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First, this seems pretty unlikely for the foreseeable future -- there's no evidence of a full sized black hole anywhere near earth (Chandrasehkar's limit says neutron stars can't occur at less and 1.44 solar mass, and stellar black holes are believed to occur at no less than 3 solar masses, and possibly more).

Smaller, primordial black holes may (or may not) once have existed, but Stephen Hawking's work on Hawking Radiation shows that, the smaller the black hole, the more energy gets expelled, hence quantum black holes (tiny ones) are likely to "evaporate".

However, if we imagine that there was a black hole very near the earth, we'd first see tidal effects as the earth responded to the gravitational field of the stellar body. Depending on how far away the earth and our imaginary black hole are, we conceivably could go into a stable orbit around it (although, dependiing on the mass, the accretion disk of the black hole might well emit enough radiation to cook us). Farther in, the earth would eventually spiral into the Schwarzchild radius. Once i9nside the Schwarzchild radius, it is postualted we could (a) see the incoming light from another universe (whimsically named "elsewhere" because "you can't get there from here"). Also, some of Hawking's work hints that, while traval along the spatial axes would no longer be mutable (as they are here in n-space, where we can travel freely spatially, but only in one direction in time), temporal travel would, in a manner of speaking, be possible.

On the other hand, Einstein's concepts of relativity give us some real problems here, particularly time dilation. Briefly, the following assumptions are made (and so far have not been disproven):

  • The effects of gravity are indistinguishable from accelleration.
  • When viewed by an external observer, an object accellerating towrds the speed of light moves more slowly through time.
  • And, from a relative observer's standpoint, that object accellerating towards the speed of light reaches c or light speed exactly an infinite number of years in the relative observer's future.

This implies that, if there was a black hole across the room from you (all other effects notwithstanding) and you fired a bullet into it, you would see the bullet slow and come to an apparent stop (relative to you), before it could cross the event horizon. This is because gravity and accelleration are indistinguishable, so the grvaity at the event horizon is equivalent to a lightspeed effect. This in turn means that, outside the black hole, one cannot observe matter passing the event horizon.

How this works in reality is a bit of a mystery. Of course, we cannot "see" a black hole -- nothing escapes the Schwarzchild radius, so cannot be "obseved". But gravitational effects outside the event horizon can be seen. And we observe the binary star, Cygnus X-1, and note that for two comparatively cool stars, that body is emmiting a huge amount of x-ray radiation. Coupling that with observations of eccentricities in X-1a and X-1b's orbits, we postulate the existing of a super-dense object of perhaps 10 solar masses, i.e. a black hole, As the black hole sucks in matter, friction heats, then superheats that matter, which forms an accretion disk as it falls into the black hole. So, we have a superhot, brightly glowing disk surrounding the black hole, as well as two stars that are sharing matter with each other and quite possibly the black hole too.

We see the xray radiation, which indicates the presence of an accretion disk, so we assume matter IS falling into the black hole.

So -- in answer to your question -- one possiblity is we enter the black hole, see the stars shining in elsewhere, and possibly travel in time, perhaps exiting the black hole an infinite number of years in the past -- or perhaps not. Also, there's the possibility that, due to Xeno's paradox, you'll never actually see anything go past the Schwarzchild radius.

Hope this helped. yes it did help sry but i wanted to add hat whoever u r who gave this answer nice job i think it is the best answer yet

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