Introduced by Anaxagoras, explains that the universe (cosmos) was once a primordial mixture composed of hydrogen, hydrogen gas, and ammonia, with a theory on the rise of the eclipses
Introduced by Leucippus and Democritus, says that the universe was composed of very small, indivisible, and indestructible building blocks called atoms
Introduced by Nicolaus Copernicus, established the heliocentric theory with the sun at the center of the solar system, based on his book "On the Revolutions of the Heavenly Bodies"
Introduced by Albert Einstein, added the cosmological constant to his general theory of relativity equation, counteracting the dynamic effects of gravity which would cause the universe to collapse
Introduced by Abbe Georges Edouard Lemaitre, the universe developed 13.8 billion years ago after a cataclysmic explosion of small, primeval "super atom" causing the inflation and expansion of the universe, the current accepted theory
Introduced by Edwin Hubble, discovered that the galaxies are moving away from each other, states that if the universe is expanding, then it could have been tiny at some moment in the past
Proposed by astronomers Fred Hoyle, Thomas Gold, and Herman Bondi, predicts that the universe expanded without a change in its density, states that matter is continually created as the universe expands, disapproved by Martin Ryle in the 1950s stating that the universe is evolving in time
Proposed by Immanuel Kent and modified by Pierre Laplace, suggests that the solar system was formed from a giant, rotating cloud of dust and gas called a nebula, gravity caused it to collapse, spin faster, and flatten into a disk, the center of the disk becomes denser and hotter, forming the Sun, and the material leftover clumped together to create planets, moons, asteroids, and comets, the current leading theory
Introduced by H.N. Russell, proposes that the solar system was formed from the collision of two stars, the immense heat and pressure of the collision would have ejected a large amount of material, clumping together and forming the solar system
Introduced by Thomas Chrowder Chemberlin and Forest Ray Moulton, proposes that a star passed very close to our sun but not enough to collide, the gravitational pull of the passing star stretched the sun, causing materials to be ejected in long streams, as the ejected material cooled and condensed, it clumped together to form small rocky bodies called planetesimals, these collided overtime and merged to create the planets we see today