the big questions
A wave is just the transfer of energy through space
Watch the red dot.
It never will make it over to the right side
Even if it seems like it, waves just pass through things, jiggling them back and forth...
Amplitude: The distance from the midline to the top of a wave
Frequency: How often a wave passes a point
Measured in meters
Measured in Hertz (waves per second)
Wavelength: the distance between each top of a wave
...or middle
...or bottom
Light is a wave.
Notice the wavelength of each color
Notice the frequency is different too!
1. Which color has the longest wavelength?
2. Which color has the greatest frequency?
Are any of them getting closer to the edge?
All light travels at the same velocity
All light travels at the same velocity
All light travels at the same velocity!
3. Which color travels fastest?
All waves work in the same ways.
We can describe a wave with only three characteristics:
Velocity (v)
Wavelength (λ)
Frequency (f)
Hooray!
That means we can use mAThs!
If we want to know the equation for wavelength, just cover up the wavelength symbol.
We are left with the equation:
Let's try to find the velocity of a wave!
We are left with the equation:
Ooh! We're trying to find v, so we cover that up
Can we paaleeease do another?!
We are left with the equation:
Ooh! We're trying to find f, so we cover that up
In the very early universe, only the smallest elements could form:
Hydrogen
Helium
and
*and maybe a tiny bit of Li and Be
This is a Nebula!
It is a clump of hydrogen dust in space, held together by gravity
Eventually, gravity will push all this hydrogen together hard enough to get fusion to happen
This explanation of where stars come from is called Nebular Theory
Bam!
This is a new star!
It starts its life fusing the smallest element, hydrogen
Bam!
Our new star that's fusing hydrogen, can be found on the HR Diagram
As it fuses hydrogen, it will sit here, on the Main Sequence
Bam!
Stars spend most of their lives on the main sequence.
Main Sequence
Our sun is in the main sequence still (that's a good thing!)
Bam!
When our sun runs out of hydrogen, it will start fusing helium, and become a Red Giant
Bam!
Once our sun has fused all of its helium into carbon, it has reached the end of its life...
And it will become a White Dwarf
That was the end of a Low Mass star.
High Mass stars have a different end to their stories...
Bam!
A High Mass star will also begin its life by fusing hydrogen.
But because it is so massive, it can fuse even larger elements in its core.
High mass stars have enough gravity to fuse elements all the way up to Iron!
For stars, it's all about that mass...
Bam!
When our high mass star reaches Iron, it begins to collapse on itself, and one of the biggest events ever happens...
Supernova
Bam!
It is these crazy-huge explosions of high mass stars that creates all the elements larger than Iron.
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