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相关概念视频

Recrystallization: Solid–Solution Equilibria01:10

Recrystallization: Solid–Solution Equilibria

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Recrystallization is a purification technique used to separate impurities from solid compounds. In this technique, no chemical reactions occur. Instead, it exploits physical properties only, specifically, the solubility differences between the desired compound and impurities, either at a single temperature or at different temperatures, and under other selected conditions. The solid-solution equilibrium (solubility equilibrium) of each component in the solution represents a binary phase...
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Phase Transitions: Vaporization and Condensation02:39

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The physical form of a substance changes on changing its temperature. For example, raising the temperature of a liquid causes the liquid to vaporize (convert into vapor). The process is called vaporization—a surface phenomenon. Vaporization occurs when the thermal motion of the molecules overcome the intermolecular forces, and the molecules (at the surface) escape into the gaseous state. When a liquid vaporizes in a closed container, gas molecules cannot escape. As these gas phase...
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Phase Transitions: Sublimation and Deposition02:33

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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...
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Coprecipitation is the contamination of a precipitate by otherwise soluble species and occurs via different processes. In colloidal precipitates, coprecipitation occurs via surface adsorption. For instance, barium sulfate has a primary layer of adsorbed barium ions and a secondary layer of nitrate counterions. This results in contamination of the precipitate by barium nitrate.
Sometimes, ions in a crystal lattice can undergo isomorphous replacement by inclusions of similar charge and size. For...
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Crystalline solids are divided into four types: molecular, ionic, metallic, and covalent network based on the type of constituent units and their interparticle interactions.
Molecular Solids
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The experimental conditions in a gravimetric analysis should be optimized to maximize the particle size and purity of the obtained precipitate. Ideally, the concentration of the precipitating reagent should be low with effective stirring to maintain low relative supersaturation for the growth of large crystals. In homogeneous precipitation, the precipitant is slowly generated by a chemical reaction in the solution to avoid local reagent excesses. For example, urea decomposes gradually to...
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相关实验视频

Updated: Sep 15, 2025

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
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在嵌入的原行星盘中检测到耐火固体凝结

M K McClure1, Merel Van't Hoff2,3, Logan Francis4

  • 1Leiden Observatory, Leiden University, Leiden, The Netherlands. mcclure@strw.leidenuniv.nl.

Nature
|July 16, 2025
PubMed
概括
此摘要是机器生成的。

天文学家在原恒星HOPS-315周围发现了行星形成的最早时刻. 这种观测揭示了构建新行星系统所需的初始热气体和固体,

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科学领域:

  • * 天文学与天体物理学
  • * 星球科学
  • * 原行星盘进化

背景情况:

  • * 地球行星由恒星间和岩石固体形成, 来自热冷气体.
  • *从这个气体中重新凝结起来的初始高温矿物质标志着行星形成的开始.
  • 这种热气体的起源及其在其他星系行星形成中的作用尚不清楚.

研究的目的:

  • * 为了检测和描述
  • 在 t=0
  • 星球形成的时刻.
  • * 探究新星系最初的构建块的组成和起源.
  • * 将早期太阳系形成过程与其他系统的形成过程进行比较.

主要方法:

  • *使用詹姆斯·韦伯太空望远镜 (JWST) 和阿塔卡马大毫米阵列 (ALMA) 观测年轻的原星HOPS-315.
  • 分析红外和毫米波长数据以确定气体和矿物成分.
  • * 观察数据与凝结和盘结构模型的比较.

主要成果:

  • * 在HOPS-315的内部盘中检测到热氧化物 (SiO) 气体和晶体矿.
  • * 确定这些物质是新行星系统的初始构建块.
  • 证据表明,类似于我们太阳系中的耐火固体正在形成.

结论:

  • 这项研究提供了首次天文探测到行星形成的"t=0"时刻.
  • *内部磁盘环境是由星际固体的升华和随后的耐火材料的再凝结形成的.
  • 这些过程发生在与我们太阳系中耐火凝结相比较的时间尺度上, 提供了对行星形成普遍性的见解.