- #71
en_pris
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One of the definitions of mass is resistance to acceleration. When it is said that mass increases, understand this statement in the context of this definition. Accelerating towards light speed relative to a particular inertial frame requires more and more energy per unit of velocity added the closer to light speed one gets.
However, there is a much more serious limitation that occurs at speeds even less than 1% of light speed, and that is encountering debris in space.
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At what speed does the interstellar medium become lethal to high speed flight? This is an important consideration if interstellar travel is to become a reality for mankind. The nearest star is over 4 light years away. Even 1 light year is an immense distance by human standards, requiring a travel time of 20,000 years at shuttle speeds. So an investigation into travel at higher velocities becomes appropriate. However, at higher velocities, encounter with debris in the interstellar medium must be considered.
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We don't really know what the interstellar medium looks like. If it is just stray hydrogen atoms you will experience a head-on flow of cosmic rays that will collide with your spacecraft and probably generate secondary radiation in the skin of your vehicle. This can be annoying, but it can be shielded so long as your speed is not near light speed. At speeds of 50 to 90% light speed, these particles are not likely to be a real problem. At speeds just below the speed of light (e.g., 99%), the particles would generate a very large x-ray and gamma-ray background in the skin of your ship. Significant shielding will be necessary to protect the crew and instruments.
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As it turns out, our solar system is inside a region called the Local Bubble, where the density of hydrogen atoms is about 1% of that in the general interstellar medium. This bubble, probably produced by an ancient supernova, extends about 300 light years from the Sun. There are thousands of stars within this region. Hydrogen atoms in interstellar space should not be a hazard while exploring the Local Bubble.
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Interstellar space also contains a few microscopic dust grains (micron-sized: 1 micron = 1 millionth meter) in a cube about a few meters on a side. At their expected densities, you are probably in for a rough ride, but it really depends on your speed. The space shuttle, encountering flecks of paint traveling at 28000 mph (0.005% light speed) is pitted and pierced by these particles, but dust grains have mass a thousand times smaller than the smallest paint fleck, so at 0.005% light speed, dust will not be a problem. However, if you want to travel even to the nearest star in a reasonable time, say in 8 to 10 years, 50% light speed will be required. Your likelihood of encountering a large dust grain at high speeds becomes significant. Only one such impact would be enough to damage your vehicle beyond repair given the energy involved. An example:
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A large dust grain may have a mass of a few milligrams. Consider the kinetic energy of a dust grain weighing just one milligram (0.001 gram) at 0.5% light speed:
KE = 0.5mv^2 = 0.5x0.001 gram x (0.5x3x10^10 cm/sec)^2 = 1.125x10^17 ergs.
This is the kinetic energy of a 10 gram bullet traveling at a speed of 1500 KILOMETERS (not meters) per second, a million times the energy that such a bullet would normally have (kinetic energy is proportional to the SQUARE of velocity). The point is, at these speeds even a dust grain would explode into an intense fireball that would melt through the skin of any vehicle. 1500 Kilometers per second is just 1/2 of 1% the speed of light. At that speed it would take 800 years for a one-way trip to the nearest star. Your likelihood of encountering such a dust grain is dependent on the volume of space your vehicle sweeps out, and the density of such dust grains. For those interested, NASA has made available a website containing a tool that will calculate the cosmic-ray transport and diffuse emission production resulting from interstellar dust grains in the Local Bubble. Check out http://galprop.stanford.edu/webrun.php and register as a user. This website requires you to show an "affiliation". However, the interstellar medium probably contains ice globules from ancient comets. Impacts with these objects even at 1/10 of 1% of light speed would be fatal. Discovering the size distribution of debris in interstellar space becomes essential in determining the survivability of vehicles.
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The conclusion is that with any technology we can reasonably imagine, interstellar travel near light speeds is not only difficult but most likely not feasible. This leaves us with cryogenics or generation ships as possibilities for methods of interstellar travel at speeds much slower than light speed, that is, until someone discovers how to warp space.
However, there is a much more serious limitation that occurs at speeds even less than 1% of light speed, and that is encountering debris in space.
.
At what speed does the interstellar medium become lethal to high speed flight? This is an important consideration if interstellar travel is to become a reality for mankind. The nearest star is over 4 light years away. Even 1 light year is an immense distance by human standards, requiring a travel time of 20,000 years at shuttle speeds. So an investigation into travel at higher velocities becomes appropriate. However, at higher velocities, encounter with debris in the interstellar medium must be considered.
.
We don't really know what the interstellar medium looks like. If it is just stray hydrogen atoms you will experience a head-on flow of cosmic rays that will collide with your spacecraft and probably generate secondary radiation in the skin of your vehicle. This can be annoying, but it can be shielded so long as your speed is not near light speed. At speeds of 50 to 90% light speed, these particles are not likely to be a real problem. At speeds just below the speed of light (e.g., 99%), the particles would generate a very large x-ray and gamma-ray background in the skin of your ship. Significant shielding will be necessary to protect the crew and instruments.
.
As it turns out, our solar system is inside a region called the Local Bubble, where the density of hydrogen atoms is about 1% of that in the general interstellar medium. This bubble, probably produced by an ancient supernova, extends about 300 light years from the Sun. There are thousands of stars within this region. Hydrogen atoms in interstellar space should not be a hazard while exploring the Local Bubble.
.
Interstellar space also contains a few microscopic dust grains (micron-sized: 1 micron = 1 millionth meter) in a cube about a few meters on a side. At their expected densities, you are probably in for a rough ride, but it really depends on your speed. The space shuttle, encountering flecks of paint traveling at 28000 mph (0.005% light speed) is pitted and pierced by these particles, but dust grains have mass a thousand times smaller than the smallest paint fleck, so at 0.005% light speed, dust will not be a problem. However, if you want to travel even to the nearest star in a reasonable time, say in 8 to 10 years, 50% light speed will be required. Your likelihood of encountering a large dust grain at high speeds becomes significant. Only one such impact would be enough to damage your vehicle beyond repair given the energy involved. An example:
.
A large dust grain may have a mass of a few milligrams. Consider the kinetic energy of a dust grain weighing just one milligram (0.001 gram) at 0.5% light speed:
KE = 0.5mv^2 = 0.5x0.001 gram x (0.5x3x10^10 cm/sec)^2 = 1.125x10^17 ergs.
This is the kinetic energy of a 10 gram bullet traveling at a speed of 1500 KILOMETERS (not meters) per second, a million times the energy that such a bullet would normally have (kinetic energy is proportional to the SQUARE of velocity). The point is, at these speeds even a dust grain would explode into an intense fireball that would melt through the skin of any vehicle. 1500 Kilometers per second is just 1/2 of 1% the speed of light. At that speed it would take 800 years for a one-way trip to the nearest star. Your likelihood of encountering such a dust grain is dependent on the volume of space your vehicle sweeps out, and the density of such dust grains. For those interested, NASA has made available a website containing a tool that will calculate the cosmic-ray transport and diffuse emission production resulting from interstellar dust grains in the Local Bubble. Check out http://galprop.stanford.edu/webrun.php and register as a user. This website requires you to show an "affiliation". However, the interstellar medium probably contains ice globules from ancient comets. Impacts with these objects even at 1/10 of 1% of light speed would be fatal. Discovering the size distribution of debris in interstellar space becomes essential in determining the survivability of vehicles.
.
The conclusion is that with any technology we can reasonably imagine, interstellar travel near light speeds is not only difficult but most likely not feasible. This leaves us with cryogenics or generation ships as possibilities for methods of interstellar travel at speeds much slower than light speed, that is, until someone discovers how to warp space.