Welcome to PF!
d=vt+1/2at^2 said:
Personally, I don't believe in the big bang. But those who do, can you explain this to me please. We all know that the Earth is exactly the right mass to orbit the sun, and that the inertia of the Earth keeps it from flying into the sun.
Hi d=vt+1/2at^2! Welcome to PF!
The mass cancels out in the equations, so the Earth (
always begin your address with a capital letter!

) could be replaced by a body with a completely different mass, and it would still go round the Sun in the same time along the same orbit.
"Mass cancelling out" happens in lots of fields … for example, the biggest acceleration that something can have without something else sliding off is determined by F = ma and F = µmg, so a = µmg/m = µg, which is the same for any m.
We also know that the velocity of the Earth is exactly the right amount so the inertia is precisely enough to keep the Earth from either flying into the sun, or flying into space. I ask you this: How did this come to be, from a random explosion? How did the Earth form exactly to the right mass, and exactly the right speed, in order for this to happen? It just seems way too random in my opinion.
The Earth didn't form from an explosion, it formed from material gradually coming
together (under gravitational attraction).
The big bang was way before the Earth formed … after the big bang, the universe had to cool down a bit, then the first stars and galaxies formed, made of only hydrogen and helium, much later a new generation was formed of slightly heavier elements, and eventually really heavy elements were made from supernova explosions, and our generation of galaxies was formed.
So the Sun and Earth
are made of material formed in lots of explosions, but way back in the past, and that material was pretty cold by the time the Earth started.
Even if there
had been an explosion, all the bits would have orbited the Sun anyway (except maybe for about .01% that might escape).
Just as
any mass will do, any
speed will do also … though that will of course affect the radius and the eccentricity (circularness) of the orbit.
