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  2. Future of Earth - Wikipedia

    en.wikipedia.org/wiki/Future_of_Earth

    The ablation and vaporization caused by Earth's fall on a decaying trajectory towards the Sun may remove Earth's mantle, leaving just the core, which will finally be destroyed after at most 200 years. [102] [103] Earth's sole legacy will be a very slight increase (0.01%) of the solar metallicity following this event. [104]: IIC

  3. List of dates predicted for apocalyptic events - Wikipedia

    en.wikipedia.org/wiki/List_of_dates_predicted...

    Earth and the Moon will be most likely be destroyed by falling into the Sun, just before the Sun reaches the largest of its red giant phase when it will be 256 times larger than it is now. Before the final collision, the Moon possibly spirals below Earth's Roche limit, breaking into a ring of debris, most of which falls to Earth's surface. [215 ...

  4. Timeline of the far future - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_the_far_future

    The Sun reaches the top of the red-giant branch of the Hertzsprung–Russell diagram, achieving its maximum radius of 256 times the present-day value. [118] In the process, Mercury, Venus and Earth are likely destroyed. [114] 8 billion The Sun becomes a carbon–oxygen white dwarf with about 54.05% of its present mass.

  5. Geologic Calendar - Wikipedia

    en.wikipedia.org/wiki/Geologic_Calendar

    Even though the Sun won't destroy Earth until December 31, all animals will die out by the end of May. Use of the geologic calendar as a conceptual aid dates back at least to the mid 20th century, for example in Richard Carrington's 1956 book A Guide to Earth History [3] and Gove Hambidge's 1941 chapter in the book Climate and Man. [4]

  6. Stability of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Stability_of_the_Solar_System

    This could eject it from the Solar System altogether [1] or send it on a collision course with Venus, the Sun, or Earth. [ 10 ] Mercury's perihelion-precession rate is dominated by planet–planet interactions, but about 7.5% of Mercury's perihelion precession rate comes from the effects described by general relativity . [ 11 ]

  7. Global catastrophe scenarios - Wikipedia

    en.wikipedia.org/wiki/Global_catastrophe_scenarios

    The Earth will naturally become uninhabitable due to the Sun's stellar evolution, within about a billion years. [148] In around 1 billion years from now, the Sun 's brightness may increase as a result of a shortage of hydrogen , and the heating of its outer layers may cause the Earth's oceans to evaporate, leaving only minor forms of life. [ 149 ]

  8. Ever see a star explode? You're about to get a chance very soon

    www.aol.com/news/ever-see-star-explode-youre...

    These explosions — billions of times brighter than the sundestroy the star, often leaving behind a black hole. Supernovas are also a useful tool for astronomers to measure distance.

  9. Runaway greenhouse effect - Wikipedia

    en.wikipedia.org/wiki/Runaway_greenhouse_effect

    Most scientists believe that a runaway greenhouse effect is inevitable in the long term, as the Sun gradually becomes more luminous as it ages, and will spell the end of all life on Earth. As the Sun becomes 10% brighter about one billion years from now, the surface temperature of Earth will reach 47 °C (117 °F) (unless Albedo is increased ...