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Nuclear Fusion02:45

Nuclear Fusion

The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

Atomic emission spectroscopy (AES) is an analytical technique used to determine the elemental composition of a sample by analyzing the light emitted from excited atoms. In AES, atoms in a sample are excited to higher energy levels by thermal energy from high-temperature sources, such as plasma, arcs, or sparks. When these excited atoms return to lower energy states, they emit light at specific wavelengths characteristic of each element. The resulting atomic emission spectrum, which consists of...
Atomic Nuclei: Nuclear Relaxation Processes01:23

Atomic Nuclei: Nuclear Relaxation Processes

In the absence of an external magnetic field, nuclear spin states are degenerate and randomly oriented. When a magnetic field is applied, the spins begin to precess and orient themselves along (lower energy) or against (higher energy) the direction of the field. At equilibrium, a slight excess population of spins exists in the lower energy state. Because the direction of the magnetic field is fixed as the z-axis,  the precessing magnetic moments are randomly oriented around the z-axis. This...
Atomic Nuclei: Magnetic Resonance01:05

Atomic Nuclei: Magnetic Resonance

The number of nuclear spins aligned in the lower energy state is slightly greater than those in the higher energy state. In the presence of an external magnetic field, as the spins precess at the Larmor frequency, the excess population results in a net magnetization oriented along the z axis. When a pulse or a short burst of radio waves at the Larmor frequency is applied along the x axis, the coupling of frequencies causes resonance and flips the nuclear spins of the excess population from the...
Emission Spectra02:39

Emission Spectra

When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
Atomic Emission Spectroscopy: Lab01:29

Atomic Emission Spectroscopy: Lab

AES is a powerful analytical technique, especially effective when used with plasma sources, producing abundant spectra in characteristic emission lines. The Inductively Coupled Plasma (ICP), in particular, yields superior quantitative analytical data due to its high stability, low noise, low background, and minimal interferences under optimal experimental conditions. However, newer air-operated microwave sources are emerging as promising alternatives that could be more cost-effective than...

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Video Experimental Relacionado

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

Supernova 1987A: Notas de todo el mundo

M M Waldrop

    Science (New York, N.Y.)
    |May 1, 1987
    PubMed
    Resumen

    La supernova 1987A en la Gran Nube de Magallanes se acerca a su brillo máximo. Los astrónomos están observando de cerca este importante evento de explosión estelar a medida que avanza hacia su eventual desvanecimiento.

    Área de la Ciencia:

    • * Astrofísica es la astrofísica.
    • * La astronomía es la ciencia.
    • * Estudios de las Supernovas.

    Sus antecedentes:

    • * La Supernova 1987A (SN 1987A) es un evento astronómico clave en la Gran Nube de Magallanes.
    • * La supernova ha alcanzado una magnitud aparente de 3.3 y se espera que siga brillando.

    Objetivo del estudio:

    • * Para documentar y analizar los desarrollos recientes en la observación en curso de la Supernova 1987A.
    • * Para seguir la progresión de SN 1987A a medida que se acerca a su luminosidad máxima.

    Principales métodos:

    • * Observación y monitoreo astronómico continuo de SN 1987A.
    • * Mediciones fotométricas para determinar la magnitud aparente y hacer un seguimiento de los cambios en el tiempo.

    Principales resultados:

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    • * SN 1987A ha alcanzado una magnitud aparente actual de 3,3.
    • * Se anticipa un mayor brillo en los próximos meses antes de que la supernova comience a desvanecerse.

    Conclusiones:

    • * Los astrónomos mantienen un gran interés en el estado de evolución de SN 1987A.
    • * La tendencia de brillo observada indica que la supernova está progresando a través de una fase crítica de su vida útil observable.