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相关概念视频

Alkali Metals03:06

Alkali Metals

18.0K
Group 1 elements are soft and shiny metallic solids. They are malleable, ductile, and good conductors of heat and electricity. The melting points of the alkali metals are unusually low for metals and decrease going down the group, while the density increases going down the group with the exception of potassium (Table 1).
Table 1: Properties of the alkali metals
18.0K
Radioactivity and Nuclear Equations03:18

Radioactivity and Nuclear Equations

18.3K
Nuclear chemistry is the study of reactions that involve changes in nuclear structure. The nucleus of an atom is composed of protons and, except for hydrogen, neutrons. The number of protons in the nucleus is called the atomic number (Z) of the element, and the sum of the number of protons and the number of neutrons is the mass number (A). Atoms with the same atomic number but different mass numbers are isotopes of the same element.
A nuclide of an element has a specific number of protons and...
18.3K
Nuclear Stability03:18

Nuclear Stability

20.5K
Protons and neutrons, collectively called nucleons, are packed together tightly in a nucleus. With a radius of about 10−15 meters, a nucleus is quite small compared to the radius of the entire atom, which is about 10−10 meters. Nuclei are extremely dense compared to bulk matter, averaging 1.8 × 1014 grams per cubic centimeter. If the earth’s density were equal to the average nuclear density, the earth’s radius would be only about 200 meters.
To hold positively...
20.5K
Radioactive Decay and Radiometric Dating02:48

Radioactive Decay and Radiometric Dating

34.6K
Radioactivity is a spontaneous disintegration of an unstable nuclide and is a random process, as all the nuclei in the sample do not decay simultaneously. The number of disintegrations per unit time is called the activity (A), which is directly proportional to the number of nuclei in the sample. The decay constant (λ) is an average probability of decay per nucleus in unit time.
34.6K
Nuclear Fission02:50

Nuclear Fission

9.5K
Many heavier elements with smaller binding energies per nucleon can decompose into more stable elements that have intermediate mass numbers and larger binding energies per nucleon—that is, mass numbers and binding energies per nucleon that are closer to the “peak” of the binding energy graph near 56. Sometimes neutrons are also produced. This decomposition of a large nucleus into smaller pieces is called fission. The breaking is rather random with the formation of a large...
9.5K
Nuclear Power02:36

Nuclear Power

7.5K
Controlled nuclear fission reactions are used to generate electricity. Any nuclear reactor that produces power via the fission of uranium or plutonium by bombardment with neutrons has six components: nuclear fuel consisting of fissionable material, a nuclear moderator, a neutron source, control rods, reactor coolant, and a shield and containment system.
Nuclear Fuels
Nuclear fuel consists of a fissile isotope, such as uranium-235, which must be present in sufficient quantity to provide a...
7.5K

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相关实验视频

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Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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实验证据表明,是行星核心中大量的放射性热源.

V Rama Murthy1, Wim van Westrenen, Yingwei Fei

  • 1Department of Geology and Geophysics, University of Minnesota, Minneapolis, Minnesota 55455, USA. vrmurthy@umn.edu

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|May 9, 2003
PubMed
概括
此摘要是机器生成的。

-40 (40K) 可以成为行星核心的重要热源. 新的实验表明,溶于硫化铁溶液中,解决了过去的模两可,并支持其在地球和火星核心热量中的作用.

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Laser-heating and Radiance Spectrometry for the Study of Nuclear Materials in Conditions Simulating a Nuclear Power Plant Accident
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A Novel Technique for Raman Analysis of Highly Radioactive Samples Using Any Standard Micro-Raman Spectrometer
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Laser-heating and Radiance Spectrometry for the Study of Nuclear Materials in Conditions Simulating a Nuclear Power Plant Accident
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科学领域:

  • 地质化学 地质化学
  • 地质物理学 地质物理学
  • 行星科学 行星科学

背景情况:

  • 几十年来,-40 (40K) 作为行星核心中的放射性热源的作用一直在争论中.
  • 之前关于在铁合金中的溶解性的实验证据是模两可的和矛盾的.

研究的目的:

  • 提供实验证据,澄清在核心条件下的富铁合金中的溶解性.
  • 评估40K作为地球和火星核心中的放射性热源的重要性.

主要方法:

  • 进行了高压和高温实验.
  • 分析的重点是在硫化铁溶液中的溶解性.

主要成果:

  • 硫化铁融中的溶性强烈依赖温度.
  • 之前的研究中,实验和分析方面的困难被认为是模两可的原因.

结论:

  • -40 (40K) 可以在包括地球和火星在内的陆地行星的核心中充当大量的热源.
  • 这一发现对理解行星热演变和核心动态具有重大意义.