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  • Me.

    No one actually has probelms like me, I hate my body

    • 5 months ago
  • storiesby-thestoner:

It’s timeeeee


Lol

    storiesby-thestoner:

    It’s timeeeee

    Lol

    (via deadlycrayons)

    Source: htdeverything
    • 6 months ago
    • 51926 notes
  • robotcosmonaut:

Wednesday


Wedensday!

    robotcosmonaut:

    Wednesday

    Wedensday!

    (via rrrick)

    Source: robotcosmonaut
    • 6 months ago
    • 166 notes
  • galaxyshmalaxy:

Startrail at the star party - HTT 2012 - (by miku.neko)

the galaxy is amazing

    galaxyshmalaxy:

    Startrail at the star party - HTT 2012 - (by miku.neko)

    the galaxy is amazing

    (via ikenbot)

    Source: Flickr / miku69
    • 7 months ago
    • 441 notes
  • just awesome

    just awesome

    (via rrrick)

    Source: etsy.com
    • 7 months ago
    • 977 notes
  • Halloween

    Halloween

    (via rrrick)

    Source: grottu
    • 7 months ago
    • 39 notes
  • “Curiouser and curiouser”
    — Alice Kingsly
    • 7 months ago
  • HALLOWEEN

    Nearly Halloween guyz

    • 7 months ago
  • dotcore:

    Pokémon Anatomy.
    by Ryan Mauskopf.

    For a more anatomically correct Charmander, take a look at Rye Bread’s dissection of your favorite Pokémon.

    via deviantART.

    Source: rye-bread.deviantart.com
    • 7 months ago
    • 10957 notes
  • sciencesoup:

    Like A Falling Apple

    Formulated in 1687, Newton’s Law of Universal Gravitation was a turning point in physics. While the legend of the apple falling on his head is an exaggeration of the truth, Newton did have a brilliant insight: that every object in the universe attracts every other object. The force of attraction between two objects depends on only two things: the mass of the objects, and the distance between them. So, more massive objects exert a stronger force, while more distant objects exert a weaker force. Newton was able to formulate a simple equation to describe this, pictured above: force is equal to Newton’s gravitational constant, multiplied by masses of the objects, then divided by the square of the distance between the objects. What’s remarkable is that the law truly is universal—not only can it predict how things move here on Earth, but it can also predict the movements of the moon, planets, stars and even galaxies millions of lightyears away. Newton believed that the movement of every object in our universe could be predicted, but we know now that while his theory generally holds true, it is not precise. Einstein’s theory of general relativity had to step in to fill the holes.

    (Image Credit: The Wonders Collection)

    Issic Newton, like a falling apple

    Source: sciencesoup
    • 7 months ago
    • 5325 notes
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