# data[].attributes.body
the brightness of a celestial object

# data[].attributes.body
a scatter plot of stars showing the relationship between the stars' absolute magnitudes or luminosity versus their stellar classifications or effective temperatures.

# data[].attributes.body
A significant release of plasma and accompanying magnetic field from the solar corona

# data[].attributes.body
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.

# data[].attributes.body
A region of turbulent plasma between a star's core and its visible photo sphere.

# data[].attributes.body
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.

# data[].attributes.body
A region of space having a gravitational field so intense that no matter or radiation can escape.

# data[].attributes.body
A white dwarf is formed when a low-mass star has exhausted all its central nuclear fuel

# data[].attributes.body
A very large star that is even brighter than a giant, often despite being relatively cool.

# data[].attributes.body
A sudden flash of increased brightness on the outer layer of the sun

# data[].attributes.body
A spot or patch appearing from time to time on the sun's surface, appearing dark by contrast with its surroundings.

# data[].attributes.body
A NASA mission which has been observing the Sun since 2010.

# data[].attributes.body
a very large star of high luminosity and low surface temperature.

# data[].attributes.body
a contracting mass of gas that represents an early stage in the formation of a star, before nucleosynthesis has begun.

# data[].attributes.body
a ring-shaped nebula formed by an expanding shell of gas around an aging star.

# data[].attributes.body
the luminous envelope of a star from which its light and heat radiate

# data[].attributes.body
A celestial object of very small radius (typically 18 miles/30 km) and very high density, composed predominantly of closely packed neutrons

# data[].attributes.body
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.

# data[].attributes.body
Main sequence stars fuse hydrogen atoms to form helium atoms in their cores. These stars can range from about a tenth of the mass of the sun to up to 200 times as massive.

# data[].attributes.body
A star that increases brightness due to a catastrophic explosion