WARNING HIGH NERD CONTENTS
Ok the exercise has already been done twice in this topic, but no one actually made a proper breakdown as where the number 8.2 comes from and how the calculation is made. Since I'm the one bitching about it, let me also be the one to give the breakdown:
Stuff needed:
- 1 g (the acceleration you experience on earth due to its gravitational field): 9.807 m/s^2 (meters per square second), in free space this means that every second our speed increases with roughly 10 m/s. So after 1 second we travel 10 meters/second, after 2 seconds we travel 20 meters/second, then 30, 40, etc.
- 1 AU (astronomical unit, the distance between the sun and the earth): 149,597,870.7 km (kilometres)
- Radius of our solar system (based on the average distance between Pluto and our sun): 39.5 AU
- So distance edge of our solar system and the earth: 39.5-1 = 38.5 AU
- As explained before, you'll need to accelerate half the distance and decelerate half the distance, so you calculate the acceleration over 38.5/2 = 19.25 AU (the half way point) and multiply the time that takes by 2 as you will be decelerating the same amount of time.
Ok now we bring in the big formula for the law of uniform acceleration which has been mentioned before: distance = 1/2 acceleration * time^2. Acceleration in this case is g so this becomes:
distance = 1/2 * g * time^2. We need time so so rewriting the equation: time = square root(2*distance/g)
In terms of units this now is: [seconds] = SQRT(2*[meters]/[meters/seconds^2])
However we like to talk about [days], [AU's] and [g's] so we need some conversion factored in. To do this lets first just do the calculation with what we've got. For this we need to at least convert 1 AU into meters which is:
1 (AU) * 149,597,870.7 (km) * 1000 (m) = 149,597,870,700 meters.
So the travelling time to the half way point is: SQRT(2 * 19.25 * 149,597,870,700 / 9,807) = 766346 seconds = 9 days (1 day = 24*60*60 = 86,400 seconds)
As the decelleration takes the same amount of time it will take 18 days (and 1 hour) to reach Earth from the edge of the solar system.
Now to obtain THE formula
To get the answer we used 3 conversion factors: 149,597,870,700 (AU in meters), 86,400 (seconds in a day) and 9.807 (g in m/s^2). So putting that into the equation:
[seconds] = SQRT(2*[meters]/[meters/seconds^2])
changing acceleration from m/s^2 to g:
[seconds] = SQRT(2*[meters]/
(9.807*[g])
)
changing answer from seconds to days:
[
days
] = SQRT(2*[meters]/(9.807*[g])) /
86,400
changing distance from meters to atronomical units (AU):
[days] = SQRT(2*
149,597,870,700[AU]
/(9.807*[g])) / 86,400
dividing the total distance by 2 (to the halfway point) and multiplying the time need by 2 (from edge to halfway and from halfway to destination):
[days] =
2 *
SQRT(2
* 1/2
* 149,597,870,700[AU] * 1/9.807 * 1/[g]) / 86,400
cleaning up the formula by moving all the numbers together and calculating the result
[days] = SQRT(15,254,192,994.80[AU] / [g]) / 43,200
[days] = SQRT((15,254,192,994.80[AU] * 1/(43,200^2) * 1/[g])
[days] = SQRT(8.17[AU]/[g])
round the number and you get the illustrious 8.2 factor mentioned before:
Time [days] = SQRT(8.2 * distance [AU] / acceleration [g])
the simpler version as mentioned before would be to simply use 50 AU as default for any solar trip so inside the sqrt you get 8.17 * 50[AU] = 408.5 :
Time [days] = SQRT(408.5 / acceleration [g])
Note:
if its possible to make a warp jump WITHOUT the need to have speed 0 then the halfway point needs to be factored out and you can then just keep accererating to the edge of the solar system. Similarly, if you EXIT the warp space you could also assume that you have the same speed as when you entered it meaning that you would only need to decelarate to get to the correct point. Of course if you accelerated from a 50AU solar made a jump to the edge of a 30AU solar system, then you'll be missing target by 20AU!!. Stuff can get a bit complex this way. Anyway, the corresponding formula assuming NO halfway point (just take out the 2* and 1/2 from the above steps):
[days] = SQRT(4.1[AU]/[g])