You don’t immediately get the maximum bonus though, as that would be exploitable. The maximum bonus provided by a side, is set in the config so we can balance it if needed. This mechanic does not change your existing ships but it allows you to now put the reactor in different positions with multiple stabilizers closer to it.Ī reactor has 6 relative sides (Front, Back, Right Left, Top, Bottom) and we simply provide a bonus to your overall stabilization for every additional side that contains a stabilization group. We worked on a method to allow this distance to be influenced indirectly by the size and placement of additional stabilizer groups. Stabilizer care about the distance between themselves and their reactor, which encourages you to build in one dimension. Our goal with this system is to make every entity shape equally viable. 6, 2004.This update contains some fixes for problems with the last update, as well as a new advanced system for reactor design. "Scientists plan to ignite tiny man-made star." Telegraph. "How to build a star on Earth." BBC News. "Can we make a star on Earth?" BBC Horizons. Learn more about stars and energy by following the links on the next page. But it remains to be seen if we can sustain such a creation and harness its astounding energy. So, we can create a star on Earth - at least for a short time. But no one has unlocked the secret just yet. Others are exploring options with plasma - the fourth state of matter. Some scientists are looking at massive lasers as a way to ignite a fusion event. The amount of power required to initiate fusion coupled with the intense heat created by the event make it difficult to build a facility capable of containing a reaction. There's no shortage of fuel - hydrogen is plentiful and the oceans have large amounts of deuterium in them.īut getting to the point where we can harness fusion for power is going to take years of research and billions of dollars in resources. If they can find a way to create sustainable and controllable reactions, scientists could use fusion to provide massive amounts of power for millions of years. Laboratories around the world are now trying to find a way to harness fusion as an energy source. For a brief moment, man had harnessed the power of the stars to create a weapon of immense power. It completely obliterated the island, leaving behind a crater 164 feet deep (nearly 50 meters) and 1.2 miles (1.9 kilometers) across. The resulting explosion was 10.4 megatons in size. That means the mass of the tiniest particle is equivalent to an enormous amount of energy. And as Einstein's famous equation tells us, energy is equal to the mass of an object times the speed of light squared. So where does that extra mass go? It's converted into energy. A helium-4 atom has less mass than four hydrogen atoms collectively. If you break all that down, it essentially means that four hydrogen atoms fuse to create a single helium-4 atom. Fusing two helium-3 atoms together creates helium-4 and two hydrogen atoms. Fusing deuterium with hydrogen creates helium-3. It's an atom with one proton and one neutron. What you're left with after this initial fusion is deuterium, an isotope of hydrogen. But if you have enough energy to overcome this force, you can fuse the two nuclei into one. If you're familiar with magnets, you know that similar charges repel each other. That's because protons are positively charged. To fuse two protons together requires enough energy to overcome electromagnetic force. The nucleus of a hydrogen atom is a single proton. The core of the sun is intensely hot - temperatures are greater than 15 million degrees Kelvin (nearly 27 million degrees Fahrenheit or just under 15 million degrees Celsius).Īt these temperatures, the hydrogen atoms absorb so much energy that they fuse together. Heavier elements make up the final percent of the sun's mass. The sun is about 75 percent hydrogen and 24 percent helium. To understand how scientists can make a star, it's necessary to learn what stars are made of and how fusion works.
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