C/2003 G1
Not currently visible. Last report 8067 days ago at mag 29.3. Historic peak was mag 15.1. Typical backyard telescopes will not show it. HST, JWST, or an 8–10 m class telescope might recover it with a good ephemeris.
Right ascension
—
J2000
Declination
—
J2000
Estimated magnitude
29.3
Professional survey · COBS consensus
Confidence
33
Class E · priority 60
Observations
67
Arc unknown
Last observation
8067d ago
Wed, 06 Oct 2004 11:02:24 GMT · COBS consensus
Perihelion
2003-01-25
4.930 au
Peak window
2003-01-22 → 2003-05-27
COBS peak mag 15.1 on 2003-05-24 · perihelion 2003-01-25. Window is those dates ±3 days — not a light-curve fit.
Historic peak
15.1
COBS / analyzed peak 2003-05-24
Catalog ingest
13h ago
Venator last wrote this row 2026-11-06 14:20:19 UTC
Brightness over time (V mag)
Gold = reported observations. Steel dashed family = ensemble (nominal / outburst / fade / disruption).
Tail length
Converted to degrees from COBS (d / arcmin / arcsec). Empty until analysis has pulled the archive.
Ensemble is a first-pass H0/n photometric model plus observed samples — not a trained ML forecast yet. The background analyzer walks the catalog one object at a time so COBS is not flooded. Disruption track rises after perihelion to stand in for solar-wind stripping.
q
4.930 au
e
1.0000
i
66.60°
Ω
246.00°
ω
11.50°
a
—
MOID
—
H
—
H0 / n
—
NEO score
—
PHA score
—
RMS
—
Elongation
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COBS comet list
okComet Observation Database magnitudes and perihelion data for the full COBS list (active and inactive).
C/2003 G1 (LINEAR)
Informal: LINEAR
C/2003 G1 · 2026-09-14 18:27:55 UTC → current
Discoverer · parsed-name · 2026-09-14 18:27:55 UTC → current
CCD Observer · HOR02 · 42 reports · last 8085d ago
CCD Observer · NAK01 · 10 reports · last 8067d ago
CCD Observer · TSU02 · 8 reports · last 8422d ago
CCD Observer · RES · 3 reports · last 8196d ago
CCD Observer · OHS · 2 reports · last 8287d ago
CCD Observer · EZA · 2 reports · last 8583d ago
Pips are observation weight on this object (log of report count). Hover for catalog-wide weight.