61P
Not currently visible. Last report 1281 days ago at mag 27.8. Historic peak was mag 14.5. 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
27.8
Professional survey · COBS consensus
Confidence
33
Class E · priority 60
Observations
153
Arc unknown
Last observation
1281d ago
Wed, 15 Mar 2023 20:52:47 GMT · COBS consensus
Perihelion
2029-11-25
2.130 au
Peak window
2022-10-13 → 2029-11-28
COBS peak mag 14.5 on 2022-10-16 · perihelion 2029-11-25. Window is those dates ±3 days — not a light-curve fit.
Historic peak
14.5
COBS / analyzed peak 2022-10-16
Catalog ingest
12h ago
Venator last wrote this row 2026-09-16 13:20:15 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
2.130 au
e
0.4230
i
5.99°
Ω
163.00°
ω
222.00°
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).
61P/Shajn-Schaldach
61P · 2026-09-14 18:27:52 UTC → current
Discoverer · parsed-name · 2026-09-14 18:27:52 UTC → current
Visual Observer · SCO01 · 19 reports · last 11907d ago
CCD Observer · HIL04 · 19 reports · last 1281d ago
Visual Observer · BEY · 12 reports · last 28058d ago
CCD Observer · FRI02 · 12 reports · last 1374d ago
Visual Observer · NAK01 · 11 reports · last 11915d ago
CCD Observer · CAR06 · 8 reports · last 1350d ago
CCD Observer · LEH02 · 7 reports · last 1369d ago
CCD Observer · YOS02 · 6 reports · last 1399d ago
CCD Observer · DEK01 · 6 reports · last 1371d ago
CCD Observer · NAK01 · 5 reports · last 9062d ago
CCD Observer · TSU02 · 5 reports · last 3914d ago
CCD Observer · PRY01 · 5 reports · last 3998d ago
CCD Observer · MAS01 · 4 reports · last 1431d ago
CCD Observer · BUI01 · 3 reports · last 1403d ago
CCD Observer · PAP04 · 3 reports · last 1430d ago
CCD Observer · SHU · 3 reports · last 3928d ago
Visual Observer · HAL · 2 reports · last 11964d ago
Visual Observer · MOR · 2 reports · last 12051d ago
CCD Observer · DEM03 · 2 reports · last 1403d ago
CCD Observer · MAI01 · 2 reports · last 1469d ago
Visual Observer · JAE · 2 reports · last 1430d ago
Visual Observer · MOD · 2 reports · last 12026d ago
Visual Observer · SZA · 2 reports · last 3962d ago
Visual Observer · BAR06 · 1 reports · last 6448d ago
CCD Observer · PEA · 1 reports · last 17577d ago
CCD Observer · HER02 · 1 reports · last 9598d ago
Visual Observer · WYA · 1 reports · last 1394d ago
CCD Observer · DEM · 1 reports · last 1420d ago
Visual Observer · GON05 · 1 reports · last 6524d ago
Visual Observer · MAR28 · 1 reports · last 6511d ago
Visual Observer · PAR03 · 1 reports · last 6621d ago
CCD Observer · LIV01 · 1 reports · last 1422d ago
Visual Observer · PRA01 · 1 reports · last 12050d ago
CCD Observer · CAR09 · 1 reports · last 1350d ago
Visual Observer · YOS04 · 1 reports · last 6529d ago
Visual Observer · SHU · 1 reports · last 4016d ago
Pips are observation weight on this object (log of report count). Hover for catalog-wide weight.