Reaching Alpha Centauri in human lifetime

In summary, if a space traveler could travel at the speed of light, they would make it to Alpha Centauri within a human lifetime. However, the closer they get to the speed of light, the higher the time dilation factor becomes, so a space traveler would only age 1 year if they traveled to Alpha Centauri and back in just two months.
  • #1
JamesCallahan
1
0
Hello,

I'm new on this forum and I hope I will blend in nicely. I happen to have a couple of questions on the Alpha Centauri star in the constellation of Centaurus. I know the distance between this star and our milk way is huge, but suppose one could travel at the speed of light X 25, would it be feasible to reach the star or one of its planets within a human lifetime.

James Callahan, University of Georgia, Department of Psychology
 
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  • #2
A couple of comments:

(1) Welcome!
(2) You say "the distance between this star and our Milky Way...". I think you are confused. The Milky Way galaxy is our galaxy, and is a collection of perhaps 100 billion stars. Both our sun, Alpha Centauri, and a whole bunch of other stars are members of the Milky Way galaxy.
(3) The distance to Alpha Centauri is about 4.2 light years, a huge distance in Earth terms, but very close in astronomical terms. This means that light takes 4.2 years to travel here from Alpha Centauri. So if you had a spaceship capable of going 1/2 the speed of light (physically possible, but far beyond our capabilities today), you could get there in about 8 years.
(4) As you get closer to the speed of light, your subjective time would slow down, so you could experience a time much less than 4.2 years if you got close enough to the speed of light. Look up "relativistic time dilation".
(5) It's impossible to go 25X the speed of light, or even to attain the speed of light.
 
  • #3
JamesCallahan said:
I know the distance between this star and our milk way is huge, but suppose one could travel at the speed of light X 25, would it be feasible to reach the star or one of its planets within a human lifetime.
There's no need for speeds faster than light (which is an unphysical assumption). The distance to Alpha Centauri is only about 4.5 light years. If he could just travel at about 0.41 times the speed of light (with respect to earth), a space traveler could get there in 10 years (according to his clocks--a bit longer according to Earth clocks).
 
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  • #4
Of course we know you can't go faster than light, at least that is the paradigm as we know it now. But, assuming some miracle happened, and we figured out some way to go 25X faster than light, you would make it to AC in just a bit over 2 months.

Or looking at it the other way 'round, you could go 25 light years in one year, 50 light years in 2 years, 500 light years in 20 years, so at that velocity, you could theoretically have a trip of 500 light years there and back within one human lifespan, 40 years in this case. That would be 1000 light years total trip distance.

There are about 15,000 stars within 100 light years of earth, so you could visit anyone of them there and back within 8 years max assuming you were actually going 25X c and there was no time dilation. So if you had 15,000 spaceships you could visit every one and the final report on them would be ready within 10 years (assuming experts would need to massage the data brought back).

We could theoretically get so close to c (speed of light) that the people on board would THINK they are going faster than the speed of light. Get close enough to c and it could be a time dilation of 25 to 1. One year of ship time would equal 25 years of Earth time.

The closer you get to c, the higher that time dilation, so closer yet to c could put time dilation at 100 to 1, 1 year of ship time, you would be going what you think is 100 times c and if you went out 100 light years and back (to a star 50 light years away) you would age only 1 year but you would find yourself 100 years in Earth's future, all your relatives would be dead.

So at a time dilation factor or 25:1, going to Alpha Centauri and back even though it might take only a couple of months on board the craft, say you spent 5 years exploring AC, you both would age 5 years in real time but the 4 months coming and going from Earth to AC and back would put yourself in your future.

That 2 month one way journey would still take 4.3 years according to Earth clocks so the total time you think you took (and biologically and every other way you would be correct, you aged less) would be 5 years and 4 months.

If you had an identical twin left behind on Earth, he would be 8.6 years older. The 5 years you spent on AC would have been at the same relative clock rates so you both aged 5 years but the time you spent so close to c it made a time dilation of 25:1, you would have aged only two months so your time spent according to your clocks would have been 5 years and 4 months.

So suppose you were both exactly 20 years old when you left on your common birthday, you would be 25 years and 4 months old when you get back. Your brother would be 33 years and 7 months old. That would be a noticeable difference in your ages.

It would be real too, suppose you were both taking courses from the same software online style, where AI would grade your work and so forth. Suppose you had to read the equivalent of 1 book per week for your course work.

Since you had only 5 years and 4 months to do your work, you would only have been able to have read a couple hundred books.

Your brother would have been way ahead of you at home, having had time to have read over 700 books and he would have his Phd while you were still only one fourth the way through. Assuming you had to read 700 books for the whole course, say some kind of world history or some such.
 
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  • #5
JamesCallahan said:
Hello,

I'm new on this forum and I hope I will blend in nicely. I happen to have a couple of questions on the Alpha Centauri star in the constellation of Centaurus. I know the distance between this star and our milk way is huge, but suppose one could travel at the speed of light X 25, would it be feasible to reach the star or one of its planets within a human lifetime.

James Callahan, University of Georgia, Department of Psychology

Hi James

Alpha Centauri is composed of three separate stars, A, B & Proxima. The Milky Way, our Galaxy, contains our Sun, the Alpha Centauri system and over 100 billion other stars in a vast system of stars that's over 100,000 light years wide. Alpha Centauri's stars are a mere 4.2-4.4 light years away (depending on which component we're talking about) and can be reached within a human lifetime without the need to go faster than light.

Perhaps you meant 1/25 of the speed of light? In that case the trip takes 105-110 years, which is a bit longer than an average human lifespan of 70-80 years.

A point your other responders neglect to mention is the need to accelerate to high speed in order to make relativistic effects usefully noticeable. For example at an acceleration of just 1 gee (equivalent to Earth's surface gravity) the trip to Alpha Centauri A or B takes 6.035 years from the point of view of people staying on Earth. On board ship the journey takes just 3.58 years. Increasing the acceleration decreases the trip-time perceived by the crew quite significantly. If the crew can be protected against a full 25 gee, then the trip takes ~0.368 years (19 weeks.) From the viewpoint of the people at home it's ~4.437 years.

An accelerometer measures, obviously enough, the acceleration, moment to moment. An integrating accelerometer produces a 'speed' (called the rapidity in relativistic terminology) that is the acceleration multiplied by the time spent accelerating, adding up all those small moments over the whole trip. According to the ship-board integrating accelerometer the top speed measured is 1.85 times lightspeed for the 1 gee trip to Alpha Centauri and 4.6 times lightspeed for the 25 gee trip. To accelerate to x25 lightspeed, according to the integrating accelerometer of the ship, the time required is 24.2 years ship-time at 1 gee and the ship travels ~16 billion light years doing so. At 25 gees that trip takes 0.97 years and the ship travels 1.4 billion light years. From a stationary observer the ship never exceeds the speed of light.

That's relativity for you!
 
  • #6
qraal said:
Hi James

Alpha Centauri is composed of three separate stars, A, B & Proxima. The Milky Way, our Galaxy, contains our Sun, the Alpha Centauri system and over 100 billion other stars in a vast system of stars that's over 100,000 light years wide. Alpha Centauri's stars are a mere 4.2-4.4 light years away (depending on which component we're talking about) and can be reached within a human lifetime without the need to go faster than light.

Perhaps you meant 1/25 of the speed of light? In that case the trip takes 105-110 years, which is a bit longer than an average human lifespan of 70-80 years.

A point your other responders neglect to mention is the need to accelerate to high speed in order to make relativistic effects usefully noticeable. For example at an acceleration of just 1 gee (equivalent to Earth's surface gravity) the trip to Alpha Centauri A or B takes 6.035 years from the point of view of people staying on Earth. On board ship the journey takes just 3.58 years. Increasing the acceleration decreases the trip-time perceived by the crew quite significantly. If the crew can be protected against a full 25 gee, then the trip takes ~0.368 years (19 weeks.) From the viewpoint of the people at home it's ~4.437 years.

An accelerometer measures, obviously enough, the acceleration, moment to moment. An integrating accelerometer produces a 'speed' (called the rapidity in relativistic terminology) that is the acceleration multiplied by the time spent accelerating, adding up all those small moments over the whole trip. According to the ship-board integrating accelerometer the top speed measured is 1.85 times lightspeed for the 1 gee trip to Alpha Centauri and 4.6 times lightspeed for the 25 gee trip. To accelerate to x25 lightspeed, according to the integrating accelerometer of the ship, the time required is 24.2 years ship-time at 1 gee and the ship travels ~16 billion light years doing so. At 25 gees that trip takes 0.97 years and the ship travels 1.4 billion light years. From a stationary observer the ship never exceeds the speed of light.

That's relativity for you!

Hi, I wonder if you have the formulae for those numbers? It seems to me 1 g would get you close to c in about a year, so how are you deriving those numbers? Thanks.
 
  • #7
litup said:
Hi, I wonder if you have the formulae for those numbers? It seems to me 1 g would get you close to c in about a year, so how are you deriving those numbers? Thanks.

Hi
You have to convert between rapidity and speed. So if the rapidity, u, is 1 c, which is reached after 30,570,323 seconds, ship time T, at 1 gee, then the speed, v, is tanh(u) - in units of c (lightspeed, c = 1.)
Tanh(u) is sinh(u)/cosh(u), where sinh(u) is used to get the stationary observer time, while cosh(u) is the Lorentz gamma-factor, what old "Blake's 7" fans would call TDF (time distortion factors.)

I'll go into more detail if you're interested still and undaunted by hyperbolic trig functions.

Qraal
 
  • #8
Another point, often unappreciated, is the fact that news of a ship's arrival arrives back at the starting point always at a speed less than, but arbitrarily close to, half lightspeed. Thus stay at home observers receive news from explorers at a minimum elapsed time of twice the target's distance (when that's measured in light years.) Thus a probe launched off at 0.5c has an effective data return speed of 1/3 c, but a much lower energy cost than a probe expensively fired off at 0.9c for example. How one determines the most economical speed depends on how the waiting time for data is costed too.
 
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  • #9
qraal said:
Hi
You have to convert between rapidity and speed. So if the rapidity, u, is 1 c, which is reached after 30,570,323 seconds, ship time T, at 1 gee, then the speed, v, is tanh(u) - in units of c (lightspeed, c = 1.)
Tanh(u) is sinh(u)/cosh(u), where sinh(u) is used to get the stationary observer time, while cosh(u) is the Lorentz gamma-factor, what old "Blake's 7" fans would call TDF (time distortion factors.)

I'll go into more detail if you're interested still and undaunted by hyperbolic trig functions.

Qraal
I would love to get all the math involved. Can you be more rigorous in your equations?That is to say, just write them out without the words? like v=Tanh(u)- what? Oh, the - is not a minus sign? So in that case V=tanh (u). Is that the same as the fitzgerald contraction?
What is the difference between speed (you mean velocity?) and 'rapidity'? If you are going to accelerate to say 0.8c there is not much in the way of time dilation, I don't think, right?
 
  • #10
Hi litup

Gamma is computed by

1/sqrt(1-(v/c)^2)

Which is a significant 5/3 at 0.8c some 2/3 higher than the Newtonian case.

There are several good websites on these issues. I'm trying to put together the equations in LaTeX format for easier reading, since ASCII and ExCel renderings aren't very readable.
 
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  • #11
And...

cosh(u) gives the gamma factor, where u = g.T for constant acceleration, g being acceleration measured by a shipboard accelerometer and T the acceleration time measured by the ship's clocks.
 
  • #12
qraal said:
And...

cosh(u) gives the gamma factor, where u = g.T for constant acceleration, g being acceleration measured by a shipboard accelerometer and T the acceleration time measured by the ship's clocks.

Are the trig functions you mentioned in degrees, grads or radians? My guess is radians. I am having a bit of trouble getting into radian mode with my simple casio, so I guess I will drag out my rusty but trusty HP48G:) You don't really need it for this simple stuff but its fun to dig it up every now and then.
 
  • #13
litup said:
Are the trig functions you mentioned in degrees, grads or radians? My guess is radians. I am having a bit of trouble getting into radian mode with my simple casio, so I guess I will drag out my rusty but trusty HP48G:) You don't really need it for this simple stuff but its fun to dig it up every now and then.

You guessed it - radians. Degrees are relative values not 'absolute' like radians.

But here's a secret... Hyperbolic trig functions are actually exponential functions. Look them up on Wikipedia for their full definitions.
 
  • #14
Ok, here goes some TeX...

[tex]\gamma=\frac{1}{\sqrt{1-\beta^2}}[/tex]

where [tex]\beta=\frac{v}{c}[/tex]
 
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  • #15
Thus...

[tex]\gamma=cosh(\frac{g.\tau}{c})[/tex]

...where g & [tex]\tau[/tex] are in [tex]m.s^{-2}[/tex] & s respectively.

Funny getting used to how Firefox, my browser, handles the LaTeX files. I have to reload fully each time I hit the Preview button.
 
  • #16
[tex]v=c.tanh(\frac{g.\tau}{c})[/tex]

[tex]x=\frac{c^2}{g}(cosh(\frac{g.\tau}{c})-1)[/tex]

[tex]t=\frac{c}{g}sinh(\frac{g.\tau}{c})[/tex]
 
  • #17
Those are the one way equations and need slight modification to be used for trips in which the vehicle accelerates then deccelerates to its destination. You can probably guess how to modify them.
 
  • #18
[tex]x=\frac{c^2}{g}(\sqrt{1+(\frac{g.t}{c})^2}-1)[/tex]

[tex]v=\frac{g.t}{\sqrt{1+(\frac{g.t}{c})^2}}[/tex]

[tex]a=\frac{dv}{dt}=\frac{g}{\sqrt[3/2]{1+(\frac{g.t}{c})^2}}[/tex]
 
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  • #19
those equations produce the distance travelled, the speed of the vehicle and the acceleration seen by a 'stationary observer'. Acceleration in this case is the instantaneous rate of change of speed as seen by the observer in the same frame as the rest frame of the ship's home or destination. Of course everything is really in relative motion and across intergalactic distances the complication of general relativity arises, but 'stationary observer' is usually understood to mean the observer to whom the ship appears to be accelerating, but its point of origin does not i.e. in the same frame as the origin.
 
  • #20
And, in case you didn't figure it out...

[tex]cosh(\frac{g.\tau}{c}) = \sqrt{1-(\frac{g.t}{c})^2} = \gamma = \frac{1}{\sqrt{1-\beta^2}}[/tex]
 
  • #21
The 'B'^2 in that last is (V^2/C^2)?
Another question on acceleration. The talk of the recent Vasimir rocket, getting folks to Mars in two months, using a 200 mw power source to an ion engine.
I understand a constant power source will end up with a reduced acceleration rate over time as the velocity increases, independent of relativistic effects. Is that true? I have seen equations of constant power inputs that says that. If so, and we are in normal ballistic velocities used in present day space probes, how does the system (the spacecraft ) know it is not say at 3 Km/sec when it is at 10 Km/sec. Why does it make for less acceleration the faster it goes? I don't understand that bit. If you are in a spacecraft with say 1 gw of power to an ion rocket and you are doing say, 0.02 G, why would it be less, say 0.01G when you start at some low velocity and end up with a higher one, say starting at 10 Km/sec and later you are at 50 Km/sec why is the resultant acceleration less than it achieved at 10Km/sec with the same power input?

I am having trouble with that one because I thought at these low velocities compared with c, there would be nearly zero relativistic effects, mass increase, etc., which it is understandable why you would get less G force when you get up to say 0.99c V 0.01C.

But if I read it right this also happens with normal velocities also. What does a spacecraft know about its velocity at low velocities, how does it know it is at a higher velocity? Sure the kinetic energy increases and all, it will make a much bigger hole if it hits something at 50 km/sec than at 10km/sec but what is it inherent in the mass/velocity that slows down the actual acceleration when using constant power?
 
  • #22
litup said:
The 'B'^2 in that last is (V^2/C^2)?
Another question on acceleration. The talk of the recent Vasimir rocket, getting folks to Mars in two months, using a 200 mw power source to an ion engine.
I understand a constant power source will end up with a reduced acceleration rate over time as the velocity increases, independent of relativistic effects. Is that true?

The power going to the jet is measured in the vehicle's frame of reference, so the velocity increase over time doesn't change the effective exhaust velocity at all. If the power is coming from an external source, say via a laser, then the Doppler effect will reduce the power received, but that's quite different to the effect you're talking about.

I suspect you're thinking of how the thrust decreases as the exhaust velocity is increased during the operation of VASIMR.

I have seen equations of constant power inputs that says that. If so, and we are in normal ballistic velocities used in present day space probes, how does the system (the spacecraft ) know it is not say at 3 Km/sec when it is at 10 Km/sec. Why does it make for less acceleration the faster it goes? I don't understand that bit. If you are in a spacecraft with say 1 gw of power to an ion rocket and you are doing say, 0.02 G, why would it be less, say 0.01G when you start at some low velocity and end up with a higher one, say starting at 10 Km/sec and later you are at 50 Km/sec why is the resultant acceleration less than it achieved at 10Km/sec with the same power input?

It doesn't happen like that and the reason why is actually due to relativity, but don't ask me to explain how. One of those subtle mathematical points about Lorentz invariance. What I do know is that changing the exhaust velocity will change the thrust, but regardless of speed the exhaust velocity won't change since it's measured in the vehicle's reference frame.

I am having trouble with that one because I thought at these low velocities compared with c, there would be nearly zero relativistic effects, mass increase, etc., which it is understandable why you would get less G force when you get up to say 0.99c V 0.01C.

But if I read it right this also happens with normal velocities also. What does a spacecraft know about its velocity at low velocities, how does it know it is at a higher velocity? Sure the kinetic energy increases and all, it will make a much bigger hole if it hits something at 50 km/sec than at 10km/sec but what is it inherent in the mass/velocity that slows down the actual acceleration when using constant power?

Don't worry as it doesn't happen - thanks to relativity.
 

What is Alpha Centauri?

Alpha Centauri is the closest star system to our Solar System, located about 4.37 light years away. It consists of three stars, Alpha Centauri A, B, and Proxima Centauri, with Proxima Centauri being the closest to Earth.

Why is it important to reach Alpha Centauri in a human lifetime?

Reaching Alpha Centauri in a human lifetime would be a significant achievement for humanity as it would open up possibilities for interstellar travel and exploration. It would also allow us to study a star system other than our own in greater detail.

How long would it take to reach Alpha Centauri in a human lifetime?

The current technology and propulsion systems available would make it impossible to reach Alpha Centauri in a human lifetime. It would take approximately 30,000 years to reach the star system with our current technology.

What advancements in technology would be necessary to reach Alpha Centauri in a human lifetime?

Significant advancements in propulsion systems, energy sources, and spacecraft design would be necessary to reach Alpha Centauri in a human lifetime. Currently, research is being conducted on technologies such as nuclear fusion and solar sails that could potentially make this journey possible.

Are there any plans or projects in place to reach Alpha Centauri in a human lifetime?

There are a few proposed projects, such as Breakthrough Starshot and Project Orion, that aim to develop technologies to reach Alpha Centauri in a shorter amount of time. However, these projects are still in the planning and development stages and it may be several decades before a feasible mission is launched.

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