With our current technology, we are already capable of observing and studying stars outside of our solar system. In fact, astronomers have been observing and studying stars beyond our solar system for many years. The field of astronomy dedicated to the study of these distant stars is known as astrophysics.
One of the key techniques used to study stars beyond our solar system is called spectroscopy. By analyzing the light emitted or absorbed by a star, astronomers can gather information about its composition, temperature, distance, and other properties. Additionally, advancements in telescopes and detectors have allowed us to detect and characterize exoplanets (planets orbiting stars outside our solar system) by observing their effects on their host stars.
As technology continues to advance, it is likely that our ability to observe and study stars outside our solar system will improve. New telescopes and instruments, both ground-based and space-based, are being developed and planned that will provide even more detailed observations of distant stars. These advancements will enable us to gather more data and increase our understanding of the universe.
However, it's important to note that there are limitations to how much detail we can obtain about individual stars located extremely far away. Factors such as distance, brightness, and atmospheric interference can impact our observations. Nevertheless, the future holds promise for further advancements in technology and techniques that will enhance our ability to study stars beyond our solar system.