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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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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

星塵のシリケートは,原始的な隕石からのものです.

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
まとめ

太陽系以前のシリケート粒子は,原始的な隕石で発見されました. シリケートの豊富さは,太陽系の初期にシリケートが一般的であったが,熱によって破壊された可能性が高いことを示唆している.

科学分野:

  • 宇宙化学 (コスモケミストリー)
  • 惑星科学は惑星科学である.
  • 天文学 天文学

背景:

  • 原始的なコンドリート隕石には,太陽系が形成される前からの残骸であるプレソラー粒子が含まれています.
  • シリケートは,原惑星円盤における支配的な固体であると考えられているが,プレソラーシリケートは,コンドライトでは発見されていない.

研究 の 目的:

  • 原始的な炭酸コンドリートにおけるプレソラーシリケート粒子の in situ 発見について報告する.
  • これらのプレソラーシリケートの起源と豊富さを調査する.

主な方法:

  • 隕石のマトリックス内のプレソラーシリケート粒 (0.1-1ミクロム) のインシット分析.
  • 発見された粒子の酸素とシリコンの同位体分析.

主要な成果:

  • 2つの原始的な炭酸性コンドライトでプレソラーシリケート粒子の発見.
  • 穀物は,高い17O濃度 (デルタ17O (SMOW) >100-400千分) と太陽電池シリコンの同位体成分を示しています.
  • 推定豊富度は100万分の3~30個で,他のプレソラー粒よりも高く,惑星間塵粒よりも低い.

結論:

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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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Scattering And Absorption of Light in Planetary Regoliths
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Scattering And Absorption of Light in Planetary Regoliths

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Last Updated: Jun 7, 2026

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

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Published on: June 5, 2014

Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions
11:50

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

Published on: June 13, 2015

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

  • プレソラー・シリケートは,酸素に富んだ赤い巨星やアシンプトティックな巨星から発生した可能性が高い.
  • 惑星間塵の粒子と比較して隕石の濃度が低いことは,太陽星雲の高温処理でシリケートが破壊されていることを示唆している.