Files
star-map/tools/etl/fetchExoplanets.ts
T
SenrokaiandClaude Opus 5.5 62f81f2c43 Number the stars the archive places after their host's name, so a refresh keeps each one's id
4c8e4a0 numbered each star it adds from the Exoplanet Archive by its place among the unmatched
hosts, in pl_name order, and the refresh workflow re-queries the archive every Monday. One host
added or dropped ahead of another renumbers it: in the review, removing a single planet row
renamed 3 276 of the 3 277 ids, and a bookmark kept on Kepler-186 (1070001620) opened Kepler-1860
under Kepler-186's stored name. HYG's and Gaia's ids do not move between refreshes; the merge's own
comment says ids are meant to hold.

archiveStarId (host-star-matching.ts, beside the matcher the ETL already imports from there) hashes
the host name with FNV-1a into the 3.7 million ids between 1 070 000 000 and 2^30, and moves a name
whose id is taken to the next free one. The added stars are sorted by id before they are appended,
so the published list stays in id order. Measured: all 4 237 archive-hosted planets change host id
once (Kepler-186 is now 1073671518), none of the others; one of the 3 277 names was probed past a
collision, and one new id falls in the old 1070000000-1070003276 range, so a bookmark saved on that
old id would open the wrong star once. Dropping the same row from a copy of the cached answer and
rerunning the exoplanet step in a scratch copy of the ETL now leaves 3 276 of 3 276 ids unchanged.
The validators pass: no duplicate id, all under 2^30.

Controls, each failing its named test: the id taken from the order of arrival, and no probing past
a taken id (1 of 801 each).

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

237 lines
12 KiB
TypeScript

import { createHash } from 'node:crypto';
import { writeFileSync } from 'node:fs';
import { propagateProperMotion, raDegDecDistanceToXyz } from '../../src/app/shared/astro/coordinates';
import { archiveStarId, buildStarNameIndex, resolveHostStarId } from '../../src/app/shared/astro/host-star-matching';
import { temperatureToColorIndex } from '../../src/app/shared/astro/spectral';
import { ExoplanetRecord } from '../../src/app/shared/models/exoplanet.model';
import { isDesignation } from '../../src/app/shared/models/star-catalog';
import { StarRecord } from '../../src/app/shared/models/star.model';
import { fetchStars, writeStarAssets } from './fetchStars';
import { parseCsvObjects, parseOptionalNumber } from './lib/csv';
import { fetchTextCached } from './lib/http';
import { dataPath, ensureDataDir } from './lib/paths';
const TAP_BASE_URL = 'https://exoplanetarchive.ipac.caltech.edu/TAP/sync';
const TAP_COLUMNS = [
'pl_name',
'hostname',
'ra',
'dec',
'sy_dist',
'sy_pmra',
'sy_pmdec',
'pl_orbsmax',
'pl_orbeccen',
'pl_orbincl',
'pl_orblper',
'pl_orbper',
'pl_rade',
'pl_bmasse',
'st_mass',
'disc_year'
].join(',');
// Ordered explicitly: without it the archive is free to return rows in any order, and a
// scheduled re-run of the ETL would then rewrite exoplanets.json — and commit a diff — when
// nothing was actually published. pl_name is unique among default_flag=1 rows, so the order
// is total and the output is a pure function of the archive's content.
const TAP_QUERY = `select+${TAP_COLUMNS}+from+ps+where+default_flag=1+order+by+pl_name&format=csv`;
const TAP_URL = `${TAP_BASE_URL}?query=${TAP_QUERY}`;
// The cache is keyed by the request it answers — endpoint included, since the cache records
// only that some response arrived: one cached before a column was added would otherwise keep
// serving rows without it, and a missing proper-motion cell reads as "does not move",
// silently wrong rather than visibly broken.
const CACHE_FILE = `exoplanet-archive-ps-${createHash('sha1').update(TAP_URL).digest('hex').slice(0, 8)}.csv`;
/**
* The host's columns from the Planetary Systems Composite table, for the cells a planet's
* default row leaves blank and for the columns that query does not ask for.
*
* The default rows are one reference each, which is what keeps a planet's orbit coherent: its
* period, semi-major axis, eccentricity and periastron come from one fit. A composite row takes
* each column from wherever it is best measured, so an orbit read from it could pair one paper's
* eccentricity with another's argument of periastron; none of its orbital columns are asked for.
* Its system columns equal the default rows' wherever both are given (6 225 distances, 6 352
* positions, none different). What it adds is the 100 distances the default rows leave blank,
* TRAPPIST-1's seven among them, 870 host masses, and the parallax, photometry and stellar
* parameters below — each of which may come from a different reference.
*/
const COMPOSITE_COLUMNS = [
'pl_name',
'ra',
'dec',
'sy_dist',
'sy_plx',
'sy_pmra',
'sy_pmdec',
'sy_bmag',
'sy_vmag',
'sy_gaiamag',
'st_spectype',
'st_teff',
'st_rad',
'st_mass',
'st_lum'
].join(',');
// pl_name is unique here too, one row per planet.
const COMPOSITE_URL = `${TAP_BASE_URL}?query=select+${COMPOSITE_COLUMNS}+from+pscomppars+order+by+pl_name&format=csv`;
const COMPOSITE_CACHE_FILE = `exoplanet-archive-pscomppars-${createHash('sha1').update(COMPOSITE_URL).digest('hex').slice(0, 8)}.csv`;
/**
* The same table's distance errors, for the stars placed from the archive. A query of its own,
* cached apart, so that asking for them did not refetch the columns above: the archive changes
* daily, and a new answer would have moved every figure the catalogue was checked against.
*/
const DISTANCE_ERRORS_URL = `${TAP_BASE_URL}?query=select+pl_name,sy_disterr1,sy_disterr2+from+pscomppars+order+by+pl_name&format=csv`;
const DISTANCE_ERRORS_CACHE_FILE = `exoplanet-archive-disterr-${createHash('sha1').update(DISTANCE_ERRORS_URL).digest('hex').slice(0, 8)}.csv`;
const ARCHIVE_SOURCE = 'exoplanet-archive';
/**
* The archive's positions are at Gaia's epoch, J2016, not the catalogue's J2000: of the 746
* matched hosts moving over 100 mas a year, 741 sit nearer their star once carried back sixteen
* years (a median 0.11″ from it, against 3.47″ as published). The matcher tries both epochs; a
* star placed from the archive has to pick one.
*/
const ARCHIVE_TO_CATALOGUE_YEARS = 2000 - 2016;
/** As in `fetchStars`: faint, for a host the archive gives neither a V nor a G magnitude. */
const UNKNOWN_MAGNITUDE = 15;
/**
* Downloads confirmed exoplanets from the NASA Exoplanet Archive (`Planetary Systems` TAP
* table), cross-references each host star to the star catalogue, adds a star from the archive's
* own figures for each host the catalogue lacks but the archive places, and writes
* `exoplanets.json` together with the star assets, which those additions change. Returns both.
*/
export async function fetchExoplanets(stars?: StarRecord[]): Promise<{ exoplanets: ExoplanetRecord[]; stars: StarRecord[] }> {
console.log('Fetching confirmed exoplanets from the NASA Exoplanet Archive...');
const knownStars = stars ?? (await fetchStars());
const nameIndex = buildStarNameIndex(knownStars);
const knownById = new Map(knownStars.map((star) => [star.id, star]));
const csv = await fetchTextCached(TAP_URL, CACHE_FILE);
const rows = parseCsvObjects(csv);
const composite = new Map(parseCsvObjects(await fetchTextCached(COMPOSITE_URL, COMPOSITE_CACHE_FILE)).map((row) => [row['pl_name'], row]));
const distanceErrors = new Map(parseCsvObjects(await fetchTextCached(DISTANCE_ERRORS_URL, DISTANCE_ERRORS_CACHE_FILE)).map((row) => [row['pl_name'], row]));
let matched = 0;
// Catalogue stars known only by their Gaia designation, which take the archive's host name —
// the only way "TRAPPIST-1" or "Teegarden's Star" can be found by search.
const renamed = new Map<number, string>();
const archiveStars = new Map<string, StarRecord>();
const archiveIds = new Set<number>();
const bands = { V: 0, G: 0, none: 0 };
const exoplanets: ExoplanetRecord[] = rows.map((row, index) => {
const compositeRow = composite.get(row['pl_name']);
// `parseOptionalNumber`, not `Number`: a blank cell would otherwise become 0, which is a
// finite, plausible-looking coordinate rather than the "not measured" it actually means.
const host = (column: string) => parseOptionalNumber(row[column] || compositeRow?.[column]);
const raDeg = host('ra') ?? Number.NaN;
const decDeg = host('dec') ?? Number.NaN;
const distancePc = host('sy_dist') ?? Number.NaN;
const pmRaMasPerYear = host('sy_pmra');
const pmDecMasPerYear = host('sy_pmdec');
let hostStarId = resolveHostStarId(
{ hostname: row['hostname'], raDeg, decDeg, distancePc, pmRaMasPerYear, pmDecMasPerYear, parallaxMas: host('sy_plx') },
knownStars,
nameIndex
);
if (hostStarId !== null) {
matched++;
const star = knownById.get(hostStarId);
if (star?.source === 'gaia' && isDesignation(star) && !renamed.has(hostStarId)) {
renamed.set(hostStarId, row['hostname']);
}
} else if ([raDeg, decDeg, distancePc].every(Number.isFinite) && distancePc > 0) {
let archiveStar = archiveStars.get(row['hostname']);
if (!archiveStar) {
// Carried back from the archive's epoch like any Gaia row, and placed at `sy_dist`.
const j2000 = propagateProperMotion(raDeg, decDeg, pmRaMasPerYear ?? 0, pmDecMasPerYear ?? 0, ARCHIVE_TO_CATALOGUE_YEARS);
// V where the archive has it, as HYG's stars are; else Gaia's G, the band the catalogue's
// Gaia stars are already in.
const v = host('sy_vmag');
const g = host('sy_gaiamag');
const b = host('sy_bmag');
const temperatureK = host('st_teff');
const band = v !== undefined ? 'V' : g !== undefined ? 'G' : undefined;
bands[band ?? 'none']++;
// B-V where the archive has both magnitudes, else the effective temperature's; with
// neither, null leaves the colour to the spectral type, as for any other star.
const colorIndex = b !== undefined && v !== undefined ? b - v : temperatureK !== undefined ? temperatureToColorIndex(temperatureK) : null;
// The archive gives the distance's error as two one-sided ones; their mean, relative.
const errors = distanceErrors.get(row['pl_name']);
const [above, below] = [parseOptionalNumber(errors?.['sy_disterr1']), parseOptionalNumber(errors?.['sy_disterr2'])];
archiveStar = {
id: archiveStarId(row['hostname'], archiveIds),
name: row['hostname'],
...raDegDecDistanceToXyz(j2000.raDeg, j2000.decDeg, distancePc),
magnitude: v ?? g ?? UNKNOWN_MAGNITUDE,
...(band === undefined ? {} : { magnitudeBand: band }),
spectralType: compositeRow?.['st_spectype'] || 'Unknown',
colorIndex,
...(colorIndex === null ? {} : { colorSystem: 'B-V' as const }),
...(above === undefined || below === undefined ? {} : { distanceError: (Math.abs(above) + Math.abs(below)) / 2 / distancePc }),
source: ARCHIVE_SOURCE
};
archiveStars.set(row['hostname'], archiveStar);
archiveIds.add(archiveStar.id);
}
hostStarId = archiveStar.id;
}
return {
id: row['pl_name'] || `exoplanet-${index}`,
hostStarId,
hostStarName: row['hostname'],
name: row['pl_name'],
radiusEarth: parseOptionalNumber(row['pl_rade']),
massEarth: parseOptionalNumber(row['pl_bmasse']),
discoveryYear: parseOptionalNumber(row['disc_year']),
// The period was already being downloaded and thrown away. With the semi-major axis it
// determines the host's gravitational parameter, so keeping it is the difference between
// propagating a planet at its real rate and pretending every host is the Sun.
periodDays: parseOptionalNumber(row['pl_orbper']),
hostStarMassSolar: host('st_mass'),
hostStarRadiusSolar: host('st_rad'),
hostStarTemperatureK: host('st_teff'),
// Published as log10(L/L☉).
hostStarLuminositySolar: ((logLuminosity) => (logLuminosity === undefined ? undefined : 10 ** logLuminosity))(host('st_lum')),
// Kept so the cross-reference can be redone without the archive; see the record's own
// documentation. Undefined rather than NaN, which JSON cannot represent.
hostRaDeg: host('ra'),
hostDecDeg: host('dec'),
hostDistancePc: host('sy_dist'),
hostPmRaMasPerYear: pmRaMasPerYear,
hostPmDecMasPerYear: pmDecMasPerYear,
orbit: {
semiMajorAxisAu: parseOptionalNumber(row['pl_orbsmax']),
eccentricity: parseOptionalNumber(row['pl_orbeccen']),
inclinationDeg: parseOptionalNumber(row['pl_orbincl']),
argumentOfPeriapsisDeg: parseOptionalNumber(row['pl_orblper'])
}
};
});
// Appended after the catalogue, whose ids all sit below ARCHIVE_ID_BASE, and sorted, so the list
// stays in the id order `fetchStars` sorted it into.
const added = [...archiveStars.values()].sort((a, b) => a.id - b.id);
const allStars = [...knownStars.map((star) => (renamed.has(star.id) ? { ...star, name: renamed.get(star.id)! } : star)), ...added];
writeStarAssets(allStars);
ensureDataDir();
writeFileSync(dataPath('exoplanets.json'), JSON.stringify(exoplanets));
console.log(
` wrote ${exoplanets.length} exoplanets: ${matched} on a catalogue star (${renamed.size} Gaia designations named after their host), ` +
`${exoplanets.filter((exoplanet) => exoplanet.hostStarId !== null).length - matched} on ${added.length} stars added from the archive ` +
`(${added.filter((star) => Math.hypot(star.x, star.y, star.z) <= 250).length} within 250 pc; magnitude in V for ${bands.V}, in G for ${bands.G}, none for ${bands.none}).`
);
return { exoplanets, stars: allStars };
}
if (require.main === module) {
fetchExoplanets().catch((error) => {
console.error(error);
process.exitCode = 1;
});
}