C/2020 S3
Not currently visible. Last report 1784 days ago at mag 29.5. Historic peak was mag 3.9. 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
29.5
Professional survey · COBS consensus
Confidence
33
Class E · priority 60
Observations
251
Arc unknown
Last observation
1784d ago
Thu, 28 Oct 2021 20:09:35 GMT · COBS consensus
Perihelion
2020-12-11
0.391 au
Peak window
2020-12-08 → 2020-12-14
COBS peak mag 3.9 on 2020-12-11 · perihelion 2020-12-11. Window is those dates ±3 days — not a light-curve fit.
Historic peak
3.9
COBS / analyzed peak 2020-12-11
Catalog ingest
2d ago
Venator last wrote this row 2026-09-14 20:00:20 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
0.391 au
e
0.9970
i
20.10°
Ω
222.00°
ω
350.00°
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).
C/2020 S3 (Erasmus)
Informal: Erasmus
C/2020 S3 · 2026-09-14 18:28:00 UTC → current
Discoverer · parsed-name · 2026-09-14 18:28:00 UTC → current
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Jose Guilherme de Souza Aguiar
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Visual Observer · CAM03 · 14 reports · last 2118d ago
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Visual Observer · GET · 10 reports · last 2131d ago
CCD Observer · LEH02 · 10 reports · last 1784d ago
Visual Observer · MAT08 · 9 reports · last 2114d ago
Visual Observer · WOL01 · 8 reports · last 2119d ago
Visual Observer · GON05 · 8 reports · last 2119d ago
Visual Observer · AMO01 · 6 reports · last 2123d ago
CCD Observer · CAR06 · 6 reports · last 1856d ago
CCD Observer · HAR10 · 5 reports · last 2125d ago
CCD Observer · HIL04 · 5 reports · last 1843d ago
Visual Observer · PEA · 4 reports · last 2122d ago
CCD Observer · HER02 · 4 reports · last 1842d ago
Visual Observer · YOS02 · 4 reports · last 2119d ago
Visual Observer · TSU02 · 4 reports · last 2123d ago
CCD Observer · CAR09 · 4 reports · last 2128d ago
CCD Observer · FRI02 · 4 reports · last 2140d ago
CCD Observer · NOV01 · 3 reports · last 2157d ago
Visual Observer · DIJ · 3 reports · last 2124d ago
CCD Observer · PAP04 · 3 reports · last 1813d ago
Visual Observer · AIK · 3 reports · last 2125d ago
Visual Observer · YOS04 · 3 reports · last 2125d ago
Visual Observer · MOR03 · 3 reports · last 2138d ago
Visual Observer · NOV01 · 2 reports · last 2118d ago
Visual Observer · GUO · 2 reports · last 2112d ago
Visual Observer · WYA · 2 reports · last 2131d ago
CCD Observer · BUI01 · 2 reports · last 2151d ago
Visual Observer · MEY · 2 reports · last 2154d ago
Visual Observer · GUT · 2 reports · last 2127d ago
Visual Observer · SZA · 2 reports · last 2125d ago
Visual Observer · LAB02 · 1 reports · last 2130d ago
Visual Observer · HAR11 · 1 reports · last 2142d ago
Visual Observer · BIE02 · 1 reports · last 2126d ago
1–40 of 46
Pips are observation weight on this object (log of report count). Hover for catalog-wide weight.