The early Universe was more uniform and less clumpy, evolving into today's vast cosmic web filled with galaxies, stars, and planets, demonstrating a profound transformation over billions of years.
As the Universe expands, it cools; photons dilute and their wavelengths stretch, which explains the transition from a hot Big Bang to the current cosmic background.
Temporal temperature relationships in the Universe’s evolution aren’t straightforward, illustrating the complexities of cosmological physics beyond just the initial hot, dense state.
The cosmic microwave background is a pivotal discovery revealing crucial insights into the Universe's hot, dense origins, framing our understanding of cosmic expansion and evolution.
#cosmic-evolution #hot-big-bang #cosmic-microwave-background #universe-expansion #temperature-and-time
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