Periodic Comets Codexery

111P/Helin–Roman–Crockett

An Encke-type comet that temporarily orbits Jupiter.

111P/Helin–Roman–Crockett

111P/Helin–Roman–Crockett is an Encke-type comet that orbits the Sun once every 8.46 years. It was discovered on 5 January 1989 by Eleanor and Ron Helin, Brian P. Roman, and Randy L. Crockett, based on images taken about one to two days earlier.

The comet is known for its extremely close approaches to Jupiter, during which it temporarily orbits the planet, classifying it as a quasi-Hilda comet. Its last such approach occurred in 1976, and the next is predicted for 2071. While orbiting Jupiter, the comet follows a highly elliptical path, and at its farthest point from Jupiter (apojove), strong solar gravitational perturbations eventually pull it out of Jovian orbit, restarting the cycle. Simulations indicate this cycle is unstable; the comet will either be captured into an encounter orbit—similar to Shoemaker–Levy 9—or be expelled into a new orbit without periodic approaches. This suggests that 111P’s current orbital configuration is only a few thousand years old.

Estimates from 2004 place the comet’s nucleus at roughly 1.2 km (0.75 mi) in diameter. Follow-up studies in 2007 generally agree, though depending on the comet’s activity, the true diameter likely falls between 0.92 and 2.78 km (0.57–1.73 mi).

Quick Facts

Discovery Ref
IAUC_4701
Discoverer
Eleanor F. Helin · Ron Helin · Brian P. Roman · Randy L. Crockett
Discovery Site
Palomar Observatory (675)
Discovery Date
5 January 1989
Mpc Name
P/1989 A2
Designations
1988 XIII, 1989bICQ1
Orbit Ref
jpldata · MPC
Epoch
25 February 2023 (JD 2460000.5)
Earliest Precovery Date
2 January 1989
Obs
152
Perihelion
3.707 AU
Aphelion
4.595 AU

Facts from the source article.

Lore & Background

Comet Helin–Roman–Crockett was co-discovered by Eleanor and Ron Helin, Brian P. Roman and Randy L. Crockett on 5 January 1989 from images obtained about 1-2 days prior. It is known for making extremely close approaches to Jupiter, being a quasi-Hilda comet. During these approaches, it actually orbits Jupiter. The last such approach was in 1976, the next will be in 2071. The Jovian orbits are highly elliptical and subject to intense Solar perturbation at apojove, which eventually pulls the comet out of Jovian orbit for the cycle to begin anew.

Simulations predict such a cycle is unstable; the object will either be captured into an encounter orbit (e.g., Shoemaker-Levy 9) or expelled into a new orbit which does not have periodic approaches. This implies that 111P's orbit is recent within the past few thousand years. Estimates for the size of its nucleus in 2004 place it roughly about 1.2 km in diameter. Follow-up studies in 2007 generally agree with this estimate, and depending on the comet's activity, the comet is likely somewhere between 0.92–2.78 km in diameter.

Reader's Guide

111P/Helin–Roman–Crockett is significant as an Encke-type comet that exhibits a rare dynamical behavior: it makes extremely close approaches to Jupiter and temporarily enters Jovian orbit as a quasi-Hilda comet. The article describes that during these approaches, the comet actually orbits Jupiter, with the last such event in 1976 and the next predicted for 2071. The Jovian orbits are highly elliptical and subject to intense Solar perturbation at apojove, which eventually pulls the comet out of Jovian orbit, restarting the cycle. Simulations indicate this cycle is unstable, leading to two possible fates: capture into an encounter orbit similar to Shoemaker-Levy 9, or expulsion into a new orbit without periodic approaches. This instability implies that the comet's current orbit is recent, within the past few thousand years. The comet's nucleus size estimates from 2004 and 2007 provide a range of 0.92–2.78 km in diameter, with a central value of about 1.2 km, though the exact size depends on the comet's activity level. These characteristics make 111P a valuable object for studying cometary dynamics and interactions with giant planets.

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