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∙ 12y agocore, radioactive zone, convection zone
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∙ 12y agoThe layers of the sun from inside out are the core, radiative zone, convective zone, photosphere, chromosphere, and corona. The core is the densest layer, with a density of about 150 g/cm3. As you move outward, the density decreases, with the corona being the least dense layer.
No, the densities of the Galilean moons do not increase with distance from Jupiter. The densities of the Galilean moons are not correlated with their distance from Jupiter, unlike the pattern seen in the densities of planets increasing with distance from the Sun.
The four main layers of the Sun are the core, radiative zone, convective zone, and the photosphere. These layers make up the internal structure of the Sun, with each layer playing a unique role in the Sun's energy production and transfer processes.
The sun has an extremely powerful gravitational field, and as a result, denser materials tend to fall to the lower layers.
They do not come from the sunspot. They can be anywhere in the sun,
No, the temperature in the layers of the sun's atmosphere is not evenly distributed. The temperature increases with height, transitioning from cooler regions like the photosphere to hotter regions like the corona. This temperature variation is due to the way energy is transported and distributed through the layers of the sun.
No, the sun's structure is not uniform throughout its interior. The sun has different layers, including the core where nuclear fusion occurs, the radiative zone, and the convective zone. These layers have different temperatures and densities, leading to distinct regions with varying properties.
The fluids with highest densities form the lowest layers. The fluids with lowest densities form the highest layers.
There are actually 5 layers. Going from the inside out they are: Thermonuclear Core, Radiative Zone, Convective Zone, Photosphere, and the Chromosphere.
It has 6 layers which are, from inside towards the surface:-CoreRadiative zoneConvective zonePhotosphereChromosphereCoronaIt also has features which appear in its outer layers:SunspotGranulesProminences
The outer layers can be seen directly; the inner layers can't, to a great extent (though neutrinos from the nuclear reactions get out immediately, and can be observed). Much of what happens inside the Sun is deduction, from what is known about how matter behaves.
The refraction of light through air layers of different densities is called atmospheric refraction. This phenomenon causes the path of light to bend as it passes through the different layers, resulting in optical effects such as mirages.
True. Liquids with different densities that do not mix will naturally separate and form distinct layers based on their respective densities, with the denser liquid settling at the bottom and the less dense liquid layering on top. This phenomenon is known as liquid stratification.
Yes, the Earth is composed of different layers with varying compositions and densities. These layers include the crust, mantle, outer core, and inner core. Each layer has distinct physical and chemical properties, which contribute to the Earth's overall structure and behavior.
Yes, that's correct. Liquids that do not mix due to differences in density will form distinct layers based on their respective densities, with the less dense liquid typically floating on top of the denser one. This phenomenon is known as stratification.
They form individual layers depending on their densities...the liquids with lighter density floats on liquid with heavier density......
No, the densities of the Galilean moons do not increase with distance from Jupiter. The densities of the Galilean moons are not correlated with their distance from Jupiter, unlike the pattern seen in the densities of planets increasing with distance from the Sun.
the outside