Chapter 71 White Dwarf Star
In the silent blackness of space.
A giant hydrogen cloud drifts slowly.
This huge hydrogen cloud was formed from an interstellar hydrogen group during a Supernova Explosion, possessing a mass of over ten Constant Star Masses.
When the nebula group attracts the light of the universe, it displays an array of colorful streams, as if a divine hand has painted an exquisitely beautiful oil painting in the universe.
Later, after a long period of drifting.
This giant hydrogen cloud slowly moved away from the remnants of the Supernova Explosion, entering deeper cosmic space.
One day, this giant hydrogen cloud encountered a White Dwarf Star formed from the death of a small-mass star, influenced by the White Dwarf Star’s gravity, they began to draw closer to each other.
This White Dwarf Star, in its lifetime, had a mass of over three thousand Constant Star Masses, after death, its surface gases dissipated, leaving only a White Dwarf composed of countless carbon atoms.
The surface temperature of the White Dwarf Star is over eight thousand degrees, emitting a faint white light, from afar, it does not look as dazzling as a Constant Star, instead, it resembles a relatively soft white light orb.
However, even a White Dwarf Star is not eternal, after about 20 billion years of a long glowing period, it will gradually cool down and darken, turning into a completely dead black dwarf star!