Relativity take two (1 of n)
Jan. 3rd, 2026 02:51 amSo, here's another go at explaining Special Relativity. I remain annoyed at how few people really get it, even amongst avid SF consumers, entirely too accustomed to generations of SF writers papering over FTL issues with technobabble, 'cause we need that galactic empire, don'tcha know.
Also, it's long past time to dump poorly motivated 1930s pedagogy that real physicists abandoned long ago (e.g.,. "Your mass increases as you go faster", "What? why?", "Fuck you, it just does" [spoiler alert: just No; forget you ever heard that. And if, in 2026, anyone is still trying to teach it that way, someone needs to sit them down for A Talk]).
All we need is basic geometry you knew or could have learned about in 6th grade plus a bit of algebra (up to Pythagorean Theorem). I think I can get by without using a single square-root sign.
But there will be fewer handwaves this time. Because we have to be clear why things have to Not Be The Way You Expected and not leave wiggle room. Here goes:
The speed of light as a constant
Shine a flashlight off of a moving boat. How fast does the light go?
- It could be like throwing a baseball, where speed of the boat matters.
- Or it could be like the waves that spread out when you jostle the boat or have it move, where replacing the boat with a possibly-moving helicopter tossing out stationary gravel makes zero difference—the wave fronts have a velocity with respect to the water and only the current/lack-thereof in the river/lake matters.
This is part of why they spent so much time from the 1600s onward arguing over whether light was a "particle" or a "wave" and they couldn't make headway because light goes so fast its speed was impossible to measure…
…until the 19th century, when the tech got good enough and the theory advanced to being able to say what light is (thanks, Maxwell), and we (sort of) get an answer: "It's like the waves in the water, but (surprise) there is no water". What we have is a number for "speed of light in a total vacuum", derived completely from constants, leaving no way to have it depend on any boat or water-current velocity, never mind there's nothing there that can have any kind of current in it.
Or, rather, the moment you try to imagine there being something there, you should then be able to infer the speed of any current in it by looking at the wave patterns you get from sources moving in various directions, even if this "water" is otherwise totally undetectable.
Except, they tried this. Result: The speed of the "current" is always zero (thanks, Michaelson and Morley).
Which then gets extra-special weird if you now arrange for there to be two boats in the same place, one stationary and one moving in some direction and somehow the magic "water" is moving in sync with both boats at the same time. How does this even work?
Answer: It can't. This is the point where Isaac Newton's head explodes.
The only way out is if one or both of the boats is having their distance and time measurements fucked with. But to get a handle on that, we need to go back to first principles on what it means to measure distance and time.
There's also the question of what it means for a boat to be "moving" when you don't have water anymore. Actually, let's start there:
I am Stationary
Let's make our lives as simple as possible by being somewhere out in interstellar space, far away from any distinguishing stars, planets, asteroids, or other landmarks of any kind, and where there's no gravity to speak of. Turn the engines off so that there's nothing accelerating us. Do shit with gyroscopes to make sure we are not spinning — gets rid of all of the weird (centrifugal, etc.) forces that would cause. (I vaguely recall Einstein spending multiple pages on what an "inertial reference frame" is, but this is all you get from me)
What we're left with is Newton's First Law: No forces on us means we are either "at rest" or moving at constant velocity in some direction. Except we can't tell the difference if all we have to look at is a bunch of distant stars that are all moving randomly. There would have to be Somebody Else local looking at us to say whether/how we're moving with respect to them. And even given that, we could still say, "No, we are stationary and you are the one who is moving."
If we can't tell the difference, perhaps it shouldn't matter. So given all of this (i.e., that I feel no forces, therefore none of the scenarios where I would know that I'm moving are in effect), I'll just declare myself Stationary and go from there.
Secondly, if I only trust measurements made by Other People Who Are Also Stationary, then I will not be relying on assumptions about how moving around affects measurements; i.e., if something is dicking with those numbers, I don't have to know in advance how that works. So, for Other People, it suffices to be able to tell whether they are also stationary; if not, then we just ignore them for now.
Measuring Time
Time is easy. Use your clock.
What is a clock? Some physical process — a totally reliable ISO Standard Gerbil In A Cage, or a spinning cesium-137 nucleus in a particular mode, we don't care, just pick something — takes a known amount of time to do a thing, making a "tick". Add some standardized mechanism to count ticks that everyone can build. As long as basic physical laws are the same everywhere (a not unreasonable assumption that may not actually be true but has sure worked really, really, really well so far), this should work. So I can now time everything happening where I am.
Measuring Distance
The trick here is to get as much mileage (pun intended) as we can out of the speed of light being this totally universal constant, which we now assume because that's what the experiments seem to be telling us..
If it's a constant, then it's like a conversion factor:
299,792,458 meters is one second;Most authors would trouble to say "light-second" or "light-year" here, but (I think) that's actually less helpful. Light goes 1 second per second, 1 year per year, or 1 meter per meter, or Just 1, Period (or "Full Stop", as my Brit friends would say). If it's already clear from context what we're measuring, the "light-" prefix is just unnecessary extra noise.
9,460,536,207,068,016 meters is one (Gregorian) year.
(I don't want to go so far as to say time and distance are the same thing; they're really not, even if it is natural to use the same units. Just like we can naturally measure distances on the surface of a sphere in degrees or radians, but we wouldn't want to say that distance and angle are the same thing; that would be confusing.)
Seems like we should now be able to use clocks and light to measure distance:
I have (1) a clock in my lap, (2) a video projector that can project an image of that clock onto a screen some distance away from me, and (3) sufficiently good eyesight to read what's on the screen
- Light needs time to get there and back, so the screen image will be delayed. If the clock image I see is, say, exactly 2 microseconds behind the clock in my lap, then the light must have traveled a total distance of 2 microseconds (≈ 2000 feet), one microsecond going out and one microsecond coming back.
- Even if the screen is moving, we can still know where it was at the exact moment that the light-ray bounced off of it: at exactly one microsecond (distance) away from me at exactly one microsecond ago.
Oh look, I just measured a distance. Go me.
What "Stationary" means
If I can now look at the screen over some period of time and see that distance does not change, i.e., that clock on the screen steadfastly remains 2 microseconds behind the clock in my lap, then I can know for certain that the screen cannot be moving. At least not in the radial (towards/away-from me) direction.
But since I'm not spinning, then transverse motions are also covered, i.e., if, I'm not having to be move my eyes or turn my head to track it, it can't be moving in those directions either, and we're done. I now have somebody located Elsewhere who I can trust.
My new friend can now put her own clock — identical construction, operating principles, and time units — next to her screen where I can see it, and I, in turn, can set up a screen next to me and return the favor.
- She has to see the same delay — light rays repeatedly covering the same distance back and forth, take the same amount of time, — so we have to agree on how far apart we are.
- If one of our clocks were to tick faster than the other, we'd have to agree on whose it is. Except that if we each have identical equipment and there's nothing else around us to distinguish where we are (e.g., if I were next to a black hole and she weren't, that would definitely be A Problem, so let's suppose there's nothing like that happening), meaning if flipping the entire universe 180° around the midpoint between us does nothing important except exchanging our identities, then how can swapping our names change the clock speeds? So this can't happen. Yay, symmetry. Which then means…
- The difference between our clock times being fixed, we can now synchronize our clocks. I suppose at this point we could have a political problem where we can't come to an agreement, but there'd still be a fixed difference, and so I will know what to subtract from her time readings to translate them to the time standard I want to use, so we may as well stipulate/assume her clock is synchronized with mine and be done with it.
Now repeat this for all of my other stationary friends. Now imagine an entire network of stationary friends located in all of the places I care about. I now know All Distances, to everyone and also between everyone because we talk to each other (over radios or whatever). This gives us a fishnet of spatial measurements, enough to derive some kind of coordinate system from (or I could take a WW2 Tokyo approach and use people's names to identify locations; whatever works).
And all of those in-synch clocks can time everything happening elsewhere on my network.
Finally, one last (temporary) simplification:
1-Dimensional Universe
Hi, we all live in the John Hancock Tower, where you never have to leave the building, where going anywhere means riding the elevator or going up and down stairs if that's more to your liking (since we're out in interstellar space with no gravity, stairs shouldn't be quite so onerous). Hey, it's got condos, offices, restaurants, movie theatres, everything you could ever want, right? (Yes, once upon a time, it really was considered Cool and Futuristic to construct buildings around the idea that people would want to live like this.)
One dimensional — we can add back the other dimensions later — means the floor number (z) is the only position coordinate we need. The aforementioned fishnet is now just an up-and-down line of stationary people, one on every floor, each of whom has a clock synched with mine.
Which then allows us to fit everything that happens on a 2-dimensional page, a spacetime grid with space going up-and-down and time scrolling left-to-right (yes this is flipped from how I've have previously done this and how most physics books do this; cope). Every horizontal line is a history of all of the events that happen on a particular floor of The Tower. Every vertical line is a snapshot of the universe/Tower at a particular time.
Some set of events will happen. I will record what happens on (or near) my floor with the time it occurs. All of my friends will do likewise. Everything goes onto the grid. And, at the End of Time, we get a picture of What Happened as far as We The Stationary People are concerned.
In the figure, we can see what a typical distance measurement looks like. I point my projector up (or down), send out a light ray at 'Sent', the light bounces off of a screen at 'Upper (Lower) Bounce' at some particular distance (n) above (below) me, and comes back to me at 'Received'. Both bounces and 'Halfway Tick' are all in the same snapshot, so they're all taking place at the same time. Easy.
What Nice Units We Have
One consequence of using the same units for distance and time — whether it's feet (= nanoseconds), microseconds (= kilofeet), seconds, etc. — is that all light rays, whether traveling upwards or downwards, will be going at 45° (traversing one distance unit per time unit) on our grid.
Why care about this? Because so much becomes more obvious when you scale time vs. distance the right way.
E.g., imagine surveying your backyard measuring north-south distances in meters and east-west distances in Astronomical Units (1AU=150 million km), i.e., compressing the east-west scale by a factor of 150 billion for basically no reason. That would be stupid, right?
But that's essentially what we were doing before 1905 and why it took 200+ years to figure out Newton had screwed something up.
And now it's time to…