Like Its 7 9 Again Words in Empire of the Sun
What Are The Layers Of The Sunday?
- The layers of the Lord's day are divided into two larger groups, the outer and the inner layers. The outer layers are the Corona, the Transition Region, the Chromosphere, and the Photosphere, while the inner layers are the Cadre, the Radiative Zone, and the Convection Zone.
- There are four outer layers of the Sun, and the Corona is the outermost one. It starts at nearly 1300 miles in a higher place the photosphere, and its temperature is measured to be around 900,000 degrees Fahrenheit.
- There are three inner layers of the Sun, and the Convection zone is the outermost one. It completely surrounds the side by side layer, the Radiative zone, after which we have the Cadre, as the innermost layer of the Sun.
Just similar our planet, and well-nigh other celestial bodies, the Lord's day is divided into distinct layers. The disquisitional difference is that the Lord's day is non solid, different Earth, so the layers are a bit harder to determine. Because the Lord's day is more often than not equanimous of helium and hydrogen and is non solid, it does not have an outer boundary that is conspicuously defined.
Still, we tin can decide the internal structure of the Dominicus, and it is made up of 7 different layers. The layers of the Dominicus are divided into two larger groups, the outer and the inner layers. The outer layers are the Corona, the Transition Region, the Chromosphere, and the Photosphere, while the inner layers are the Core, the Radiative Zone, and the Convection Zone.
The Outer Layers
- Corona
- Transition region
- Chromosphere
- Photosphere
There are iv outer layers of the Sun, and the Corona is the outermost ane. It starts at about 1300 miles higher up the photosphere, and its temperature is measured to be around 900,000 degrees Fahrenheit. It is incommunicable to see the Corona with the naked middle, but there is an exception. We are able to run into it during a solar eclipse, or by using a special device called the coronagraph. There is no upper limit to the Corona.
It is followed by the Transition region, which is an extremely narrow layer that divides the Chromosphere from the Corona. Its width is simply 60 miles, which is incredibly small for a layer on a body every bit big every bit the Sun. This layer marks the spot where the temperatures rise tremendously since the Corona layer is much hotter than the Chromosphere.
The Chromosphere is the layer we detect between the distances of 250 and 1300 miles from the solar surface. The temperatures in this layer vary greatly, with the parts that are further from the solar surface being much hotter than the ones that are closer to it. Still, it does not compare to the temperatures that are reached in the Corona layer. It is an interesting affair to notice how the temperature in these layers grows the further away we motion from the center of the Sun.
The Photosphere is the last, innermost layer of the outer layers of the Dominicus. Nosotros are able to observe this layer straight, and its temperatures vary between xi,000 and 6,700 degrees Fahrenheit. The majority of this layer is covered by granulation, which is acquired past bubbling gases and sunspots from magnetic fields.
The Inner Layers
- Convection zone
- Radiative zone
- Cadre
At that place are three inner layers of the Lord's day, and the Convection zone is the outermost one. It completely surrounds the next layer, the Radiative zone.
In this layer, all of the hot textile plant near the center of the Sun rises cools down and drops back into the radiative zone to go more heat. This is the movement that creates sunspots and solar flares. This layer marks the border of what we unremarkably refer to as the Lord's day.
The radiative zone is the second inner layer of the Sun. It sits exterior of the cadre, and it holds its extremely loftier temperature. The zone itself has a temperature of around seven million degrees Fahrenheit. This layer serves as a passage for all the energy that is released by the core. Photons travel through the radiative zone, and they can't travel through long ranges of space, so it takes almost 50 million years for a photon to travel through this layer of the Sun.
Finally, we have the core, every bit the innermost layer of the Lord's day. The core is plasma, simply its movement is extremely similar to that of a gas. The temperature of the core of the Sun is around 27 million degrees Fahrenheit. In the cadre, nuclear reactions occur that create helium from hydrogen atoms. This releases huge amounts of energy, and it starts to move outwards toward the other layers. This energy eventually becomes the light and heat we receive on World.
Source: https://www.worldatlas.com/articles/what-are-the-layers-of-the-sun.html
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