相关实验视频
Updated: Jul 12, 2026

10:35
Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
概括
研究人员分析了木星的木星.
科学领域:
- 行星科学 行星科学
- 大气物理学 大气物理学
- 红外光谱学 红外光谱学
背景情况:
- 木星的大气表现出复杂的热辐射模式.
- 了解红外不透明度对于大气分析至关重要.
- 分子是木星大气层的主要组成部分.
研究的目的:
- 为了确定木星的垂直压力-温度概况.
- 量化木星大气中的分子混合比率.
- 为了分析1640微米波段的热辐射光谱.
主要方法:
- 对木星热辐射的光谱分析.
- 使用压力扩大分子转换模型的红外不透明度.
- 从光谱数据中推导大气参数.
主要成果:
- 确定了木星大气层的垂直压力-温度概况.
- 分子混合比率计算为0.89 ± 0.11.
- 导出的混合比与公认的太阳能值保持一致.
结论:
- 压力扩展的分子过渡占据了木星的红外不透明度.
- 确定的分子丰度支持太阳系形成模型.
- 精确的气体巨星大气概况可以通过光谱分析来实现.
相关概念视频
Infrared (IR) Spectroscopy: Overview
When electromagnetic radiation passes through a material, atoms or molecules transition from a lower to a higher energy state by absorbing radiation corresponding to the energy difference between the two states. The absorption of infrared (IR) radiation causes transitions between vibrational energy levels in a molecule. Therefore, IR spectroscopy is a useful analytical tool for determining the molecular structure of molecules.
Different compounds display unique properties due to their...
Different compounds display unique properties due to their...
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.
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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...
IR Spectrometers
There are two main infrared (IR) spectrophotometers: dispersive IR spectrometers and Fourier transform infrared (FTIR) spectrometers. In a dispersive IR spectrometer, a beam of infrared radiation produced by a hot wire is divided into two parallel equal-intensity beams using mirrors. One beam passes through the sample, while another is a reference beam. The beams then move through the monochromator, which separates the radiations into a continuous spectrum of different frequencies. The...
IR Spectroscopy: Molecular Vibration Overview
When Infrared (IR) radiation passes through a covalently bonded molecule, the bonds transition from lower to higher vibrational levels. The fundamental vibrational motions that result in infrared absorption can be classified as stretching or bending vibrations.
Stretching vibrations are vibrational motions that occur along the bond line, changing the bond length or distance between two bonded atoms. They are further distinguished as symmetric or asymmetric. In symmetric stretching, the...
Stretching vibrations are vibrational motions that occur along the bond line, changing the bond length or distance between two bonded atoms. They are further distinguished as symmetric or asymmetric. In symmetric stretching, the...
IR Spectrum Peak Intensity: Amount of IR-Active Bonds
When infrared radiation is passed through a molecule, absorption occurs if the molecule's vibration leads to a substantial change in its bond dipole moment. Transitions between vibrational energy levels, typically corresponding to infrared frequencies (4000–400 cm−1), allow absorption if the vibration significantly alters the dipole moment, making the molecule infrared active. The molecular bonds have different stretching and bending vibrations, resulting in various peaks with varying...
The Electromagnetic Spectrum
Electromagnetic waves are categorized according to their wavelengths and frequencies, giving the electromagnetic spectrum. These waves are classified as radio, infrared, ultraviolet, etc. Radio waves refer to electromagnetic radiation with wavelengths ranging from millimeters to kilometers. Radio waves are commonly used for audio communications (i.e., radios) and typically result from an alternating current in the wires of a broadcast antenna. They cover a broad wavelength range and are used...

