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相关概念视频

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.
The Fossil Record02:56

The Fossil Record

The fossil record documents only a small fraction of all organisms that have ever inhabited Earth. Fossilization is a rare process, and most organisms never become fossils. Moreover, the fossil record only exhibits fossils that have been discovered. Nevertheless, sedimentary rock fossils of long-lived, abundant, hard-bodied organisms dominate the fossil record. These fossils offer valuable information, such as an organism's physical form, behavior, and age. Studying the fossil record helps...
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.
Types of Collisions - II01:19

Types of Collisions - II

When two or more objects collide with each other, they can stick together to form one single composite object (after collision). The total mass of the object after the collision is the sum of the masses of the original objects, and it moves with a velocity dictated by the conservation of momentum. Although the system's total momentum remains constant, the kinetic energy decreases, and thus such a collision is an inelastic collision. Most of the collisions between objects in daily life are...
Origin of Cellular Life01:24

Origin of Cellular Life

The origin of life on Earth is a complex and enigmatic event rooted in ancient biochemical processes and geological conditions. Experimental evidence supports the hypothesis that life began with the spontaneous formation of organic molecules such as RNA nucleotides, amino acids, and lipids under early Earth conditions. Factors like volcanic activity, intense UV radiation, and a reducing atmosphere without free oxygen likely facilitated these reactions. Hydrothermal vents on the ocean floor are...
Microbes and Other Elemental Cycles01:24

Microbes and Other Elemental Cycles

Microbial activity plays a pivotal role in the biogeochemical cycling of iron and manganese, especially at the redox gradients characteristic of stratified aquatic environments. These cycles are driven by microbial transformations between oxidized and reduced forms of the metals, allowing organisms to exploit them for metabolic energy and structural purposes.Iron Cycling Across Redox GradientsIn neutral, oxygen-rich surface waters, iron is predominantly found in its oxidized, insoluble ferric...

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相关实验视频

Updated: May 10, 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

铁石证据证明了原行星的早期形成和灾难性破坏.

Jijin Yang1, Joseph I Goldstein, Edward R D Scott

  • 1Department of Mechanical and Industrial Engineering, University of Massachusetts, Amherst, Massachusetts 01003, USA. jiyang@ecs.umass.edu

Nature
|April 20, 2007
PubMed
概括

铁石的冷却速度揭示了早期的原行星比以前认为的要大. 这些发现挑战了行星积聚的传统模型,并表明更大的撞击事件形成了第一个行星.

科学领域:

  • 行星科学 行星科学
  • 宇宙化学 宇宙化学
  • 天体物理学 天体物理学

背景情况:

  • 行星是通过较小的天体的碰撞成长而形成的,包括原行星.
  • 铁石提供了关于早期行星积聚的见解,因为它们的起源很古老.
  • 传统模型表明,根据石冷却速度,差异化的物体直径为5-200公里.

研究的目的:

  • 为了研究IVA组铁石的冷却速度.
  • 重新评估早期分化物体的大小和性质.
  • 为了测试行星积聚的传统模型.

主要方法:

  • 使用改进模型分析IVA组铁石的冷却速度.
  • 从独立的冷却速率指标中纳入新的数据.
  • 测量石中的大量含量.

主要成果:

  • 对于IVA铁石的冷却速度在100到6000K Myr (-1) 之间,随着散装Ni的减少而增加.
  • 在小物体中采用同热冷却的传统模型不再可行.
  • 结果表明,IVA石冷却在一个直径为300公里的金属体内,缺乏绝缘地幔.

结论:

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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

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Last Updated: May 10, 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

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

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  • 大约10^3公里的原行星在最初的1.5亿年内形成.
  • 这些大型原行星可能是通过"撞击逃跑"碰撞形成的.
  • 这些早期的大型天体的碎片可能作为小行星存活下来.