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What is an Ecosystem?01:17

What is an Ecosystem?

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The total amount of energy acquired by primary producers in an ecosystem is called gross primary production (GPP). However, of this energy, producers use some for metabolic processes, and some is lost as heat, decreasing the amount of energy available to the next trophic level. The remaining usable amount of energy is called the net primary productivity (NPP). In terrestrial ecosystems, NPP is driven by climate, while light penetration and nutrient availability drive NPP in aquatic ecosystems.
Sustainable Development01:43

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As the human population continues to grow and use resources, we must be mindful of our planet’s natural limits. Sustainable development provides a pathway to maintain and improve human life now while also ensuring that future generations will have the resources that they need. The long-term success of sustainability efforts rests on understanding the interplay between human actions and ecological systems.
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Effect of Sea Water on Concrete

Concrete exposed to seawater can undergo degradation like the dissolution of ettringite and gypsum, increasing the material's porosity and decreasing its strength. In contrast, the crystallization of salts within the concrete's pores can cause expansion, particularly above the waterline where evaporation occurs. Nonetheless, this expansion only happens when seawater, enabled by the concrete's permeability, manages to infiltrate the structure.
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Marine Microbial Ecology

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Deep Sea Microbial Ecology

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Video Experimental Relacionado

Updated: Jun 24, 2026

Methods for Image-based Surveys of Benthic Macroinvertebrates and Their Habitat Exemplified by the Drop Camera Survey for the Atlantic Sea Scallop
07:43

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¿Hay océanos en Titán?

F M Flasar

    Science (New York, N.Y.)
    |July 1, 1983
    PubMed
    Resumen
    Este resumen es generado por máquina.

    El titán Titan es un titán.

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    Área de la Ciencia:

    • Ciencias planetarias Ciencias planetarias.
    • Astrobiología Astrobiología.

    Sus antecedentes:

    • La atmósfera de Titán puede contener océanos de metano.
    • Los datos de ocultación de radio de la Voyager proporcionan información sobre las condiciones de la superficie de Titán.

    Objetivo del estudio:

    • Para evaluar la probabilidad de océanos de metano en Titán basado en los niveles de saturación atmosférica.
    • Para determinar las condiciones bajo las cuales podrían existir océanos de metano en Titán.

    Principales métodos:

    • Análisis de los datos de ocultación de radio de la Voyager.
    • Modelado atmosférico de las condiciones cercanas a la superficie de Titán.

    Principales resultados:

    • Se requiere una saturación de metano atmosférico cercana al 100% para los océanos de metano.
    • Los datos de la Voyager sugieren una baja humedad en la superficie, lo que implica que la tierra en los lugares de sondeo.
    • Las bajas velocidades de viento zonales (< 4 cm/s) son necesarias para océanos potenciales de baja latitud.

    Conclusiones:

    • Los océanos de metano pueden existir en regiones inexploradas de baja latitud de Titán.
    • Las condiciones atmosféricas y de viento específicas son críticas para la presencia de metano líquido en la superficie.