How did the solar system take shape?
How did the solar system take shape?
The Sun and the planets formed together, 4.6 billion years ago, from a cloud of gas and dust called the solar nebula. A shock wave from a nearby supernova explosion probably initiated the collapse of the solar nebula. The Sun formed in the center, and the planets formed in a thin disk orbiting around it.
How we think the solar system is vs how it actually is?
Many scientists think our solar system formed from a giant, rotating cloud of gas and dust known as the solar nebula. As the nebula collapsed because of its gravity, it spun faster and flattened into a disk. Most of the material was pulled toward the center to form the sun.
Why is our solar system shaped like a disk?
It’s thought to have arisen from an amorphous cloud of gas and dust in space. The original cloud was spinning, and this spin caused it to flatten out into a disk shape. The sun and planets are believed to have formed out of this disk, which is why, today, the planets still orbit in a single plane around our sun.
How long did it take for Earth to become roughly the size and shape it is today?
According to nebular theory, planetesimals formed by accretion, with the primordial Earth being estimated as likely taking anywhere from 70 to 100 million years to form. Estimates of the age of the Moon range from 4.5 Ga to significantly younger.
Is there a black hole in the solar system?
There’s a growing consensus among astronomers that beyond the gas giants of the outer solar system lurks a mysterious object — perhaps a black hole — influencing the massive cloud of small, icy bodies in the Oort cloud.
Is our solar system actually flat?
Our solar system is actually pretty flat, with most of its planets orbiting within three degrees of the plane of the Earth’s orbit around the sun, called the ecliptic. It’s out of this rotating protoplanetary disk of gas and dust that planets are born, resulting in a relatively flat solar system.
Why do spinning things flatten?
The equilibrium shape of a rotating star–or planet, for that matter–is not a sphere, but rather an flattened oblate spheroid. The reason is that centrifugal effects are greatest at the rotational equator and work against the object’s self-gravity.