5 ms·
I was wrong, see edit below. No, there is still an lower limit of 4.37 years to get to alpha-centauri within any frame of reference no matter how much you acce
by TrainedMonkey 12y ago
I was wrong, see edit below.
No, there is still an lower limit of 4.37 years to get to alpha-centauri within any frame of reference no matter how much you accelerate within conventional space.
What relativity does, is that if you travel close to speed of light time taken for the trip as measured on ship versus on earth could be different by many orders of magnitude.
edit: Was wrong, as per [0] "This is something many readers don't understand well, so it bears repeating: The journey times as experienced by those on the ship are not limited by the speed of light. Instead what they experience is the planetary reference frame getting relativistic."
[0] http://en.wikipedia.org/wiki/Space_travel_using_constant_acceleration#Ship_reference_frame http://en.wikipedia.org/wiki/Space_travel_using_constant_acc...
- lfuller 12y agoThat's not true. From the perspective of the travelers space will appear to contract dramatically - though the speed of light remains constant, the distance traveled is reduced.
- readerrrr 12y agolfuller is right. For example, if you have a ship capable of continuous acceleration at 1g, you can reach any point in the universe on the order of ~50 years.
- ikeboy 12y agoCan you continuously accelerate at g for 50 years without going over the speed of light? According to wolfram alpha http://www.wolframalpha.com/input/?i=speed+of+light%2Flittle+g http://www.wolframalpha.com/input/?i=speed+of+light%2Flittle... it would take a year to get to the speed of light at 1g (if my equation was right.) Then you can't speed up anymore.
- pdonis 12y ago> it would take a year to get to the speed of light at 1g (if my equation was right.) It isn't. Wolfram Alpha apparently doesn't know about the relativistic rocket equation. Try here: http://math.ucr.edu/home/baez/physics/Relativity/SR/rocket.html http://math.ucr.edu/home/baez/physics/Relativity/SR/rocket.h...
- gizmo686 12y agoYour equation is correct in a Newtonian universe, but does not consider relativistic effects. Generally when we talk about an object's acceleration, we are talking about its acceleration in its own reference frame. By definition, an object's velocity in its own reference frame is always 0, so acceleration does not become more difficult (ignoring the fact that the surrounding matter will be impacting you at higher speeds). From the perspective of an outside observer who is not accelerating, time would appear to slow down on the accelerating object, and the outside observer would record a decreasing acceleration.
- readerrrr 12y agoFun fact, from the perspective of the observer on the ship, time outside the ship would also appear to slow down.
- ikeboy 12y agoSo why is it difficult to maintain a constant acceleration? Is 1g really that impractical right now?
- gizmo686 12y ago1) Maintaining an acceleration requires fuel. 2) Even though you don't observe yourself moving at increasing speeds, you do observe the rest of the universe moving at increasing speeds. This means that small particles impacting your ship will hit it with increasing energy.
- snowwrestler 12y agoI'm being accelerated at 1g right now and I'm about 40...so in another decade or so I should be able to get to anywhere in the universe! Jokes aside, there's no fuel source we know of that would allow a ship to accelerate continuously for 50 years at 1g.
- readerrrr 12y agoAfter a year of acceleration at 1g, a stationary observer would observe a speed of 215184620 m/s or 71.7% the speed of light. After two years: 89.9% After four years: 97.2% After eight years: 99.3%
- EGreg 12y agoWait why can't you get under 4 years if you accelerate really fast?
- joshuahutt 12y agoBecause it's 4.367 light years away [1]. [1] https://www.google.com/search?q=distance+to+alpha+centauri https://www.google.com/search?q=distance+to+alpha+centauri
- EGreg 12y agoBut from the point of view of the traveler, it an take far less time.