関連する実験動画
Updated: Jun 18, 2026

12:39
Gold Nanostar Synthesis with a Silver Seed Mediated Growth Method
Published on: January 15, 2012
まとめ
分子酸素のヘルツバーグII帯は,金星の夜空の輝きの中で最も強いスペクトル特徴です. 実験室での実験では,酸素原子が二酸化炭素と再結合すると,金星の上層大気中にこれらの帯が生成されると示唆されています.
科学分野:
- 大気化学 大気化学
- 惑星科学は惑星科学である.
- スペクトル顕微鏡検査です.
背景:
- 金星の夜空の輝きは,複雑なスペクトル特徴を示しています.
- 分子酸素の排出量を理解することは,大気モデルにとって極めて重要です.
研究 の 目的:
- 金星の夜空の輝き (3000~8000アングストーム) の支配的なスペクトル特徴を特定する.
- 金星の上層大気圏でこれらの放射を発生させる可能性のあるメカニズムを調査する.
主な方法:
- 金星の夜空の光スペクトルの分析.
- 実験室での実験では,アフターグローを用いて大気の状態をシミュレートします.
主要な成果:
- 分子酸素のヘルツバーグII帯 (c(1) シグマ((-) u) - X(3) シグマ(-) a)) は,最も強いスペクトル特徴として特定されました.
- これらの帯は,二酸化炭素の存在下での酸素原子再結合により,実験室のアフターグローで成功裏に再現されました.
結論:
- 酸素原子と二酸化炭素の再結合が,金星の夜空の輝きにおけるヘルツバーグII放射の主なメカニズムであると仮定されています.
- この発見は,金星の有意な大気現象に対する妥当な説明を提供する.
関連する概念動画
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.
Rocket Propulsion in Empty Space - I
The driving force for the motion of any vehicle is friction, but in the case of rocket propulsion in space, the friction force is not present. The motion of a rocket changes its velocity (and hence its momentum) by ejecting burned fuel gases, thus causing it to accelerate in the direction opposite to the velocity of the ejected fuel. In this situation, the mass and velocity of the rocket constantly change along with the total mass of ejected gases. Due to conservation of momentum, the rocket's...
Rocket Propulsion In Empty Space - II
The motion of a rocket is governed by the conservation of momentum principle. A rocket's momentum changes by the same amount (with the opposite sign) as the ejected gases. As time goes by, the rocket's mass (which includes the mass of the remaining fuel) continuously decreases, and its velocity increases. Therefore, the principle of conservation of momentum is used to explain the dynamics of a rocket's motion. The ideal rocket equation gives the change in velocity that a rocket experiences by...
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 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...
Focusing of Light in the Eye
Light rays enter the eye through the cornea, a transparent dome-shaped tissue that is the eye's outermost layer. The cornea bends or refracts, light rays traveling to the pupil. The shape of the cornea determines how much of the light is bent and whether the image will be focused correctly on the retina at the back of the eye. Once the light has passed through both refraction layers, it converges into a single focal point onto a small area. This is where photoreceptors start transforming...

