1999/05/31 by Eugene Chiang, E. I. Chiang, Michael E. Brown +1 · 4 citations
Physics and Astronomy · #Astro and Planetary Science #Planetary Science and Exploration #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1086/301005
Accepted to AJ. Final proof-edited version: references added, discussion of G98 revised in sections 4.3 and 5.1
arxiv created 1999/07/24 · openalex publication_date 1999/09/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31
We present the results of a pencil-beam survey of the Kuiper Belt using the Keck 10 m telescope. A single 0.01 deg 2 field is imaged 29 times for a total integration time of 4.8 hr. Combining exposures in software allows the detection of Kuiper Belt objects (KBOs) having visual magnitude m V ≲ 27.9. Two new KBOs are discovered. One object having m V = 25.5 lies at a probable heliocentric distance R ≈ 33 AU. The second object at m V = 27.2 is located at R ≈ 44 AU. Both KBOs have diameters of about 50 km, assuming comet-like albedos of 4%. Data from all surveys are pooled to construct the luminosity function from m R = 20 to 27. The cumulative number of objects per square degree, Σ(< m R ), is fitted to a power law of the form Σ = α( m R - 23.5), where the slope α = 0.52 ± 0.02. Differences between slopes reported in the literature are due mainly to which survey data are incorporated in the fit and not to the method of analysis. The luminosity function is consistent with a power-law size distribution for objects having diameters s = 50–500 km within 50 AU; dN ∝ s - q ds , where the differential size index q = 3.6 ± 0.1. We estimate to order of magnitude that 0.2 M ⊕ and 1 × 10 10 comet progenitors lie between 30 and 50 AU. Though our inferred size index nearly matches that derived by Dohnanyi, it is unknown whether catastrophic collisions are responsible for shaping the size distribution. Impact strengths may increase strongly with size from 50 to 500 km, whereas the derivation by Dohnanyi assumes impact strength to be independent of size. Collisional lifetimes of KBOs having diameters 50–500 km exceed the age of the solar system by at least 2 orders of magnitude in the present-day Belt, assuming bodies consist of solid, cohesive rock. Implications of the absence of detections of classical KBOs beyond 50 AU are discussed.