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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.
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.
Rocket Propulsion In Empty Space - II01:12

Rocket Propulsion In Empty Space - II

The motion of a rocket is governed by the conservation of momentum principle. A rocket's momentum changes by the same amount (with the opposite sign) as the ejected gases. As time goes by, the rocket's mass (which includes the mass of the remaining fuel) continuously decreases, and its velocity increases. Therefore, the principle of conservation of momentum is used to explain the dynamics of a rocket's motion. The ideal rocket equation gives the change in velocity that a rocket experiences by...
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...
Sulfur Assimilation01:20

Sulfur Assimilation

Sulfur is an essential element in biological systems, contributing to synthesizing key biomolecules, including amino acids such as cysteine and methionine, and cofactors such as coenzyme A and biotin. Microorganisms primarily assimilate sulfur as sulfate (SO₄²⁻) from the environment, which must undergo a series of biochemical transformations before it can be incorporated into cellular components. As sulfate is highly oxidized, it must undergo assimilatory sulfate reduction to become...

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相关实验视频

Updated: Jun 7, 2026

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

来自原始石的星尘酸盐.

Kazuhide Nagashima1, Alexander N Krot, Hisayoshi Yurimoto

  • 1Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Ookayama, Meguro, Tokyo 152-8551, Japan. kazu@geo.titech.ac.jp

Nature
|May 1, 2004
PubMed
概括

太阳前的酸盐粒,早于我们的太阳系,在原始的石中被发现. 它们的丰富性表明,在太阳系早期,酸盐是常见的,但很可能被热量破坏了.

科学领域:

  • 太空化学 太空化学
  • 行星科学 行星科学
  • 天文学 天文学

背景情况:

  • 原始的体石含有太阳前颗粒,这些颗粒是我们太阳系形成前的遗留物.
  • 预计在原行星盘中酸盐是主导的固体,但在氏体中没有发现前极酸盐.

研究的目的:

  • 报告在原始碳状地质中发现的前太阳性酸盐颗粒的现场发现.
  • 为了研究这些前极性酸盐的起源和丰富性.

主要方法:

  • 在石矩阵内对前极酸盐颗粒 (0.1-1微米) 的现场分析.
  • 在发现的颗粒中对氧和的同位素分析.

主要成果:

  • 在两个原始的碳酸中发现了前极酸盐颗粒.
  • 颗粒显示高17O丰富度 (delta17O(SMOW) >100-400每千) 和太阳能同位素组成.
  • 估计的丰度为每百万分之3-30个部分,高于其他太阳前颗粒,但低于行星间尘埃颗粒.

结论:

  • 太阳前酸盐可能起源于富含氧气的红巨星或非对称巨星分支恒星.
  • 与行星间尘埃颗粒相比,石的丰度较低,这表明在太阳星云中的高温处理过程中酸盐的破坏.

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