Os cálculos batem: nosso universo pode ser um holograma
Teoria que diz que o universo é um holograma – enquanto o mundo "real" seria um cosmo de uma dimensão e sem gravidade, ditado pelas leis da física quântica - pode ser verdadeira
21 Breathtaking Images Of Moon That Will Make You Think If It's Real Or Not
Who doesn't love the glory and shine of Moon? Here's some of breathtaking pictures of Moon that will surely make you think twice if it's real or photoshopped.
Billions and Billions
thedemon-hauntedworld: “Antennae Galaxy by Hubble The Antennae Galaxies, also known as NGC 4038/NGC 4039, are a pair of interacting galaxies in the constellation Corvus. They are currently going...
NGC 3576: Glowing Gas in the Milky Way (NASA, Chandra, 10/28/13)
A region of glowing gas in the Sagittarius arm of the Milky Way galaxy, NGC 3576 is located about 9,000 light years from Earth. Such nebulas present a tableau of the drama of the evolution of massive stars, from the formation in vast dark clouds, their relatively brief (a few million years) lives, and the eventual destruction in supernova explosions. The diffuse X-ray data detected by Chandra (blue) are likely due to the winds from young, massive stars that are blowing throughout the nebula…
Some 60 million light-years away in the southerlyconstellation Corvus, two large galaxies are colliding. Stars in the two galaxies, cataloged as NGC 4038 and NGC 4039, very rarely collide in the course of the ponderous cataclysm that lasts for hundreds of millions of years. But the galaxies' large clouds of molecular gas and dust often do, triggering furious episodesof star formation near the center of the cosmic wreckage
NGC 602 is a young, bright open cluster of stars located in the Small Magellanic Cloud (SMC), a satellite galaxy to the Milky Way. Radiation and shock waves from the stars have pushed away much of the lighter surrounding gas and dust that compose the nebula known as N90, and this in turn has triggered new star formation in the ridges (or "elephant trunks") of the nebula.