相关实验视频
Updated: Jul 19, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
太阳星云异质性在p过程中的萨马和新同位素
Rasmus Andreasen1, Mukul Sharma
1Radiogenic Isotope Geochemistry Laboratory, Department of Earth Sciences, Dartmouth College, 6105 Sherman Fairchild Hall, Hanover, NH 03755, USA.
概括
碳状地石显示出萨马-144 (144Sm) 的缺陷,这表明它在早期太阳星云中分布异质. 这表明p过程和r过程元素有不同的超新星来源.
科学领域:
- 宇宙化学 宇宙化学
- 核天体物理学 核天体物理学
- 行星科学 行星科学
背景情况:
- 大量碳状地铁体呈现出显著的144Sm (约. 100 ppm) 与其他石和地面标准相比.
- 这个赤字与142Nd/144Nd比率大约下降有关. 在这些石中11ppm.
研究的目的:
- 为了研究碳酸中萨马 (Sm) 和 (Nd) 的同位素异常.
- 确定来自早期太阳星云中不同核合成过程的Sm和Nd同位素的分布模式.
主要方法:
- 在散装碳状地中对和的同位素分析.
- 同位素比率与陆地和其他石标准的比较.
- 基于核合成起源的同位素异质性的建模 (p-过程,r-过程,s-过程).
主要成果:
- 在碳状地石中证实了144Sm的显著赤字和142Nd/144Nd比率的相应下降.
- 超新星中p过程产生的同位素在太阳星云中分布异质.
- 通过r过程 (超新星) 和s过程 (红巨星) 生产的同位素被发现分布均.
结论:
- 对于这些核素来说,p过程中Sm和Nd同位素的异质分布意味着不同的或弱连接的超新星源.
- r-过程和s-过程同位素的均分布表明,这些元素从各自的来源中混合得更均.
- 这种同位素证据限制了负责早期太阳星云元素组成的天体物理地点和混合过程.
更多相关视频
相关概念视频
Atomic Emission Spectroscopy: Overview
Atomic emission spectroscopy (AES) is an analytical technique used to determine the elemental composition of a sample by analyzing the light emitted from excited atoms. In AES, atoms in a sample are excited to higher energy levels by thermal energy from high-temperature sources, such as plasma, arcs, or sparks. When these excited atoms return to lower energy states, they emit light at specific wavelengths characteristic of each element. The resulting atomic emission spectrum, which consists of...
Atomic Nuclei: Nuclear Spin State Population Distribution
Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
Atomic Emission Spectroscopy: Lab
AES is a powerful analytical technique, especially effective when used with plasma sources, producing abundant spectra in characteristic emission lines. The Inductively Coupled Plasma (ICP), in particular, yields superior quantitative analytical data due to its high stability, low noise, low background, and minimal interferences under optimal experimental conditions. However, newer air-operated microwave sources are emerging as promising alternatives that could be more cost-effective than...
Other Nuclides: 31P, 19F, 15N NMR
Many organic, inorganic, and biological molecules contain spin-half nuclei such as nitrogen-15, fluorine-19, and phosphorus-31. As a result, NMR studies of these nuclei have found extensive applications in chemical and biological research.
While fluorine-19 and phosphorous-31 have high natural abundances (100%) and positive gyromagnetic ratios, nitrogen-15 has a low natural abundance and a negative gyromagnetic ratio. However, nitrogen-15 is still preferred over nitrogen-14 (which has a high...
While fluorine-19 and phosphorous-31 have high natural abundances (100%) and positive gyromagnetic ratios, nitrogen-15 has a low natural abundance and a negative gyromagnetic ratio. However, nitrogen-15 is still preferred over nitrogen-14 (which has a high...
Emission Spectra
When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
Atomic Nuclei: Larmor Precession Frequency
The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession, and the angular frequency...

