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total amount of energy emitted per unit of time by a star, galaxy, or other astronomical object

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release of plasma and accompanying magnetic field from the solar corona.

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1. the rarefied gaseous envelope of the sun and other stars. The sun's corona is normally visible only during a total solar eclipse when it is seen as an irregularly shaped pearly glow surrounding the darkened disk of the moon.

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hot plasma rises, cools as it nears the surface, and falls to be heated and rise again.

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a reddish gaseous layer immediately above the photosphere of the sun or another star. Together with the corona, it constitutes the star's outer atmosphere

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A region of space-time exhibiting such strong gravitational effects that nothing—not even particles and electromagnetic radiation such as light can escape from inside it. The theory of general relativity predicts that a sufficiently compact mass can deform space-time to form a black hole.

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a small very dense star that is typically the size of a planet. A white dwarf is formed when a low-mass star has exhausted all its central nuclear fuel and lost its outer layers as a planetary nebula.

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a very large star that is even brighter than a giant, often despite being relatively cool.

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A sudden flash of increased brightness on the Sun, usually observed near its surface and in close proximity to a sunspot group. Powerful flares are often, but not always, accompanied by a coronal mass ejection. Even the most powerful flares are barely detectable in the total solar irradiance.

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a spot or patch appearing from time to time on the sun's surface, appearing dark by contrast with its surroundings.

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a very large star of high luminosity and low surface temperature. Red giants are thought to be in a late stage of evolution when no hydrogen remains in the core to fuel nuclear fusion.

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a contracting mass of gas that represents an early stage in the formation of a star, before nucleolus thesis has begun

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a ring-shaped nebula formed by an expanding shell of gas around an aging star.

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the luminous envelope of a star from which its light and heat radiate.

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the collapsed core of a large star which before collapse had a total of between 10 and 29 solar masses

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a cloud of gas and dust in outer space, visible in the night sky either as an indistinct bright patch or as a dark silhouette against other luminous matter.

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continuous and distinctive band of stars that appear on plots of stellar color versus brightness.

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The brilliant point of light is the explosion of a star that has reached the end of its life, otherwise known as a supernova. Supernovae can briefly outshine entire galaxies and radiate more energy than our sun will in its entire lifetime. They're also the primary source of heavy elements in the universe.