226P
Not currently visible. Last report 972 days ago at mag 24.0. Historic peak was mag 15.5. 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
24.0
Professional survey · COBS consensus
Confidence
33
Class E · priority 60
Observations
96
Arc unknown
Last observation
972d ago
Sat, 09 Mar 2024 19:26:24 GMT · COBS consensus
Perihelion
2023-12-26
1.780 au
Peak window
2023-11-24 → 2023-12-29
COBS peak mag 15.5 on 2023-11-27 · perihelion 2023-12-26. Window is those dates ±3 days — not a light-curve fit.
Historic peak
15.5
COBS / analyzed peak 2023-11-27
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.
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
1.780 au
e
0.5280
i
44.00°
Ω
54.00°
ω
341.00°
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).
226P/Pigott-LINEAR-Kowalski
226P · 2026-09-14 18:27:53 UTC → current
Discoverer · parsed-name · 2026-09-16 13:20:16 UTC → current
Discoverer · parsed-name · 2026-09-16 13:20:16 UTC → current
Discoverer · parsed-name · 2026-09-16 13:20:16 UTC → current
Discoverer · parsed-name · 2026-09-16 13:20:16 UTC → current
Discoverer · parsed-name · 2026-09-14 18:27:53 UTC → 2026-09-16 13:20:16 UTC
CCD Observer · PEA · 14 reports · last 1032d ago
CCD Observer · NAG05 · 12 reports · last 3599d ago
CCD Observer · HIL04 · 12 reports · last 1013d ago
CCD Observer · LEH02 · 11 reports · last 972d ago
CCD Observer · DEK01 · 5 reports · last 1031d ago
CCD Observer · NAK01 · 4 reports · last 8616d ago
CCD Observer · PAP04 · 4 reports · last 1037d ago
Visual Observer · GUZ · 3 reports · last 3722d ago
CCD Observer · RAM02 · 3 reports · last 3622d ago
Visual Observer · SZA · 3 reports · last 3599d ago
Visual Observer · PEA · 2 reports · last 3797d ago
Visual Observer · HAR11 · 2 reports · last 3681d ago
Visual Observer · DIJ · 2 reports · last 3631d ago
CCD Observer · MAS01 · 2 reports · last 1057d ago
CCD Observer · TSU02 · 2 reports · last 3657d ago
Visual Observer · CAM03 · 2 reports · last 3713d ago
CCD Observer · CAR06 · 2 reports · last 1030d ago
CCD Observer · SHU · 2 reports · last 3677d ago
CCD Observer · NOV01 · 1 reports · last 3665d ago
Visual Observer · WYA · 1 reports · last 3779d ago
CCD Observer · BUI01 · 1 reports · last 1034d ago
Visual Observer · WOL01 · 1 reports · last 3684d ago
CCD Observer · KII · 1 reports · last 1035d ago
CCD Observer · YOS02 · 1 reports · last 3743d ago
Visual Observer · PAR03 · 1 reports · last 3718d ago
CCD Observer · LOS02 · 1 reports · last 1021d ago
CCD Observer · TIR01 · 1 reports · last 1040d ago
Visual Observer · YOS04 · 1 reports · last 3718d ago
Visual Observer · SCA02 · 1 reports · last 8696d ago
Pips are observation weight on this object (log of report count). Hover for catalog-wide weight.