0:00
Hi, everybody.
00:01
So we got to compare the following stages.
00:04
So a human being with a star.
00:06
And what does a star with mass of the sun in doing each of these stages? so stars have a life cycle, which we obviously know because of the question.
00:16
And so we have like a human life.
00:20
So we start from output.
00:23
Let's do this.
00:24
Let's do human and star over here.
00:32
Okay, so we start as a zygote, and we grow up to become a fetus, and we grow up to become a fetus, okay? and it takes to birth and grows in a small kid to adolescence.
00:48
So we get fetus, baby, child, young adult, adult, old age.
01:10
And then i guess we have death.
01:13
And you guys, you can delete some of these if you feel like it.
01:16
So stars have the same pattern.
01:19
So a star is concentrated in a cloud's inner serum.
01:22
So we have a nebula.
01:27
And so whenever it becomes dense, so this nebula comes dense, we'll write, becomes dense and collapse.
01:50
And while the collapsing in the region is considered matter, it will heat up and grow to form a new star.
01:56
And so then then heats up and then we have a new star.
02:09
Okay.
02:10
And this phenomenon can be called a birth of a star.
02:12
So we'll put birth.
02:17
Okay.
02:18
And that can line up to about here on our graph.
02:22
I just didn't write birth, but we can write birth here.
02:26
Okay.
02:29
And so if a star has enough matter, then the central temperature will reach 15 million degrees.
02:35
So we'll put 15 million degrees...