関連する実験動画
Updated: Jul 8, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
まとめ
ヴィーナス (Venus) ヴィーナス (Venus) ヴィーナス (Venus) ヴィーナス (Venus) ヴィーナス (Venus) ヴィーナス (Venus) ヴィーナス (Venus) とは
科学分野:
- 惑星科学は惑星科学である.
- 地質学 地質学 地質学
- 大気科学 大気科学
背景:
- 金星の表面は,可視光では暗い,無色な外観を示しています.
- 厚い金星の大気は,発生する放射線にオレンジ色を与える.
研究 の 目的:
- 金星の玄武岩表面の多スペクトル画像を分析するために.
- 金星の表面の鉱物学的組成を決定するために.
- 金星の表面材料の酸化状態を調査するために.
主な方法:
- ベネラ13号からの多スペクトル画像の処理.
- 大気中の光の散乱と吸収を補正する.
- 高温下における玄武岩物質の反射スペクトルの実験室分析.
- ヴェネラ13号の観測データとヴェネラ9号と10号の観測データとの比較.
主要な成果:
- 金星の表面は暗く見られ,大気修正後の可視波長で有意な色が欠けています.
- 実験室のスペクトルは,地表鉱物には鉄酸または鉄状鉄が含まれていることを示唆しています.
- 近くの場所での高い近赤外線反射は,鉄鉱物の存在を示しています.
結論:
- 金星の玄武岩表面は,鉄を含有する鉱物集合体と一致しています.
- 証拠によると,金星の表面の物質は,特にヴェネラ9号と10号の場所では,比較的酸化している可能性があります.
関連する概念動画
Emission Spectra
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Metallic Solids
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All metallic solids exhibit high thermal and electrical conductivity, metallic luster, and malleability. Many...
All metallic solids exhibit high thermal and electrical conductivity, metallic luster, and malleability. Many...
Colors and Magnetism
Color in Coordination Complexes
When atoms or molecules absorb light at the proper frequency, their electrons are excited to higher-energy orbitals. For many main group atoms and molecules, the absorbed photons are in the ultraviolet range of the electromagnetic spectrum, which cannot be detected by the human eye. For coordination compounds, the energy difference between the d orbitals often allows photons in the visible range to be absorbed and emitted, which is seen as colors by the human eye.
When atoms or molecules absorb light at the proper frequency, their electrons are excited to higher-energy orbitals. For many main group atoms and molecules, the absorbed photons are in the ultraviolet range of the electromagnetic spectrum, which cannot be detected by the human eye. For coordination compounds, the energy difference between the d orbitals often allows photons in the visible range to be absorbed and emitted, which is seen as colors by the human eye.
Hückel's Rule Diagram of π MOs: Frost Circle
The Frost circle or the inscribed polygon method is a graphical method for determining the relative energies of π molecular orbitals (MOs) for planar, fully conjugated, and monocyclic compounds. This method was first described by A. A. Frost and Boris Musulin in 1953.
A Frost circle is constructed by drawing a polygon whose number of edges is equal to the number of carbons of the given cyclic system, with one of the vertices pointing down. Then, a circle is drawn enclosing the polygon so that...
A Frost circle is constructed by drawing a polygon whose number of edges is equal to the number of carbons of the given cyclic system, with one of the vertices pointing down. Then, a circle is drawn enclosing the polygon so that...
Flame Photometry: Overview
Flame photometry, also known as flame emission spectrometry, is a technique used for the qualitative and quantitative analysis of elements present in a sample using a flame as the source of excitation energy. The concept of flame photometry was realized in the early 1860s by Kirchhoff and Bunsen, who discovered that specific elements emit characteristic radiation when excited in flames. The first instrument developed for this purpose was used to measure sodium (Na) in plant ash using a Bunsen...
Flame Photometry: Lab
In a flame photometer, when a solution like potassium chloride is aspirated into the flame, the solvent evaporates, leaving behind dehydrated salt. This salt dissociates into free gaseous atoms in their ground state. Some of these atoms absorb energy from the flame, leading to their excitation. The excited atoms return to the ground state, emitting photons at characteristic wavelengths. Because only electronic transitions are involved, the resulting emission lines are very narrow. The intensity...

