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関連する概念動画

Geoid and Ellipsoid01:28

Geoid and Ellipsoid

The Earth's shape is best described as an ellipsoid, a slightly flattened sphere created by rotating an ellipse around its minor axis. This flattening results in the polar axis being about 21 kilometers shorter than the equatorial axis. In contrast, the geoid represents the Earth's gravitational shape and aligns with the mean sea level (MSL). The geoid is an irregular equipotential surface where gravity is perpendicular at every point. Variations in Earth's mass distribution cause geoid...
Trigonometric Substitution01:23

Trigonometric Substitution

Trigonometric substitution is a technique used to simplify integrals that contain square root expressions involving quadratic forms. It is particularly effective when the integrand includes terms resembling those found in standard geometric equations, such as circles or ellipses.Molniya satellites follow highly elliptical orbits, repeatedly sweeping out the same regions of space as they revolve around Earth. To estimate the area enclosed by such an orbit, the path is modeled as an ellipse...
Application of Linearization and Approximation01:29

Application of Linearization and Approximation

A drone flying through complex terrain often relies on more than one sensing method to estimate small changes in altitude. Along with direct measurements, air pressure provides a useful indirect indicator of vertical movement. Atmospheric pressure decreases as altitude increases, and this relationship is commonly described using an exponential model. Although accurate, converting pressure measurements into altitude values requires calculations that are too complex to perform repeatedly during...
Influence of Earth's Curvature and Atmospheric Refraction on Leveling01:26

Influence of Earth's Curvature and Atmospheric Refraction on Leveling

During leveling, the Earth's curvature and atmospheric refraction introduce deviations in the line of sight from a true horizontal reference. When the line of sight is leveled, it remains perpendicular to the plumb line only at a single point. Beyond this, it deviates due to the Earth’s curvature, represented by the correction C. For a sight distance D, the deviation can be derived using the relationship:This relationship shows that the deviation increases quadratically with distance. Over a...
Circular Orbits and Critical Velocity for Satellites01:16

Circular Orbits and Critical Velocity for Satellites

The Moon orbits around the Earth. In turn, the Earth (and other planets) orbit the Sun. The space directly above our atmosphere is filled with artificial satellites in orbit. One can examine the circular orbit, the simplest kind of orbit, to understand the relationship between the speed and the period of planets and satellites with respect to their positions and the bodies that they orbit.
Nicolaus Copernicus (1473-1543) first suggested that the Earth and all other planets orbit the Sun in...
Simple Harmonic Motion and Uniform Circular Motion01:42

Simple Harmonic Motion and Uniform Circular Motion

While simple harmonic motion and uniform circular motion may be two separate concepts, they correlate and interlink with each other. Simple harmonic motion is an oscillatory motion in a system where the net force can be described by Hooke's law, while uniform circular motion is the motion of an object in a circular path at constant speed.
There is an easy way to produce simple harmonic motion by using uniform circular motion. For instance, consider a ball attached to a uniformly rotating...

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関連する実験動画

Updated: Jul 12, 2026

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
06:14

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

アポロ・レーザー高度計による月の形状.

W L Sjogren, W R Wollenhaupt

    Science (New York, N.Y.)
    |January 19, 1973
    PubMed
    まとめ

    アポロミッションは月面の高さを正確に測定し,月面の近側と遠側との大きな違いを明らかにした. 組み合わせたデータは,月が月であることを示しています.

    科学分野:

    • 月面地質学と地球物理学
    • 惑星科学は惑星科学である.
    • ジオデシ (Geodesy) とは

    背景:

    • 正確な月の地形は,惑星の進化を理解するために不可欠です.
    • 以前の月の高さデータには,精度と範囲の制限がありました.

    研究 の 目的:

    • レーザー高度測定を用いて月面上の高さ差を正確に測定する.
    • 月の形状と内部構造のモデルを精査する.

    主な方法:

    • アポロ15号とアポロ16号からのレーザー高度計データを活用した.
    • 高度測定結果を,既存の月面地図データと比較した.
    • 月の重力場と質量中心をモデル化するために不一致を分析した.

    主要な成果:

    • 月球半球の高度差異を明らかにした.
    • マレ・ヌビウムとマレ・トランキリタティスにおける地域的な標高変動を特定した.
    • 半径1737.7kmの月の最適な球形モデルを確立しました.
    • 質量の中心から地球へ向けて2km,東へ向けて1kmの偏移を決定した.

    結論:

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    Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

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    関連する実験動画

    Last Updated: Jul 12, 2026

    Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
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    Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

    Published on: July 30, 2020

    Shaping the Amplitude and Phase of Laser Beams by Using a Phase-only Spatial Light Modulator
    08:39

    Shaping the Amplitude and Phase of Laser Beams by Using a Phase-only Spatial Light Modulator

    Published on: January 28, 2019

    Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
    06:48

    Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

    Published on: May 10, 2020

    • 月は,近辺と遠辺の間のトポグラフィック・アシンメトリが顕著である.
    • レーザー高度計は,月面のマッピングに前例のない精度を提供します.
    • 月の質量の中心は,その幾何学的中心から偏移しており,内部密度の変化を示しています.