Cosmic microwave background offers evidence of gas flowing in galaxy clusters
The cosmic microwave background (CMB) is a faint glow in the universe dating back to roughly 380,000 years after the Big Bang, long before stars or galaxies emerged. Detecting this light and mapping its fluctuations provide valuable insights into the age and composition of the un
The cosmic microwave background (CMB) is a faint glow in the universe dating back to roughly 380,000 years after the Big Bang, long before stars or galaxies emerged. Detecting this light and mapping its fluctuations provide valuable insights into the age and composition of the un This story matters for Science & Discovery readers tracking student. Reported by phys.org. Read the full original at the source link below.
Originally reported by phys.org. StudentNewsletter.com curates and briefs the science & discovery stories that matter. Our editorial policy →
Get the daily student signal