长时间的核心形成和原行星的快速积聚
T S Kruijer1, M Touboul2, M Fischer-Gödde3
1Institut für Planetologie, Westfälische Wilhelms-Universität Münster, Wilhelm-Klemm-Strasse 10, DE-48149 Münster, Germany. ETH Zürich, Inst. of Geochemistry and Petrology, Clausiusstrasse 25, CH-8092 Zürich, Switzerland.
早期的太阳系过程塑造了石母体. -182的变化揭示了核心形成需要100万年左右的时间,这表明尽管存在挥发性差异,但并发积累.
科学领域:
- 行星科学 行星科学
- 太空化学 太空化学
- 太阳系早期的进化过程
背景情况:
- 石母体中的核心形成是理解原行星积聚和分化的关键.
- 太阳原行星盘的过程是行星形成的基础.
研究的目的:
- 研究石母体中核心形成的时间和过程.
- 了解核心形成时间对挥发性内容变化的影响.
主要方法:
- 分析了五个岩铁石群中的-182 ((182) W) 变化.
- 使用已灭绝的 hafnium-182 ((182) Hf) 的衰变作为计时器.
主要成果:
- 观察到的182W变化为每百万分之5至20的变化表明核形成延长了约100万年.
- 证据表明Fe-FeS的早期分离,随后在核心形成过程中分离了Fe融.
- 铁石母体可能同时积累,大约在含丰富含量 (CAI) 后的0.1到030万年.
结论:
- 石母体中的核心形成是一个漫长的过程,而不是瞬间的.
- 挥发性含量变化不是由于不同的积累时间,而是由于局部星云过程.
- 这项研究完善了我们对早期太阳系动力学和小行星形成的理解.
更多相关视频
09:44Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
Published on: June 5, 2014
11:50Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions
Published on: June 13, 2015
相关概念视频
Acceleration due to Gravity on Other Planets
Astronomical observations are thus used to measure the acceleration due to gravity on other planets. This can be determined by observing the effect of a planet's gravity on objects close to it. The crucial factor that helps in this...
Kepler's First Law of Planetary Motion
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
Precipitate Formation and Particle Size Control
The obtained precipitate should be either a pure substance of known composition or easily converted to one by a simple process, such as ignition or drying. In addition, the precipitate should be insoluble and easily filterable. In general, filterability...
Kepler's Second Law of Planetary Motion
While in an elliptical orbit, the total energy of the planet is conserved. Therefore, the planet slows down when it is at apogee and...
Kepler's Third Law of Planetary Motion
Conditions on Early Earth
