A quasi-Hilda comet (QHC) is a Jupiter-family comet that interacts strongly with Jupiter and undergoes extended temporary capture by it. These comets are associated with the Hilda asteroid zone in the 3:2 inner mean-motion resonance with Jupiter. Typically, asteroids in this zone have a semimajor axis between 3.70 and 4.20 AU, eccentricities below 0.30, and inclinations of no more than 20°.[1] Comets can be temporarily perturbed into this group and then perturbed back out again.[2] Eight percent of the comets that leave the 3:2 resonance end up impacting Jupiter.[1]
Known quasi-Hilda comets
These numbered comets belong to the group of quasi-Hilda comet:[1]
39P/Oterma was a quasi-Hilda before a close approach to Jupiter in 1963.[1]77P/Longmore falls outside of the bulk distribution because of its large eccentricity and inclination.[1]Comet Shoemaker–Levy 9 impacted with Jupiter in 1994.
^Spratt, Christopher E. (December 1989). "The Hilda group of minor planets". Journal of the Royal Astronomical Society of Canada. 83: 393–404. Bibcode:1989JRASC..83..393S.
^Chandler, Colin Orion; Oldroyd, William J.; Trujillo, Chadwick A.; Burris, William A.; Hsieh, Henry H.; Kueny, Jay K.; Farrell, Kennedy A.; DeSpain, Jarod A.; Sedaghat, Nima; Magbanua, Mark Jesus Mendoza; Sheppard, Scott S.; Mazzucato, Michele T.; Bosch, Milton K. D.; Shaw-Diaz, Tiffany; Gonano, Virgilio (November 2023). "New Active Quasi-Hilda Asteroid 2004 CV50: A Citizen Science Discovery". Research Notes of the AAS. 7 (11): 237. doi:10.3847/2515-5172/ad09c1. ISSN2515-5172.