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X-ray Crystallography02:18

X-ray Crystallography

The size of the unit cell and the arrangement of atoms in a crystal may be determined from measurements of the diffraction of X-rays by the crystal, termed X-ray crystallography.
Diffraction
Diffraction is the change in the direction of travel experienced by an electromagnetic wave when it encounters a physical barrier whose dimensions are comparable to those of the wavelength of the light. X-rays are electromagnetic radiation with wavelengths about as long as the distance between neighboring...
Energy of a Satellite in a Circular Orbit01:11

Energy of a Satellite in a Circular Orbit

Thousands of artificial satellites orbit the Earth every day at various distances from the Earth. Satellites that orbit the Earth below an altitude of 1,600 km are considered to be orbiting in low-Earth orbit (LEO). Research satellites and Earth observation satellites are usually placed in LEO, and mostly orbit the Earth in elliptical orbits. Navigation satellites are placed in medium-Earth orbit (MEO), ranging from 2,000 km to 36,000 km from the surface of the Earth. Meanwhile, communication...
Impact: Problem Solving01:26

Impact: Problem Solving

In an experiment conducted during a Mars mission, a rover propels a projectile with an initial velocity, and the projectile rebounds after colliding with the Martian surface. To ascertain the maximum height attained by the projectile after this collision, the known restitution coefficient and acceleration due to gravity are employed.
By designating the launch point as the origin and utilizing kinematic equations, the vertical component of the projectile's velocity at the point of impact is...
Minerals01:26

Minerals

Minerals are essential nutrients that the human body needs in small amounts to work properly. They play a vital role in many bodily functions, such as building strong bones and transmitting nerve impulses. Some minerals are needed for hormone production or to maintain a normal heartbeat. Major minerals include calcium, phosphorus, potassium, sulfur, sodium, chlorine, and magnesium, while trace minerals include iron, manganese, copper, iodine, zinc, cobalt, fluoride, and selenium.
Types of Building Stone01:30

Types of Building Stone

Building stones, essential materials for construction, are extracted from natural rock deposits and processed into specific forms and dimensions suitable for various building applications. These stones are broadly classified into three types based on their geological formation: igneous, sedimentary, and metamorphic.
Igneous rocks are formed from the solidification of magma or lava. An example is granite, known for its durability and resistance to weathering, making it ideal for parts of...
Quarrying of Stone01:15

Quarrying of Stone

Quarrying is the process of extracting stone from a quarry, where specialized techniques are employed to remove large blocks of stone safely and efficiently. This process can involve controlled explosions or more precision-oriented methods such as cutting and drilling.
One common method involves using a diamond belt saw to cut large blocks from the quarry face. These blocks can be about 50 feet long and 12 feet high. After the initial vertical cut, drilling is performed at the base of the block.

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Updated: Jul 5, 2026

Synchrotron X-ray Microdiffraction and Fluorescence Imaging of Mineral and Rock Samples
10:12

Synchrotron X-ray Microdiffraction and Fluorescence Imaging of Mineral and Rock Samples

Published on: June 19, 2018

NASAは彗星から岩を回収した.

Don S Burnett1

  • 1Department of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA. burnett@gps.caltech.edu

Science (New York, N.Y.)
|December 16, 2006
PubMed
まとめ
この要約は機械生成です。

スターダストミッションは彗星粒子,主に太陽系からのシリケート物質を帰還した. これらの粒子は太陽の近くで形成され,後に彗星を組み込む前にカイパーベルトに移動しました.

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Synchrotron X-ray Microdiffraction and Fluorescence Imaging of Mineral and Rock Samples
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科学分野:

  • 宇宙塵分析 コスミックダスト分析
  • 惑星科学は惑星科学である.
  • 太陽系形成 太陽系形成について

背景:

  • 彗星粒子は,太陽系の初期状態についての洞察を提供します.
  • スターダストミッションは,彗星ワイルド2から原始サンプルを採取した.
  • 彗星の組成を理解することは,太陽系の歴史を再構築するのに役立ちます.

研究 の 目的:

  • 星の塵彗星サンプルの鉱物学と起源を特徴付けるために.
  • 彗星塵の粒子の熱史と輸送経路を調査する.
  • 太陽系物質と彗星体の関係を決定する.

主な方法:

  • 高度な顕微鏡とスペクトロスコピーを用いて帰還した彗星粒子の分析.
  • シリケート粒子の同位体および元素組成分析.
  • 太陽系初期における粒子の形成と運搬のモデリング.

主要な成果:

  • 彗星の粒子は,主に太陽系起源のシリケート物質である.
  • 証拠によると,太陽に近い高温でいくつかの粒子が形成されたという.
  • これらの高温粒子は,カイパーベルト地域を含む太陽系の外側へと運ばれた.

結論:

  • 彗星には,様々な太陽の中心距離で形成された物質の混合物が含まれる.
  • 星塵のサンプルは,太陽系内の物質輸送の直接的な証拠を提供します.
  • 彗星の塵の構成は,形成と移動の複雑な歴史を反映しています.