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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...
Rocket Propulsion in Gravitational Field - I01:20

Rocket Propulsion in Gravitational Field - I

Rockets range in size from small fireworks that ordinary people use to the enormous Saturn V that once propelled massive payloads toward the Moon. The propulsion of all rockets, jet engines, deflating balloons, and even squids and octopuses are explained by the same physical principle: Newton's third law of motion. The matter is forcefully ejected from a system, producing an equal and opposite reaction on what remains.
The motion of a rocket in space changes its velocity (and hence its...
Rocket Propulsion in Gravitational Field - II01:03

Rocket Propulsion in Gravitational Field - II

A rocket's velocity in the presence of a gravitational field is decreased by the amount of force exerted by Earth's gravitational field, which opposes the motion of the rocket. If we consider thrust, that is, the force exerted on a rocket by the exhaust gases, then a rocket's thrust is greater in outer space than in the atmosphere or on a launch pad. In fact, gases are easier to expel in a vacuum.
A rocket's acceleration depends on three major factors, consistent with the equation for the...
Atomic Nuclei: Larmor Precession Frequency01:11

Atomic Nuclei: Larmor Precession Frequency

The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession, and the angular frequency...
Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

An object absorbing an electromagnetic wave would experience a force in the direction of propagation of the wave. This force occurs because electromagnetic waves contain and transport momentum. The force accounts for the wave's radiation pressure exerted on the object. Maxwell's prediction was confirmed in 1903 by Nichols and Hull by precisely measuring radiation pressures with a torsion balance. The measuring instrument had mirrors suspended from a fiber kept inside a glass container. Nichols...
Rapidly Varying Flow01:24

Rapidly Varying Flow

Rapidly varying flow (RVF) in open channels is characterized by abrupt changes in flow depth over a short distance, with the rate of depth change relative to distance often approaching unity. These flows are inherently complex due to their transient and multi-dimensional nature, making exact analysis difficult. However, approximate solutions using simplified models provide valuable insights into their behavior.Key Features of Rapidly Varying FlowRVF is commonly observed in scenarios involving...

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Video Experimental Relacionado

Updated: May 13, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

Published on: July 2, 2012

Acreción pulsada en una protoestrella variable.

James Muzerolle1, Elise Furlan, Kevin Flaherty

  • 1Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218, USA. muzerol@stsci.edu

Nature
|January 4, 2013
PubMed
Resumen
Este resumen es generado por máquina.

Las protoestrellas jóvenes exhiben acreción pulsada, un fenómeno en el que la luminosidad aumenta periódicamente debido a tasas de acreción variables. Este estudio observó una protoestrella con un sorprendente y regular aumento de diez veces la luminosidad infrarroja cada 25,34 días.

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Área de la Ciencia:

  • La astrofísica es la astrofísica.
  • Evolución Estelar Evolución Estelar
  • Investigación de exoplanetas Investigación de exoplanetas.

Sus antecedentes:

  • Las estrellas binarias cercanas de la pre-secuencia principal acumulan material de los discos circumbinarios.
  • La acreción pulsada, caracterizada por aumentos periódicos de la luminosidad, influye en la evolución binaria y la formación de planetas.
  • La variabilidad de la acreción es común en estrellas jóvenes, pero las señales periódicas de acreción pulsada rara vez se observan en binarios jóvenes.

Objetivo del estudio:

  • Para investigar las variaciones periódicas de luminosidad en una protoestrella joven.
  • Para determinar si las variaciones observadas son consistentes con la acreción pulsada.
  • Comprender las implicaciones de la fuerte y regular acreción pulsada en sistemas estelares muy jóvenes.

Principales métodos:

  • Observaciones infrarrojas de varias épocas de una joven protoestrella.
  • Análisis de las variaciones de luminosidad en el tiempo.
  • Comparación de los patrones observados con los modelos teóricos de la acreción pulsada.

Principales resultados:

  • Una joven protoestrella (edad ~10^5 años) mostró un aumento de diez veces en la luminosidad infrarroja durante aproximadamente una semana.
  • Este aumento de la luminosidad se repitió con una regularidad notable cada 25,34 días.
  • El fenómeno observado se atribuye a la acreción pulsada de un compañero binario invisible.

Conclusiones:

  • La señal de acreción pulsada observada es inusualmente fuerte y regular para un sistema de esta edad tan joven.
  • Este hallazgo sugiere que la acreción pulsada puede jugar un papel importante en la evolución temprana de estrellas binarias cercanas.
  • La regularidad y la intensidad de la señal pueden estar vinculadas a la edad muy joven de la protoestrella en comparación con los sistemas estudiados anteriormente.