関連する実験動画
Updated: Jul 15, 2026

11:10
Conducting Miller-Urey Experiments
Published on: January 21, 2014
隕石の中の古代のシリケート星塵の発見
1Laboratory for Space Sciences and the Physics Department, Washington University, St. Louis, MO 63130, USA. nguyen@wustl.edu
まとめ
Acfer 094隕石で発見された9つのプレソラーシリケート粒子は,進化した星についての洞察を提供します. 異常な酸素同位体とマグネシウム26濃縮は,恒星の核合成と混合プロセスに関する詳細を明らかにします.
科学分野:
- 宇宙化学 (コスモケミストリー)
- 星の天体物理学 星の天体物理学
- 惑星科学は惑星科学である.
背景:
- プレソラー粒子は,太陽が形成される前に存在した微小な塵の粒子です.
- Acfer 094のような炭酸性コンドライトは,初期の太陽系材料を保存した原始的な隕石です.
- プレソーラー粒子の同位体異常は,それらの恒星起源のヒントを提供します.
研究 の 目的:
- Acfer 094隕石からのプレソラーシリケート粒子を特定し,特徴づけること.
- 恒星の環境と,その形成に起因する核合成過程を研究する.
- これらの粒子を太陽系の初期状態と恒星の進化の探査機として利用する.
主な方法:
- プレソラー粒子の顕微鏡検査と同位体分析.
- 形成条件を決定するための酸素とマグネシウムの同位体測定.
- ミネラロジカル識別 (例えば,ピロキセン,オリビン,GEMS,Al豊富なシリケート).
主要な成果:
- 9つのプレソラーシリケート粒子がAcfer 094.から成功裏に分離されました.
- 異常な酸素同位体組成は,進化した星の形成を強く示唆している.
- 一粒の穀物は26Mg濃度の濃度が高く,26Alの放射性崩壊を示していた.
- ピロキセン,オリヴィン,GEMS,アルミニウムの豊富なシリケートを含む多様な鉱物学が観察されました.
結論:
- これらのプレソラー粒子は,初期の太陽星雲に組み込まれた進化した星からの物質の直接的な証拠を提供します.
- 同位体データは,恒星の核合成と母星内の混合プロセスに制約を与える.
- この発見は,初期の太陽系物質と恒星の進化の源として,太陽前塵の理解を深める.
関連する概念動画
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.
Elements: Chemical Symbols and Isotopes
A chemical symbol is an abbreviation used to indicate an element or an atom of an element. For example, the symbol for mercury is Hg. The same symbol is used to indicate one atom of mercury (microscopic domain) or to label a container of many atoms of the element mercury (macroscopic domain).
Some symbols are derived from the common English name of the element; others are abbreviations of the name in another language — Latin, Greek or German. For example, the symbol for aluminum (common name)...
Some symbols are derived from the common English name of the element; others are abbreviations of the name in another language — Latin, Greek or German. For example, the symbol for aluminum (common name)...
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.
Quarrying of Stone
Quarrying is the process of extracting stone from a quarry, where specialized techniques are employed to remove large blocks of stone safely and efficiently. This process can involve controlled explosions or more precision-oriented methods such as cutting and drilling.
One common method involves using a diamond belt saw to cut large blocks from the quarry face. These blocks can be about 50 feet long and 12 feet high. After the initial vertical cut, drilling is performed at the base of the block.
One common method involves using a diamond belt saw to cut large blocks from the quarry face. These blocks can be about 50 feet long and 12 feet high. After the initial vertical cut, drilling is performed at the base of the block.
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...
Origin of Photosynthesis
Photosynthesis represents a fundamental biological process that transformed Earth's atmosphere and paved the way for complex life. Emerging roughly 3.4–3.8 billion years ago, the earliest photosynthetic organisms harnessed light energy to produce organic compounds. These anoxygenic phototrophs used electron donors like hydrogen sulfide (H₂S) or ferrous iron (Fe²⁺), rather than water, and did not release molecular oxygen (O₂) as a byproduct. Various groups, including green sulfur and purple...

