40P
Not visible to typical instruments. Current estimate mag 23.6. Historic peak was mag 15.4. Visual and most CCD amateur setups will not see it. Space telescopes or large ground telescopes are the remaining path.
Right ascension
—
J2000
Declination
—
J2000
Estimated magnitude
23.6
Professional survey · COBS consensus
Confidence
33
Class E · priority 60
Observations
185
Arc unknown
Last observation
58d ago
Mon, 20 Jul 2026 20:52:48 GMT · COBS consensus
Perihelion
2025-11-12
1.820 au
Peak window
2025-11-09 → 2025-11-22
COBS peak mag 15.4 on 2025-11-19 · perihelion 2025-11-12. Window is those dates ±3 days — not a light-curve fit.
Historic peak
15.4
COBS / analyzed peak 2025-11-19
Catalog ingest
10h ago
Venator last wrote this row 2026-09-16 13:20:17 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
1.820 au
e
0.6310
i
11.60°
Ω
129.00°
ω
52.10°
a
—
MOID
—
H
—
H0 / n
—
NEO score
—
PHA score
—
RMS
—
Elongation
—
COBS comet list
okComet Observation Database magnitudes and perihelion data for the full COBS list (active and inactive).
40P/Vaisala
40P · 2026-09-14 18:27:55 UTC → current
Discoverer · parsed-name · 2026-09-14 18:27:55 UTC → current
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CCD Observer · PEA · 12 reports · last 201d ago
Visual Observer · MIK · 12 reports · last 12142d ago
Visual Observer · KUT · 12 reports · last 8193d ago
Visual Observer · SCO01 · 9 reports · last 12108d ago
Visual Observer · HAL · 8 reports · last 12176d ago
CCD Observer · SRB · 8 reports · last 8122d ago
CCD Observer · DEK01 · 7 reports · last 186d ago
CCD Observer · NAK01 · 6 reports · last 8147d ago
CCD Observer · TSU02 · 6 reports · last 4278d ago
CCD Observer · PRY01 · 6 reports · last 4168d ago
CCD Observer · OHS · 6 reports · last 8187d ago
CCD Observer · KOU · 5 reports · last 58d ago
CCD Observer · HOR02 · 5 reports · last 8117d ago
CCD Observer · OLA · 5 reports · last 229d ago
Visual Observer · MOR · 4 reports · last 12149d ago
CCD Observer · RES · 4 reports · last 8130d ago
CCD Observer · SHU · 4 reports · last 8177d ago
Visual Observer · NAK07 · 4 reports · last 12157d ago
CCD Observer · YUS · 4 reports · last 209d ago
Visual Observer · LEH · 3 reports · last 8190d ago
Visual Observer · BOU · 3 reports · last 12202d ago
Visual Observer · PEA · 2 reports · last 8189d ago
Visual Observer · COM · 2 reports · last 12202d ago
Visual Observer · CAV · 2 reports · last 12169d ago
CCD Observer · FRI02 · 2 reports · last 194d ago
CCD Observer · KAL02 · 2 reports · last 8175d ago
CCD Observer · MOR · 1 reports · last 8190d ago
CCD Observer · PAP04 · 1 reports · last 223d ago
CCD Observer · YOS02 · 1 reports · last 235d ago
Visual Observer · SAR02 · 1 reports · last 8244d ago
CCD Observer · MAS01 · 1 reports · last 265d ago
CCD Observer · MAT08 · 1 reports · last 242d ago
CCD Observer · ORI · 1 reports · last 4281d ago
CCD Observer · PIL01 · 1 reports · last 201d ago
Visual Observer · HAS02 · 1 reports · last 12234d ago
CCD Observer · NAG08 · 1 reports · last 219d ago
Visual Observer · TOT03 · 1 reports · last 8160d ago
Pips are observation weight on this object (log of report count). Hover for catalog-wide weight.