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460P

460P/PANSTARRS

CometClass Ecatalogued
Unknown

Not currently visible. Last report 3814 days ago at mag 23.4. Historic peak was mag 21.9. Typical backyard telescopes will not show it. HST, JWST, or an 8–10 m class telescope might recover it with a good ephemeris.

Active comet in COBS

Right ascension

—

J2000

Declination

—

J2000

Estimated magnitude

23.4

Professional survey · COBS consensus

Confidence

33

Class E · priority 60

Observations

27

Arc unknown

Last observation

3814d ago

Sat, 28 May 2016 22:19:11 GMT · COBS consensus

Perihelion

2026-09-21

1.020 au

Peak window

2021-06-13 → 2026-09-24

COBS peak mag 21.9 on 2021-06-16 · perihelion 2026-09-21. Window is those dates ±3 days — not a light-curve fit.

Historic peak

21.9

COBS / analyzed peak 2021-06-16

Catalog ingest

13h ago

Venator last wrote this row 2026-11-06 14:20:24 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.

No tail measures stored yet for this object.

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

1.020 au

e

0.6640

i

18.90°

Ω

181.00°

ω

352.00°

a

—

MOID

—

H

—

H0 / n

—

NEO score

—

PHA score

—

RMS

—

Elongation

—

Reporting sources

  • COBS comet list

    ok

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

Name history

  • 460P/PANSTARRS

    460P · 2026-09-14 18:28:01 UTC → current

Discoverers

  • PANSTARRS

    Discoverer · parsed-name · 2026-09-14 18:28:01 UTC → current

Contributors

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