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Precipitate Formation and Particle Size Control01:16

Precipitate Formation and Particle Size Control

947
In precipitation gravimetry, the precipitating agent should react specifically or selectively with the analyte. While a specific reagent reacts with the analyte alone, a selective reagent can react with a limited number of chemical species.
The obtained precipitate should be either a pure substance of known composition or easily converted to one by a simple process, such as ignition or drying. In addition, the precipitate should be insoluble and easily filterable. In general, filterability...
947
Conditions on Early Earth02:06

Conditions on Early Earth

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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.
96.4K
Phase Transitions: Sublimation and Deposition02:33

Phase Transitions: Sublimation and Deposition

17.9K
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...
17.9K
Solution Formation02:16

Solution Formation

32.7K
There is no one solvent that can dissolve every type of solute. Some substances that readily dissolve in a certain solvent might be insoluble in a different solvent. A simple way to predict which substances dissolve in which solvent is the phrase "like dissolves like". This means that polar substances, such as salt and sugar, dissolve in a polar substance like water. In contrast, non-polar substances are more soluble in non-polar solvents such as carbon tetrachloride.
This selective...
32.7K
Formation of Complex Ions03:45

Formation of Complex Ions

24.0K
A type of Lewis acid-base chemistry involves the formation of a complex ion (or a coordination complex) comprising a central atom, typically a transition metal cation, surrounded by ions or molecules called ligands. These ligands can be neutral molecules like H2O or NH3, or ions such as CN− or OH−. Often, the ligands act as Lewis bases, donating a pair of electrons to the central atom. These types of Lewis acid-base reactions are examples of a broad subdiscipline called coordination...
24.0K
Elastic Collisions: Introduction01:00

Elastic Collisions: Introduction

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An elastic collision is one that conserves both internal kinetic energy and momentum. Internal kinetic energy is the sum of the kinetic energies of the objects in a system. Truly elastic collisions can only be achieved with subatomic particles, such as electrons striking nuclei. Macroscopic collisions can be very nearly, but not quite, elastic, as some kinetic energy is always converted into other forms of energy such as heat transfer due to friction and sound. An example of a nearly...
13.1K

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Updated: Sep 10, 2025

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

Published on: June 5, 2014

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由木星形成引发的含有挥发物质的行星体碰撞形成

Sin-Iti Sirono1, Diego Turrini2

  • 1Graduate School of Earth and Environmental Sciences, Nagoya University, Nagoya, Japan. sirono@eps.nagoya-u.ac.jp.

Scientific reports
|August 25, 2025
PubMed
概括
此摘要是机器生成的。

含有挥发性物质的行星之间的碰撞解释了圆柱体的形成. 木星的形成引发了这些撞击,产生了由气体分散的酸盐融化,与体大小和冷却速度相匹配.

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Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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Simulation of the Planetary Interior Differentiation Processes in the Laboratory

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

Last Updated: Sep 10, 2025

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

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Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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Simulation of the Planetary Interior Differentiation Processes in the Laboratory

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

Published on: June 13, 2015

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科学领域:

  • 星球科学
  • 宇宙化学
  • 天体物理学

背景情况:

  • 圆柱体是圆柱体石的关键组成部分,为早期太阳系过程提供了洞察力.
  • 观察到的圆柱体大小和冷却速度很难与现有的形成模型相协调.
  • 对于确定太阳系早期的年代和了解行星的形成至关重要.

研究的目的:

  • 提出和数值验证一个新的chondrule形成模型.
  • 解释孔德鲁的特征大小和冷却速度.
  • 为了将体形成与木星和太阳星云形成的早期阶段联系起来.

主要方法:

  • 高速行星碰撞的数值模拟.
  • 通过挥发性驱动气体扩张生成和分散的酸盐模型.
  • 分析与木星气体积聚相关的融化速度.

主要成果:

  • 具有挥发性丰富的行星体的高速碰撞 (> 2 公里/秒) 会产生大量的化物.
  • 从加热的挥发物中膨胀的气体分散并冷却化物, 形成圆柱体大小的水滴.
  • 化的峰值与木星的气体积聚开始相关.

结论:

  • 星球微小碰撞提供了一个自然的机制,解释了它们的观测特性.
  • 圆柱体形成提供了一个时间标记,表明木星在含丰富的含量 (CAI) 后大约形成了1.8亿年.
  • 这个模型与早期太阳系动态和木星的形成时间表相协调.