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260P

260P/McNaught

CometClass Ecatalogued
Northern hemisphere

Difficult — CCD / large telescope. Around mag 15.0. A large amateur CCD or a professional telescope is required.

Active comet in COBS

Right ascension

06h 17m 04s

J2000

Declination

+50° 29′ 54″

J2000

Estimated magnitude

15.0

CCD / citizen telescope · COBS consensus

Confidence

33

Class E · priority 76

Observations

42

80.00 d arc

Last observation

26h ago

Fri, 06 Nov 2026 01:26:23 GMT · COBS consensus

Perihelion

2026-08-05

1.420 au

Peak window

2026-08-02 → 2026-08-08

COBS peak mag 15.1 on 2026-08-05 · perihelion 2026-08-05. Window is those dates ±3 days — not a light-curve fit.

Historic peak

15.1

COBS / analyzed peak 2026-08-05

Catalog ingest

3m ago

Venator last wrote this row 2026-11-07 03:00:09 UTC

Light curve

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.

Orbital elements

q

1.420 au

e

0.6090

i

15.00°

Ω

349.00°

ω

18.50°

a

3.620 au

MOID

—

H

—

H0 / n

14.4 / 1

NEO score

—

PHA score

—

RMS

—

Elongation

126°

Reporting sources

  • COBS comet list

    ok

    Comet Observation Database magnitudes and perihelion data for the full COBS list (active and inactive).

  • COBS orbits

    ok

    Osculating elements and photometric parameters (H0, n) for active comets.

Name history

  • 260P/McNaught

    260P · 2026-09-08 02:09:56 UTC → current

Discoverers

  • McNaught

    Discoverer · parsed-name · 2026-09-08 17:27:23 UTC → current

Contributors

Pips are observation weight on this object (log of report count). Hover for catalog-wide weight.