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相关概念视频

Reduced Mass Coordinates: Isolated Two-body Problem01:12

Reduced Mass Coordinates: Isolated Two-body Problem

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In classical mechanics, the two-body problem is one of the fundamental problems describing the motion of two interacting bodies under gravity or any other central force. When considering the motion of two bodies, one of the most important concepts is the reduced mass coordinates, a quantity that allows the two-body problem to be solved like a single-body problem. In these circumstances, it is assumed that a single body with reduced mass revolves around another body fixed in a position with an...
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Classifying Matter by Composition03:35

Classifying Matter by Composition

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Matter: Pure Substances and Mixtures
According to its composition, the matter can be classified into two broad categories — pure substances and mixtures. 
A pure substance is a form of matter that has a constant composition throughout with uniform properties. For example, any sample of sucrose has the same composition and same physical properties, such as melting point, color, and sweetness, regardless of the source from which it is isolated. 
A mixture is composed of two or...
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Atomic Orbitals02:44

Atomic Orbitals

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An atomic orbital represents the three-dimensional regions in an atom where an electron has the highest probability to reside. The radial distribution function indicates the total probability of finding an electron within the thin shell at a distance r from the nucleus. The atomic orbitals have distinct shapes which are determined by l, the angular momentum quantum number. The orbitals are often drawn with a boundary surface, enclosing densest regions of the cloud.
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Mass Spectrometry: Isotope Effect01:13

Mass Spectrometry: Isotope Effect

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Most elements exist in nature as a mixture of isotopes. The isotopes differ in weight due to their respective number of neutrons. The molecular weight of a molecule is different depending on the specific isotope of its elements involved. As a result, the mass spectrum of the molecule exhibits peaks from the same fragment at multiple positions. The positions of these mass signals depend on the mass differences between isotopes. Furthermore, the intensity of these signals is dependent on the...
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Kepler's First Law of Planetary Motion01:10

Kepler's First Law of Planetary Motion

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In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. He formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe.
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,...
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Atomic Absorption Spectroscopy: Lab01:21

Atomic Absorption Spectroscopy: Lab

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For AAS measurements, samples must be introduced as clear solutions, often requiring extensive preliminary treatment to dissolve materials like soils, animal tissues, and minerals. Common methods for sample preparation include treatment with hot mineral acids, wet ashing, combustion in closed containers, high-temperature ashing, or fusion with reagents.
 Solutions containing organic solvents, such as low-molecular-mass alcohols, esters, or ketones, enhance absorbances by increasing...
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相关实验视频

Updated: Feb 21, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

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小行星中没有异国情调的物质.

Alan E Rubin1,2, Thomas H Burbine3

  • 1Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA 90095-1567 USA.

European physical journal plus
|February 20, 2026
PubMed
概括

小行星密度通常在预期的物理极限内. 根据目前的证据,在像波利希姆尼亚这样的小行星中存在异常物质的说法,比如超重元素或暗物质,是极不可能的.

科学领域:

  • 行星科学 行星科学
  • 天体物理学 天体物理学
  • 太空化学 太空化学

背景情况:

  • 太阳系天体表现出不易挥发的元素的均丰度.
  • 小行星被分类为未化的体或由化的体祖先形成的差异化物体.
  • 基于反射光谱的小行星组成与石组成一致,石组成由酸盐和金属铁等常见材料组成.

研究的目的:

  • 批判性地评估声称小行星 (33) Polyhymnia具有异常高的密度,暗示异国情调的组成.
  • 为了评估含有超重元素 (SHEs),α物质或退化的暗物质的小行星的可能性.
  • 根据已确定的物理和化学原理,加强对小行星组成的理解.

主要方法:

  • 审查和分析已公布的小行星密度数据,包括异常值.
  • 对小行星光谱数据与已知的石组成进行比较.
  • 对理论模型的评估,建议在小行星中与观测证据和物理约束相对应的异国情调物质.

主要成果:

  • 报告的小行星 (33) Polyhymnia (75.3 ± 9.7 g cm−3) 的散装密度被认为是不现实的和非物理的.
  • 石,主要来自小行星,由非异国材料组成.
  • 来自小行星的光谱数据,包括那些被标记为"紧超密物体" (CUDO) 的数据,与其分类学类内的其他小行星没有显著差异.

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Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
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Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas

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Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
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Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

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Last Updated: Feb 21, 2026

Scattering And Absorption of Light in Planetary Regoliths
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Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

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Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
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Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas

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Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
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Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

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结论:

  • 极其不太可能Polyhymnia或其他小行星含有外来物质,如稳定的超重元素或退化的暗物质.
  • SHE和退化暗物质的存在仍然未被证明,而α物质通常只在极端的天体物理环境中发现.
  • 小行星密度受到已知的物理和石组成的约束,支持非异国情调的物质基础.