When the white dwarf nears the old star, the strong gravitational pull causes the material of the old star to boil, forming a torrent that throws itself at the white dwarf.

Undoubtedly, a spectacle was formed in the Gemini galaxy at this time.

Two white dwarfs orbit the star, constantly devouring the material of the older star.

However, such devouring is too slow for a white dwarf asteroid.

At this rate, I am afraid that it will take tens of millions of years before this old star can be swallowed cleanly.

So in the end, the white dwarf asteroid rushed straight into the old star.

In an instant, with the entry of the white dwarf asteroid, a hole appeared in the body of the old star, and this hole moved with the movement of the white dwarf asteroid, so that the material flow of the old star began to accelerate.

The size of the white dwarf asteroid also begins to slowly increase over time.

This process lasted a month!

Over the course of a month, the mass of the aged stars has lost more than 15 percent!

This massive mass loss also caused the internal structure of the old star to begin to collapse rapidly.

In three months at most, the elderly star will have an earth-shattering supernova explosion because it is approaching the end of its life!

As a result, both white dwarfs and white dwarf asteroids will be pushed far away due to violent supernova explosions.

So the white dwarf asteroid immediately shifted its target and rushed towards the white dwarf.

When two white dwarfs collided with each other, a violent explosion occurred.

The only thing to be thankful for is that the white dwarf asteroid was manipulated by Wang Dashu and had its own wisdom, so the collision between the two ended in the victory of the white dwarf asteroid.

The white dwarf asteroid that devoured the white dwarf has doubled in size, but due to the violent impact and engulfment, its otherwise smooth surface has some wrinkles.

But that didn't mean much, and the white dwarf asteroid crashed into the old star's body again and headed straight for its core.

For today's white dwarf asteroids, the only valuable place for an old star is the core.

The whole is already full of empty old stars, and then slowly devoured, the efficiency is too poor, and the core area with ultra-high temperature and high density is different.

Here, white dwarf asteroids can easily swallow massive amounts of stellar material.

That's almost four-fifths the size of the white dwarf that preceded it!

The most important thing is to devour fast enough.

In less than three days, the core of the old star becomes blank, and the material of the entire star begins to collapse inward due to its own gravitational pull.

Before that, the white dwarf asteroid quickly separated from the star, and after pulling a distance of billions of kilometers, Wang Dashu planned to take a closer look at the grandeur of this supernova explosion.

That's right, in the real universe, supernova explosions should be called the most spectacular astronomical phenomenon.

This supernova explosion is indeed spectacular.

In an instant, the brightness of the old star reached its limit, as if the entire universe was enveloped in white light.

Massive amounts of stellar material are ejected, forming a torrent that rushes outward.

Even the white dwarf asteroids were pushed by this torrent for a long distance.

After the white dwarf asteroid returned, Wang Dashu was a little surprised.

That old star didn't end up forming a white dwarf, but a neutron star!

Neutron star, Wang Dashu knows.

If three to ten percent of stars form white dwarfs after a supernova explosion, then neutron stars form only a few thousandths of a thousandth, and only stars with masses between 8 and 30 times the mass of the Sun are possible.

The old star before this was less than 20 percent larger than the Sun.

Such an old star actually formed a neutron star after the supernova explosion, which really made Wang Dashu a little unexpected.

But then again, when the white dwarf asteroid got closer, it was discovered that the size of this neutron star was unexpectedly small.

The normal size of a neutron star is between 2,000 meters and 10,000 meters in diameter, but the diameter of this neutron star is only about 300 meters!

Well, with a diameter of three hundred meters, it is almost several times larger than the volume of an aircraft carrier, and if you put it on the Blue Star, it is only the volume of a skyscraper.

And a neutron star of this size still has a gravitational pull tens of millions of times stronger than that of a white dwarf!

When the white dwarf came too close to the miniature neutron star, the gravitational pull of the two sides created a huge suction force, making it impossible for the white dwarf to break free and had to rush towards the neutron star.

Wang Dashu is not too worried about this.

If it is a neutron star of normal size, it is very dangerous for a white dwarf asteroid to collide with it.

But this neutron star is only one-seventh the diameter of a normal neutron star and 3.5 thousandths of a volume, and an impact is dangerous, but not that big.

The collision occurred two hours after the two sides approached.

The white dwarf asteroid, which is already more than 1,100 kilometers in diameter, is like a piece of tofu being shot into it, and the bullet stops in the core of the white dwarf asteroid in an instant.

The next moment, the white dwarf asteroid collapsed under the incomparably strong gravitational pull of the neutron star.

The white dwarf asteroid, which relies on electron degeneracy pressure to support its structure, began to shrink rapidly, and electrons were pressed into protons to form neutrons, and the distance between neutrons began to be infinitely closer.

To put it bluntly, the electron orbital of the atom disappears completely, and the nucleus and the nucleus are close together as if they were brothers.

The whole process is like a magic shrinkage, the white dwarf asteroid quickly shrinks, and finally becomes a layer of skin that clings to the neutron star!

Of course, the neutron star has also increased in size by a factor of about 1.78, and its diameter has increased by about 50 meters.

This time, the soul of the white dwarf asteroid was scattered at the first time, so it did not suffer much damage in the subsequent compression collapse.

The only problem is that it will take more than three months for the white dwarf asteroid to regain its soul, and it needs Wang Dashu to keep his mind connected and fully blessed!

Don't think that full stat blessings are useless against white dwarf asteroids!

On the contrary, the use of comprehensive attribute blessings on white dwarf asteroids is far greater than that of other clones!

The main reason for this is that the blessing of intelligence and perception attributes plays the greatest role, which can make the souls of the white dwarf asteroid accelerate the speed of convergence and control a part of the neutron star body in the shortest time.

I have to say that Wang Dashu is satisfied with this.

As long as the white dwarf asteroid swallows up this neutron star, then it is equivalent to controlling two neutron war stars in your own hands!