Files
star-map/tools/etl/fetchStars.ts
T
SenrokaiandClaude Opus 5.5 ff744a00de Place a naked-eye star HYG gives no distance for by its Hipparcos parallax, where that is 2.5 times its error
c64eea0 left out 41 naked-eye stars "because neither survey gives them a distance". Hipparcos does:
HYG's distances are 1 000 over van Leeuwen's 2007 parallaxes, which the ETL already downloads for
their errors, but HYG writes its 100 000 pc placeholder for every parallax under 1 mas whatever its
error, while keeping far less certain ones above it (Alnilam at 1.65 ± 0.45 mas is drawn). 30 of
the 41 have a positive parallax in the new reduction and 7 have one at least 2.5 times its error:
HD 74180 at 0.67 ± 0.16 mas (4.2 σ), Mu Cep at 0.55 ± 0.20.

hipparcosDistancePc (star-merge.ts, with HYG's placeholder constant moved beside it) keeps HYG's
distance and, where it gives the placeholder, takes 1 000 over the parallax when that is 2.5 times
its error; fetchHipparcosParallaxErrors now returns the parallax with its error. From cache the ETL
keeps 73 563 HYG rows against 73 556 and publishes 455 571 stars; the seven are Alp Cam (1.4 to 3.0
kpc), Psi-1 Aur, HD 74180 (1.2 to 2.0 kpc), HD 86352, HD 96918, Mu Cep (1.3 to 2.9 kpc) and HD
217476, each printed as the range its parallax's error gives. The other 34 stay out: no parallax,
or one within 2.5 times its error of zero. Parallax distances printed as ranges go from 1 109 to
1 116; the validators hold.

Controls, each failing its named test: placeholder rows given no distance, and any parallax 1.25
times its error placing a star (1 of 807 each).

Co-Authored-By: Claude Opus 5.5 (1M context) <noreply@anthropic.com>
2026-09-29 21:45:12 +02:00

233 lines
10 KiB
TypeScript

import { writeFileSync } from 'node:fs';
import { hipparcosDistancePc, mergeStarCatalogues, 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 { fetchGaiaDistancesByHip, fetchHipparcosParallaxErrors, GaiaAnswerError } from './sources/gaia';
import { positionalSources } from './sources/registry';
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, unions the other positional
* sources, and writes `stars.bin` (packed positions) + `stars-index.json` (everything else).
*/
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 stars: StarRecord[] = [];
let atGaiaDistance = 0;
let pastCutoff = 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 gaia = row['hip'] ? gaiaByHip.get(Number(row['hip'])) : undefined;
const gaiaPc = gaia?.distancePc;
const magnitudeV = parseOptionalNumber(row['mag']);
const magnitude = magnitudeV ?? UNKNOWN_MAGNITUDE;
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.
const x = Number(row['x']);
const y = Number(row['y']);
const z = 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 (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.`);
const merged = await mergeWithOtherSources(stars);
merged.sort((a, b) => a.id - b.id);
writeStarAssets(merged);
return merged;
}
/**
* 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));
}
if (require.main === module) {
fetchStars().catch((error) => {
console.error(error);
process.exitCode = 1;
});
}