Files
star-map/tools/etl/build.ts
T
SenrokaiandClaude Opus 5.5 1d42be2ad5 Add Charon, the moons of Uranus, Saturn's other large moons and the four dwarf planets past Pluto's table
The solar system stopped at 18 bodies: Pluto without Charon, Uranus without a moon, Saturn with
Titan alone, no dwarf planet but Pluto (audit #22). bodies.json now holds 38: the eight planets,
the five IAU dwarf planets, and every moon in JPL's mean-element table more than 100 km in mean
radius. New: Ceres, Eris, Haumea, Makemake; Mimas, Enceladus, Tethys, Dione, Rhea, Hyperion,
Iapetus, Phoebe; Miranda, Ariel, Umbriel, Titania, Oberon; Nereid, Proteus; Charon. Search finds
each by name (it indexes bodies.json), each has a body page, and the Sun's system draws them.

Where they come from
- Moons: the same archived JPL satellite table as the others. Uranus's and Pluto's are given
  against the planet's equator, with the IAU WGCCRE 2015 poles: Pluto's as the IAU gives it
  (132.993, -6.163), Uranus's at the end the table measures inclinations from (77.311, 15.175)
  with its nodes counted 180 degrees on, from the IAU pole's crossing; read without that offset
  every Uranian moon was 180 degrees from Horizons at every date from 1980 to 2100.
- Two rows are corrected where they disagree with JPL's own ephemeris and the reason is known.
  Pluto's section prints epoch 2000 Jan 1.0; JPL's current table gives Charon's as 2000-01-01.5,
  and at 1.0 Charon was 27.8-28.2 degrees from Horizons at every date, half a day of its motion.
  Phoebe's mean motion gives 548.02 days where its Horizons page and the current table give
  550.30 (the table's own note says its source misstated retrograde moons' mean motions); on the
  row's figure Phoebe was 24.6 degrees out by 2025 and 100 by 2075.
- Dwarf planets: JPL SBDB osculating heliocentric elements with their epoch (2026 Jun 9), carried
  at their own n. Against Horizons (heliocentric, 1950-2300; the clock only runs forward from now):
  Ceres 0.02 degrees in 2025, 1.9 in 2050, 4.0 in 2075, 5.3 in 2100, 11.6 in 2200 (Jupiter pulls
  on it and nothing here carries that); Eris within 0.06 to 2100 and 0.5 to 2300; Haumea within
  0.35 to 2100; Makemake within 0.25 to 2100 and 1.7 by 2200.
- Size and spin: Horizons pages for the moons (Charon 606 km, Miranda 235.7 as the mean of its
  three axes). The SBDB for Ceres (469.7 km, 9.074 h) and for the other three's spins (Eris 25.9 h,
  Haumea 3.915 h, Makemake 22.83 h). Neither source nor the WGCCRE 2015 report has a radius for
  Eris, Haumea or Makemake, so each carries its stellar-occultation measurement: Eris 1163 km
  (Sicardy et al. 2011), Makemake 715 (Brown 2013, the mean of 1434 x 1434 x 1422 km), and
  Haumea 797.6, the radius of a sphere of its volume: it is triaxial, 1161 x 852 x 513 km
  (Ortiz et al. 2017), and is drawn as that sphere.
- Rotation uses the branch's model. Every moon is locked except three: Hyperion's page says
  "Chaotic" and Nereid's gives no spin, so both are left still; Phoebe turns in 9.274 h.
- Charon carries massRatio 0.12205, the GM ratio of the two Horizons pages (106.10 / 869.326), so
  it and Pluto are drawn round their barycentre 2 131 km from Pluto's centre.

Validators (tools/etl/build.ts, on the real catalogue; full npm run etl passes)
- Offsets from Horizons on 2025-01-01, new bodies: dwarf planets at most 0.016 degrees (Ceres),
  under the 0.25 ceiling; moons Dione 0.009, Ariel 0.058, Rhea 0.070, Charon 0.111, Oberon 0.142,
  Titania 0.185, Umbriel 0.219, Proteus 0.245, Enceladus 0.309, Phoebe 0.984, Miranda 1.162,
  Tethys 2.042, under the 2.5 ceiling, which is unchanged.
- Four moons get their own ceiling, each just above its worst offset at twelve dates from 1980
  to 2100 and each named with its reason: Mimas 46 (measured up to 44.7: its resonance with
  Tethys swings its longitude 44 degrees either way over 70.8 years, which the table has no
  column for), Hyperion 21 (20.2; held in resonance by Titan, and the row's eccentricity 0.0232
  is under a quarter of the current table's 0.105), Iapetus 11 (10.1; the row sits 9.4 degrees
  behind Horizons at its own epoch and keeps that, with its plane within 0.07 degrees and its
  period within 0.001 per cent), Nereid 3 (2.6 in 2025; eccentricity 0.75).
- New checks: every body has a radius over 0 (Charon's would have been 0 before the page
  parser learnt its form); a freely spinning moon is not locked; a moon with a mass ratio puts
  the barycentre outside its planet; there are 5 dwarf planets.
- Negative controls, each a full npm run etl on the real catalogue refused with the named
  message: Uranus's node offset removed (Miranda 172.50 degrees), Charon at the printed epoch
  (28.08), Phoebe on the row's mean motion (24.61), Charon's radius unread (no radius),
  free spinners locked (Hyperion), mass ratio inverted (barycentre 17 460 km out).

Measured in the running app (port 4311): the Sun's system has 38 members ("13 + 25 moons");
Charon comes back to within 0.0004 degrees of where it started after 6.38723 days and is 179.98
degrees round after half that; Pluto is 2 130.6 km from the barycentre and Charon 17 456.8,
exactly opposite; Saturn's moons in order of distance now: Mimas 185 617 km, Enceladus 238 042,
Tethys 294 648, Dione 376 805, Rhea 526 964, Titan 1 231 389, Hyperion 1 470 453, Iapetus
3 637 059, Phoebe 11 740 900. At the arrival framing the dwarf planets are held at the 3 px
floor and the moons at 1.5 px, half their planet's drawn radius, the scene's existing rule.
Searching Charon, Enceladus, Ceres, Titania, Makemake and Phoebe each finds the body; the body
pages show Charon 6.39 d and 606 km, Titania 8.71 d, Ceres 4.6 yr and 470 km, Haumea 283 yr and
798 km, Hyperion 21.3 d, each with its orbit source. Long tasks on entering: see the previous
commit.

The Sun's note now says the four dwarf planets are on the SBDB's osculating elements. Holding
Eris's orbit, the arrival framing widens: 192 AU of range on a 1600 x 1000 window, under the
200 AU ceiling.

Co-Authored-By: Claude Opus 5.5 (1M context) <noreply@anthropic.com>
2026-09-24 21:54:56 +02:00

348 lines
19 KiB
TypeScript

import { statSync } from 'node:fs';
import { BodyRecord, OrbitalElements } from '../../src/app/shared/models/body.model';
import { eclipticToEquatorial, laplacePlaneToEquatorial } from '../../src/app/shared/astro/coordinates';
import { meanElementsAt, positionAtEpoch } from '../../src/app/shared/astro/kepler';
import { DeepSkyRecord } from '../../src/app/shared/models/deepsky.model';
import { ExoplanetRecord } from '../../src/app/shared/models/exoplanet.model';
import { StarRecord, SUN_STAR_ID } from '../../src/app/shared/models/star.model';
import { fetchDeepSky } from './fetchDeepSky';
import { fetchExoplanets } from './fetchExoplanets';
import { fetchSolarSystem, FREELY_SPINNING_MOONS } from './fetchSolarSystem';
import { BYTES_PER_STAR_META, BYTES_PER_STAR_POSITION, decodeStarCatalog, encodeStarCatalog } from '../../src/app/shared/models/star-catalog';
import { fetchStars } from './fetchStars';
import { describeSources } from './sources/registry';
import { dataPath } from './lib/paths';
class ValidationError extends Error {}
function assertCondition(condition: boolean, message: string): void {
if (!condition) {
throw new ValidationError(message);
}
}
function validateStars(stars: StarRecord[]): void {
assertCondition(stars.length > 0, 'No stars were produced.');
const ids = new Set<number>();
for (const star of stars) {
assertCondition(Number.isFinite(star.id), `Star has a non-numeric id: ${JSON.stringify(star)}`);
assertCondition(!ids.has(star.id), `Duplicate star id: ${star.id}`);
ids.add(star.id);
assertCondition(!!star.name, `Star ${star.id} has no name.`);
assertCondition([star.x, star.y, star.z].every(Number.isFinite), `Star ${star.id} has a non-finite position.`);
}
const positionBytes = statSync(dataPath('stars.bin')).size;
assertCondition(positionBytes === stars.length * BYTES_PER_STAR_POSITION, `stars.bin size (${positionBytes}) does not match ${stars.length} stars.`);
const metaBytes = statSync(dataPath('stars-meta.bin')).size;
assertCondition(metaBytes === stars.length * BYTES_PER_STAR_META, `stars-meta.bin size (${metaBytes}) does not match ${stars.length} stars.`);
// Round-trips the written assets back through the decoder the app uses, so a format change
// that only half-lands fails here rather than as a silently wrong star map.
const { index, positions, meta } = encodeStarCatalog(stars);
const decoded = decodeStarCatalog(index, positions, meta);
assertCondition(decoded.length === stars.length, `Star catalogue round-trip lost records: ${decoded.length} of ${stars.length}.`);
for (let i = 0; i < stars.length; i++) {
assertCondition(decoded[i].id === stars[i].id && decoded[i].name === stars[i].name, `Star catalogue round-trip altered record ${i}.`);
assertCondition(decoded[i].spectralType === stars[i].spectralType, `Star catalogue round-trip lost the spectral type of star ${stars[i].id}.`);
assertCondition(decoded[i].colorIndex === null === (stars[i].colorIndex === null), `Star catalogue round-trip changed whether star ${stars[i].id} has a colour index.`);
}
}
/**
* What a good merge looks like, in two numbers the unit suite cannot see.
*
* The catalogues are regenerated by a scheduled job that pushes straight to `main` once the unit
* tests and a production build pass — and both passed, for weeks, on a catalogue carrying 23 000
* stars twice: the suite tests code against fixtures, and no fixture is 400 000 real stars. The
* two ways the merge has actually failed both show up here.
*
* A star kept twice leaves its two entries near each other on the sky, from *different* sources —
* one catalogue does not list a star twice. Under an arcsecond that is never two stars at this
* depth, so every such pair is a miss. Nineteen survive today, all of them a second HYG row
* wanting a Gaia entry that already absorbed one (Gliese lists some doubles twice); the merge
* that trusted a Hipparcos parallax over direction left 1 112.
*
* The other failure leaves no close pair at all, because proper motion had already carried the
* two entries tens of arcseconds apart — the 2026-08-24 refresh, where HYG sat at epoch 2000.0
* and Gaia at J2016.0. What it does leave is HYG rows that found no counterpart: 36 056 of them
* against the 10 886 today, and no counterpart was possible for most of those. Two thirds of them,
* 6 835, are the stars Gaia measures but the main query never downloads, because Gaia's parallax
* puts them past `ETL_GAIA_DISTANCE_PC` while Hipparcos put them inside `ETL_STAR_DISTANCE_PC`;
* they are every star in the published catalogue beyond 250 pc. The rest are what Gaia genuinely
* lacks: bright stars it saturates on, red dwarfs past its magnitude cut. So the headroom left to
* the ceiling tracks the gap between those two cutoffs as much as Gaia's completeness.
*
* This bounds a merge that went wrong, and — loosely — a Gaia download that came back short: a
* truncated answer leaves the HYG rows whose counterpart it dropped without one, so survivors go
* *up*, not down. Measured against the published catalogue: 10 886 today, 11 004 at nine tenths of
* the rows, 12 711 at half, 16 258 at a third. So this ceiling only catches a truncation past about
* two thirds, and `fetchGaiaStars` catches the shallower ones with its own row floor.
*/
const MAX_UNMERGED_TWINS = 100;
const MAX_HYG_SURVIVORS = 15_000;
const TWIN_TOLERANCE_RAD = (1 / 3600) * (Math.PI / 180);
function validateMerge(stars: StarRecord[]): void {
// Checked first and on its own: an unreachable Gaia is skipped rather than thrown, and would
// otherwise surface below as "68 000 HYG stars found no counterpart" — true, and no help.
assertCondition(
stars.some((star) => star.source === 'gaia'),
'Gaia DR3 contributed no stars — the archive was unreachable or returned nothing, and a catalogue without it is not one to publish.'
);
const survivors = stars.filter((star) => star.source === 'hyg').length;
assertCondition(
survivors <= MAX_HYG_SURVIVORS,
`${survivors} HYG stars found no Gaia counterpart (at most ${MAX_HYG_SURVIVORS} expected) — the two catalogues are not being matched.`
);
// Sorted by declination, so each star is only compared against the handful sharing its
// parallel — an arcsecond of declination holds one or two of 400 000 stars.
const byDec = stars
.map((star) => {
const distance = Math.hypot(star.x, star.y, star.z);
return { star, distance, dec: distance === 0 ? 0 : Math.asin(Math.max(-1, Math.min(1, star.z / distance))) };
})
.filter((entry) => entry.distance > 0)
.sort((a, b) => a.dec - b.dec);
const cosTolerance = Math.cos(TWIN_TOLERANCE_RAD);
let twins = 0;
let example = '';
for (let i = 0; i < byDec.length; i++) {
const a = byDec[i];
for (let j = i + 1; j < byDec.length && byDec[j].dec - a.dec <= TWIN_TOLERANCE_RAD; j++) {
const b = byDec[j];
if (a.star.source === b.star.source) {
continue;
}
const cosine = (a.star.x * b.star.x + a.star.y * b.star.y + a.star.z * b.star.z) / (a.distance * b.distance);
if (cosine >= cosTolerance) {
twins++;
example ||= `${a.star.name} (${a.star.source}) and ${b.star.name} (${b.star.source})`;
}
}
}
assertCondition(
twins <= MAX_UNMERGED_TWINS,
`${twins} stars from different catalogues sit within an arcsecond of each other (at most ${MAX_UNMERGED_TWINS} expected), starting with ${example} — the merge is keeping the same star twice.`
);
console.log(` ${survivors} HYG stars have no Gaia counterpart; ${twins} unmerged cross-catalogue pairs within an arcsecond.`);
}
/**
* How far a body's mean elements may put it from where Horizons has it, on the one date the ETL
* asks Horizons about (2025-01-01), seen from the Sun for a planet and from its planet for a moon.
*
* Measured on this catalogue: the planets at most 0.10 degrees (Uranus; Standish's own stated
* error for his fit is 2 000 arcseconds, 0.56 degrees), the moons at most 1.41 (the Moon, whose
* evection and variation, 1.27 and 0.66 degrees, no mean ellipse has). What this catches is a
* table read wrongly: a moon read against the ecliptic instead of its Laplace plane, a precession
* run the wrong way, or a column taken for its neighbour, which put Triton 26 degrees out and Io
* 0.9.
*/
const MAX_PLANET_OFFSET_DEG = 0.25;
const MAX_MOON_OFFSET_DEG = 2.5;
const KM_PER_AU = 149597870.7;
/**
* The moons whose table row cannot come within that, each for a reason no mean ellipse carries,
* with a ceiling just above its worst offset from Horizons at twelve dates from 1980 to 2100:
*
* - Mimas, 44.7 degrees: its resonance with Tethys swings its mean longitude 44 degrees either
* way over 70.8 years, and the table has no column for it (Tethys, on the other end, swings 2).
* - Hyperion, 20.2: held in a 4:3 resonance by Titan; the row's eccentricity, 0.0232, is less than
* a quarter of the 0.105 JPL's current table gives.
* - Iapetus, 10.1: the row sits 9.4 degrees behind Horizons at its own epoch, 2000 Jan 1.5, and
* keeps that offset; its plane agrees with Horizons' to 0.07 degrees and its period to 0.001 per
* cent, so the fault is in the row's longitude, which this has no second source to correct.
* - Nereid, 2.6: an eccentricity of 0.75, the largest here, which a mean ellipse follows least
* well: under 0.9 degrees in every year measured but 2025 and 2030 (2.6 and 2.3) and 2100 (1.7).
*/
const MOON_OFFSET_CEILINGS_DEG: Record<string, number> = { mimas: 46, hyperion: 21, iapetus: 11, nereid: 3 };
function angleBetweenDeg(a: { x: number; y: number; z: number }, b: { x: number; y: number; z: number }): number {
const cosine = (a.x * b.x + a.y * b.y + a.z * b.z) / (Math.hypot(a.x, a.y, a.z) * Math.hypot(b.x, b.y, b.z));
return (Math.acos(Math.min(1, Math.max(-1, cosine))) * 180) / Math.PI;
}
function validateBodies(bodies: BodyRecord[], horizonsOrbits: Map<string, OrbitalElements>): void {
assertCondition(bodies.length > 0, 'No solar-system bodies were produced.');
const ids = new Set(bodies.map((body) => body.id));
assertCondition(ids.size === bodies.length, 'Duplicate body ids were found.');
const offsets: string[] = [];
for (const body of bodies) {
const orbitValues = Object.values(body.orbit);
assertCondition(orbitValues.every(Number.isFinite), `Body ${body.id} has non-finite orbital elements.`);
assertCondition(body.rates.meanMotionDegPerDay > 0, `Body ${body.id} has no mean motion.`);
// Horizons' elements are osculating, exact at their own epoch; both sets are placed there.
const horizons = horizonsOrbits.get(body.id);
assertCondition(horizons !== undefined, `Body ${body.id} has no Horizons elements to be checked against.`);
const truth = eclipticToEquatorial(positionAtEpoch(horizons!));
const mean = positionAtEpoch(meanElementsAt(body.orbit, body.rates, horizons!.epochJd));
const offset = angleBetweenDeg(body.laplacePole ? laplacePlaneToEquatorial(mean, body.laplacePole) : eclipticToEquatorial(mean), truth);
const ceiling = body.kind === 'moon' ? (MOON_OFFSET_CEILINGS_DEG[body.id] ?? MAX_MOON_OFFSET_DEG) : MAX_PLANET_OFFSET_DEG;
assertCondition(
offset <= ceiling,
`${body.name}'s mean elements put it ${offset.toFixed(2)} degrees from where Horizons has it (at most ${ceiling} expected) — the elements were read wrongly.`
);
offsets.push(`${body.id} ${offset.toFixed(3)}`);
// A radius of 0 is what a page whose radius no pattern reads comes out as — Charon's did.
assertCondition(body.radiusKm > 0, `Body ${body.id} has no radius; its page states it in a form the ETL does not read.`);
if (body.kind === 'moon') {
const parent = bodies.find((candidate) => candidate.id === body.parentBodyId);
assertCondition(parent !== undefined, `Moon ${body.id} has no valid parentBodyId.`);
const orbitHours = (360 / body.rates.meanMotionDegPerDay) * 24;
if (FREELY_SPINNING_MOONS.has(body.id)) {
// Hyperion tumbles and Nereid's page gives no spin, so they have none; Phoebe turns in
// 9.27 hours against a 550-day orbit. A lock here would be the rule below misapplied.
assertCondition(
body.rotationPeriodHours === undefined || Math.abs(body.rotationPeriodHours - orbitHours) > orbitHours * 0.1,
`Moon ${body.id} does not keep one face to its planet, yet turns once in ${body.rotationPeriodHours} hours against an orbit of ${orbitHours}.`
);
} else {
// Every other moon here is tidally locked: its day is its orbit, from the same mean motion
// that carries it round, or its face turns away from its planet: the Kepler period of the
// osculating orbit this used to take would turn the Moon's five degrees an orbit.
assertCondition(
body.rotationPeriodHours !== undefined && Math.abs(body.rotationPeriodHours - orbitHours) <= orbitHours * 1e-9,
`Moon ${body.id} turns once in ${body.rotationPeriodHours} hours but goes round in ${orbitHours} — it will not keep one face to its planet.`
);
}
if (body.massRatio !== undefined) {
// The pair's barycentre, which the planet's elements place, must lie outside the planet —
// that is why the two are drawn going round it — and nearer the planet than the moon.
const offsetKm = (body.orbit.semiMajorAxisAu * KM_PER_AU * body.massRatio) / (1 + body.massRatio);
assertCondition(
body.massRatio > 0 && body.massRatio < 1 && offsetKm > parent!.radiusKm,
`${body.name}'s mass ratio ${body.massRatio} puts its barycentre ${offsetKm.toFixed(0)} km from ${parent!.name}'s centre, which is not between its surface, ${parent!.radiusKm} km out, and the moon.`
);
}
}
}
const planetCount = bodies.filter((body) => body.kind === 'planet').length;
assertCondition(planetCount === 8, `Expected 8 planets, found ${planetCount}.`);
const dwarfCount = bodies.filter((body) => body.kind === 'dwarf').length;
assertCondition(dwarfCount === 5, `Expected the IAU's 5 dwarf planets, found ${dwarfCount}.`);
console.log(` mean elements against Horizons, degrees: ${offsets.join(', ')}.`);
}
function validateExoplanets(exoplanets: ExoplanetRecord[], starIds: Set<number>): void {
assertCondition(exoplanets.length > 0, 'No exoplanets were produced.');
let crossReferenced = 0;
for (const exoplanet of exoplanets) {
assertCondition(!!exoplanet.name, `Exoplanet ${exoplanet.id} has no name.`);
if (exoplanet.hostStarId !== null) {
assertCondition(starIds.has(exoplanet.hostStarId), `Exoplanet ${exoplanet.id} references unknown star id ${exoplanet.hostStarId}.`);
// The Sun has no exoplanets, so any match to it is a matching failure — historically a
// blank distance column parsing as 0, which puts the host at the origin and matches Sol
// exactly. Free, permanent tripwire for that whole class of bug.
assertCondition(
exoplanet.hostStarId !== SUN_STAR_ID,
`Exoplanet ${exoplanet.id} was matched to the Sun, which has no exoplanets — the host-star match is wrong.`
);
crossReferenced++;
}
assertCondition(
exoplanet.periodDays === undefined || exoplanet.periodDays > 0,
`Exoplanet ${exoplanet.id} has a non-positive orbital period.`
);
assertCondition(
exoplanet.hostStarMassSolar === undefined || exoplanet.hostStarMassSolar > 0,
`Exoplanet ${exoplanet.id} has a non-positive host star mass.`
);
}
console.log(` ${crossReferenced}/${exoplanets.length} exoplanets cross-referenced to a HYG host star.`);
// How many can be propagated at their real rate rather than as if the host were the Sun.
const withPeriod = exoplanets.filter((exoplanet) => exoplanet.periodDays !== undefined).length;
const withHostMass = exoplanets.filter((exoplanet) => exoplanet.hostStarMassSolar !== undefined).length;
console.log(` ${withPeriod}/${exoplanets.length} have a measured period, ${withHostMass} a host star mass.`);
}
const UNIT_VECTOR_TOLERANCE = 1e-6;
function validateDeepSky(objects: DeepSkyRecord[]): void {
assertCondition(objects.length > 0, 'No deep-sky objects were produced.');
const ids = new Set<string>();
for (const object of objects) {
assertCondition(!!object.id, `Deep-sky object has no id: ${JSON.stringify(object)}`);
assertCondition(!ids.has(object.id), `Duplicate deep-sky id: ${object.id}`);
ids.add(object.id);
assertCondition(!!object.name, `Deep-sky object ${object.id} has no name.`);
// Positions are directions, so every one of them must be a unit vector — a zero-length
// or mis-scaled entry would silently collapse onto the origin on the backdrop shell.
const length = Math.hypot(object.x, object.y, object.z);
assertCondition(Math.abs(length - 1) < UNIT_VECTOR_TOLERANCE, `Deep-sky object ${object.id} has a non-unit direction (length ${length}).`);
assertCondition(object.angularSizeDeg >= 0, `Deep-sky object ${object.id} has a negative angular size.`);
assertCondition(object.distancePc === null || object.distancePc > 0, `Deep-sky object ${object.id} has a non-positive distance.`);
// The distance and its provenance have to travel together, or the UI cannot say where a
// number came from.
assertCondition(
(object.distancePc === null) === (object.distanceMethod === null),
`Deep-sky object ${object.id} has a distance/method mismatch.`
);
}
const kinds = new Set(objects.map((object) => object.kind));
for (const kind of ['galaxy', 'nebula', 'cluster'] as const) {
assertCondition(kinds.has(kind), `No deep-sky objects of kind "${kind}" were produced.`);
}
const withDistance = objects.filter((object) => object.distancePc !== null).length;
console.log(` ${withDistance}/${objects.length} deep-sky objects have a derived distance.`);
}
/**
* Orchestrates the whole ETL pipeline: fetches every source (each caches its own raw
* responses under `tools/etl/.cache/`), writes the static assets under `src/assets/data/`,
* then validates the combined output for completeness before declaring success.
*/
async function build(): Promise<void> {
console.log('=== NASA star map ETL ===\n');
console.log('Catalogues:');
console.log(describeSources());
console.log();
const stars = await fetchStars();
console.log();
const { bodies, horizonsOrbits } = await fetchSolarSystem();
console.log();
const exoplanets = await fetchExoplanets(stars);
console.log();
const deepSky = await fetchDeepSky();
console.log();
console.log('Validating output...');
validateStars(stars);
validateMerge(stars);
validateBodies(bodies, horizonsOrbits);
validateExoplanets(exoplanets, new Set(stars.map((star) => star.id)));
validateDeepSky(deepSky);
console.log('\nETL completed successfully:');
console.log(` stars: ${stars.length}`);
console.log(` bodies: ${bodies.length}`);
console.log(` exoplanets: ${exoplanets.length}`);
console.log(` deep sky: ${deepSky.length}`);
}
build().catch((error) => {
console.error('\nETL failed:', error instanceof Error ? error.message : error);
process.exitCode = 1;
});