The concept of "seeing" the Big Bang is a bit complex because the Big Bang itself was not an explosion that occurred at a specific point in space. It was the beginning of the expansion of the universe from an extremely hot and dense state. The universe has been expanding and cooling down ever since.
As we trace the expansion of the universe back in time, we eventually reach a point called the cosmic microwave background (CMB). The CMB is the residual radiation left over from the hot, dense early universe. It is like a faint glow that permeates space and can be detected as microwave radiation. The CMB provides valuable information about the early universe, including its temperature and density fluctuations.
If we were able to travel back in time to the epoch of the CMB, we would not "see" the Big Bang directly. Instead, we would encounter a hot and dense plasma, the primordial soup of particles and radiation that existed during the early stages of the universe. The conditions would be extremely intense, and it is uncertain what we would perceive or experience in such an environment.
However, it's important to note that our current understanding of physics breaks down when we try to describe the exact conditions at the very beginning of the universe. The laws of physics as we know them may not be applicable in such extreme scenarios. The concept of time itself becomes uncertain near the Big Bang, so the idea of "traveling back" to that point is a challenging one to address within our current scientific framework.