Files
star-map/tools/etl/fetchStars.ts
T
SenrokaiandClaude Opus 5.5 8c3a86097c Place a star at whichever of its two distances is the more precise, not at Gaia's regardless
placementDistancePc took Gaia's distance wherever the cross-match gave a usable one, and its
docstring and c64eea0 called that "the better measurement", adding that Gaia saturates on the
brightest stars "so those sit at their Hipparcos distance". For 273 of the 88 781 HYG stars with
both, Gaia's relative error is the larger, 257 of them naked-eye and 38 by more than twice: Eta Leo
was drawn at Gaia's 556.6 pc ±17 % against Hipparcos's 389 pc ±6.2 %, Schedar and Tarazed at
Gaia's though both have Gaia G of about 2.

placementDistancePc now takes both relative errors and picks the smaller, Gaia's as before when
either is missing; fetchStars gives the placed star the error and the Gaia-distance flag of the
distance it took. The merge's combine keeps the Gaia entry's direction, and now takes the other
entry's distance with its error where that is the more precise, so a bright star Gaia's main query
also holds lands at its Hipparcos distance too. Gaia still wins for the rest, whose parallaxes are
some fifty times more precise.

From cache: 424 stars move, 386 of them naked-eye; HYG rows at Gaia's distance 58 379 -> 58 109 and
HYG stars flagged so 8 129 -> 8 095. Eta Leo 556.6 -> 389.1 pc, Tarazed 178.9 -> 121.1, Imai 139.5 ->
105.8, Schedar 71.0 -> 70.0, Alphecca 23.7 -> 23.0, each now "±" its Hipparcos error. Where the two
disagree by more than 5 σ (21 stars, Iot Gem 11 σ), one of the formal errors is wrong, and this
takes the smaller one at its word. The validators pass unchanged.

Controls, each failing its named test: the placement ignoring the errors, the merge keeping Gaia's
distance whatever the errors, and taking the distance but not its error (1 of 805 each).

Co-Authored-By: Claude Opus 5.5 (1M context) <noreply@anthropic.com>
2026-09-29 21:37:35 +02:00

233 lines
10 KiB
TypeScript

import { writeFileSync } from 'node:fs';
import { 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';
const HYG_UNKNOWN_DISTANCE_PC = 100000; // HYG's placeholder for unmeasured/unreliable parallax
/**
* 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 hipparcosPc = Number.isFinite(hygPc) && hygPc > 0 && hygPc < HYG_UNKNOWN_DISTANCE_PC ? hygPc : undefined;
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 = row['hip'] ? hipparcosErrors.get(Number(row['hip'])) : undefined;
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;
});
}