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  2. Habitable zone for complex life - Wikipedia

    en.wikipedia.org/.../Habitable_Zone_for_Complex_Life

    Milankovitch cycle The Milankovitch cycle and ice age have been key is shaping Earth. [96] [97] Life on Earth today is using water melting from the last ice age. The ice ages cannot be too long or too cold for life to survive. Milankovitch cycle has an impact on the planet's obliquity also. [98] [99] [100]

  3. Future of Earth - Wikipedia

    en.wikipedia.org/wiki/Future_of_Earth

    The biological and geological future of Earth can be extrapolated based on the estimated effects of several long-term influences. These include the chemistry at Earth's surface, the cooling rate of the planet's interior, gravitational interactions with other objects in the Solar System, and a steady increase in the Sun's luminosity.

  4. Timeline of the evolutionary history of life - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_the...

    The earliest evidence for life on Earth includes: 3.8 billion-year-old biogenic hematite in a banded iron formation of the Nuvvuagittuq Greenstone Belt in Canada; [30] graphite in 3.7 billion-year-old metasedimentary rocks in western Greenland; [31] and microbial mat fossils in 3.48 billion-year-old sandstone in Western Australia.

  5. Life on Our Planet - Wikipedia

    en.wikipedia.org/wiki/Life_on_Our_Planet

    Life on Our Planet is an American television nature documentary series released on Netflix and produced by Amblin Television and Silverback Films. Executive-produced by Steven Spielberg and narrated by Morgan Freeman, the series focuses on the evolutionary history of complex life on Earth. Upon its release, the series received generally mixed ...

  6. Planetary habitability - Wikipedia

    en.wikipedia.org/wiki/Planetary_habitability

    It took 4.5 billion years before humanity appeared on Earth, and life as we know it will see suitable conditions for 1 [95] to 2.3 [96] billion years more. Red dwarfs, by contrast, could live for trillions of years because their nuclear reactions are far slower than those of larger stars, meaning that life would have longer to evolve and survive.

  7. Gaia hypothesis - Wikipedia

    en.wikipedia.org/wiki/Gaia_hypothesis

    Lovelock formulated the Gaia Hypothesis in journal articles in 1972 [1] and 1974, [2] followed by a popularizing 1979 book Gaia: A new look at life on Earth. An article in the New Scientist of February 6, 1975, [ 42 ] and a popular book length version of the hypothesis, published in 1979 as The Quest for Gaia , began to attract scientific and ...

  8. Carbon-based life - Wikipedia

    en.wikipedia.org/wiki/Carbon-based_life

    The carbon cycle is a biogeochemical cycle that is important in maintaining life on Earth over a long time span. The cycle includes carbon sequestration and carbon sinks. [4] [5] Plate tectonics are needed for life over a long time span, and carbon-based life is important in the plate tectonics process. [6]

  9. Prebiotic atmosphere - Wikipedia

    en.wikipedia.org/wiki/Prebiotic_atmosphere

    Putative evidence of life on Earth from older times (e.g. 3.8 and 4.1 billion years ago [15] [16]) lacks additional context necessary to claim it is truly of biotic origin, so it is still debated. [17] Thus, the prebiotic atmosphere concluded 3.5 billion years ago or earlier, placing it in the early Archean Eon or mid-to-late Hadean Eon. [18]