215P
Not visible to typical instruments. Current estimate mag 22.7. Historic peak was mag 20.4. Visual and most CCD amateur setups will not see it. Space telescopes or large ground telescopes are the remaining path.
Right ascension
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J2000
Declination
—
J2000
Estimated magnitude
22.7
Professional survey · COBS consensus
Confidence
33
Class E · priority 60
Observations
42
Arc unknown
Last observation
127d ago
Tue, 12 May 2026 23:17:31 GMT · COBS consensus
Perihelion
2028-11-22
3.620 au
Peak window
2019-07-24 → 2028-11-25
COBS peak mag 20.4 on 2019-07-27 · perihelion 2028-11-22. Window is those dates ±3 days — not a light-curve fit.
Historic peak
20.4
COBS / analyzed peak 2019-07-27
Catalog ingest
11h ago
Venator last wrote this row 2026-09-16 13:20:16 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
3.620 au
e
0.1650
i
10.60°
Ω
56.70°
ω
262.00°
a
—
MOID
—
H
—
H0 / n
—
NEO score
—
PHA score
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RMS
—
Elongation
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COBS comet list
okComet Observation Database magnitudes and perihelion data for the full COBS list (active and inactive).
215P/NEAT
215P · 2026-09-14 18:27:52 UTC → current
Discoverer · parsed-name · 2026-09-14 18:27:52 UTC → current
CCD Observer · HIL04 · 22 reports · last 127d ago
CCD Observer · NAK01 · 7 reports · last 8363d ago
CCD Observer · NOV01 · 7 reports · last 5389d ago
CCD Observer · TSU02 · 3 reports · last 5864d ago
CCD Observer · PAP04 · 1 reports · last 2143d ago
CCD Observer · MAI01 · 1 reports · last 562d ago
CCD Observer · SHU · 1 reports · last 5943d ago
Pips are observation weight on this object (log of report count). Hover for catalog-wide weight.