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関連する概念動画

Thomson's e/m Experiment01:19

Thomson's e/m Experiment

In a beam of charged particles created by a heated cathode, the particles move at different speeds. However, many applications need a beam with uniform particle speeds. An arrangement known as a velocity selector uses electric and magnetic fields to pick particles with a particular speed from the beam.
A particle with charge q, speed v, and mass m enters an area from the top, where the magnetic and electric fields are perpendicular both to the particle's motion and to one another. The magnetic...
Rocket Propulsion in Empty Space - I01:13

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 - II01:12

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...
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...
Flame Photometry: Lab01:16

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...
Azimuths and Bearings01:19

Azimuths and Bearings

Azimuths and bearings are essential concepts in surveying, providing methods to express the direction of a line relative to a meridian. Azimuths refer to the clockwise angle measured from the north end of a reference meridian to the given line, ranging from zero to 360 degrees. This method gives a comprehensive directional reference within a full 360-degree circle, making it a straightforward way to communicate direction in various fields, including navigation, cartography, and...

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関連する実験動画

Updated: Jul 12, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

フォボス:マリナー7からの予備的な結果

B A Smith

    Science (New York, N.Y.)
    |May 15, 1970
    PubMed
    まとめ

    火星の衛星であるフォボスは,以前考えられていたよりも大きく,暗く,アルベドが非常に低い. 新しい分析によると,惑星と共に形成されたのではなく,火星によって捕獲された可能性が高い.

    科学分野:

    • 惑星科学は惑星科学である.
    • 天文学 天文学
    • 太陽系研究 太陽系研究

    背景:

    • フォボス (Phobos) は火星の2つの衛星の1つである.
    • 以前のフォボスの大きさと表面特性の推定は,限られたデータに基づいていた.
    • フォボスの特徴を理解することは,火星の歴史を理解するための鍵です.

    研究 の 目的:

    • フォボスのサイズと表面特性を再評価する.
    • フォボスの起源を特定するために.

    主な方法:

    • マリナー7の特定の画像 (フレーム7F91) の分析.
    • フォボスの四肢プロフィールの画像からの測定.
    • 視覚的幾何学的アルベドの計算.

    主要な成果:

    • フォボスの四肢のプロフィールは18×22キロメートルで,以前考えられていたより大きな大きさを示しています.
    • フォボスの表面はより暗く,視覚的幾何学的なアルベドは0.065.5である.
    • このアルベドは,既知の他の太陽系天体のアルベドよりも低い.

    結論:

    さらに関連する動画

    Optimization, Test and Diagnostics of Miniaturized Hall Thrusters
    12:22

    Optimization, Test and Diagnostics of Miniaturized Hall Thrusters

    Published on: February 16, 2019

    Emission Spectroscopic Boundary Layer Investigation during Ablative Material Testing in Plasmatron
    09:41

    Emission Spectroscopic Boundary Layer Investigation during Ablative Material Testing in Plasmatron

    Published on: June 9, 2016

    関連する実験動画

    Last Updated: Jul 12, 2026

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    Optimization, Test and Diagnostics of Miniaturized Hall Thrusters
    12:22

    Optimization, Test and Diagnostics of Miniaturized Hall Thrusters

    Published on: February 16, 2019

    Emission Spectroscopic Boundary Layer Investigation during Ablative Material Testing in Plasmatron
    09:41

    Emission Spectroscopic Boundary Layer Investigation during Ablative Material Testing in Plasmatron

    Published on: June 9, 2016

    • フォボスは,以前見積もっていたよりも大きく,暗くなっています.
    • 低いアルベドと大きさは,フォボスが火星の周りにインシトゥで形成されたわけではないことを示唆しています.
    • フォボスはおそらく,火星によって後に捕らえられた.