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Might be converting said heat into microwaves or other as of yet undiscovered states of energy, then beaming it to other star systems or areas of the universe where required. They could even utilize said microwaves beams or streams of energy for transportation purposes, you would be bound by light speed all the same.
originally posted by: RAY1990
a reply to: andy06shake
Might be converting said heat into microwaves or other as of yet undiscovered states of energy, then beaming it to other star systems or areas of the universe where required. They could even utilize said microwaves beams or streams of energy for transportation purposes, you would be bound by light speed all the same.
I hinted at such things in my first post but as you mentioned in your first post, such concepts of energy production could be so primitive for where they are.
Trying to fathom the unfathomable gets my brain going in circles though, it always comes to "how you get there" and then I can only use ourselves as examples.
Here are my conclusions.
1. A "wireless" format of energy distribution where shear volume trumps efficiency. Or it could be efficient but limited by light speed.
2. Localising your civilization around the star, this makes gathering raw materials a logistical nightmare.
3. Faster than light travel.
Now those conclusions of mine (I'm not exactly educated) rely on some technologies to be mastered and potentialy sciences we don't have a clue about. Which gets me in circles... Who knows?
Super batteries and wormholes?
Power from the ether?
It keeps bringing me back to the point that the Dyson Sphere idea might be utterly pointless.
Fusion Torch Can Create New Raw Materials
January 1, 2004 • 1:00AM
Marjorie Mazel Hecht reports:
How soon the world might run out of necessary resources and raw materials, from drinkable water to strategic minerals, should be no concern for panic, rationing, or calls for population control. We have the ability now to create the resources we need, using advanced technology. Conventional nuclear reactors can provide the energy to desalinate seawater, and high-temperature nuclear reactors can efficiently create hydrogen to replace petroleum fuel. The even higher temperatures available from thermonuclear fusion will provide working plasmas that can reduce garbage and waste down to its constituent elements, eliminating disposal problems; these high-temperature plasmas will also be able to “mine” strategic minerals directly from the ordinary rock.
The material in a white dwarf no longer undergoes fusion reactions, so the star has no source of energy. As a result, it cannot support itself by the heat generated by fusion against gravitational collapse but is supported only by electron degeneracy pressure, causing it to be extremely dense. The physics of degeneracy yields a maximum mass for a non-rotating white dwarf, the Chandrasekhar limit—approximately 1.44 times of M☉—beyond which it cannot be supported by electron degeneracy pressure. A carbon-oxygen white dwarf that approaches this mass limit, typically by mass transfer from a companion star, may explode as a type Ia supernova via a process known as carbon detonation.[1][5] (SN 1006 is thought to be a famous example.)
A white dwarf is very hot when it forms, but because it has no source of energy, it will gradually radiate its energy and cool. This means that its radiation, which initially has a high color temperature, will lessen and redden with time. Over a very long time, a white dwarf will cool and its material will begin to crystallize (starting with the core). The star's low temperature means it will no longer emit significant heat or light, and it will become a cold black dwarf.[5] Because the length of time it takes for a white dwarf to reach this state is calculated to be longer than the current age of the universe (approximately 13.8 billion years),[9] it is thought that no black dwarfs yet exist.[1][4] The oldest white dwarfs still radiate at temperatures of a few thousand kelvins.
There are currently thought to be eight white dwarfs among the hundred star systems nearest the Sun.
The idea is to build the entire swarm in iterative steps and not all at once. We would only need to build a small section of the Dyson sphere to provide the energy requirements for the rest of the project. Thus, construction efficiency will increase over time as the project progresses. "We could do it now," says Armstrong. It's just a question of materials and automation.
And yes, you read that right: we're going to have to mine materials from Mercury. Actually, we'll likely have to take the whole planet apart. The Dyson sphere will require a horrendous amount of material so much so, in fact, that, should we want to completely envelop the sun, we are going to have to disassemble not just Mercury, but Venus, some of the outer planets, and any nearby asteroids as well.