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Lifecycle of the Sun - Contenido educativo

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Subido el 15 de mayo de 2024 por Maria Jesús T.

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This project shows how to calculate the rotational period of the Sun, as well as its lifecycle through history.

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Welcome to the next video about our beloved star, the Sun. 00:00:01
We are a team of scientists and engineers who study the stars and outer space. 00:00:05
Have you ever wondered how the stars are born, or how then our Sun will die? 00:00:11
Or even, does the Sun rotate? 00:00:18
If that is the case, then keep watching to see the answers of my teammates. 00:00:20
Hi! We are Erika, Kike and me, Akram, and we are going to show you how the Sun evolved during its life. 00:00:26
At the very beginning, about 5 billion years ago, our star was just a large cloud of gas and dirt with many different colors, 00:00:33
called stellar nebula, just like confetti. 00:00:40
Then it began to shrink and its density increased, forming a baby Sun. 00:00:43
Observing other stars with similar sizes, astronomers have been able to say how it will evolve during the following billions of years. 00:00:48
of years that's right and don't worry the Sun won't die in the near future and 00:00:55
we won't be able to see it as it will happen in another five billion years but 00:01:01
before its death it will grow and grow and grow to become a red giant and it 00:01:07
will engulf Mercury and Venus and perhaps Earth then it will start to 00:01:14
shrink again and when it fades away it will become a small white dwarf. There 00:01:20
won't be any explosions or supernovas? I'm sorry but that will never happen to 00:01:28
our Sun. It's way too small to become a black hole like many people may think. 00:01:34
Now I guess you want to see some experiments right? Well Kike will show 00:01:39
you how to represent the life of the Sun in just two easy experiments. The first 00:01:45
In the next experiments we will show you how the atoms are expelled from the star throughout its life cycle. 00:01:48
To do so, we will hold a tennis ball on a basketball and let them fall. 00:01:55
The tennis ball will be launched into the air really fast. 00:02:01
To try it, our second experiment consists of showing how the sun will die. 00:02:05
We will represent the sun with a balloon full of color powder. 00:02:11
We need to inflate the balloon as much as we can and then pop it. 00:02:14
This is the form of a cloud of colors called the planetary nebula. 00:02:20
And that is the way that a normal star will die, but our sun, no. 00:02:27
That sounds really nice. 00:02:33
You've explained everything about the sun's life cycle, but we don't know yet if it rotates. 00:02:35
Can you tell us, Diego? 00:02:40
Yes, the Sun rotates, indeed, but not like our parent does. The Sun is made of plasma and there is no soil to hold it together. 00:02:42
Therefore, the Earth's middle equator rotates faster than the one at the poles. 00:02:54
Interesting, but how can we know that? 00:02:59
By comparing the latitudes and longitudes of a sunspot during a period of time. 00:03:03
This way, we know the speed at which it is moving, and we can calculate the Euler's rotational period and the differential rotation. 00:03:08
And why did you all decide to talk about these two topics? 00:03:17
We thought it was important that everyone knew that the Sun was an average star, which won't die as a supernova, 00:03:21
or that it doesn't rotate at the same speed as Euler's old RS. 00:03:27
The Sun is, after all, our nearest star, and it would so learn as much as possible we could about it. 00:03:33
And you? Do you think it's important to know a lot of information about the universe outside our world? 00:03:42
We hope you have enjoyed the video and that it has inspired you to share some more about the Sun. Goodbye! 00:03:49
Idioma/s:
en
Idioma/s subtítulos:
en
Autor/es:
Enrique G., Akram O., Erika R., Diego S., Victoria P.
Subido por:
Maria Jesús T.
Licencia:
Todos los derechos reservados
Visualizaciones:
5
Fecha:
15 de mayo de 2024 - 10:08
Visibilidad:
Clave
Centro:
IES PRINCIPE FELIPE
Duración:
04′ 05″
Relación de aspecto:
1.00:1
Resolución:
1080x1080 píxeles
Tamaño:
54.55 MBytes

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