Spatial Displacement Theory · Start Here
Nothing in the universe pulls.
Everything gets pushed. Once you see why, a lot of strange things stop being strange. Here is the whole idea, from the very beginning, in plain words.
J. C. Harvey · Melbourne · Simplified edition
Step 1
Space is a thing, not a nothing
Most people picture space as emptiness. An empty stage, and stars and planets are the actors standing on it.
That is not what space is. Space is made of something. It is built from grains — unimaginably tiny beads, all exactly the same size, packed against each other with no gaps in between. There is no such thing as a bit of space with nothing in it. Space is the stuff.
One grain on its own will not squash. Push it and it holds. But a huge crowd of them together can bend, flow and part — the way a crowd of people can let you through even though no single person is squishy.
Step 2
Everything is moving, and "now" is the only time there is
Nothing in this universe ever sits perfectly still. Everything moves, always.
So what is time? Time is not a river you float down. There is no yesterday sitting in a room behind you, and no tomorrow waiting in a room ahead. There is only now. It always was now, and it always will be.
What we call time is just counting. Count how much things have moved and you have made a clock. The past is the count you already made. The future is the count you expect. Neither one is a place you could visit.
Step 3
The whole sky is squeezing you, right now
Here is the strange part. Space is being pushed inward at you from every direction at once — from above, below, both sides, and from every distance out to the very edge of everything we can see.
The push is enormous. So why can't you feel it?
Because it is perfectly even. The push from your left exactly matches the push from your right. Balanced pushes cancel, and you feel nothing at all. That is the only reason space seems empty to us. It isn't empty. It is balanced.
Step 4
Shadows are what we call forces
Now — what happens if something blocks part of that push?
Put two objects near each other. Each one blocks a little of the push heading toward the other. So between them the push is slightly weaker, while behind them it is still full strength.
Full push on the outside, weaker push in the middle. So they get squeezed together.
This is the whole idea behind every force you have ever felt. Gravity is this. Magnets are this. The force holding the middle of an atom together is this. They look wildly different in strength only because the shadows are different sizes — not because they are different kinds of thing.
Step 5
What matter actually is
So what does the blocking? What is a particle?
A particle is a knot. Take movement, loop it around, and tie it so it cannot come undone. That knot is a thing — a proton, say. It is not a tiny ball, and it is not a fuzzy cloud. It is tied movement.
And here is the one genuinely new idea in this whole theory, the sentence everything else grows out of:
The grains it shoves aside have to go somewhere. Where they go — crowding up ahead of it, trailing behind it, casting a shadow — is every force in the universe.
Step 6
Why heavy things are hard to push
Try to shove a heavy thing and it resists. We call that mass. But what is actually resisting?
Not the object. The space around it. A knot of matter has already squashed the space it sits in. To move it somewhere else, all that squashing has to be undone here and redone over there. That rearranging takes effort — and that effort is the mass.
Mass isn't a substance the object is carrying around. It is the price of changing its mind about which way to go.
Step 7
Everything moves at the same speed. Yes, everything.
This one sounds impossible, so read it slowly.
Everything in the universe is moving at exactly the speed of light — all the time, including you, right now, sitting still.
The trick is that a thing can spend its movement in two ways: spinning on the spot, or travelling somewhere. You only get one allowance, and it never changes size.
Sit still and you spend the whole allowance spinning inside. Move fast and you must take some out of the spin to pay for the travel. Since your inner spinning is what your clock is made of, a fast-moving clock ticks slower. It isn't magic and time isn't stretching. You just spent your movement on something else.
Step 8
Gravity is a slope, not a bend
Near a big object like a star, space is squashed. Close in, it's squashed a lot; further out, less. So there is a slope.
Everything drifts along that slope, because that is simply the easiest path through it. A planet going around the Sun isn't held by an invisible rope. It has found a loop that costs it the least, and it keeps going around because nothing stops it.
Light feels the slope too. Deep in the squash, light travels a touch slower — so a radio signal that grazes past the Sun arrives a fraction of a second late. That delay has actually been measured by real spacecraft, and this theory now gets it right to about one part in sixty thousand.
Step 9
Building atoms out of shadows
The middle of an atom is built from a few standard pieces that fit together like gear teeth — and there is a strict rule: each piece only ever meshes with the opposite kind, never its own kind. Because of that rule the whole thing turns together without ever jamming.
Chemists have known for a century that some atoms are unusually sturdy — the ones with 2, 8, 20, 28, 50, 82 or 126 neutrons. Nobody could say why those numbers and no others. They were just a list you memorised.
In 2026 that list stopped being a mystery. Those numbers are what you get when you count how many pieces fit on each layer as an atom is built up, shelf by shelf. Two small counting rules give you all seven numbers — and they predict the next one, which should be 184, in a kind of atom nobody has made yet.
Step 10
The universe is not blowing up like a balloon
Distant galaxies look redder than they should. The usual story is that everything is flying apart and space itself is stretching.
This theory says something quieter: light gets tired-looking for two ordinary reasons instead. It leaves from deep inside a squashed patch of space, and then it gets gently squeezed on its long journey to us. Nothing has to be running away.
If that's right, then there is no dark energy, no expansion, and no mysterious invisible matter needed either. Just space, doing what space does.
The honest part
What we still cannot do
Any theory that only tells you its wins is trying to sell you something. So here is the list of things this one cannot do yet.
Most of these are half-solved rather than untouched, so here is both halves each time — what works, and what still doesn't.
The size of the grain
We cannot work it out. We have to measure it and hand it to the theory.
But: we proved this is unavoidable. You can never build a length out of pure numbers — someone has to give you one ruler to start with. Knowing exactly why you're stuck is better than not knowing you are.
How galaxies spin
Our first big model was 66% wrong against real galaxy data. Not close. It's still on the website, with the failure written in the same size letters as the wins.
But part of it works. We can predict the "floor" — the gentlest push a galaxy can feel — from the size of the visible universe, with nothing fitted. And one single rule ties atoms to stars to galaxies to within 8.8%. When we deliberately fed that test a wrong floor to see if it would notice, it got six times worse — so the test genuinely can tell right from wrong.
What's still missing is the shape of the spin. The curve we use for that is borrowed from someone else's theory, and borrowing isn't explaining.
Big atoms
We cannot yet predict how hard it is to pull an electron off a large atom. Some are out by 500%.
But: for hydrogen — one proton, one electron — we get the colours of its light right to about three parts in ten thousand, with nothing adjusted. The simple case works; the crowded case doesn't yet.
The beautiful number
A proton is 1836 times heavier than an electron. The expression 6π⁵ gives 1836.118 — a match to 19 parts in a million, and no other tidy expression comes anywhere near.
But we don't know why, so we are not allowed to claim it. It sits on the site marked OPEN. The same goes for the rule that fixes the proton's size: it lands within 0.02% of the measurement, and it is still labelled a conjecture, because nobody has proved it from the knot's geometry yet.
A good theory earns trust by being clear about where it fails, and then going and fixing it. Every claim on this website has a number attached, and every number can be checked by running the code yourself.
When you want more depth, the same story is told twice more: once in full for the general reader, and once in equations for physicists. Same twenty-one steps, three different levels.