据的支持.
  • 目前产生石行星地的机制仍然有效,不需要修改.