Chapter 138: Core Area Collision
After the core areas of the Galaxy Nebula and the Andromeda Nebula were exposed,
one could see that they were mostly composed of old Constant Stars, and there were even quite a few White Dwarf Stars.
The spacing between these old Constant Stars was not nearly as wide as that in the spiral arms; the closest ones were less than an astronomical unit apart, and the farthest ones were no more than ten light years away.
Moreover, due to their closer proximity to the central Black Hole, these old Constant Stars were bound by strong Gravity and unable to break free, only to rotate in tight circles around the central Black Hole.
Under normal circumstances, apart from the central Black Hole, the most abundant objects in the core areas of a Celestial Nebula are the old Constant Stars.
These old Constant Stars seem to huddle together to form clusters, collectively making up about ten percent of the total mass of the nebula, and because so many stars are clustered together, the core area is generally one of the thickest and highest parts of the nebula.
At the same time, the core area is also the brightest spot in the nebula.
Typically, there exists a halo layer at the edges of the core area, formed by the combined light emitted by billions of Constant Stars within the core area.
Besides, numerous gases and dust particles are bound by Gravity within this halo layer, becoming an interstellar medium layer that absorbs and reflects light.
One could imagine, when the densely packed core areas of these two nebulas collide, the energy released would be more terrifying than the combination of the previous four spiral arms, and the spectacle it displays would be the most brilliant, the most shocking, and the most spectacular scene in the entire grand collision.