C/2008 Q1
Not currently visible. Last report 6284 days ago at mag 33.2. Historic peak was mag 17.4. 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
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J2000
Declination
—
J2000
Estimated magnitude
33.2
Professional survey · COBS consensus
Confidence
33
Class E · priority 60
Observations
5
Arc unknown
Last observation
6284d ago
Mon, 24 Aug 2009 04:33:36 GMT · COBS consensus
Perihelion
2008-12-29
2.970 au
Peak window
2008-12-26 → 2009-01-19
COBS peak mag 17.4 on 2009-01-16 · perihelion 2008-12-29. Window is those dates ±3 days — not a light-curve fit.
Historic peak
17.4
COBS / analyzed peak 2009-01-16
Catalog ingest
13h ago
Venator last wrote this row 2026-11-06 14:20:18 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.
No tail measures stored yet for this object.
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
2.970 au
e
0.9950
i
119.00°
Ω
9.61°
ω
105.00°
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/2008 Q1 (Maticic)
Informal: Maticic
C/2008 Q1 · 2026-09-14 18:27:53 UTC → current
Discoverer · parsed-name · 2026-09-14 18:27:53 UTC → current
CCD Observer · CHE09 · 1 reports · last 6348d ago
CCD Observer · BRE03 · 1 reports · last 6397d ago
CCD Observer · HAU · 1 reports · last 6383d ago
CCD Observer · SHU · 1 reports · last 6284d ago
CCD Observer · YUS · 1 reports · last 6367d ago
Pips are observation weight on this object (log of report count). Hover for catalog-wide weight.