Chapter 1033: Chapter 1028 Trouble 4_1 Chapter 1033: Chapter 1028 Trouble 4_1 “This is a dying star entering its final phase; of course, that’s in stellar terms.
For humans, it’s still a lengthy period, but it has reached the final stage of a star’s life.
Therefore, its state is extrely unstable.
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Just by using so special weapons, we can directly trigger a violent solar wind and a super ion electromagnetic stream that will sweep through the entire Heritage System.
These will complete all of our work for us,” Lucy Watson said calmly.
Finn Lewis kept a poker face, but couldn’t help a wry smile in his heart.
...
He didn’t even know what to say; what kind of girl begins with such a destructive level of action?
“I disagree,” Miles spoke up directly.
“Why?” Finn Lewis turned to Miles.
“The temper of a star is sothing we can’t fully grasp.
If the explosion goes as we plan, that’s great.
But what if it goes beyond that?
The complete eruption of a star could even affect the entire galaxy, not to ntion that there’s more than one such star here.
So we can’t take such risks to complete our mission.
If sothing goes wrong, the entire galaxy could be destroyed,” Miles said without hesitation.
“The probability of that is lower than 1%,” Lucy Watson stated impassively.
“But there’s still a 1% chance,” Miles countered unwaveringly.
“I also don’t mind proceeding this way,” Sekata Brown’s voice also rose among them, “because indeed, the power of nature is unstoppable.”
“Although this is the simplest and most effective thod, there is also the possibility of an accident.
We warriors of the Sanctuary have always believed in overcoming enemies with our strength,” Adriana Wilson added.
“That’s why you were defeated by enemies,” Lucy Watson glanced at them faintly.
“Let’s not argue.
Other than this, are there any other ways?” Finn Lewis was sowhat helpless; actually, he didn’t really agree with this idea either.
Stars were terrifying, and perhaps he hadn’t been fully aware of it before, but now Finn Lewis was no longer the sa Finn Lewis.
His understanding was naturally far more advanced.
Let’s put it this way, a star in its normal stage isn’t that scary.
Take the sun, for example, with a surface temperature of roughly 6,000 Celsius and a core temperature around 20 million Celsius.
And man-made nuclear fusion reactors can reach temperatures of one hundred million Celsius!
With such temperatures, there are now many materials and technologies that allow spacecraft to get close to the surface of the sun, or even deep inside without any problems.
But that’s during a star’s normal period.
Once a star enters its final stage and starts to beco unstable, the energy it releases is beyond any creature’s control.
Be it White Dwarf Star or the even more terrifying Neutron Star, they represent the current limits for humanity.
Once you’re close enough to such gravity, there’s no way to leave!
Not to ntion sothing even more frightening than a Neutron Star, which is smaller—can you imagine a star as big as the sun becoming a planet only a few dozen kiloters in diater?
The terrible mass eventually condenses into such a small point, and it’s no exaggeration to say that anything that reaches it will be directly compressed, and essentially no matter would exist anymore.
Not to ntion, there are even more terrifying black holes, like the one at the center of the Heritage System.
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