With the recent rogue bolts flying around space, I am pondering how big an object has to be to not completely burn up in the atmosphere and impact the Earth's surface.
What would the formula be to solve for mass?
For the purpose of my inquiry, let's keep it simple. Assume the object was not in orbit, but rather entered orbit perpendicular to Earth's sphere traveling at a negligible speed such that at the initiation of the gravitational pull it's initial speed was zero and began its acceleration at that point.
Also assume that there are no lateral atmospheric forces, (e.g., falling through a jet stream or 50 m.p.h. wind perpendicular to it's travel) and that the atmosphere is still.
For the object, assume a solid sphere so that it's orientation and rotation have no affect, even though it is known that as it starts to burn away it will no longer stay a perfect sphere.
As for material, assume 1010/1020 Low Carbon Steel.
So what would the formula look like? What is the transition point? Meaning "x" diameter and smaller will completely burn up whereas everything larger will impact. For those objects that are of sufficient size to impact, how much of them will impact? Meaning, is the amount that burns away a fixed percentage or a ratio proportionate to their original mass? Example, will 75% of the original mass be lost whether it starts as a 10 foot diameter sphere or a 500 foot diameter sphere or would the graph be more parabolic in nature?
This is way outside my realm of knowledge so I appreciate your input in satisfying my curiosity. Unfortunately, I leave for two weeks tomorrow and will not have internet access so you've got time to ponder on this one... Thanks Again!