74P
Not currently visible. Last report 269 days ago at mag 18.8. 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
—
J2000
Declination
—
J2000
Estimated magnitude
18.8
Professional survey · COBS consensus
Confidence
33
Class E · priority 60
Observations
318
Arc unknown
Last observation
269d ago
Tue, 10 Feb 2026 22:33:35 GMT · COBS consensus
Perihelion
2026-01-17
4.830 au
Peak window
2026-01-14 → 2026-01-20
COBS peak mag 18.2 on 2026-01-17 · perihelion 2026-01-17. Window is those dates ±3 days — not a light-curve fit.
Historic peak
18.2
COBS / analyzed peak 2026-01-17
Catalog ingest
2m ago
Venator last wrote this row 2026-11-07 03:00:09 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
4.830 au
e
0.0787
i
5.74°
Ω
45.90°
ω
58.70°
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).
74P/Smirnova-Chernykh
74P · 2026-09-13 22:21:22 UTC → current
Discoverer · parsed-name · 2026-09-13 22:21:22 UTC → current
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Visual Observer · LEH · 19 reports · last 9305d ago
CCD Observer · MAS01 · 19 reports · last 2626d ago
CCD Observer · HOR02 · 17 reports · last 9266d ago
CCD Observer · TSU02 · 11 reports · last 3656d ago
CCD Observer · NAG05 · 10 reports · last 3513d ago
CCD Observer · KAD02 · 10 reports · last 8955d ago
CCD Observer · PEA · 9 reports · last 15481d ago
CCD Observer · FRI02 · 8 reports · last 3108d ago
CCD Observer · BAR06 · 7 reports · last 4368d ago
CCD Observer · HAE · 6 reports · last 6043d ago
CCD Observer · LEH02 · 6 reports · last 3107d ago
CCD Observer · ROQ · 5 reports · last 9296d ago
Visual Observer · BOU · 5 reports · last 9276d ago
CCD Observer · YOS04 · 5 reports · last 9792d ago
Seiichi Yoshida and KenIchi Kadota
CCD Observer · YOS05 · 5 reports · last 9792d ago
Visual Observer · REN · 4 reports · last 9326d ago
CCD Observer · NOV01 · 4 reports · last 5760d ago
Visual Observer · SCO01 · 4 reports · last 12275d ago
CCD Observer · WAR01 · 4 reports · last 3121d ago
CCD Observer · DEK01 · 4 reports · last 3176d ago
CCD Observer · RAM02 · 4 reports · last 3546d ago
Visual Observer · MOD · 4 reports · last 12230d ago
Visual Observer · KUT · 4 reports · last 6524d ago
Visual Observer · HAE · 3 reports · last 6043d ago
CCD Observer · YOS02 · 3 reports · last 2725d ago
Visual Observer · NAK07 · 3 reports · last 12219d ago
Visual Observer · HAL · 2 reports · last 12646d ago
Visual Observer · BAR06 · 2 reports · last 3572d ago
CCD Observer · PRA02 · 2 reports · last 10502d ago
Visual Observer · HER02 · 2 reports · last 11392d ago
Visual Observer · HOR02 · 2 reports · last 9743d ago
Visual Observer · RES · 2 reports · last 9709d ago
CCD Observer · HAU · 2 reports · last 6073d ago
CCD Observer · PAR03 · 2 reports · last 3136d ago
CCD Observer · YUS · 2 reports · last 6041d ago
CCD Observer · NEV · 2 reports · last 6881d ago
1–40 of 52
Pips are observation weight on this object (log of report count). Hover for catalog-wide weight.