There are several problems that will prevent us from interstellar transit in the foreseeable future. The most fundamental is just the mass of propellant required to even achieve speeds to travel the distance between stars in a human lifespan. As every freshman physics student discovers, rocket propulsion (regardless of power source) requires that you eject mass rearward in order to make the vessel go forward, maintaining conservation of momentum per the rocket equation. This means that some of the initial mass of your vessel includes this material, which is generically called propellant. In the chemical rockets that we use to launch satellites into space this is composed of fuel (such as kerosene, liquid hydrogen, or some form of hydrazine) and oxidizer (typically liquid oxygen, but can be stabilized nitric acid or even more exotic substances) which also provide the power source in the form of exothermic chemical combustion which heats the products to high temperatures and pressures, forcing them out the nozzle. Nuclear thermal rockets are more of the same, except the propellant is generally hydrogen (favored in vacuum for the low molecular weight). Other systems, like fission fragment, fissionable salt water, nuclear pulse propulsion, et cetera use other propellants such as the fission products themselves combined with water or other propellants, but in the end, there has to be mass ejected in order to effect a change in momentum.
The efficacy of propellants, called specific impulse (Isp) is measured in terms of thrust divided by the rate of consumption by weight or mass of propllant per interval of time, giving a mass-independent result in units of seconds. The best chemical rockets have a hard time achieving an Isp of 400 seconds even with the best possible mass fraction (mass of propellant over the total gross liftoff weight of the vehicle). Nuclear thermal may give on close order of 1000 seconds. Fission fragment and nuclear pulse propulsion could potentially offer up to around 5000 seconds. Using a hypothetical nuclear fusion power source could give specific impulse (using diatomic hydrogen as the propellant) of somewhere around 10,000 to 20,000 seconds. By comparison, to have a vessel with a reasonable mass fraction–say, 1 kilogram of spacecraft/payload to 2000 kilograms of propellant–capable of achieving even 0.01c and then decelerating would require a specific impulse on the order of 80,000 seconds, and that is still a four century transit to our nearest interstellar neighbor. Anything less will strand the spacecraft and its hapless inhabitants in the interstellar void for thousands of years. This capability is radically beyond anything we could hope to develop in ten years, or indeed, likely within the next century, and would require some kind of fundamental breakthrough in either energy or propulsion, it just isn’t feasible to send any craft, manned or unmanned, to another star in less than millennia.
The other major issue is the devil that pops up to cause no end of trouble in every area of natural science, thermodynamics. Specifically, the inevitable buildup of heat–not just from this energetic propulsion system, but also from all the other life-sustaining and vehicle maintaining activities–which has to be transferred away lest amount of the heat and thus temperature of the system keeps increasing until it physically breaks down. On Earth, this is not problem; the air and water carry heat away by convection, and the Earth as a whole spends about twelve hours a day radiating all of the heat energy it absorbs from the Sun (except for that used in driving the hydrological cycle) which dwarfs the production by any human activity (provided we don’t significantly alter the composition and resulting emissivity of the atmosphere). In space, however, the only way to reject (get rid of) heat that is produced without having to exhaust more mass to carry it way is to radiate it away. Also the space background is very cold (at 2.7 Kelvin) for a vessel of any significant volume the amount of radiative area required to exhaust excess heat is going to be huge, not withstanding all of the systems needed to convey heat to the radiators. Basically, the vessel would consist of a habitat of some suitable size surrounded by a giant spheroid bubble of radiating surface.
Mind you, this is not a theoretical problem; spacecraft that have onboard energy generation systems or high power avionics have to be actively cooled, and the Shuttle Orbiter of the now retired Space Transportation System always had the cargo bay doors open in orbit not because it looked cool but so that the radiators on the inside could keep the Shuttle at a liveable temperature. These systems are good for missions of limited duration or low energy output, but for a habitat of indefinite duration that has to produce food, distill water, and propel itself it becomes a massive hurdle which is not readily overcome by any kind of brute force methods, e.g. just make it bigger or throw more power at it. Adding a high power propulsion system or nuclear power plant just magnifies the problem by many orders of magnitude.
There are, of course, other more prosaic issues, such as how you would provision for such a long journey, ensure the health and survival of the crew against hazards, boredom, and personal strife, ensure the functionality of electrical and mechanical devices over such a long duration without impractical levels of redundancy, et cetera, but these are the two fundamental issues which no extant or developing technology will address in the foreseeable future.
[QUOTE=lazybratsche]
I believe the most plausible method of interstellar travel, using technology mostly available today, is with nuclear pulse propulsion. Basically, the spacecraft will carry a bunch of small nuclear bombs and detonate them periodically behind the craft. One of the early studies of the concept is “Project Orion”. An Orion based craft (or one of the later developments of the concept) could conceivably make it to Alpha Centauri in 50-100 years.
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Although Dyson promoted Project ORION based upon an advertised capability to achieve interstellar speeds, a very simple simulation using realistic impulse values demonstrates that it just isn’t feasible over a human lifespan, and the amount of nuclear “fuel pods” required for a single transit radically dwarfs the yield of all nuclear weapons every produced. Nuclear pulse propulsion is adequate for exploring the planetary system, but traveling to the stars will squire a fundamentally more efficient form of propulsion, or a much longer tolerance for duration.
Stranger