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States of Water01:23

States of Water

46.6K
Water exists in any one of the three classical states: solid (ice), liquid (water), and gas (steam or water vapor). The state of water depends on i) the intermolecular forces that draw molecules together and ii) the kinetic energy that leads to movements that pull them apart.
Water freezes when the intermolecular forces are greater than the kinetic energy. Unlike most other substances, water is less dense in its solid state than in its liquid state. This is because each water molecule can form...
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The Water Cycle01:00

The Water Cycle

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The Earth’s hydrosphere includes all of the areas where the storage and movement of water occurs. Since water is the basis of all living processes, the cycling of water is extremely important to ecosystem dynamics.
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The Carbon Cycle01:14

The Carbon Cycle

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Carbon is the basis of all organic matter on Earth, and is recycled through the ecosystem in two primary processes: one in which carbon is exchanged among living organisms, and one in which carbon is cycled over long periods of time through fossilized organic remains, weathering of rocks, and volcanic activity. Human activities, including increased agricultural practices and the burning of fossil fuels, has greatly affected the balance of the natural carbon cycle.
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Global Climate Change01:50

Global Climate Change

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Throughout its ~4.5 billion year history, the Earth has experienced periods of warming and cooling. However, the current drastic increase in global temperatures is well outside of the Earth’s cyclic norms, and evidence for human-caused global climate change is compelling. Paleoclimatology, the study of ancient climate conditions, provides ample evidence for human-caused global climate change by comparing recent conditions with those in the past.
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The Fossil Record02:56

The Fossil Record

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The fossil record documents only a small fraction of all organisms that have ever inhabited Earth. Fossilization is a rare process, and most organisms never become fossils. Moreover, the fossil record only exhibits fossils that have been discovered. Nevertheless, sedimentary rock fossils of long-lived, abundant, hard-bodied organisms dominate the fossil record. These fossils offer valuable information, such as an organism's physical form, behavior, and age. Studying the fossil record helps...
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Phase Transitions: Melting and Freezing02:39

Phase Transitions: Melting and Freezing

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Heating a crystalline solid increases the average energy of its atoms, molecules, or ions, and the solid gets hotter. At some point, the added energy becomes large enough to partially overcome the forces holding the molecules or ions of the solid in their fixed positions, and the solid begins the process of transitioning to the liquid state or melting. At this point, the temperature of the solid stops rising, despite the continual input of heat, and it remains constant until all of the solid is...
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Updated: May 6, 2026

Removal of Exogenous Materials from the Outer Portion of Frozen Cores to Investigate the Ancient Biological Communities Harbored Inside
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Removal of Exogenous Materials from the Outer Portion of Frozen Cores to Investigate the Ancient Biological Communities Harbored Inside

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Las recientes edades de hielo en Marte han sido muy recientes.

James W Head1, John F Mustard, Mikhail A Kreslavsky

  • 1Department of Geological Sciences, Brown University, Providence, Rhode Island 02912, USA. James_Head@brown.edu

Nature
|December 20, 2003
PubMed
Resumen
Este resumen es generado por máquina.

Marte experimentó una reciente edad de hielo entre hace 2,1 y 0,4 millones de años, evidenciada por extensos depósitos de hielo polvoriento. Esta edad de hielo marciana presentó polos más cálidos y transporte de polvo hacia el ecuador, a diferencia de las edades de hielo de la Tierra.

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Área de la Ciencia:

  • Ciencias planetarias Ciencias planetarias.
  • Ciencias del clima Ciencias del clima Ciencias del clima
  • Geología Geología Geología.

Sus antecedentes:

  • Las edades de hielo de la Tierra son impulsadas por variaciones orbitales.
  • Marte exhibe depósitos en capas, polvorientos y ricos en hielo de agua a través de los hemisferios.
  • Estos depósitos dependen de la latitud y tienen varios metros de espesor.

Objetivo del estudio:

  • Para investigar la formación y el momento de los depósitos marcianos ricos en hielo.
  • Para entender el papel de las variaciones orbitales en la historia del clima marciano.
  • Para comparar las edades de hielo marcianas con las de la Tierra.

Principales métodos:

  • Análisis de los datos de la exploración de Marte sobre los depósitos del manto.
  • Modelado de la estabilidad del hielo de agua y el polvo bajo diferentes oblicuidades.
  • Datación geológica de los períodos de formación de depósitos.

Principales resultados:

  • La evidencia sugiere que la edad de hielo marciana ocurrió hace entre 2,1 y 0,4 millones de años.
  • Los depósitos se colocan simétricamente hacia abajo a ~ 30 grados de latitud en respuesta a los cambios de oblicuidad (30-35 grados).
  • Marte se encuentra actualmente en un período interglacial con depósitos de hielo en retroceso.

Conclusiones:

  • Las edades de hielo marcianas se caracterizan por climas polares más cálidos.
  • El transporte mejorado hacia el ecuador de agua y polvo se produjo durante las edades de hielo marcianas.
  • A diferencia de la Tierra, Marte muestra depósitos extendidos de latitudes medias de edades de hielo.