Files
star-map/tools/etl/fetchStars.ts
T
SenrokaiandClaude Opus 5.5 e7c420b296 Fold a Gliese star into its Gaia source in Gaia's photometry, wherever HYG already put it, and place two naked-eye stars by SIMBAD's name for them
The Gliese fold (030447b) kept HYG's magnitude, band and colour over the Gaia entry's, putting
CNS3's V at Gaia's distance. Of the 49 folded, 15 lost a measured BP-RP and 6 their temperature and
radius (Gl 700.1C, Gl 632.2B, GJ 9800B, Gl 734B, Gl 323B, GJ 3605), and GJ 4285, V 11.45 where
SIMBAD has G 13.05, was drawn five times too luminous. A folded star now keeps the photometry of the
entry already there; HYG's name, id and type still come with the fold. Published catalogue, before
-> after: GJ 4285 V 11.45, 3 850 K, 0.491 R☉, 4.76e-2 L☉ -> G 13.05, BP-RP 2.74, 3 291 K, 0.297 R☉,
9.29e-3 L☉; GJ 3207 0.574 -> 0.278 R☉; Gl 700.1C no temperature, 4.54 L☉ -> 5 155 K, 1.214 R☉,
0.937 L☉; Gl 632.2B -> 9 044 K, 0.018 R☉; Gl 734B -> 3 360 K, 0.381 R☉.

The fold also looked its target up by name, so it saw only Gaia entries still bare. Where a
Hipparcos row of HYG's had already taken the source, the Gliese-only row of the same star stayed
beside it and the check counted none: Gl 251 at 5.76 pc beside HD 265866 (the host of GJ 251 b and
c) at 5.58, Gl 422 beside HD 304043. Gaia entries now carry their DR3 designation through the merge
(ETL only; the assets do not store it) and the fold looks it up; into an entry a HYG star already
describes it folds only where the two V agree within 0.5, so a companion SIMBAD gives its primary's
source stays. 14 more rows fold, 63 in all, each within 0.47 of the star it joins: Gl 251, Gl 422,
Gl 162, Gl 794, Gl 225.2C, Gl 905.2B, GJ 3232, GJ 4046, GJ 9490C, GJ 9608, 69 Tau Oph (Gl 700.1A)
and the second rows of HD 65277, HD 120237 and HD 336196. Stars within 10 pc 367 -> 366, within
25 pc 5 479 -> 5 468; distances without an error 346 -> 332; HYG survivors 11 478 -> 11 465.

validateMerge's count of Gliese rows beside their source took SIMBAD's map from the function the
fold takes it from, so a slip in the map turned both off: with it empty, GJ 2097 and GJ 4285 were
back inside 10 pc and the ETL passed. It now also asks for GJ 2097 and GJ 4285 beyond 20 pc and for
no Gl 251 or Gl 422 by name, and glieseGaiaDesignations refuses fewer than 3 200 HYG rows matched to
SIMBAD (3 352 of HYG's 3 801 measured).

4d47896 left 22 naked-eye HYG rows out as having no distance anywhere; two had one. HD 45951 (K0 III,
V 6.2) was on the map only as "Gaia DR3 3369454521490604416", HYG's declination being 31.7' out,
and θ¹ Ori A (HD 37020, HIP 26220) sits 0.1" from Gaia DR3 3017364132050194688, 2.643 ± 0.072 mas,
which the magnitude test refused because HYG gives V 4.98 against G 6.63. One cached SIMBAD query
now names the Gaia DR3 source of each naked-eye HYG row with no distance (199 of 206 HD numbers),
and a row nothing else places takes that source from the bright list, at its position: HD 45951 at
112.0 pc, under its name, and θ¹ Ori A at 378.4 pc. HD 45951 joins the required names. The twenty
still left out are named in build.ts; none has a bright source with a parallax five times its error
within a minute of arc nor under its SIMBAD name. Naked-eye stars 8 898 -> 8 899; 455 532 -> 455 519
stars.

The fold and the identity lookup are tested in star-merge.spec.ts. Guarded mutants (1 of 833
failed unless noted):
- the Gliese row's photometry kept: caught by "...in Gaia's photometry" (and the Hipparcos-row fold test, 2 failed)
- combine dropping the designation: caught by "folds one into a Gaia entry a HYG star of the same brightness..."
- folding whatever the brightness; tolerance 2 magnitudes: caught by "leaves a star with a Hipparcos error alone..."
- folding into bare entries only: caught by the Hipparcos-row fold test (and the leave-alone test, 2 failed)

Co-Authored-By: Claude Opus 5.5 (1M context) <noreply@anthropic.com>
2026-09-30 19:55:25 +02:00

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import { writeFileSync } from 'node:fs';
import { foldByIdentity, hipparcosDistancePc, HYG_UNKNOWN_DISTANCE_PC, mergeStarCatalogues, NAKED_EYE_MAGNITUDE, placementDistancePc } from '../../src/app/shared/astro/star-merge';
import { encodeStarCatalog } from '../../src/app/shared/models/star-catalog';
import { StarRecord, SUN_STAR_ID } from '../../src/app/shared/models/star.model';
import { BrightGaiaSource, fetchBrightGaiaSources, fetchGaiaDistancesByHip, fetchHipparcosParallaxErrors, GaiaAnswerError } from './sources/gaia';
import { positionalSources } from './sources/registry';
import { fetchGaiaDesignationsByGj, fetchGaiaDesignationsByHd } from './sources/simbad';
import { PARALLAX_PRECISION_MAS } from './sources/star-sources';
import { parseCsvObjects, parseOptionalNumber } from './lib/csv';
import { fetchTextCached } from './lib/http';
import { dataPath, ensureDataDir } from './lib/paths';
const HYG_CSV_URL = 'https://raw.githubusercontent.com/astronexus/HYG-Database/main/hyg/CURRENT/hygdata_v41.csv';
/**
* Stand-in magnitude for a star with no photometry. Faint rather than 0, because 0 would mean
* "as bright as Vega" and render it as one of the largest points on the map.
*/
const UNKNOWN_MAGNITUDE = 15;
/**
* Stars either survey places within this distance (parsecs) of the Sun are kept for the galaxy
* view, and every naked-eye star wherever it is; `placementDistancePc` decides which distance a
* kept star is drawn at.
*
* Set at the range Hipparcos's own measurements reach rather than at a round number: its
* parallaxes are good to roughly a milliarcsecond, so at 250 pc (4 mas) a distance is uncertain
* by some tens of per cent. That is why it is not applied to the Hipparcos distance alone:
* Gaia puts 6 833 of the stars Hipparcos places inside it outside, and 3 666 the other way
* round. Only the *radial* placement blurs; a star's direction on the sky stays exact.
*
* The catalogue is also magnitude-limited, so this is not a volume-complete sample beyond about
* 50 pc: it thins to the intrinsically bright, which is the same selection the naked eye makes.
*/
const DISTANCE_CUTOFF_PC = Number(process.env['ETL_STAR_DISTANCE_PC'] ?? 250);
function resolveName(row: Record<string, string>): string {
if (row['proper']) {
return row['proper'];
}
if (row['bayer'] && row['con']) {
return `${row['bayer']} ${row['con']}`;
}
if (row['flam'] && row['con']) {
return `${row['flam']} ${row['con']}`;
}
if (row['hd']) {
return `HD ${row['hd']}`;
}
if (row['gl']) {
// Already a complete designation ("Gl 581", "GJ 3512"), unlike the bare numbers in `hd`
// and `hip` — prefixing it again produced 2331 stars named "Gl GJ 1076", which broke
// search, the on-screen labels, and exoplanet host-star name matching alike.
return row['gl'];
}
if (row['hip']) {
return `HIP ${row['hip']}`;
}
return `HYG ${row['id']}`;
}
/**
* HYG's spectral type, without the `...` that 2 127 of the map's stars end in, all of them
* Hipparcos stars: the Hipparcos catalogue's mark for a classification it does not print in full
* (Sirius is "A0m..."). On the map it read as text the app had cut short.
*/
function spectralTypeOf(row: Record<string, string>): string {
return (row['spect'] ?? '').replace(/\.\.\.$/, '') || 'Unknown';
}
/**
* Downloads the HYG (Hipparcos/Yale/Gliese) stellar database, places each star along its
* equatorial direction (epoch J2000.0) at whichever of its Hipparcos and Gaia distances has the
* smaller error, keeps the ones either survey puts within range, and unions the other positional
* sources. Writes nothing: fetchExoplanets adds the hosts the catalogue lacks and renames the
* ones known only by a designation, then writes the star assets once. Written here as well, they
* stood on disk without those 3 277 stars whenever a run stopped between the two — and that
* catalogue left 4 237 planets pointing at stars it did not have.
*/
export async function fetchStars(): Promise<StarRecord[]> {
console.log(`Fetching HYG star catalog (distance cutoff: ${DISTANCE_CUTOFF_PC} pc)...`);
const csv = await fetchTextCached(HYG_CSV_URL, 'hygdata_v41.csv');
const rows = parseCsvObjects(csv);
// Not skipped when unreachable, unlike the positional sources below; see its own comment.
const gaiaByHip = await fetchGaiaDistancesByHip();
const hipparcosErrors = await fetchHipparcosParallaxErrors();
const brightGaia = await fetchBrightGaiaSources();
const brightByDesignation = new Map(brightGaia.map((source) => [source.designation, source]));
const nakedEyeDesignations = await fetchGaiaDesignationsByHd(
rows.filter((row) => row['hd'] && Number(row['dist']) >= HYG_UNKNOWN_DISTANCE_PC && (parseOptionalNumber(row['mag']) ?? Infinity) <= NAKED_EYE_MAGNITUDE).map((row) => row['hd'])
);
const stars: StarRecord[] = [];
let atGaiaDistance = 0;
let pastCutoff = 0;
let identified = 0;
for (const row of rows) {
const id = Number(row['id']);
if (id === SUN_STAR_ID) {
stars.push({ id, name: 'Sol', x: 0, y: 0, z: 0, magnitude: parseOptionalNumber(row['mag']) ?? UNKNOWN_MAGNITUDE, magnitudeBand: 'V', spectralType: row['spect'] || 'G2V', colorIndex: parseOptionalNumber(row['ci']) ?? null, colorSystem: 'B-V' });
continue;
}
const hygPc = Number(row['dist']);
const hipparcos = row['hip'] ? hipparcosErrors.get(Number(row['hip'])) : undefined;
const hipparcosPc = hipparcosDistancePc(hygPc, hipparcos);
const magnitudeV = parseOptionalNumber(row['mag']);
const magnitude = magnitudeV ?? UNKNOWN_MAGNITUDE;
const unplaced = hipparcosPc === undefined && magnitude <= NAKED_EYE_MAGNITUDE;
const crossMatched = row['hip'] ? gaiaByHip.get(Number(row['hip'])) : undefined;
const positional = crossMatched === undefined && unplaced ? brightCounterpart(row, magnitude, brightGaia) : undefined;
// Where HYG's position leads to no bright source, the one SIMBAD names it as: HD 45951, whose
// declination HYG has 31.7′ out, and θ¹ Ori A (HD 37020), whose V it has 1.65 brighter than G.
const byIdentity = crossMatched === undefined && positional === undefined && unplaced ? brightByDesignation.get(nakedEyeDesignations.get(`HD ${row['hd']}`) ?? '') : undefined;
const gaia = crossMatched ?? positional ?? byIdentity;
const gaiaPc = gaia?.distancePc;
const hipparcosError = hipparcos?.relativeError;
const distancePc = placementDistancePc(hipparcosPc, gaiaPc, magnitude, DISTANCE_CUTOFF_PC, hipparcosError, gaia?.relativeError);
if (distancePc === null) {
continue;
}
const fromGaia = gaia !== undefined && distancePc === gaiaPc;
// HYG's own Cartesian columns rather than its `ra`/`dec`, which are in the same frame as
// `raDecDistanceToXyz` and would be redundant if the two agreed. They do not, for the stars
// that move: the right ascension was carried from the Hipparcos epoch to 2000.0 without the
// cos δ its motion needs, which puts Proxima 17.9″ from where HYG's own x/y/z — and Gaia,
// once brought to the same epoch — have it. 1813 stars differ by over an arcsecond, and the
// Cartesian columns are the ones Gaia agrees with for 1155 of them against 156 (one of those,
// HIP 57146, has x/y/z 161″ from its own ra/dec and stays double).
//
// Only their direction is used. They sit at HYG's own distance, or at its 100 000 pc
// placeholder where it has none, and are carried along that direction to the one chosen above —
// Gaia's, for a star found by its identity, where HYG's may be the thing that is wrong.
const [x, y, z] = byIdentity ? [byIdentity.direction.x, byIdentity.direction.y, byIdentity.direction.z] : [Number(row['x']), Number(row['y']), Number(row['z'])];
const length = Math.hypot(x, y, z);
if (![x, y, z].every(Number.isFinite) || length === 0) {
continue;
}
const scale = distancePc / length;
if (fromGaia) {
atGaiaDistance++;
}
if (byIdentity) {
identified++;
}
if (distancePc > DISTANCE_CUTOFF_PC) {
pastCutoff++;
}
// Gaia's error with Gaia's distance, Hipparcos's with its own; a Gliese row, with neither, has
// no published error, and its distance is as often photometric as measured.
const distanceError = fromGaia ? gaia.relativeError : hipparcosError;
const colorIndex = parseOptionalNumber(row['ci']);
stars.push({
id,
name: resolveName(row),
x: x * scale,
y: y * scale,
z: z * scale,
magnitude,
...(magnitudeV === undefined ? {} : { magnitudeBand: 'V' as const }),
spectralType: spectralTypeOf(row),
colorIndex: colorIndex ?? null,
...(colorIndex === undefined ? {} : { colorSystem: 'B-V' as const }),
...(distanceError === undefined ? {} : { distanceError }),
distanceFromGaia: fromGaia,
// Only for the Gliese-only rows, whose positions are what the merge needs the motion to see
// past. A Hipparcos position is good to under an arcsecond; given its motion too, 15 stars
// took their co-moving companion's Gaia entry, and the companion was kept twice.
...(row['hip'] ? {} : { pmRaMasYr: parseOptionalNumber(row['pmra']), pmDecMasYr: parseOptionalNumber(row['pmdec']) })
});
}
console.log(
` kept ${stars.length} stars (of ${rows.length} in the catalog): ${atGaiaDistance} at Gaia's distance, ${pastCutoff} of them past ${DISTANCE_CUTOFF_PC} pc; ${identified} naked-eye stars placed by the Gaia source SIMBAD names them as.`
);
const { stars: merged, folded } = foldByIdentity(await mergeWithOtherSources(stars), await glieseGaiaDesignations(rows));
console.log(` ${folded} Gliese entries folded into the Gaia source SIMBAD names them as.`);
merged.sort((a, b) => a.id - b.id);
return merged;
}
/** How far a naked-eye star may be from its Gaia source, and how much brighter or fainter in G. */
const BRIGHT_COUNTERPART_TOLERANCE_RAD = (5 / 3600) * (Math.PI / 180);
const BRIGHT_COUNTERPART_MAGNITUDES = 1;
/**
* The Gaia source that is a naked-eye HYG star neither survey places otherwise: the nearest within
* 5″ of its direction and a magnitude of its V. Found this way, HD 152249 is 4.1″ from where HYG
* has it, the rest within 1.1″. At 15″, θ¹ Ori (HIP 26220) took the source of θ¹ Ori C, 12.9″ away
* and already on the map.
*/
function brightCounterpart(row: Record<string, string>, magnitudeV: number, sources: readonly BrightGaiaSource[]): { distancePc: number; relativeError: number } | undefined {
const [x, y, z] = [Number(row['x']), Number(row['y']), Number(row['z'])];
const length = Math.hypot(x, y, z);
let best: BrightGaiaSource | undefined;
let bestCosine = Math.cos(BRIGHT_COUNTERPART_TOLERANCE_RAD);
for (const source of sources) {
const cosine = (x * source.direction.x + y * source.direction.y + z * source.direction.z) / length;
if (cosine >= bestCosine && Math.abs(source.magnitudeG - magnitudeV) <= BRIGHT_COUNTERPART_MAGNITUDES) {
best = source;
bestCosine = cosine;
}
}
return best;
}
/** HYG's Gliese designation as SIMBAD writes it: "Gl 734B" is "GJ 734 B". */
function simbadGliese(gl: string): string {
return gl.trim().replace(/^Gl\s+/, 'GJ ').replace(/^(GJ \d+(?:\.\d+)?)\s*([A-Z]+)$/, '$1 $2');
}
/**
* How many HYG rows with a Gliese number SIMBAD names a Gaia source for: 3 352 of HYG's 3 801 on
* 2026-09-30. SIMBAD's side has its own floor; this one is on the join, where HYG's "Gl 94" has to
* become SIMBAD's "GJ 94". Joined on HYG's names as they stand, 38 rows were folded instead of 49
* and the check in build.ts, which takes this map too, still counted none left.
*/
const MIN_GLIESE_IDENTITIES = 3_200;
/**
* The Gaia DR3 designation SIMBAD gives each HYG star with a Gliese number, by HYG id: what the
* merge folds its Gliese-only rows by, and what build.ts checks it did. `rows` are HYG's, read
* again from the cache when not given.
*/
export async function glieseGaiaDesignations(rows?: Record<string, string>[]): Promise<Map<number, string>> {
const hyg = rows ?? parseCsvObjects(await fetchTextCached(HYG_CSV_URL, 'hygdata_v41.csv'));
const byGj = await fetchGaiaDesignationsByGj();
const designations = new Map<number, string>();
for (const row of hyg) {
const designation = row['gl'] ? byGj.get(simbadGliese(row['gl'])) : undefined;
if (designation) {
designations.set(Number(row['id']), designation);
}
}
if (designations.size < MIN_GLIESE_IDENTITIES) {
throw new Error(`Only ${designations.size} HYG stars with a Gliese number were matched to SIMBAD's (at least ${MIN_GLIESE_IDENTITIES} expected) — HYG's designations are no longer written as SIMBAD writes them.`);
}
return designations;
}
/**
* Unions HYG with every other positional source that is wired in and reachable.
*
* A source that cannot be reached is reported and skipped here rather than thrown, so a run still
* gets as far as validation and says what it has. Whether that may be published is decided
* there: `validateMerge` in build.ts refuses a catalogue Gaia contributed nothing to. A source
* that answered with something unusable ({@link GaiaAnswerError}) is a different matter, and stops
* the run where it happened rather than being reported later as an outage.
*/
async function mergeWithOtherSources(hygStars: StarRecord[]): Promise<StarRecord[]> {
const others = positionalSources().filter((source) => source.id !== 'hyg');
if (others.length === 0) {
return hygStars;
}
const candidates = [{ sourceId: 'hyg', parallaxPrecisionMas: PARALLAX_PRECISION_MAS['hyg'], stars: hygStars }];
for (const source of others) {
try {
candidates.push({
sourceId: source.id,
parallaxPrecisionMas: PARALLAX_PRECISION_MAS[source.id] ?? 1,
stars: await source.fetch!()
});
} catch (error) {
// An answer that cannot be worked with is not an outage: skipping it would write a
// half-catalogue over the published assets before the merge gate got to say so.
if (error instanceof GaiaAnswerError) {
throw error;
}
console.log(` skipping ${source.name}: ${error instanceof Error ? error.message : error}`);
}
}
if (candidates.length === 1) {
return hygStars;
}
const { stars, summary } = mergeStarCatalogues(candidates);
console.log(` merged ${summary.total} stars from ${candidates.length} catalogues (${summary.duplicates} entries folded into a better-measured one):`);
for (const [sourceId, count] of Object.entries(summary.bySource)) {
console.log(` ${sourceId}: ${count}`);
}
return stars;
}
export function writeStarAssets(stars: StarRecord[]): void {
ensureDataDir();
// The layout lives in `star-catalog.ts`, which the app decodes with — one definition, so the
// writer and the reader cannot drift.
const { index, positions, meta } = encodeStarCatalog(stars);
writeFileSync(dataPath('stars.bin'), Buffer.from(positions.buffer));
writeFileSync(dataPath('stars-meta.bin'), Buffer.from(meta));
writeFileSync(dataPath('stars-index.json'), JSON.stringify(index));
}
// On its own it writes what the ETL would, hosts included; imported late, since fetchExoplanets imports this module.
if (require.main === module) {
import('./fetchExoplanets').then(({ fetchExoplanets }) => fetchExoplanets()).catch((error) => {
console.error(error);
process.exitCode = 1;
});
}