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Atomic Structure01:33

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Protons and neutrons, collectively called nucleons, are packed together tightly in a nucleus. With a radius of about 10−15 meters, a nucleus is quite small compared to the radius of the entire atom, which is about 10−10 meters. Nuclei are extremely dense compared to bulk matter, averaging 1.8 × 1014 grams per cubic centimeter. If the earth’s density were equal to the average nuclear density, the earth’s radius would be only about 200 meters.
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The Greek philosopher Democritus proposed that everything on Earth is made up of tiny particles called atomos, Greek for "indivisible," from which the modern term "atom" is derived. In the 19th century, John Dalton proposed the atomic theory that is still largely correct today. He put forth five postulates to explain how atoms made up the world around us. (1) All matter is composed of infinitely small particles or atoms. (2) All atoms of a given element are identical to one another and (3) are...

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Synthesis of Core-shell Lanthanide-doped Upconversion Nanocrystals for Cellular Applications
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Marte: un nuevo régimen de cristalización del núcleo.

Andrew J Stewart1, Max W Schmidt, Wim van Westrenen

  • 1Institute for Mineralogy and Petrology, Eidgenössische Technische Hochschule Zurich, CH 8092 Zurich, Switzerland.

Science (New York, N.Y.)
|June 2, 2007
PubMed
Resumen

El núcleo de Marte es líquido y carece de un núcleo interno rico en hierro como el de la Tierra. El enfriamiento planetario puede causar la cristalización a través de un modelo de "núcleo de nieve" o "núcleo interno de sulfuro".

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Área de la Ciencia:

  • Ciencias planetarias Ciencias planetarias.
  • La geofísica es la geofísica.
  • La geoquímica de la tierra sólida La geoquímica de la tierra sólida

Sus antecedentes:

  • La evolución del núcleo marciano a menudo se compara con la de la Tierra.
  • Los modelos anteriores asumieron estructuras centrales y caminos evolutivos similares.

Objetivo del estudio:

  • Para investigar el estado físico y el comportamiento de cristalización del núcleo marciano.
  • Para determinar si Marte desarrolla un núcleo interno rico en hierro.

Principales métodos:

  • Experimentos de alta presión y alta temperatura en sistemas de hierro-azufre y hierro-níquel-azufre.
  • Simulaciones en presiones representativas del núcleo de Marte.

Principales resultados:

  • El núcleo marciano es actualmente completamente líquido.
  • Los datos experimentales sugieren que Marte no formará un núcleo interno rico en hierro.
  • Se predice que la cristalización seguirá un modelo de "núcleo de nieve" o de "núcleo interno de sulfuro".

Conclusiones:

  • La evolución del núcleo marciano diverge de la de la Tierra.
  • La futura cristalización del núcleo en Marte diferirá significativamente de la de la Tierra.
  • Se necesitan nuevos modelos para explicar la dinámica del núcleo marciano.