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feat(sky): replace the blocky default sky box with catalogue stars
Cesium's default Tycho-2 sky box is six 1024² JPEGs stretched 3–6× around the whole-globe view, so space read as an over-compressed JPEG (HAL-627). The scene now draws its own sky in the Scene#skyBox slot: the 9,096 stars of the Yale Bright Star Catalogue as point sprites sized in CSS pixels (magnitude → width and opacity, B−V → colour), over a soft, star-free Milky Way cube map built from ESO/S. Brunier's panorama (CC BY 4.0). Both layers share one ICRF→Earth-fixed rotation at the scene clock, with the TEME rotation filling in until Cesium's IAU 2006 tables load. Assets total 482 KB, built by scripts/build-bright-stars.mjs and scripts/build-milky-way.mjs. Frame time and the idle render governor are unchanged. Co-Authored-By: Claude Opus 5.5 <[email protected]>
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#!/usr/bin/env node
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/**
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* Build src/data/local_data/sky/bright_stars.json from the Yale Bright Star
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* Catalogue, 5th Revised Edition (Hoffleit & Warren 1991).
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*
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* Source: CDS VizieR catalogue V/50, https://cdsarc.cds.unistra.fr/viz-bin/cat/V/50
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* Fetched: https://cdsarc.cds.unistra.fr/ftp/V/50/catalog.gz
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* Format: fixed-width ASCII, 197 bytes per record, byte layout in
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* https://cdsarc.cds.unistra.fr/ftp/V/50/ReadMe
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* License: public domain (Yale University Observatory / NASA ADC); CDS asks
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* for an acknowledgement, which DATA_SOURCES.md carries.
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*
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* Transform (deterministic):
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* 1. J2000 RA/Dec (bytes 76-90), V magnitude (103-107) and B−V (110-114).
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* 2. The 14 records without a J2000 position (novae and other objects later
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* found not to be stars) are dropped.
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* 3. RA/Dec rounded to 3 decimals of a degree (3.6″ — a fraction of a pixel
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* at any field of view the globe uses), magnitudes to 2.
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* 4. Missing B−V is stored as null; the renderer gives it a neutral colour.
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* 5. Records keep catalogue (HR) order for a stable diff.
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*
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* Usage:
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* node scripts/build-bright-stars.mjs [catalog | catalog.gz]
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* With no argument it downloads the catalogue from CDS.
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*/
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import fs from 'node:fs';
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import path from 'node:path';
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import zlib from 'node:zlib';
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import { fileURLToPath } from 'node:url';
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const SOURCE_URL = 'https://cdsarc.cds.unistra.fr/ftp/V/50/catalog.gz';
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const OUT = path.join(
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path.dirname(fileURLToPath(import.meta.url)),
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'..',
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'src',
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'data',
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'local_data',
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'sky',
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'bright_stars.json',
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);
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/** Slice 1-based inclusive byte columns the way the CDS ReadMe numbers them. */
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function columns(line, from, to) {
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return line.slice(from - 1, to).trim();
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}
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/** Parse a fixed-width float; blank fields are null. */
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function parseField(text) {
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if (text === '') return null;
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const value = Number(text);
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return Number.isFinite(value) ? value : null;
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}
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/**
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* Parse one BSC5 record. Returns null for records without a J2000 position
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* or V magnitude.
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*/
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export function parseBscRecord(line) {
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const hr = parseField(columns(line, 1, 4));
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const raH = parseField(columns(line, 76, 77));
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const raM = parseField(columns(line, 78, 79));
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const raS = parseField(columns(line, 80, 83));
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const sign = columns(line, 84, 84);
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const deD = parseField(columns(line, 85, 86));
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const deM = parseField(columns(line, 87, 88));
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const deS = parseField(columns(line, 89, 90));
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const vmag = parseField(columns(line, 103, 107));
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const bv = parseField(columns(line, 110, 114));
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if (
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hr === null ||
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raH === null ||
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raM === null ||
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raS === null ||
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deD === null ||
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deM === null ||
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deS === null ||
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vmag === null ||
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(sign !== '+' && sign !== '-')
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)
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return null;
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const raDeg = (raH + raM / 60 + raS / 3600) * 15;
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const decDeg = (sign === '-' ? -1 : 1) * (deD + deM / 60 + deS / 3600);
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return { hr, raDeg, decDeg, vmag, bv };
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}
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const round = (value, decimals) => {
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const scale = 10 ** decimals;
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return Math.round(value * scale) / scale;
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};
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/** Build the committed pack from the raw catalogue text. */
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export function buildStarPack(text, { fetched = null } = {}) {
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const stars = [];
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let dropped = 0;
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for (const line of text.split('\n')) {
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if (line.trim() === '') continue;
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const record = parseBscRecord(line);
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if (!record) {
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dropped += 1;
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continue;
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}
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stars.push(
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round(record.raDeg, 3),
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round(record.decDeg, 3),
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round(record.vmag, 2),
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record.bv === null ? null : round(record.bv, 2),
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);
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}
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return {
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meta: {
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source:
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'Yale Bright Star Catalogue, 5th Revised Ed. (Hoffleit & Warren 1991), CDS V/50',
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url: SOURCE_URL,
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license: 'public domain',
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fetched,
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frame: 'ICRF/J2000, epoch 2000.0',
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columns: ['raDeg', 'decDeg', 'vmag', 'bv'],
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count: stars.length / 4,
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dropped,
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},
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stars,
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};
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}
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async function readCatalogue(file) {
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if (!file) {
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const response = await fetch(SOURCE_URL);
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if (!response.ok) throw new Error(`${SOURCE_URL}: HTTP ${response.status}`);
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return zlib
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.gunzipSync(Buffer.from(await response.arrayBuffer()))
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.toString('latin1');
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}
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const bytes = fs.readFileSync(file);
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return (file.endsWith('.gz') ? zlib.gunzipSync(bytes) : bytes).toString(
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'latin1',
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);
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}
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async function main() {
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const [file] = process.argv.slice(2);
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const text = await readCatalogue(file);
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const pack = buildStarPack(text, {
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fetched: new Date().toISOString().slice(0, 10),
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});
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// One star per line keeps the JSON compact and the diff readable.
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const rows = [];
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for (let i = 0; i < pack.stars.length; i += 4)
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rows.push(JSON.stringify(pack.stars.slice(i, i + 4)).slice(1, -1));
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const body = `{"meta":${JSON.stringify(pack.meta)},\n"stars":[\n${rows.join(',\n')}\n]}\n`;
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fs.mkdirSync(path.dirname(OUT), { recursive: true });
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fs.writeFileSync(OUT, body);
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console.log(
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`wrote ${pack.meta.count} stars (${pack.meta.dropped} dropped) → ${path.relative(process.cwd(), OUT)} (${body.length} bytes)`,
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);
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}
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if (process.argv[1] === fileURLToPath(import.meta.url)) await main();
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@@ -0,0 +1,372 @@
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#!/usr/bin/env node
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/**
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* Build the soft Milky Way cube map in src/data/local_data/sky/ from the ESO
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* all-sky Milky Way panorama.
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*
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* Source page: https://www.eso.org/public/images/eso0932a/
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* Fetched: https://cdn.eso.org/images/original/eso0932a.tif
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* (6000×3000 8-bit sRGB TIFF, 27.7 MB; sha256 in README.md)
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* Credit: ESO/S. Brunier
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* License: CC BY 4.0 (https://www.eso.org/public/outreach/copyright/).
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* Modified: stars removed, blurred, reprojected to ICRF cube
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* faces and tone-mapped, as below.
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* Frame: plate carrée in galactic coordinates, centred on the Galactic
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* Centre, galactic longitude increasing to the left.
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*
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* Transform (deterministic):
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* 1. Resample to WORK_WIDTH×WORK_WIDTH/2 and convert sRGB to linear light.
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* 2. Paint out the planets the 2008–2010 exposures caught (PLANETS): they
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* sit where today's sky has nothing and are far brighter than any star.
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* 3. Remove stars with a morphological opening (minimum, then maximum, over
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* a (2·OPEN_RADIUS+1)² window): anything smaller than the window — every
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* star — drops to the surrounding sky; the renderer draws catalogue stars
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* itself, sharp and in the right place.
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* 4. Blur with a three-pass box approximation of a Gaussian, σ = BLUR_DEG on
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* the sky: rows wrap in longitude and widen by 1/cos(latitude) so the
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* blur stays round towards the poles.
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* 5. Resample into six FACE_SIZE² cube faces in the standard WebGL face
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* orientation (the renderer uploads them without flipY), with the ICRF
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* axes as the cube axes — +X to the March equinox, +Z to the north
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* celestial pole — rotating each direction into galactic coordinates
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* with the IAU J2000 matrix.
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* 6. Map the darkest 25 % of the sky to black and the brightest 0.01 % to
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* white, encode with gamma 1/2.2 and ±0.5 LSB dither against banding;
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* WebP.
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*
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* Usage:
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* node scripts/build-milky-way.mjs <eso0932a.tif>
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* Needs the sharp dev dependency.
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*/
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import path from 'node:path';
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import { fileURLToPath } from 'node:url';
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export const FACE_SIZE = 1024;
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export const BLUR_DEG = 0.4;
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const WORK_WIDTH = 4096;
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const OPEN_RADIUS = 3;
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const WEBP_QUALITY = 96;
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// The darkest quarter of the sky is the black level: away from the galactic
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// plane the panorama carries a mottled glow of unresolved stars that would
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// read as grey fog around the globe.
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const BLACK_PERCENTILE = 0.25;
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const WHITE_PERCENTILE = 0.9999;
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const OUT_DIR = path.join(
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path.dirname(fileURLToPath(import.meta.url)),
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'..',
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'src',
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'data',
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'local_data',
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'sky',
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);
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/**
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* Bright planets in the panorama, galactic longitude/latitude in degrees and
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* the radius painted over with the surrounding sky. By position both are
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* Jupiter, in Sagittarius (2008) and Aquarius (2010); no catalogue star lies
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* under either.
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*/
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export const PLANETS = Object.freeze([
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{ l: 13.4, b: -16.6, radiusDeg: 2.5 },
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{ l: 69.0, b: -58.4, radiusDeg: 2.5 },
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]);
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/** Cube faces in WebGL upload order. */
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export const CUBE_FACES = Object.freeze([
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'positiveX',
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'negativeX',
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'positiveY',
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'negativeY',
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'positiveZ',
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'negativeZ',
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]);
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export const FACE_FILE_SUFFIX = Object.freeze({
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positiveX: 'px',
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negativeX: 'nx',
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positiveY: 'py',
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negativeY: 'ny',
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positiveZ: 'pz',
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negativeZ: 'nz',
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});
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/**
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* ICRF (J2000 equatorial) → galactic rotation, rows = galactic axes
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* (Hipparcos catalogue, ESA SP-1200 vol. 1 §1.5.3).
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*/
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export const ICRF_TO_GALACTIC = Object.freeze([
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[-0.0548755604162154, -0.873437090234885, -0.4838350155487132],
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[0.4941094278755837, -0.4448296299600112, 0.7469822444972189],
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[-0.867666149019004, -0.1980763734312015, 0.4559837761750669],
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]);
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/**
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* Direction (not normalized) that the WebGL cube-map lookup sends to texel
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* coordinate (s, t) ∈ [0, 1]² of `face`, t = 0 being the first image row.
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* Inverse of the OpenGL ES 3.0 §3.8.10 major-axis table.
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*/
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export function cubeFaceDirection(face, s, t) {
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const sc = 2 * s - 1;
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const tc = 2 * t - 1;
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switch (face) {
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case 'positiveX':
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return [1, -tc, -sc];
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case 'negativeX':
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return [-1, -tc, sc];
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case 'positiveY':
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return [sc, 1, tc];
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case 'negativeY':
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return [sc, -1, -tc];
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case 'positiveZ':
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return [sc, -tc, 1];
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case 'negativeZ':
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return [-sc, -tc, -1];
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default:
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throw new RangeError(`Unknown cube face ${face}`);
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}
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}
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/** Rotate an ICRF direction into galactic coordinates. */
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export function icrfToGalactic([x, y, z]) {
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return ICRF_TO_GALACTIC.map((row) => row[0] * x + row[1] * y + row[2] * z);
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}
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/**
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* Map a direction to (u, v) ∈ [0, 1)² of a plate carrée centred on
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* longitude 0 with longitude increasing to the left and v = 0 at +90°.
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*/
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export function directionToPlateCarree(x, y, z) {
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const longitude = Math.atan2(y, x);
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const latitude = Math.atan2(z, Math.hypot(x, y));
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let u = 0.5 - longitude / (2 * Math.PI);
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u -= Math.floor(u);
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return [u, 0.5 - latitude / Math.PI];
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}
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/** Box widths whose three passes approximate a Gaussian of `sigma` (Kovesi). */
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function boxRadii(sigma) {
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const ideal = Math.sqrt((12 * sigma * sigma) / 3 + 1);
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let lower = Math.floor(ideal);
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if (lower % 2 === 0) lower -= 1;
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const upper = lower + 2;
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const m = Math.round(
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(12 * sigma * sigma - 3 * lower * lower - 12 * lower - 9) /
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(-4 * lower - 4),
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);
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return [0, 1, 2].map((i) => ((i < m ? lower : upper) - 1) / 2);
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}
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/** Index along a line, wrapped or clamped at the ends. */
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function lineIndex(i, length, wrap) {
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if (wrap) return ((i % length) + length) % length;
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return i < 0 ? 0 : i >= length ? length - 1 : i;
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}
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/** Running-sum box blur of one strided line. */
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function boxLine(src, dst, offset, stride, length, radius, wrap) {
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if (radius < 1) {
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for (let i = 0; i < length; i++)
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dst[offset + i * stride] = src[offset + i * stride];
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return;
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}
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const r = wrap ? Math.min(radius, Math.floor((length - 1) / 2)) : radius;
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const at = (i) => src[offset + lineIndex(i, length, wrap) * stride];
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let sum = 0;
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for (let i = -r; i <= r; i++) sum += at(i);
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const scale = 1 / (2 * r + 1);
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for (let i = 0; i < length; i++) {
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dst[offset + i * stride] = sum * scale;
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sum += at(i + r + 1) - at(i - r);
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}
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}
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/** Minimum or maximum over a (2r+1) window of one strided line. */
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function extremumLine(src, dst, offset, stride, length, radius, wrap, pick) {
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for (let i = 0; i < length; i++) {
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let value = src[offset + lineIndex(i - radius, length, wrap) * stride];
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for (let k = -radius + 1; k <= radius; k++)
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value = pick(
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value,
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src[offset + lineIndex(i + k, length, wrap) * stride],
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);
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dst[offset + i * stride] = value;
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}
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}
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/** Separable minimum or maximum filter over a plate-carrée plane, in place. */
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function extremumPlane(plane, width, height, radius, pick) {
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const scratch = new Float32Array(plane.length);
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for (let y = 0; y < height; y++)
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extremumLine(plane, scratch, y * width, 1, width, radius, true, pick);
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for (let x = 0; x < width; x++)
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extremumLine(scratch, plane, x, width, height, radius, false, pick);
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}
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/** Blur one plate-carrée channel in place, round on the sphere. */
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function blurPlane(plane, width, height, sigmaPx) {
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const scratch = new Float32Array(plane.length);
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for (let y = 0; y < height; y++) {
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const latitude = (0.5 - (y + 0.5) / height) * Math.PI;
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const sigmaX = Math.min(
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width / 4,
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sigmaPx / Math.max(Math.cos(latitude), 1e-3),
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);
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for (const radius of boxRadii(sigmaX)) {
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boxLine(plane, scratch, y * width, 1, width, Math.round(radius), true);
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plane.set(scratch.subarray(y * width, (y + 1) * width), y * width);
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}
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}
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for (const radius of boxRadii(sigmaPx)) {
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for (let x = 0; x < width; x++)
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boxLine(plane, scratch, x, width, height, Math.round(radius), false);
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plane.set(scratch);
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}
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}
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/** Unit vector for galactic longitude and latitude in degrees. */
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function galacticVector(l, b) {
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const lr = (l * Math.PI) / 180;
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const br = (b * Math.PI) / 180;
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return [
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Math.cos(br) * Math.cos(lr),
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Math.cos(br) * Math.sin(lr),
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Math.sin(br),
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];
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}
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/**
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||||
* Replace a disc of the sky with the mean of the ring just outside it, per
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* channel. The blur that follows hides the seam.
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*/
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||||
function paintOut(planes, width, height, { l, b, radiusDeg }) {
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const centre = galacticVector(l, b);
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const inner = Math.cos((radiusDeg * Math.PI) / 180);
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const outer = Math.cos(((radiusDeg + 0.5) * Math.PI) / 180);
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const disc = [];
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const ring = [];
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const span = Math.ceil(((radiusDeg + 0.5) / 180) * height);
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const row = Math.round((0.5 - b / 180) * height);
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for (let y = Math.max(0, row - span); y < Math.min(height, row + span); y++) {
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const latitude = 90 - ((y + 0.5) * 180) / height;
|
||||
for (let x = 0; x < width; x++) {
|
||||
const longitude = (0.5 - (x + 0.5) / width) * 360;
|
||||
const p = galacticVector(longitude, latitude);
|
||||
const cos = p[0] * centre[0] + p[1] * centre[1] + p[2] * centre[2];
|
||||
if (cos >= inner) disc.push(y * width + x);
|
||||
else if (cos >= outer) ring.push(y * width + x);
|
||||
}
|
||||
}
|
||||
for (const plane of planes) {
|
||||
let sum = 0;
|
||||
for (const index of ring) sum += plane[index];
|
||||
const mean = sum / ring.length;
|
||||
for (const index of disc) plane[index] = mean;
|
||||
}
|
||||
}
|
||||
|
||||
/** Bilinear sample with longitude wrap and latitude clamp. */
|
||||
function samplePlane(plane, width, height, u, v) {
|
||||
const fx = u * width - 0.5;
|
||||
const fy = Math.min(Math.max(v * height - 0.5, 0), height - 1);
|
||||
const x0 = Math.floor(fx);
|
||||
const y0 = Math.floor(fy);
|
||||
const ax = fx - x0;
|
||||
const ay = fy - y0;
|
||||
const xa = ((x0 % width) + width) % width;
|
||||
const xb = (xa + 1) % width;
|
||||
const yb = Math.min(y0 + 1, height - 1);
|
||||
const top = plane[y0 * width + xa] * (1 - ax) + plane[y0 * width + xb] * ax;
|
||||
const bottom =
|
||||
plane[yb * width + xa] * (1 - ax) + plane[yb * width + xb] * ax;
|
||||
return top * (1 - ay) + bottom * ay;
|
||||
}
|
||||
|
||||
/** Deterministic hash noise in [-0.5, 0.5) for dithering. */
|
||||
function dither(index, channel) {
|
||||
let h = (index * 374761393 + channel * 668265263) | 0;
|
||||
h = Math.imul(h ^ (h >>> 13), 1274126177);
|
||||
h ^= h >>> 16;
|
||||
return (h >>> 0) / 4294967296 - 0.5;
|
||||
}
|
||||
|
||||
/** Value at `fraction` of the sorted luminance. */
|
||||
function luminancePercentile(planes, fraction) {
|
||||
const [r, g, b] = planes;
|
||||
const lum = new Float32Array(r.length);
|
||||
for (let i = 0; i < lum.length; i++) lum[i] = (r[i] + g[i] + b[i]) / 3;
|
||||
lum.sort();
|
||||
return lum[Math.min(lum.length - 1, Math.floor(fraction * lum.length))];
|
||||
}
|
||||
|
||||
const srgbToLinear = (value) =>
|
||||
value <= 0.04045 ? value / 12.92 : ((value + 0.055) / 1.055) ** 2.4;
|
||||
|
||||
async function decodePanorama(sharp, file) {
|
||||
const width = WORK_WIDTH;
|
||||
const height = WORK_WIDTH / 2;
|
||||
const raw = await sharp(file)
|
||||
.resize(width, height, { fit: 'fill', kernel: 'lanczos3' })
|
||||
.removeAlpha()
|
||||
.raw()
|
||||
.toBuffer();
|
||||
const lut = Float32Array.from({ length: 256 }, (_, i) =>
|
||||
srgbToLinear(i / 255),
|
||||
);
|
||||
const planes = [0, 1, 2].map(() => new Float32Array(width * height));
|
||||
for (let i = 0; i < width * height; i++)
|
||||
for (let c = 0; c < 3; c++) planes[c][i] = lut[raw[i * 3 + c]];
|
||||
return { width, height, planes };
|
||||
}
|
||||
|
||||
async function main() {
|
||||
const [file] = process.argv.slice(2);
|
||||
if (!file) throw new Error('usage: build-milky-way.mjs <eso0932a.tif>');
|
||||
const { default: sharp } = await import('sharp');
|
||||
const { width, height, planes } = await decodePanorama(sharp, file);
|
||||
const sigmaPx = (BLUR_DEG / 180) * height;
|
||||
for (const planet of PLANETS) paintOut(planes, width, height, planet);
|
||||
for (const plane of planes) {
|
||||
extremumPlane(plane, width, height, OPEN_RADIUS, Math.min);
|
||||
extremumPlane(plane, width, height, OPEN_RADIUS, Math.max);
|
||||
blurPlane(plane, width, height, sigmaPx);
|
||||
}
|
||||
const black = luminancePercentile(planes, BLACK_PERCENTILE);
|
||||
const white = luminancePercentile(planes, WHITE_PERCENTILE);
|
||||
let total = 0;
|
||||
for (const face of CUBE_FACES) {
|
||||
const pixels = Buffer.alloc(FACE_SIZE * FACE_SIZE * 3);
|
||||
for (let j = 0; j < FACE_SIZE; j++) {
|
||||
for (let i = 0; i < FACE_SIZE; i++) {
|
||||
const direction = cubeFaceDirection(
|
||||
face,
|
||||
(i + 0.5) / FACE_SIZE,
|
||||
(j + 0.5) / FACE_SIZE,
|
||||
);
|
||||
const [u, v] = directionToPlateCarree(...icrfToGalactic(direction));
|
||||
const index = j * FACE_SIZE + i;
|
||||
for (let c = 0; c < 3; c++) {
|
||||
const linear = Math.max(
|
||||
(samplePlane(planes[c], width, height, u, v) - black) /
|
||||
(white - black),
|
||||
0,
|
||||
);
|
||||
const encoded = Math.min(linear, 1) ** (1 / 2.2) * 255;
|
||||
pixels[index * 3 + c] = Math.min(
|
||||
255,
|
||||
Math.max(0, Math.round(encoded + dither(index, c))),
|
||||
);
|
||||
}
|
||||
}
|
||||
}
|
||||
const out = path.join(OUT_DIR, `milkyway_${FACE_FILE_SUFFIX[face]}.webp`);
|
||||
const info = await sharp(pixels, {
|
||||
raw: { width: FACE_SIZE, height: FACE_SIZE, channels: 3 },
|
||||
})
|
||||
.webp({ quality: WEBP_QUALITY, smartSubsample: true, effort: 6 })
|
||||
.toFile(out);
|
||||
total += info.size;
|
||||
console.log(`${path.relative(process.cwd(), out)}: ${info.size} bytes`);
|
||||
}
|
||||
console.log(`total ${total} bytes`);
|
||||
}
|
||||
|
||||
if (process.argv[1] === fileURLToPath(import.meta.url)) await main();
|
||||
@@ -1062,5 +1062,10 @@
|
||||
"src/ui/flyToDataSource.test.mjs",
|
||||
"scripts/assemble-changelog.mjs",
|
||||
"src/tooling/changelogFragments.test.mjs",
|
||||
"src/data/gbfsProxyRateLimit.test.mjs"
|
||||
"src/data/gbfsProxyRateLimit.test.mjs",
|
||||
"scripts/build-bright-stars.mjs",
|
||||
"scripts/build-milky-way.mjs",
|
||||
"src/sky/stars.test.mjs",
|
||||
"src/sky/starrySky.test.mjs",
|
||||
"src/tooling/skyAssets.test.mjs"
|
||||
]
|
||||
@@ -22,7 +22,14 @@
|
||||
},
|
||||
"viewer": {
|
||||
"exports": ["./application/viewer"],
|
||||
"modules": ["src/app/viewer.js", "src/app/atmosphereCompat.js"],
|
||||
"modules": [
|
||||
"src/app/viewer.js",
|
||||
"src/app/atmosphereCompat.js",
|
||||
"src/sky/starrySky.js",
|
||||
"src/sky/stars.js",
|
||||
"src/data/bundledJson.js",
|
||||
"src/renderGovernor.js"
|
||||
],
|
||||
"external": ["cesium"]
|
||||
},
|
||||
"vite-build": {
|
||||
@@ -1708,6 +1715,8 @@
|
||||
"src/app/surfaceServices.js",
|
||||
"src/app/tools.js",
|
||||
"src/app/viewer.js",
|
||||
"src/sky/starrySky.js",
|
||||
"src/sky/stars.js",
|
||||
"src/app/atmosphereCompat.js",
|
||||
"src/bloom.js",
|
||||
"src/camera.js",
|
||||
|
||||
Reference in new issue
Block a user