OrbitStanding on the Moon
Since the Moon was first built, tapping it gave a line of fact. Now it takes you there. Once the Moon is made, a tap leaves the Earth: the camera dives, the Moon doubles on the screen at a steady beat until it fills the frame, the ground comes up under a sheet of dust, and you are standing on it. No air, so the stars are out at noon and every shadow is black to the bottom. The dust the landing throws flies in arcs and falls straight back, because there is nothing for it to hang in. The horizon is a hard line. Close it and you lift off and fall back into orbit exactly where you were.
The Earth in that sky is the one you left. It is the same globe, the same clouds and the same sunlight, drawn a second time into the lunar sky and turned so that the face that looks at the Moon looks at you. Its phase is the real one: the angle between Earth, Moon and Sun is taken from the orbit as it stood when you tapped, and the Sun is placed on this ground from the same geometry, low when the geometry allows it. When it does not, it is night here and the Earth lights the ground, which is what a full Earth does. In the Jurassic the orbit can carry the Moon through the Earth's shadow, and then you stand in that shadow: the Earth is a dark disk with a ring of red air, and the ground goes copper. The Earth hangs where it hangs and never rises or sets, since the Moon keeps one face toward it, and in the early worlds it is larger, because the Moon was closer then. It is drawn a little larger than it would look from here, so the world on it can be read, and the page says so.
The reason it exists is on its way. A slice of Northeast Africa 104, a lunar troctolite melt breccia found in 2025 and one of thirteen of its kind ever classified, was bought on the 28th and arrives the first week of October. The panel on the surface describes it and says it is on its way; the record comes when it is in the collection, and the panel will say so then. Where on the Moon it left from is not known, so the ground is no place in particular, and it is drawn.
One sound was added, for those who have the sound on: the feet meeting the ground, a low thump, the one sound the Moon can carry, through the boots. Nothing else here makes a noise, and the page says why.
A second pass the same night, after the first look. The cut to the surface is now a camera move: the dive ends looking straight down at the Moon, and the surface opens forty meters up looking straight down at the ground, falling and tilting to the horizon as the dust thins, so the eye is carried in rather than handed across. The sky is no longer still. The Earth turns at a pace that can be seen, the stars wheel slowly, the finest dust drifts above the ground the way the Surveyor landers photographed it, and now and then something small arrives from space at speed: no streak, because there is no air to make one, only the flash where it lands and the ground thrown up. Hundreds of pebbles lie in the near ground, and the grain of the regolith was calmed. A second panel on the right draws a section through the Moon under your feet, regolith to mantle, with the depth the troctolite grew at and the line a strike took to throw it clear. Back to orbit moved above the text it used to cover. Time does not move while you are away from the planet.
Third pass. Both panels wider, the type larger, and no small print anywhere on the Moon. Depths on the section lead with feet, its names sit at an even pitch with a hairline to each layer, and the line that carries the rock out runs through no word. The section now plays the story it only told before: something falls out of the top right, the ground opens, the break runs down through the crust to the depth the troctolite grew at, and a piece rides the break up and out along the line toward the Earth, every twelve seconds. The boulders lost their razor edges, the shadow map was widened until no seam crossed the ground, and a little more of the fine dust drifts.
Fourth pass. The section carries depths now, feet and miles first: fifty feet of regolith, two miles of shattered crust, twenty-five miles of anorthosite, and the six to twenty-five miles the troctolite grew at, every one marked as an estimate. The panel says how old the rock is, which it had not: no age has been measured on the stone, so the age is by its kind, the 4.3 billion years of the Apollo troctolites. The grid that crossed the ground was the grain of the regolith meeting itself at every tile edge; the tiles now mirror, and there is no edge to meet. Two faults in the page were fixed on the way: a stop chosen on the rail while Travel through time was running took you there and then dragged you back, since the journey kept going; now a chosen moment ends the journey. And the panels lingered after lift-off, because the wait on the way in was applied on the way out; they leave at once now.
Fifth pass, the one that makes it a place. You can look around: drag turns your head, and on a phone the phone does, so the Earth is where the Earth is when you hold the phone up. Time runs on the Moon. The rail stays, the arrow keys work, and the planet keeps updating underneath, undrawn, so the Earth in that sky is the Earth of whatever moment you scroll to: stand still and watch Pangaea open. Tap the Earth and you fall back toward it. Things on the ground carry gold callouts in Scale's language, and each says how it is known: a young crater, a boulder, the regolith, and beyond the horizon the two kinds of Moon the collection wants next, the dark seas and the white crust, marked as wants. The slice hangs in front of you as a projection at its true proportions until the scan exists. The Sun creeps so the shadows can be seen to move; a strike in the distance is heard a moment late, through the ground; the galaxy is a band across the sky; the visitor crosses now and then, far off. The hills at the edge give the horizon a shape. And the frame is finished softer, a touch of diffusion folded over the whole picture, so no edge on the Moon ends on a razor line.
Sixth and seventh passes, after a night's look: the screen was doing three jobs in one column of words. Now one box opens folded, the name of the place and one line on how to move, with three toggles under it. Open one and it opens; open it again and it folds back, and the Moon gets the room. The section moved inside the third toggle. The hills at the edge became worn domes; they had come out as cones. The callouts and the rock's label sit on dark chips so they read against white ground, and the projection of the slice carries a shade behind its light for the same reason. The two wants point at the hills, not at the sky. A Sun below the horizon lights nothing: the undersides of the rocks had glowed at night. More of the fine dust drifts, and some of it close. The sound of the Moon is what the astronauts said it was: your own suit, the fans and a slow breath, with the dark beyond. And a world chosen on the rail while Travel through time was running still dragged you back, because the world stops took a different road from the other stops; every stop ends the journey now.
Eighth and ninth passes, into the small hours, from the phone in one hand. Holding the phone up and finding the Earth was the first thing to feel like being somewhere, so the rest of the night went to the things a place has. On a phone the box opens full screen when a toggle is chosen, with a Close that breathes the first time so it is seen, and folds back to one line; the toggles are named for what they hold, Here, The troctolite, Where it came from, since the rock is not a rock but one of thirteen of its kind. The thermometer came to the Moon, reading the ground under you: about +250 °F in the Sun and −208 °F in the dark, the Apollo and Diviner numbers, swinging with the light as the Sun creeps. The air and the day-length stayed off, because the answers are none and twenty-nine days, and the Here text already says so.
Then the events. An eclipse comes on its own about forty seconds after landing and every few minutes after: the creeping Sun passes behind the Earth, the ground goes to almost nothing and turns copper, the Earth goes black with a ring of red air around it, the Sun's glow stands out from behind the disk, and the thermometer falls. From the Earth this is a lunar eclipse; from where you stand it is the Earth eclipsing the Sun, which no camera has ever been placed to see. A row under the one-liner, Watch, calls any of four events rather than waiting: the eclipse; a strike, close and in front of you, with the flash, the ground thrown up, the thud through your boots a beat later and the ground shaking under you; night, the Sun carried under the horizon and the two-week dark arriving in half a minute, the stars taking the sky and the Earth lighting the ground blue, then dawn; and a shower, a minute of strikes across the plain, because when the Earth crosses a comet's trail the Moon crosses it too, and with no air to burn them up the meteors land. Astronomers watch for those flashes from here. On a phone, Motion on at the top right hands the looking to the phone or gives it back to the finger. Fourteen versions of Orbit in one day, all of them the Moon.