The expansion of the universe is a concept that can be difficult to visualize, especially when it comes to the question of where we will end up. However, it's important to note that the expansion of the universe does not necessarily imply a specific destination or an endpoint that we are moving towards.
The expansion of the universe refers to the idea that the distances between galaxies and other cosmic structures are increasing over time. It is often described as the stretching of the fabric of space itself. To help understand this concept, imagine drawing dots on the surface of an inflating balloon. As the balloon expands, the dots move away from each other, but there is no central point to which they are all converging.
Similarly, in the context of the universe, the expansion means that galaxies are moving away from each other as space itself expands. However, this expansion is happening on a cosmological scale and does not have a specific "end" or direction in the conventional sense. It is more accurate to think of the expansion as a stretching of the fabric of space on a grand scale, rather than a motion towards a particular location.
It's worth noting that our current understanding of the universe's expansion is based on observations and theoretical models. There is ongoing research to refine and expand our understanding of this complex phenomenon. While we may not have a complete picture yet, scientists continue to study the expansion of the universe to deepen our understanding of its nature and implications.