Dabih is catalogued in this registry as a star, held in the frame of Milky Way, from Gaia DR3 — naked-eye bright sky (G ≤ 7).
Registry id GAIA_6875990375999580544 ·
source layer gaia-bright ·
provenance PROCESSED — derived deterministically from source catalogues (unit, frame and epoch conversions, cross-source reconciliation) — no value invented
Open Dabih 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.
| Kind | star |
|---|---|
| Origin | natural |
d=119.10 pc · σ_d/d 8% · G=2.8 · RV missing (tangential-only drift) [Gaia DR3] · designation Gaia DR3 6875990375999580544 [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 — naked-eye bright sky (G ≤ 7) |
|---|---|
| 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-bright.ts (fetched 2026-07-10T10:36Z) |
| Snapshot | 2026-07-10 |
| Coverage | 19,122 stars, G ≤ 7 at ALL distances — the familiar bright sky. RELAXED precision gate (deliberate, unlike the ≤50 pc layer's σ_d/d<1%): parallax > 3σ only, the per-star distance σ carried; 522 rows without a usable parallax excluded, never placed at an invented distance; deduplicated by source_id against the ≤50 pc layer (1656) and positionally against curated stars + exoplanet hosts. 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. |
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