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  2. Colonization of Venus - Wikipedia

    en.wikipedia.org/wiki/Colonization_of_Venus

    Geoffrey A. Landis of NASA's Glenn Research Center has summarized the perceived difficulties in colonizing Venus as being merely from the assumption that a colony would need to be based on the surface of a planet: However, viewed in a different way, the problem with Venus is merely that the ground level is too far below the one atmosphere level.

  3. Space colonization - Wikipedia

    en.wikipedia.org/wiki/Space_colonization

    The two most common reasons in favor of colonization are the survival of humans and life independent of Earth, making humans a multiplanetary species, [7] in the event of a planetary-scale disaster (natural or human-made), and the commercial use of space particularly for enabling a more sustainable expansion of human society through the ...

  4. Seasons on planets - Wikipedia

    en.wikipedia.org/wiki/Seasons_on_planets

    Given the different Sun incidence in different positions in the orbit, it is necessary to define a standard point of the orbit of the planet, to define the planet position in the orbit at each moment of the year w.r.t such point; this point is called with several names: vernal equinox, spring equinox, March equinox, all equivalent, and named considering northern hemisphere seasons.

  5. Terraforming of Venus - Wikipedia

    en.wikipedia.org/wiki/Terraforming_of_Venus

    However, the length of a solar day on Venus is significantly shorter than the sidereal day; to an observer on the surface of Venus, the time from one sunrise to the next would be 116.75 days. Therefore, the slow Venerian rotation rate would result in extremely long days and nights, similar to the day-night cycles in the polar regions of earth ...

  6. How climate change made Venus impossible to inhabit - AOL

    www.aol.com/climate-change-made-venus-impossible...

    Venus currently has a surface temperature of 450℃ (the temperature of an oven’s self-cleaning cycle) and an atmosphere dominated by carbon dioxide (96%) with a density 90 times that of Earth’s.

  7. Timeline of the far future - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_the_far_future

    The Sun will likely expand sufficiently to overwhelm most of the inner planets (Mercury, Venus, and possibly Earth) but not the giant planets, including Jupiter and Saturn. Afterwards, the Sun will be reduced to the size of a white dwarf, and the outer planets and their moons will continue to orbit this diminutive solar remnant.

  8. Discovery and exploration of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Discovery_and_exploration...

    One important discovery made at different times in different places is that the bright planet sometimes seen near the sunrise (called Phosphorus by the Greeks) and the bright planet sometimes seen near the sunset (called Hesperus by the Greeks) were actually the same planet, Venus. [7] Animation depicting Eudoxus' model of retrograde planetary ...

  9. The Founder of OceanGate Wants to Send 1,000 People to ...

    www.aol.com/founder-oceangate-wants-send-1...

    Venus is one of the most inhospitable planets, but OceanGate cofounder Guillermo Söhnlein wants to form a colony in its atmosphere. Venus is one of the most inhospitable planets, but OceanGate ...

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