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Articles tagged: carbon dioxide

  • abiogenesis zone, Kepler 452b, plate tectonics, stagnant lid planets, ultraviolet (UV) light 03 August 2018 Plate tectonics not needed for life, but UV light is

    ...are in fact not required. Temperatures on Earth are kept to a reasonable habitable level by the release and capture of carbon dioxide (CO2). After it is released from the ground, it is then returned to the subsurface when it has been sequestered into...

    • abiogenesis zone
    • Kepler 452b
    • plate tectonics
    • stagnant lid planets
    • ultraviolet (UV) light
  • coastal management, Copernicus Sentinel-3, image data, NASA, oceans October 2017 Colouring our view of the oceans

    ... is one of the Essential Climate Variables (ECV) listed by the World Meteorological Organization (WMO). Phytoplankton pull carbon dioxide from the atmosphere for photosynthesis and a given population of phytoplankton can double its numbers in a day...

    • coastal management
    • Copernicus Sentinel-3
    • image data
    • NASA
    • oceans
    Authors: Ewa Kwiatkowska    
  • Enceladus, Europa, Europa Clipper, JUICE mission 02 January 2021 Life beneath glaciers is good news in the search for life on icy worlds

    ... team, was that the microbial communities under the glaciers could combine that hydrogen gas with carbon dioxide to generate biomass. Biomass is biological material derived from living, or recently living organisms that can be used to generate...

    • Enceladus
    • Europa
    • Europa Clipper
    • JUICE mission
  • Janet G. Luhmann, Mars Atmosphere and Volatile EvolutioN, Maven, Space Sciences Laboratory December 2014 MAVEN and the evolution of Mars

    ..., unlike Mercury, are far enough from the Sun to have retained at least their heavier constituents like carbon dioxide. Endeavour Crater, with Pillinger Point in the foreground, as viewed in false colour by NASA’s Mars Exploration Rover Opportunity...

    • Janet G. Luhmann
    • Mars Atmosphere and Volatile EvolutioN
    • Maven
    • Space Sciences Laboratory
    Authors: Janet G. Luhmann    
  • 02 March 2016 Using MUSCLES to test for life on other planets

    ... stars. The first abiotic method identified to produce this result is when a star's ultraviolet (UV) light splits apart carbon dioxide (CO2) molecules, freeing some of the oxygen atoms to form into O2, the kind of oxygen present in Earth's atmosphere...

  • Ceres, megasatellite, Space Exploration, space habitats November 2021 Megasatellite habitat at Ceres

    ... for Earth, and this makes it necessary to regulate the carbon dioxide level to prevent fluctuations. To achieve this, some biomass will...then burned cleanly at the right rate to keep the carbon dioxide level optimal for plants and people. Just as on ...

    • Ceres
    • megasatellite
    • Space Exploration
    • space habitats
    Authors: Pekka Janhunen    
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