The latest catalog of spin rates suggests more massive stars spin more slowly than less massive stars.

At their peak spin rates, these maturing stars eject large amounts of stellar wind.

Kepler measures spin rates of stars in Pleiades cluster

In the 'ballet' of the Pleiades, we see that slow rotators tend to be more massive, whereas the fastest rotators tend to be very light stars, said Rebull.

As a star ages, its spin rate begins to slow down.

And they say, Oh, yeah. Constant acceleration.

Kepler measures each star's spin rate by tracking the time between the appearance of recognizable starspots like sunspots.

So what you would expect is that if you measured the orbital speed of the stars, that they should be slower on the edges than on the inside.

Flying speed is determined by convolutions

Star Density

Star color intensity

Constant

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Rebull likens the stars to dancers, larger ones pirouetting more slowly than smaller ones.

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Because the Pleiades cluster is so close, it serves as an ideal cosmic laboratory to compare stellar qualities with spin rates.

Law of Conservation of Mass

That's a limit imposed on the mass of stars.

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Let's say that you have the same thing, and let's say the initial velocity you're given the initial velocity, you're given the final velocity, you're given the acceleration, and you want to figure out the distance.

And this precise oxygen concentration, 10 parts per million, that caused suspended animation, is conserved.

The latest mission by the Kepler space telescope has helped astronomers collect the most complete catalog of spin rates among the stars of the Pleiades cluster.

We've learned over the last several videos that if we have a system undergoing constant pressure, or it's in an environment with constant pressure, that its change in enthalpy is equal to the heat added to the system.

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So once you have gravity, here's this increase the speed by something, increase the ship's speed.

Vessel contents should be heated at a constant rate independent of the heat being generated by the organic peroxide or self reactive substance.

Unable to determine maximum speed for some reason. Ignoring.

I've always been kind of slow making up my mind.

Cv the specific heat at constant volume

We still have a lot we want to learn about how, when and why stars slow their spin rates and hang up their 'dance shoes,' so to speak.

If it's constant, that means that the stars out here are feeling the gravitational effects of matter that we do not see.

We know that the average velocity is the final velocity plus the initial velocity divided by 2, so that's the average velocity let me highlight this is the same thing as this, and then that times time.

He was fast, fast on the draw.

Wants speed, let's give it to him.

The self was not constant.

Cv is the specific heat at constant volume.

The new data is helping astronomers understand why stars in the cluster spin at varying rates, as well as how rotation periods relate to planet formation.

And once again, I'm assuming constant pressure.