Back to Contributors

C/1988 A1

C/1988 A1 (Liller)

CometClass Ecatalogued
Unknown

Not currently visible. Last report 13915 days ago at mag 33.2. Historic peak was mag 6.5. 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

33.2

Professional survey · COBS consensus

Confidence

33

Class E · priority 60

Observations

1156

Arc unknown

Last observation

13915d ago

Fri, 12 Aug 1988 04:19:11 GMT · COBS consensus

Perihelion

1988-04-13

0.818 au

Peak window

1988-04-10 → 1988-04-16

COBS peak mag 6.5 on 1988-04-13 · perihelion 1988-04-13. Window is those dates ±3 days — not a light-curve fit.

Historic peak

6.5

COBS / analyzed peak 1988-04-13

Catalog ingest

9h ago

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

0.818 au

e

0.9970

i

73.70°

Ω

31.90°

ω

57.10°

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

  • C/1988 A1 (Liller)

    Informal: Liller

    C/1988 A1 · 2026-09-14 18:27:55 UTC → current

Discoverers

  • Liller

    Discoverer · parsed-name · 2026-09-14 18:27:55 UTC → current

Contributors

140 of 145

1 / 4

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