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Wendy Freedman

👤 Person
333 total appearances

Appearances Over Time

Podcast Appearances

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

And then WMAP, the Wilkinson Microwave Anisotropy Probe,

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

first measurements of all sky in space for the microwave background got a value of 71.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

So it looked pretty good.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

And the acceleration of the universe had been discovered.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

The age was something like 13.7 or 13.8 billion years.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

And wow, here you are measuring locally using stars and you're using

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

The redshift of 1100, 380,000 years after the Big Bang, you're making these tiny measurements of the temperature differences.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

And boy, they agree pretty well.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

That is a measurement of how fast the universe is expanding at the current time.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

It has units of inverse time.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

So it is also a way of getting at the age of the universe.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

in detail is kilometers per second per megaparsec.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

So when we talk about a Hubble constant of 70, we mean 70 kilometers per second per megaparsec.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

Yes.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

Exactly.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

That was Edwin Hubble's original discovery.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

What he showed is the farther away a galaxy is, the faster it's moving away from us.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

The slope of that correlation is the Hubble constant.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

That is the expansion rate at time t equals zero, now.

StarTalk Radio
Solving the Crisis in Cosmology with Wendy Freedman

We could be missing things.