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Electron Orbital Model01:18

Electron Orbital Model

Orbitals are the areas outside of the atomic nucleus where electrons are most likely to reside. They are characterized by different energy levels, shapes, and three-dimensional orientations. The location of electrons is described most generally by a shell or principal energy level, then by a subshell within each shell, and finally, by individual orbitals found within the subshells.The first shell is closest to the nucleus, and it has only one subshell with a single spherical orbital called the...
Subatomic Particles03:37

Subatomic Particles

Dalton was only partially correct about the particles that make up matter. All matter is composed of atoms, and atoms are composed of three smaller subatomic particles: protons, neutrons, and electrons. These three particles account for the mass and the charge of an atom.
Kinetic Theory of an Ideal Gas01:12

Kinetic Theory of an Ideal Gas

A mole is defined as the amount of any substance that contains as many molecules as there are atoms in exactly 12 grams of carbon-12. An Italian scientist Amedeo Avogadro (1776–1856) formed the  hypothesis that equal volumes of gas at equal pressure and temperature contain equal numbers of molecules, independent of the type of gas. Later, the hypothesis was developed to form the SI unit for measuring the amount of any substance.
The number of molecules in one mole is called Avogadro's number...
Faraday Disk Dynamo01:23

Faraday Disk Dynamo

A Faraday disk dynamo is a DC generator, producing an emf that is constant in time. It consists of a conducting disk that rotates with a constant angular velocity in the magnetic field, perpendicular to the disk's plane. The rotation of the disk causes a change in magnetic flux, which induces an emf, causing opposite charges to develop on the rim and in the center of the disk. The polarity of the induced emf can be determined by the direction of the magnetic field and the direction of the...
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...
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Vectors in Space: Problem Solving

A chandelier suspended by multiple cables can be analyzed using principles of three-dimensional static equilibrium. In this setup, a chandelier weighing 1000 N is positioned at the origin of a three-dimensional coordinate system, while three ceiling anchor points are fixed at known locations above it. Each cable connects the chandelier to one anchor point and transmits a tensile force along its length.To find out the forces in the cables, the spatial direction of each cable must first be...

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Video Experimental Relacionado

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Gold Nanostar Synthesis with a Silver Seed Mediated Growth Method
12:39

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Published on: January 15, 2012

El experimento del globo Venus de VEGA.

R Z Sagdeev, V M Linkin, J E Blamont

    Science (New York, N.Y.)
    |March 21, 1986
    PubMed
    Resumen

    Dos globos exploraron la atmósfera de Venus en 1985, midiendo los factores ambientales clave y los vientos. Estos datos de la misión VEGA proporcionaron información sobre la dinámica y las condiciones atmosféricas de Venus.

    Área de la Ciencia:

    • Ciencias planetarias Ciencias planetarias.
    • Ciencias de la atmósfera Ciencias atmosféricas.
    • La aeronomía es la aeronomía.

    Sus antecedentes:

    • Venus posee una densa atmósfera con una dinámica compleja.
    • Las exploraciones atmosféricas anteriores de Venus se basaron en datos limitados.
    • Comprender las condiciones atmosféricas de Venus es crucial para la planetología comparativa.

    Objetivo del estudio:

    • Para desplegar y operar globos instrumentados en la atmósfera de Venus.
    • Para recopilar mediciones in situ de las propiedades atmosféricas.
    • Para monitorear los patrones de viento de Venus utilizando técnicas avanzadas de seguimiento.

    Principales métodos:

    • Despliegue de dos globos instrumentados durante la misión VEGA de 1985.

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  • Detección in situ de la presión, la temperatura, la velocidad del viento, la retrodispersión de las nubes, la luz y los rayos.
  • Seguimiento de globos a través de interferometría de línea de base muy larga (VLBI) utilizando una red global de antenas de radio.
  • Principales resultados:

    • Los globos atravesaron con éxito aproximadamente el 30% de la circunferencia de Venus.
    • Recogió datos completos sobre las variables atmosféricas a una altitud de ~54 km.
    • VLBI proporcionó un seguimiento preciso para las mediciones de la velocidad del viento.

    Conclusiones:

    • El experimento del globo VEGA caracterizó con éxito los parámetros atmosféricos clave en Venus.
    • Los datos recopilados ofrecen información valiosa sobre la circulación atmosférica de Venus y su composición.
    • El experimento demostró la viabilidad de un monitoreo atmosférico de larga duración en Venus.