# data[].attributes.body
http://solarsystem.nasa.gov/planets/sun/facts

https://www.nasa.gov/sun

# data[].attributes.body
The sun sends us more than heat and light; it sends lots of other energy and small particles our way. The protective magnetic field around Earth shields us from most of the energy and particles, and we don’t even notice them.

# data[].attributes.body
A solar flare is a sudden flash of brightness observed near the Sun's surface

# data[].attributes.body
A solar prominence is a large, bright feature extending outward from the Sun's surface.

# data[].attributes.body
A spot or patch appearing from time to time on the sun's surface

# data[].attributes.body
A corona is an aura of plasma that surrounds the sun and other stars. The Sun's corona extends millions of kilometres into space and is most easily seen during a total solar eclipse.

# data[].attributes.body
The chromosphere is the second of the three main layers in the Sun's atmosphere and is roughly 3,000 to 5,000 kilometers deep. The chromosphere's red color is only apparent during eclipses.

# data[].attributes.body
The photosphere is the visible surface of the Sun that we are most familiar with. Since the Sun is a ball of gas, this is not a solid surface but is actually a layer about 100 km thick

# data[].attributes.body
It extends from a depth of 200,000 km up to the visible surface of the Sun. Energy is transported by convection in this region.

# data[].attributes.body
The section of the solar interior between the innermost core and the outer convective zone. In the radiative zone, energy generated by nuclear fusion in the core moves outward as electromagnetic radiation.

# data[].attributes.body
The central region where nuclear reactions consume hydrogen to form helium