# data[].attributes.body
The nebula and the supernova are the most similar because they both have to be compressed to create something.

# data[].attributes.body
Once all the gasses are pushed back a white dwarf appears. A white dwarf can be the size of a planet.

# data[].attributes.body
After the super giant explodes, a shock wave blows of the outer layers of the star.

# data[].attributes.body
In the few millions of years that the a star has is a super giant. A super giant will not stay for a long period because it rapidly is losing energy to power it self.

# data[].attributes.body
The star begins to release energy, stopping it from contracting even more and causes it to shine.

# data[].attributes.body
A protostar contains enough matter the central temperature reaches 15 million degrees centigrade.

# data[].attributes.body
The starting phase for all stars, including our Sun, begins when a dense region in a nebula begins to shrink and warm up.

# data[].attributes.body
A star is a ball of energy made out of 75% hydrogen and 15% helium. Our star (sun) is a yellow dwarf or also known as G2V. A star has 5 main layers. The core, the radiation zone, the convection zone, the photosphere, the chromosphere, and the corna which can only be seen during a solar eclipse. Our star is in its main sequence right now which means that is is halfway through its life.