Sure. One would think for such a proponent of evolution, at least you'd be familiar with its concepts. It's not that hard as the myth that the planets were spit out of stars, where life just happened to "poof", is all over the place. Here are a few 'non-reputable' sources for you, like Space.com and Harvard University.
The Big Bang: What Really Happened at Our Universe's Birth?
Over time, stars gravitated together to form galaxies, leading to more and more large-scale structure in the universe. Planets coalesced around some newly forming stars, including our own sun. And 3.8 billion years ago, life took root on Earth.
5(a). Evolution of the Universe
As the Universe expanded, matter began to coalesce into gas clouds, and then stars and planets. Our solar system formed about 5 billion years ago when the Universe was about 65% of its present size
5(b). Early History of the Earth
The Earth formed as cosmic dust lumped together to form larger and larger particles until 150 million years had passed. At about 4.4 billion years, the young Earth had a mass similar to the mass it has today. The continents probably began forming about 4.2 billion years ago as the Earth continued to cool. The cooling also resulted in the release of gases from the lithosphere, much of which formed the Earth's early atmosphere. Most of the Earth's early atmosphere was created in the first one million years after solidification (4.4 billion years ago). Carbon dioxide, nitrogen, and water vapor dominated this early atmosphere.
As the Earth continued to cool, the water vapor found in the atmosphere condensed to form the oceans and other fresh water bodies on the continents. Oxygen began accumulating in the atmosphere through
photo-dissociation of O2 from water, and by way of
photosynthesis (life). The emergence of living organisms was extremely important in the creation of atmospheric oxygen and
ozone. Without ozone, life could not exist on land because of harmful
ultraviolet radiation.
Astronomy 280: Evolution of the Universe
The course includes the origin of the simplest chemical elements shortly after the Big Bang, the condensation of matter in the early universe into large structures such as galaxies and clusters of galaxies, and scenarios that explain why we find different types of galaxies in the universe. The Milky Way is used as a specific example of a spiral galaxy to examine how matter is cycled from the interstellar medium into stars that evolve and eventually die, putting their matter back into the interstellar medium. This process creates more complex elements, including those necessary for life as we know it.
Here's a video for you:
Watch the entire evolution of the universe in under 3 minutes
https://www.cfa.harvard.edu/~ejchaisson/cosmic_evolution/docs/text/text_plan_2.html
Current consensus envisions the genesis of a planetary system as a natural, perhaps frequent, outgrowth of the birth of a star. The condensation model can generally account for each of the 7, earlier-noted properties characterizing our Solar System today. But exactly how those atoms of gas and grains of dust managed to coalesce into the present planets and moons remains one of the great riddles of modern science.
5.1 - Planetary Evolution
a large, slowly rotating cloud of interstellar gas and dust about a light-year in diameter begins to slowly shrink. As it draws itself together gravitationally over a period of perhaps ten million years,1945 it becomes denser...As the protostar collapses, its magnetic field lines of force are dragged closer together but are held firmly in place...The planets themselves form in the disk of matter surrounding the protostar.