60P
Not currently visible. Last report 2665 days ago at mag 22.9. Historic peak was mag 16.9. 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
22.9
Professional survey · COBS consensus
Confidence
33
Class E · priority 60
Observations
202
Arc unknown
Last observation
2665d ago
Sat, 01 Jun 2019 22:33:36 GMT · COBS consensus
Perihelion
2025-07-20
1.650 au
Peak window
2025-07-16 → 2025-07-23
COBS peak mag 16.9 on 2025-07-19 · perihelion 2025-07-20. Window is those dates ±3 days — not a light-curve fit.
Historic peak
16.9
COBS / analyzed peak 2025-07-19
Catalog ingest
14h ago
Venator last wrote this row 2026-09-17 13:20:21 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
1.650 au
e
0.5340
i
3.58°
Ω
267.00°
ω
217.00°
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).
60P/Tsuchinshan
60P · 2026-09-14 18:27:54 UTC → current
Discoverer · parsed-name · 2026-09-14 18:27:54 UTC → current
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CCD Observer · LEH02 · 13 reports · last 2699d ago
Visual Observer · HAL · 12 reports · last 10024d ago
CCD Observer · HIL04 · 12 reports · last 2665d ago
Visual Observer · BIV · 9 reports · last 2753d ago
CCD Observer · FRI02 · 9 reports · last 2697d ago
CCD Observer · NAK01 · 8 reports · last 10026d ago
Visual Observer · WYA · 8 reports · last 2721d ago
CCD Observer · NOV01 · 7 reports · last 2812d ago
Visual Observer · SCH19 · 6 reports · last 2720d ago
CCD Observer · WAR01 · 4 reports · last 2698d ago
Visual Observer · LEH · 4 reports · last 10050d ago
CCD Observer · YOS04 · 4 reports · last 10042d ago
Seiichi Yoshida and KenIchi Kadota
CCD Observer · YOS05 · 4 reports · last 10042d ago
Visual Observer · HAR11 · 3 reports · last 2759d ago
Visual Observer · DIJ · 3 reports · last 2759d ago
CCD Observer · YOS02 · 3 reports · last 2755d ago
Visual Observer · SAR02 · 3 reports · last 10051d ago
CCD Observer · TSU02 · 3 reports · last 2691d ago
CCD Observer · PAU02 · 3 reports · last 2746d ago
Visual Observer · HAS02 · 3 reports · last 2729d ago
CCD Observer · PAR03 · 2 reports · last 2756d ago
Visual Observer · CAM03 · 2 reports · last 2752d ago
Visual Observer · GUZ · 2 reports · last 2759d ago
Visual Observer · SZA · 2 reports · last 2797d ago
Visual Observer · YOS04 · 2 reports · last 2811d ago
Visual Observer · PEA · 1 reports · last 10075d ago
CCD Observer · HAD02 · 1 reports · last 2708d ago
CCD Observer · SRB · 1 reports · last 7538d ago
Visual Observer · GON05 · 1 reports · last 2835d ago
Visual Observer · HOR02 · 1 reports · last 10085d ago
CCD Observer · SHU · 1 reports · last 2918d ago
CCD Observer · PRY01 · 1 reports · last 2778d ago
Visual Observer · KAR02 · 1 reports · last 2750d ago
CCD Observer · KUT · 1 reports · last 2862d ago
CCD Observer · OHS · 1 reports · last 7596d ago
Pips are observation weight on this object (log of report count). Hover for catalog-wide weight.