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Yes it is! Just like the sun. Its Corona is very hot.
When a star runs out of energy, its mass is so great that the remaining energy cannot force the outer edges of a star away from its core, so the gravity causes the star to implode on itself.
The layer of gases that covers a planet, star or moon is called the atmosphere.
The explosion of novae hardly disturb the white dwarf or its companion star. Mass transfer resumes and a new layer of fuel can accumulate so that the process can happen all over again. In a supernovae, its the death of a star. Its theory that the outer layers of a massive star produces the supernovae while the core collapses to form a neutron star or black hole.
An average star, which is what our sun is, will actively fuse hydrogen into helium for a few billion years (exact time varies based on mass), then it slowly expands int a giant star. Then, the star's outer layer of gases puff off and become a planetary nebula, where its hot core is exposed as a white dwarf. The star reddens and cools, then stops burning and becomes a black dwarf.
Magnetosphere is the layer above the photospere.
The photosphere is the outer part of the star that is visible, inside which the star becomes opaque to visible light. The photosphere is the layer below the star's atmosphere (the chromosphere, and so forth).
A Red Giant
Yes it is! Just like the sun. Its Corona is very hot.
The color of the light radiated by the spectra can show the internal composition as well as the gases burning on the outer layer. Red stars are colder and blue stars are hotter.
Meteors come from outer space and crash into our atmosphere which burns them. That's what a shooting star is.
A simple version - Draw a star (on a transparent background and fill the start with white. Go to Layer - Layer style and set the layer style to outer glow , set the size to about 80% and the opacity to 40% The star shape may also be in the default shapes in the tool bar depending on you version of PS
When a star runs out of energy, its mass is so great that the remaining energy cannot force the outer edges of a star away from its core, so the gravity causes the star to implode on itself.
Depends on the mass of the star. A star the size of our Sun will eject its outer layers, forming a planetary nebula with the core of the star exposed, cooling to become a white dwarf. Larger mass stars will explode as a supernova, creating a shock wave of stellar matter, the core either condensing to a neutron star or a black hole.
Our sun release energy by a process called convection. Inside the star, energy is transported towards the surface through radiation, but about 1/3 of the outer layer of the star is markedly cooler than the core and the energy is transported by convection from the core to this layer.
When hydrogen in the core of the star is depleted, a balance no longer exists between pressure and gravity. Core contracts, temperatures incrase. This causes outer layers to expand and cool. This star is called a GIANT.
The corona of a star is the outer layer, mostly comprised of plasma. In the case of the Sun, the corona is what becomes visible in the event of a solar eclipse. Do not look directly at it. It can and will blind you.