Alchiba is catalogued in this registry as a star, held in the frame of Milky Way, from Gaia DR3 — local star field 4D.
Registry id GAIA_3489338019475637760 ·
source layer gaia ·
provenance PROCESSED — derived deterministically from source catalogues (unit, frame and epoch conversions, cross-source reconciliation) — no value invented
Open Alchiba in the live scene → The scene composes a position for any date and is where a figure becomes a picture. It downloads the whole catalogue first: measured against the built product, an object outside the core resolves after about 16 s over a local network and about 147 s over a 4 Mbit link, having transferred roughly 70 MB. If you cannot wait that long, this page is the answer.
| Quantity | Value | Uncertainty | Source |
|---|---|---|---|
| Temperature | 6900 K | no published uncertainty in this registry | Gaia DR3 — local star field 4D |
Each row carries its own uncertainty and its own source. Where a row says no uncertainty is published, that is what the catalogue says — it is not a claim that the value is exact.
| Kind | star |
|---|---|
| Origin | natural |
d=14.98 pc · G=3.9 · RV 2.8±0.3 km/s [XHIP, positional] [Gaia DR3] · designation Gaia DR3 3489338019475637760 [IAU-CSN]
Reproduced as the source wrote it. Author-year citations link to their DOI where one is registered.
These are absences in the catalogues aggregated here, not measurements of zero, and not statements that the quantity is unknown to science:
| Database | Gaia DR3 — local star field 4D |
|---|---|
| Authority | ESA Gaia DR3 (gaia_source) |
| Address | https://gea.esac.esa.int/tap-server/tap/sync |
| Licence | ESA Gaia data — free use with attribution (Gaia DPAC) |
| How it entered | RAW snapshot via scripts/ingest-gaia.ts (fetched 2026-06-10T06:47Z) |
| Snapshot | 2026-06-10 |
| Coverage | 36,835 stars ≤50 pc, σ_d/d<1% (I15 in-query); 26,777 with radial velocity; cross-joined to the exoplanet hosts (dedup + teff corroboration). Positions are REAL positions at the simulated instant, not the sky as seen from Earth: each catalogue position is displaced along the star's own measured velocity by (J2000 − catalogue epoch) PLUS the light-travel time d/c, since a catalogue records where a star APPEARED. A star with no measured motion is not displaced at all. |
This database remains the property of its owners and is reused under its own licence. If you quote a value from this page, name that database alongside SolarSystemRegistry.org.