Resonance Occupation in the Kuiper Belt: Case Examples of the 5:2 and Trojan Resonances

Details Resonance Occupation in the Kuiper Belt: Case Examples of the 5:2 and Trojan Resonances Resonance Occupation in the Kuiper Belt: Case Examples of the 5:2 and Trojan Resonances

2003-01-22

arxiv.org/abs/astro-ph/0301458v3

Astron.J. 126 (2003) 430

Astronomy and Astrophysics

Astrophysics

Accepted to AJ, final version, contains list of names of all resonant KBOs known to humanity as of Feb 1 2003

Scientific paper

10.1086/375207

As part of our ongoing Deep Ecliptic Survey (DES) of the Kuiper belt, we report on the occupation of the 1:1 (Trojan), 4:3, 3:2, 7:4, 2:1, and 5:2 Neptunian mean-motion resonances (MMRs). The occupation of the 1:1 and 5:2 MMRs is not easily understood within the standard model of resonance sweeping by a migratory Neptune over an initially dynamically cold belt. Our dynamically hot, 5:2 resonant objects can librate with modest amplitudes of 90 deg within the resonance for at least 1 Gyr. Their trajectories cannot be explained by close encounters with Neptune alone, given the latter's current orbit. The hot orbits of such 5:2 resonant KBOs, unlike hot orbits of previously known resonant KBOs, may imply that these objects were pre-heated to large inclination and large eccentricity prior to resonance capture by a migratory Neptune. Our first discovered Neptunian Trojan, 2001QR322, may not owe its existence to Neptune's migration at all. The trajectory of 2001QR322 is remarkably stable; the object can undergo tadpole-type libration about Neptune's leading Lagrange (L4) point for at least 1 Gyr with a libration amplitude of 24 deg. Trojan capture probably occurred while Neptune accreted the bulk of its mass. For an assumed albedo of 12--4%, our Trojan is 130--230 km in diameter. Model-dependent estimates place the total number of Neptune Trojans resembling 2001QR322 at 20--60. Their existence might rule out violent orbital histories for Neptune.

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