A perspective camera leans everything away from the centre of the frame. In a
system that means the orbits are ellipses whose shape depends on where they
happen to sit on screen, so two planets on the same circular orbit do not look
like they are on the same circle. Plan view, in the Display panel, swaps the
projection for a parallel one and swings to look down the plane the current
scale is read against — the galactic plane out in the field, this system's own
orbital plane inside one. Circles are circles again, wherever they are.
Both halves are the feature and neither alone is it. The projection is what
makes the shape honest; the swing is what makes it worth looking at. Orbiting
still works afterwards, so a plan is where the view starts rather than a cage.
The engine now holds both cameras and keeps them in step, rather than making
one on demand: a camera that exists only while it is being looked through is a
camera whose pose is always one swap out of date. The orthographic frustum is
derived, never stored — it is the perspective camera's own frustum at the
current orbit distance, made parallel — which is why the camera flights work
through it untouched. They move the camera; the frame follows.
Three things had to be taught that a projection had changed.
Sprites. three.js turns an angular size into a world size only when it is
compiling against a perspective camera (SpriteNodeMaterial: `camera
.isPerspectiveCamera && sizeAttenuation === false`). Under a parallel one that
step is silently skipped and every star in the field collapses to a thousandth
of a parsec. The same arithmetic is now done in the node graph behind a
uniform, so one material serves both cameras without being recompiled — and
picking follows it exactly, since a star has to be clickable where it is drawn.
Depth. A parallel camera does not back away as its frame grows, so at galactic
framing the backdrop shell and half the Milky Way sit behind its own plane. Its
depth range is symmetric about it instead, which a linear depth buffer can
afford and a perspective one could not.
And distance. Half the map was keyed on how far back the camera was pulled —
the scale ladder, the crossfade, the label radius, the range readout — which
under a parallel projection says nothing at all, because the frustum sets the
extent. They all read one honest equivalent now: the distance a perspective
camera would need to frame the same thing.
Two defects found while verifying, both mine, both from this change:
The per-frame work was computed against the camera captured at bootstrap while
the renderer drew through the other one, so after a swap every label was
projected by a camera nobody was looking through.
And the zoom limits were derived from the orbit limits, which are in whichever
unit space the view is in. Reading them on the frame the scene swaps parsecs
for astronomical units pinned the zoom at the ratio between the two, and
leaving a system landed the view three kiloparsecs out. Zoom is a plain
multiplier on a frame the distance already sets, so it is bounded by a factor.
Verified: build clean, 595/595 unit including a new spec for the projection
arithmetic, 13/13 end-to-end including two that flatten a system and check the
ladder still knows how far out it is, design detector clean, screenshots of
both scales in both projections.
Co-Authored-By: Claude Fable 5 <noreply@anthropic.com>
Claude-Session: https://claude.ai/code/session_016jxMkwA2rbicdGxHosecYi
SenrokaiandClaude Fable 5
d9bd913458