在早期太阳系中,Hf-W同位素证实了快速积聚和分化
1Department of Geological Sciences, University of Michigan, Ann Arbor, MI 48109-1063 USA.
概括
内部太阳系的物体在几百万年内迅速增加和分化. 来自石的同位素数据揭示了太阳系早期的快速母体形成和金属分离.
科学领域:
- 行星科学 行星科学
- 太空化学 太空化学
- 地质时间学 (Geochronology)
背景情况:
- 由于石同位素系统受到干扰,太阳系内部天体的积聚和分化的时间表仍然不确定.
- 哈夫尼-182 (182Hf) 衰变为-182 (182W) 提供了一种有价值的计时器,因为这两种元素的耐火性和不移性.
研究的目的:
- 为了确定早期太阳系物体的积累和分化时间尺度.
- 使用182Hf-182W同位素系统进行精确的时间测量.
主要方法:
- 分析各种类型的石中的同位素组成,包括IIA,IIIA,IVA,异常铁石和H,L和LL石.
- 用182Hf-182W衰变系统作为计时器的应用.
主要成果:
- 的同位素数据表明,研究石的母体迅速增加.
- 有证据表明,金属分离发生在太阳系形成的头几百万年内.
结论:
- 早期的太阳系经历了快速的形成和分化过程.
- 182Hf-182W系统是确定太阳系早期事件日期的强大工具.
相关概念视频
Speciation Rates
Speciation can proceed at markedly different rates, and evolutionary biologists commonly describe these differences through the models of gradualism and punctuated equilibrium. Both patterns explain how new species arise, but they differ in the tempo and continuity of evolutionary change. In both cases, evolutionary change arises from heritable variation within populations, with natural selection often shaping traits that improve survival and reproduction under specific environmental conditions.
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.
What is Evolutionary History?
Scientists record evolutionary history by analyzing fossil, morphological, and genetic data. The fossil record documents the history of life on Earth and provides evidence for evolution. However, both fossil and living organisms offer evidence that outlines Earth’s evolutionary history.Phylogenetic trees illustrate the evolutionary relationships among these organisms. Scientists infer organisms’ common ancestry by evaluating shared morphological and genetic characteristics. Together, the fossil...
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 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.
High-Resolution Mass Spectrometry (HRMS)
The resolution of a mass spectrometer depends on the efficiency of separating ions with different ion masses. The mass of an atom is approximated to the sum of the masses of protons and neutrons inside, considering the masses of protons and neutrons as equal. However, the masses of the proton (1.6726 × 10−24 g) and neutron (1.6749 × 10−24 g) are not truly equal. There is a minor error in the expression of atomic masses relative to the simplest atom of hydrogen. For example, the mass of helium...


