can travel vast distances, although is limited by the mass of any propellant it carries. A spaceship using significant constant acceleration will approach the
speed of light over
interstellar distances, so
special relativity effects including
time dilation become important.
Expressions for covered distance and elapsed time The distance traveled, under constant
proper acceleration, from the point of view of Earth as a function of the traveler's time is expressed by the
coordinate distance x as a function of
proper time τ at constant proper acceleration
a. It is given by: :x(\tau) = \frac{c^2}{a} \left(\cosh \frac{a \ \tau}{c} -1 \right) , where
c is the speed of light. Under the same circumstances, the time elapsed on Earth (the
coordinate time) as a function of the traveler's time is given by: :t(\tau) = \frac{c}{a} \sinh \frac{a \ \tau}{c} .
Feasibility A limitation of constant acceleration is adequate fuel. Constant acceleration is only feasible with the development of fuels with a much higher
specific impulse than presently available. There are two broad approaches to higher specific impulse propulsion: • Higher efficiency fuel (the motor ship approach). Two possibilities for the motor ship approach are nuclear and matter–antimatter based fuels. • Drawing propulsion energy from the environment as the ship passes through it (the sailing ship approach). One hypothetical sailing ship approach is discovering something equivalent to the
parallelogram of force between wind and water which allows sails to propel a sailing ship. Picking up fuel along the way — the
ramjet approach — will lose efficiency as the space craft's speed increases relative to the planetary reference. This happens because the fuel must be accelerated to the spaceship's velocity before its energy can be extracted, and that will cut the
fuel efficiency dramatically. A related issue is
drag. If the near-light-speed space craft is interacting with matter that is moving slowly in the planetary reference frame, this will cause drag which will bleed off a portion of the engine's acceleration. A second big issue facing ships using constant acceleration for interstellar travel is colliding with matter and radiation while en route. In mid-journey any such impact will be at near light speed, so the result will be dramatic.
Interstellar traveling speeds If a space ship is using constant acceleration over interstellar distances, it will approach the speed of light for the middle part of its journey when viewed from the planetary
frame of reference. This means that the effects of relativity will become important. The most important effect is that time will appear to pass at different rates in the ship frame and the planetary frame, and this means that the ship's speed and journey time will appear different in the two frames.
Planetary reference frame From the planetary frame of reference, the ship's speed will appear to be limited by the speed of light — it can approach the speed of light, but never reach it. If a ship is using 1
g constant acceleration, it will appear to get near the speed of light in about a year, and have traveled about half a light year in distance. For the middle of the journey the ship's speed will be roughly the speed of light, and it will slow down again to zero over a year at the end of the journey. As a rule of thumb, for a constant acceleration at 1
g (
Earth gravity), the journey time, as measured on
Earth, will be the distance in light years to the destination, plus 1 year. This rule of thumb will give answers that are slightly shorter than the exact calculated answer, but reasonably accurate.
Ship reference frame From the frame of reference of those on the ship the acceleration will not change as the journey goes on. Instead the planetary reference frame will look more and more relativistic. This means that for voyagers on the ship the journey will appear to be much shorter than what planetary observers see. At a constant acceleration of 1
g, a rocket could travel the diameter of our galaxy in about 12 years ship time, and about 113,000 years planetary time. If the last half of the trip involves deceleration at 1
g, the trip would take about 24 years. If the trip is merely to the nearest star, with deceleration the last half of the way, it would take 3.6 years. == In fiction ==