Gyrok, on 09 April 2015 - 10:23 AM, said:
Wrong, gravity is impacted by density.
Consider a neutron star the size of the earth would have gravity so strong that everything in our solar system would have been pulled into the orbit of such a spatial body.
Then you have singularities that have gravitational fields so strong that venturing beyond the event horizon of such objects is to be forever banished into the depths of whatever lies beyond. Whether you believe that to be a white hole, or a terminal singularity is up to you, but that does not change the fact that gravity behaves weirdly all the time. That is why M theory is the pursuit of a unified theory of gravity. Even einstein could not explain gravity in every instance, and had 2 separate theories that do not comingle about how gravity behaves. Both were proved accurate for specific cases and were the best "guesses" humanity has made to this point; however, that does not preclude them proving that gravity is far from completely predictable, or even uniform in nature.
If you are outside the event horizon for any body, no matter how dense, you will have a force between you and it given by Gmm/r^2. Show me where I'm wrong. Pretending that when we go to some corner of the IS that gravity will no longer be Gmm/r^2 is stupidly arbitrary and has no basis in reality.
Do you know how large the event horizon is for these super dense structures? Look at the Great Annihilator, or other suspected large scale superdense entities. We are far outside their event horizons, and until you want to play around in the plank lengths of distance, we're not going to be working in that regime. So my theory of gravity that got Sputnik in orbit and people to the moon and rovers to Mars is it. It's not going to change no matter what planet I go to in the IS.
For those who can't understand what I am saying, try the following:
"
Black hole event horizons are widely misunderstood. Common, although erroneous, is the notion that black holes “vacuum up” material in their neighborhood, where in fact they are no more capable of “seeking out” material to consume than any other gravitational attractor. As with any mass in the universe, matter must come within its gravitational scope for the possibility to exist of capture or consolidation with any other mass. Equally common is the idea that matter can be observed “falling into” a black hole. This is not possible. Astronomers can only detect accretion disks around black holes, where material moves with such speed that friction creates high-energy radiation which can be detected. (Similarly, some matter from these accretion disks is forced out along the axes of spin of the black hole, creating visible jets when these streams interact with matter such as interstellar gas or when they happen to be aimed directly at earth.) Further, a distant observer will never actually see it cross the horizon. Instead, while approaching it, it will seem to go ever more slowly, while any light it emits will be further and further redshifted."
"The description of event horizons given by general relativity is thought to be incomplete. When the conditions under which event horizons occur are modeled using a more comprehensive picture of the way the universe works, that includes both relativity and quantum mechanics, event horizons are expected to have properties that are different from those predicted using general relativity alone.
At present, it is expected that the primary impact of quantum effects is for event horizons to possess a
temperature and so emit radiation. For
black holes, this manifests as
Hawking radiation, and the larger question of how the black hole possesses a temperature is part of the topic of
black hole thermodynamics. For accelerating particles, this manifests as the
Unruh effect, which causes space around the particle to appear to be filled with matter and radiation.
A complete description of event horizons is expected to, at minimum, require a theory of
quantum gravity. One such candidate theory is
M-theory. Another such candidate theory is
loop quantum gravity."
The notion that macro behaviors all of a sudden change (and do so radically) when we refine our understanding of the quantum underpinnings is ridiculous
by the way no matter how dense an object is, if I am 10m from its center and i am totally outside of it, then it will have a gravitational pull equal to Gmm/(10^2) - doesn't matter if it's an apple, or a black hole with the mass of an apple.
Additional material and reference:
"[color=black]
Gravity and quantum mechanics[/color][color=#252525]
Main articles: Graviton and Quantum gravity[/color]
[color=#252525]
In the decades after the discovery of general relativity it was realized that general relativity is incompatible with quantum mechanics.[18] It is possible to describe gravity in the framework of quantum field theory like the other fundamental forces, such that the attractive force of gravity arises due to exchange of virtual gravitons, in the same way as the electromagnetic force arises from exchange of virtual photons.[19][20] This reproduces general relativity in the classical limit. However, this approach fails at short distances of the order of the Planck length,[18] where a more complete theory of quantum gravity (or a new approach to quantum mechanics) is required."[/color]
http://en.wikipedia....i/Planck_length
Edited by Dino Might, 09 April 2015 - 11:01 AM.