The most efficient chemical rockets, e.g. those of the space shuttle, burn hydrogen and oxygen to form water (or more accurately, superheated steam). The molecular formula of water is H2O, and since the atom of oxygen (O) is 16 times heavier than that of hydrogen (H), the water molecule has 18 times the weight of the atom of hydrogen, and 9 times the weight of the H2 molecule, the form in which hydrogen usually exists.
If only the exhaust jet consisted not of water H2O but of hydrogen H2! Then at the same temperature (as shown above) its molecules would move 3 times faster, and the exhaust jet would be faster too. Unfortunately, there exists no practical chemical reaction which produces H2.
With unlimited nuclear power, however, it is not necessary to burn anything--instead, hydrogen gas could be heated inside a nuclear reactor and then ejected backwards from a big nozzle. That was the idea of the NERVA project, NASA's attempt in the 1960s to build a nuclear rocket.
It is difficult to imagine running a nuclear reactor at the same high temperature as a rocket engine. But with a factor of 3 in one's favor, even a lower temperature can still give a great advantage. Some experimental models of the nuclear rocket ran quite well when tested on the ground, but in the end, the risk of environmental contamination and of the reactor melting down were too high and the project was stopped.
A completely different approach to spaceflight was taken by Theodore Taylor, a nuclear physicist. Taylor led a successful career in designing bigger and more powerful nuclear bombs, until personal doubts focused his talents elsewhere.
Taylor visualized nothing less than a spaceship propelled by atomic bombs. Its rear would hold a massive metal plate, with an opening in the middle. At suitable intervals an atomic bomb would be ejected from there and after it reached some specific distance, it would be exploded. The bomb would be wrapped in a hydrogen-rich plastic casing, which the enormous heat of the bomb would instantly turn into extremely hot gas, much of it hydrogen. That gas would then be blown off into space, but some would first hit the plate, and its pressure would propel the spaceship upwards.
The idea was first raised by Ulam and Everett in 1955, before any practical spaceflight was achieved (Stanislaw Ulam was also the mind behind the first practical design for an H-bomb; see "Dark Sun" by Richard Rhodes). In 1958 Taylor obtained Air Force support and the project, named "Orion", was begun. It attracted a crew of practical dreamers, among them Freeman Dyson, a distinguished theoretical physicist from the Institute of Advanced Studies in Princeton.
| Test model of "Orion," pro-
pelled by ordinary
(Exhibited in the Smithsonian)
Over the seven years that followed, at the cost of about 10 million dollars, plans for a bomb-propelled spaceship were developed. Small models of such a ship were actually built, and in one successful experiment a model was propelled upwards by a series of conventional explosive charges, ejected from its rear. Although the detailed design remains classified (it involved a great deal of bomb technology), the designers have claimed that no technical problem posed a stumbling block--neither the wearing-down of the "pusher plate" exposed to the explosions, nor the radiation hazard to the spaceship passengers, nor any other details.
"Orion" called for huge spaceships, weighing thousands of tons. One design proposed a flight to distant stars using a "conservatively designed" spaceship of 40 million tons, powered by 10 million bombs! But in the end, the project was abandoned, because the prospect of exploding a large number of nuclear bombs in the atmosphere or close to it seemed too frightening. The world woke up to realize the extent to which radioactive debris contaminated the atmosphere, and signed in 1963 a treaty banning nuclear tests, which also spelled the end of "Orion".
And yet... the "Orion" propulsion method could one day be the only practical way of protecting Earth from asteroid impact.
Most asteroids move between Mars and Jupiter, far from Earth, but a few have orbits which cross that of the Earth. Geology suggests that a fairly large one has hit Earth in the past about every 30 million years, with devastating results. An impact structure (partially under water) near the top of the Yucatan peninsula in Mexico was apparently formed by a 10-kilometer asteroid some 65 million years ago, and many scientists believe that was the impact which caused the extinction of the dinosaurs and of other early life.
Even a 1-kilometer asteroid can cause huge damage. Currently NASA is conducting a search for all near-Earth asteroids down to that size; the project extends to 2008, and as of now (2003) about 800 objects have been identified and tracked. Many smaller objects exist around Earth's orbit (one hit Siberia in 1908), but it's the big ones NASA worries about.
Supposing an asteroid is found to move on a path that hits Earth--what can be done about it? Blowing it up would just convert it into a collection of fragments, still headed for Earth. However, the "Orion" propulsion method could spoil its aim and make it miss Earth
One would have to send out a probe with a very powerful nuclear fusion bomb (H-bomb), and make it fly (not too close) alongside the asteroid, on the side where we would like to apply the push. When the bomb explodes, it vaporizes the surface layer of the asteroid next to it and turns it into hot gas, which then expands to space. By Newton's laws, the center of gravity of the asteroid material does not change (see section on the rocket principle), so as the gas expands to one side, the asteroid is pushed to the other.
It isn't easy to push a billion-ton rock, suggesting that any such maneuver should be done very far from Earth, where (one hopes) no more than a small nudge is needed to move the asteroid into a non-colliding trajectory. Right now this is just an idea for the very distant future (although it has already appeared in science fiction movies). Luckily, this does not seem to be an urgent matter, since the risk of a serious impact within one's lifetime is rather small.