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P/2015 D5

P/2015 D5 (Kowalski)

CometClass Ecatalogued
Unknown

Not currently visible. Last report 4115 days ago at mag 25.8. Historic peak was mag 18.4. 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

25.8

Professional survey · COBS consensus

Confidence

33

Class E · priority 60

Observations

1

Arc unknown

Last observation

4115d ago

Fri, 12 Jun 2015 12:14:23 GMT · COBS consensus

Perihelion

2014-04-14

4.540 au

Peak window

2014-01-03 → 2014-04-17

COBS peak mag 18.4 on 2014-01-06 · perihelion 2014-04-14. Window is those dates ±3 days — not a light-curve fit.

Historic peak

18.4

COBS / analyzed peak 2014-01-06

Catalog ingest

13h ago

Venator last wrote this row 2026-09-16 13:20:17 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

4.540 au

e

0.4920

i

20.50°

Ω

74.10°

ω

39.70°

a

MOID

H

H0 / n

NEO score

PHA score

RMS

Elongation

Reporting sources

  • COBS comet list

    down

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

Name history

  • P/2015 D5 (Kowalski)

    Informal: Kowalski

    P/2015 D5 · 2026-09-14 18:27:56 UTC → current

Discoverers

  • Kowalski

    Discoverer · parsed-name · 2026-09-14 18:27:56 UTC → current

Contributors

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