Files
star-map/tools/etl/fetchExoplanets.ts
T
SenrokaiandClaude Opus 5.5 23547defe0 Read an archive host's colour off the dwarf sequence at its temperature, and say it was not measured
For an archive-placed host with a temperature and no B magnitude, fetchExoplanets took B−V from
Ballesteros' blackbody fit, which runs 0.1 to 0.2 redder than Pecaut & Mamajek's dwarf sequence
below 3 800 K, and the luminosity then read its correction off that sequence at that colour: 3 500 K
came back as 3 102 K with a correction 1.15 magnitudes too large, anything under about 3 170 K was
clamped to B−V 2.00, and the card printed it as a measured "Colour B−V 2.00". CFBDSIR
J145829+101343, a 580 K brown dwarf, read "Spectral type ~M6, from colour".

temperatureToColorIndex now reads the table itself backwards, interpolating B−V between the two
types the temperature falls between, so the temperature and correction read back off the colour
are the table's at that temperature; it has no answer outside 2 420 to 31 400 K. The colour is
flagged colorFromTemperature, a fifth bit in the photometry byte (the format, README and the ETL's
round-trip check follow), and the card prints it "B−V 1.66, from its temperature", marked derived.

From cache: 57 archive stars change colour; 54 carry the flag and 3, CFBDSIR J145829+101343 among
them, now have none. For the 47 of them the archive gives a luminosity, the one derived from
magnitude and colour moves from a median 0.228 dex off it to 0.124; Kepler-445 (3 157 K) from
0.0282 L☉ to 0.0080 against the archive's 0.0079. Its colour goes from 2.00 to 1.67. The card shows
the archive's luminosity where it has one since earlier on this branch, so this is the figure used
for the rest and for their radii.

Controls, each failing its named test: the nearest hotter row taken without interpolating (2 of
803 failed), no refusal outside the table, the flag not encoded, and the card calling the colour
measured (1 of 803 each).

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

238 lines
12 KiB
TypeScript

import { createHash } from 'node:crypto';
import { writeFileSync } from 'node:fs';
import { propagateProperMotion, raDegDecDistanceToXyz } from '../../src/app/shared/astro/coordinates';
import { ARCHIVE_EPOCH, archiveStarId, buildStarNameIndex, CATALOGUE_EPOCH, 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 DR2's epoch, J2015.5, not the catalogue's J2000 (see
* `ARCHIVE_EPOCH`): of the 746 matched hosts moving over 100 mas a year, 741 sit nearer their star
* once carried back (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 = CATALOGUE_EPOCH - ARCHIVE_EPOCH;
/** 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 }),
...(colorIndex !== null && (b === undefined || v === undefined) ? { colorFromTemperature: true } : {}),
...(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;
});
}