The star cluster Westerlund 2 in the Milky Way galaxy, with an estimated age of about one or two million years. It contains some of the hottest, brightest, and most massive stars known. The cluster resides inside a stellar breeding ground known as Gum 29, located 20,000 light-years away in the constellation Carina.
The star cluster Westerlund 2 in the Milky Way galaxy, with an estimated age of about one or two million years. It contains some of the hottest, brightest, and most massive stars known. The cluster resides inside a stellar breeding ground known as Gum 29, located 20,000 light-years away in the constellation Carina.

Solving the Crisis in Cosmology with Wendy Freedman

NASA, ESA, the Hubble Heritage Team (STScI/AURA), A. Nota (ESA/STScI), and the Westerlund 2 Science Team, Public domain, via Wikimedia Commons
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About This Episode

Can we resolve the crisis in cosmology? Neil deGrasse Tyson and co-host Matt Kirshen take on Hubble Tension, the difference between the estimated ages of the universe, and how to solve it with legendary astronomer Wendy Freedman.

We trace the debate from the early days with Henrietta Leavitt’s discovery of Cepheid variables through today’s most precise measurements. Why do local distance measurements (Cepheids, tip of the red-giant branch, carbon stars) give a different expansion rate than the cosmic microwave background? Could dust be dimming our view, or systematic errors biasing our results? Or do we require discovering new physics?

We break down the Hubble tension and what caused it. How did the Hubble telescope complicate the existing debate, between 10 and 20 billion years old, through more precise measurements? We explore possible explanations: local density fluctuations, evolving dark energy, or something missing from the standard model. Are we missing something fundamental hiding in plain sight? Could the Hubble constant vary with time, or even by location in the universe?

Listener questions push the frontier further: Could dark energy distort our distance calculations? How would we measure expansion if we traveled to another galaxy? Would it matter scientifically, or emotionally, if the universe is finite or infinite? Through it all, Neil reminds us that science isn’t democracy, it’s data.

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