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Ep 255: Prebiotic evolution part 2: DNA and RNA

Ep 255: Prebiotic evolution part 2: DNA and RNA

Prebiotic evolution part 2: DNA and RNA

DNA cannot copy itself. It needs enzymes, very large complicated proteins to replicate from one cell to a new one. The way the proteins are produced requires DNA and RNA. All three types of molecule have to be present in a cell for the cell to work. What exactly are DNA and RNA, and how did all this complicated business get started? Join us for the conclusion of our look at the evolution that happened before evolution.

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Ep 254: Prebiotic evolution part 1: proteins

Ep 254: Prebiotic evolution part 1: proteins

Prebiotic evolution part 1: proteins

Most of the way your cells do what they do is by using proteins. Proteins are made by life. But if life makes proteins and life needs proteins, where did the first proteins come from? Join us for part 1 of our investigation of the evolution before evolution—the building up of the complex chemicals needed for the beginning of life.

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Ep 253: The solar system’s greatest hits

Ep 253: The solar system’s greatest hits

The solar system’s greatest hits

After gravity managed to make some decent sized planets, they started getting smashed together with almost planet sized bits and pieces. These impacts may be responsible for our oceans, and perhaps even for life on our planet, but it was not an easy ride. Join us for a look at some of the biggest collisions in our inner solar system, and the huge scars that were left behind.

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Ep 252: From gas and dust, to all of us

Ep 252: From gas and dust, to all of us

From gas and dust, to all of us

The general idea is simple—a cloud of gas and dust collapses in on itself, driven by gravity, until roughly in the middle of it, our sun began to shine. But the details are somewhat odd, especially when we compare our solar system to what we’re able to observe of planets around other stars. What triggered the original collapse? Why does our sun spin so slowly? Where did the earth’s water come from? How and why did our solar system end up with nice stable, nearly circular orbits that gave life on earth billions of years of relative peace? There’s plenty of room for competing theories and interesting side trips as we take a look at the birth of our sun and planets.

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Ep 251: making the ingredients

Ep 251: making the ingredients

making the ingredients

Before our planet could form, all the stuff one would like to make a planet out of had to be made. Starting with hydrogen and helium, stars had to cook up the rest of the periodic table over a nice long period. Toss in some explosions and collisions, and everything we’re made of was ready to make us. But, all those giant stars couldn’t even get started, if it weren’t for a quirk of how the tiniest pieces of the universe interact. But hey, what’s a little quantum physics amongst friends?

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Ep 250: Just after the beginning

Ep 250: Just after the beginning

Just after the beginning

The standard model of cosmology has been worked out, slowly and painfully and oh so very carefully. Only trouble is, some recent observations don’t quite match what the theory predicts. Join us for a timeline of the early universe, and some of what doesn’t quite match what we were expecting.

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Ep 249: Figuring out the neighborhood

Ep 249: Figuring out the neighborhood

Figuring out the neighborhood

From the surface of Earth, the sun and moon look to be about the same size. Other planets are tiny specks of light, and everything seemingly spins around us. But that’s not what our solar system is really like. So, how did we find out what was where, and which way things were moving?

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Ep 248: The matter of dark matter

Ep 248: The matter of dark matter

The matter of dark matter

From the rotation of our own Milky Way galaxy, to the expansion of the universe, much of the night sky is moving in ways we can’t quite explain. To plug the wholes in our understanding we have dark energy and dark matter. We don’t actually know what they are, but they can still surprise us.

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Ep 247: In the beginning, part 2: the lost episode

Ep 247: In the beginning, part 2: the lost episode

In the beginning, part 2.

After covering history and background in the last episode, we can relax and play with the strange ideas and concepts surrounding the theory of the big bang. The event horizon around our universe, the way that time flows differently depending on where you are, how parts of the early universe may have run away and become impossible to observe, and even a theory we propose with no math and fewer reasons.

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Ep 246: In the beginning, part 1.

Ep 246: In the beginning, part 1.

In the beginning, part 1.

Before 1923, the universe was thought to be static and eternal, unchanging and without beginning or end. Its size was likely just a few tens of thousands of lightyears across, with one large island of stars, our galaxy, the Milky Way. Discoveries showed us that the universe is much larger than we thought, and is getting bigger all the time. The universe seems to have had a beginning, and might even, one day, come to an end. Join us for a talk about how we got notions like the big bang and the expanding universe.

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