C/2005 YW
Not currently visible. Last report 7140 days ago at mag 33.7. Historic peak was mag 14.8. 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
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J2000
Estimated magnitude
33.7
Professional survey · COBS consensus
Confidence
33
Class E · priority 60
Observations
7
Arc unknown
Last observation
7140d ago
Sat, 21 Apr 2007 08:52:48 GMT · COBS consensus
Perihelion
2006-11-30
1.990 au
Peak window
2006-11-27 → 2006-12-30
COBS peak mag 14.8 on 2006-12-27 · perihelion 2006-11-30. Window is those dates ±3 days — not a light-curve fit.
Historic peak
14.8
COBS / analyzed peak 2006-12-27
Catalog ingest
13h ago
Venator last wrote this row 2026-11-06 14:20:20 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
1.990 au
e
0.9860
i
41.10°
Ω
302.00°
ω
234.00°
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/2005 YW (LINEAR)
Informal: LINEAR
C/2005 YW · 2026-09-14 18:27:56 UTC → current
Discoverer · parsed-name · 2026-09-14 18:27:56 UTC → current
Visual Observer · RAE · 3 reports · last 7140d ago
CCD Observer · YOS02 · 1 reports · last 7252d ago
Visual Observer · MAT08 · 1 reports · last 7144d ago
Visual Observer · YOS04 · 1 reports · last 7311d ago
Visual Observer · ROB06 · 1 reports · last 7194d ago
Pips are observation weight on this object (log of report count). Hover for catalog-wide weight.