SimplePrimate said:In the detection of Cosmic Microwave Background Radiation I understand there's still some low frequency radio astronomy left to do before hitting the 'opaque universe' boundary where/when light could not propagate. What, if anything, can we still hope see?
Scientists have gathered evidence of the early Universe through various methods such as observing the cosmic microwave background radiation, studying the distribution of galaxies and clusters, and measuring the abundance of elements in the Universe. These pieces of evidence provide insights into the conditions and events that occurred in the early Universe.
The farthest we can see back in time is to about 380,000 years after the Big Bang, when the Universe was still in its infancy. This is when the cosmic microwave background radiation was released and can be observed today. Beyond this point, the Universe was too hot and dense for light to travel freely, making it impossible for us to see any further back in time.
Studying the early Universe allows us to understand the fundamental laws of physics and how the Universe evolved over time. It also helps us to answer fundamental questions about the origin of the Universe, the formation of galaxies and structures, and the nature of dark matter and dark energy. This knowledge can also lead to technological advancements and further our understanding of our place in the Universe.
Scientists have determined the age of the Universe to be approximately 13.8 billion years old through various methods, including measuring the expansion rate of the Universe, studying the cosmic microwave background radiation, and observing the ages of the oldest stars in the Universe. These methods all point to a similar age, providing strong evidence for the age of the Universe.
While we have made significant progress in understanding the early Universe, there are still many mysteries that remain. Some of these include the nature of dark matter and dark energy, the origin of cosmic inflation, and the reason for the asymmetry between matter and antimatter in the Universe. Scientists continue to study and gather evidence to unravel these mysteries and gain a deeper understanding of the early Universe.