相关实验视频
Updated: Jul 7, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
紫外线成像光谱显示了一个活跃的土星系统
Larry W Esposito1, Joshua E Colwell, Kristopher Larsen
1University of Colorado, Laboratory for Atmospheric and Space Physics, 234 Innovation Drive, Boulder, CO 80303-7814, USA. larry.esposito@lasp.colorado.edu
概括
土星 土星 土星 土星
科学领域:
- 行星科学 行星科学
- 空间物理 空间物理
- 天体化学是天体化学.
背景情况:
- 土星系统表现出影响其大气组成和环结构的动态过程.
- 了解这些过程是解读气体巨星及其环境演变的关键.
研究的目的:
- 为了研究中性氧气,极光活动和土星系内的水冰分布的变化.
- 为了确定菲比的起源和土星环的进化历史.
主要方法:
- 对有关中性氧气丰度的观测数据的分析.
- 土星的极光与木星的极光的光谱比较.
- 对菲比星和土星环中的水冰含量变化的评估.
主要成果:
- 在土星系中,中性氧呈现出可变性,其峰值丰富度为4 x 10 (34) 个原子.
- 土星的极光响应太阳风的强迫,并与木星的光谱相似.
- 菲比的表面表现出可变的水冰含量,这表明它起源于外太阳系.
- 土星的环在水的丰富性上显示了辐射变化,A环中最纯的冰.
结论:
- 观测到的土星环的辐射变化支持初始纯度的模型,随后是石轰炸.
- 较小的辐射结构表明,土星环最近在过去的10~7~10~8年内发生了更新事件.
- 菲比的组成指向了太阳系外层的形成,有助于我们了解行星天体的起源.
相关概念视频
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.
Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview
Ultraviolet–visible (UV–visible or UV–Vis) spectroscopy is an analytical technique that investigates the interaction between matter and UV–Vis light within the electromagnetic spectrum. This method is widely used for its versatility, simplicity, and relatively quick data acquisition, making it valuable for both qualitative and quantitative analysis. When UV–Vis radiation passes through a material, molecules absorb light depending on the energy required for electronic transitions. As a result...
UV–Vis Spectrum
When light passes through a substance, a portion of the light is absorbed while the remaining light is reflected or transmitted. If the molecule absorbs light between the wavelengths of 180–400 nm range, the UV spectrum is obtained, and if it absorbs light in the 400–780 nm wavelength range, the visible spectrum is obtained.
The UV–Vis spectrum of a molecule is the plot of its absorbance versus wavelength. The plot is drawn by taking molar absorptivity (ε) or log ε on the y-axis (ordinate)...
The UV–Vis spectrum of a molecule is the plot of its absorbance versus wavelength. The plot is drawn by taking molar absorptivity (ε) or log ε on the y-axis (ordinate)...
IR Spectrum
When infrared (IR) radiation passes through a molecule, the bonds stretch or bend by absorbing the radiation. This absorption creates the molecule's absorption spectrum, which is the plot of its percentage transmittance versus wavenumber.
Transmittance is defined as the ratio of the radiant power passing through a sample to that from the radiation's source. Multiplying the transmittance by 100 gives the percent transmittance (%T), which varies between 100% (no absorption) and 0% (complete...
Transmittance is defined as the ratio of the radiant power passing through a sample to that from the radiation's source. Multiplying the transmittance by 100 gives the percent transmittance (%T), which varies between 100% (no absorption) and 0% (complete...
UV–Vis Spectroscopy of Conjugated Systems
Organic compounds with conjugated double bonds show strong absorption features in the UV–visible region of the electromagnetic spectrum attributed to π → π* electronic excitations. Generally, a UV–vis absorption spectrum is recorded as a plot of absorbance vs wavelength. The wavelength of maximum absorbance, which manifests as a peak in the absorption spectrum, is denoted as λmax.
One of the factors influencing λmax is the extent of conjugation in the...
One of the factors influencing λmax is the extent of conjugation in the...
UV–Vis Spectroscopy: Molecular Electronic Transitions
In Ultraviolet–Visible (UV–Vis) spectroscopy, the absorption of electromagnetic radiation is used to probe the electronic structure of molecules. This technique provides insights into molecular electronic transitions, particularly the movement of electrons between different molecular orbitals. Radiation is absorbed if the energy of the electromagnetic radiation passing through the molecule is precisely equal to the energy difference between the excited and ground states. During this process,...

