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関連する概念動画

Eccentricity of an Ellipse01:27

Eccentricity of an Ellipse

An ellipse is a fundamental conic section defined by the constant sum of distances from any point on its curve to two fixed points, known as the foci. This geometric property can be physically demonstrated using a pencil, string, and two pins. By anchoring the string at both ends and maintaining it taut with a pencil, one can trace the outline of an ellipse.The shape and extent of the ellipse are determined by its eccentricity, e, defined as the ratio of the distance between the center and a...
Kepler's First Law of Planetary Motion01:10

Kepler's First Law of Planetary Motion

In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. He formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe.
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
Maximum Size of Aggregate01:12

Maximum Size of Aggregate

The maximum size of aggregate is defined as the aperture of the sieve retaining 15 percent or more of the particles present in the aggregate sample. The aggregate's maximum size impacts the concrete's water requirement, workability, and strength. Larger aggregates reduce the surface area needing cement paste coverage, which can lower water needs, thereby allowing a decrease in the water-to-cement ratio when the desired workability and richness of the mix are to be maintained, which can result...
Ellipses01:30

Ellipses

An ellipse is formed when a right circular cone is intersected by an inclined plane that does not cut through its base. This intersection yields a closed, symmetric curve characterized by distinctive geometric properties. Most notably, an ellipse is defined as the collection of all points in a plane for which the combined distances to two fixed points—called the foci—remain constant.The ellipse features two principal axes: the major and the minor axes. The major axis is the longest diameter,...
Hyperbolas01:30

Hyperbolas

A hyperbola is a conic section produced when a double-napped cone is intersected by a plane at an angle steeper than the slope of the cone, such that it cuts through both nappes. This intersection yields two separate, mirror-image curves known as branches, which open away from each other along the transverse axis. The nearest points on each branch to the hyperbola’s center are termed vertices, and the distance from the center to a vertex is denoted by a. Perpendicular to the transverse axis is...
Conformations of Ethane and Propane02:18

Conformations of Ethane and Propane

In an organic molecule, free rotation about the carbon-carbon single bond results in energetically different conformers of the molecule. Due to this rotation, called the internal rotation, ethane has two major conformations — staggered and eclipsed.
Staggered conformation is a low energy and more stable conformation with the C-H bonds on the front carbon placed at 60°dihedral angles relative to the C-H bonds on the back carbon, leading to a reduced torsional strain. In staggered ethane, the...

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関連する実験動画

Updated: Jul 11, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

ヘクトル:最も大きな高度に伸びた小惑星.

W K Hartmann, D P Cruikshank

    Science (New York, N.Y.)
    |February 29, 1980
    PubMed
    まとめ

    新しい観測により,トロイの小惑星624 (ヘクター) が発見された.

    科学分野:

    • 天文学と天体物理学について
    • 惑星科学は惑星科学である.

    背景:

    • 小惑星624 (ヘクター) はトロイの木馬類の小惑星である.
    • その回転光の曲線は高振幅を示し,異常な特徴を示唆しています.

    研究 の 目的:

    • ヘクターの回転光の曲線の高振幅の原因を調査するために.
    • 小惑星624の物理的特徴と形成仮説を評価するために,ヘクター.

    主な方法:

    • 1979年4月に得られた小惑星624 (ヘクター) の新しい観測データの分析.
    • オブジェクトの形状と表面特性を推論するために,回転光線曲線データの解釈.

    主要な成果:

    • ヘクターの回転光線曲線の高い振幅は,その伸びた形状に起因する.
    • 観測により,光の曲線の振幅の主な原因としてアルベドの変動は排除されています.

    結論:

    • 小惑星624のヘクターは,かなり伸びた形をしている.
    • この発見は,ヘクターが2つの同じサイズのトロイの木馬の衝突によって形成された複合小惑星であるという仮説を支持し,惑星の増殖の洞察を提供している.

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