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Related papers: The Absolute Magnitude Distribution of Kuiper Belt…

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We measure the absolute magnitude, $H$, distribution, $dN(H) \propto 10^{\alpha H}$ of the scattering Trans-Neptunian Objects (TNOs) as a proxy for their size-frequency distribution. We show that the H-distribution of the scattering TNOs is…

Earth and Planetary Astrophysics · Physics 2016-02-03 C. Shankman , J. J. Kavelaars , B. J. Gladman , M. Alexandersen , N. Kaib , J. -M. Petit , M. T. Bannister , Y. -T Chen , S. Gwyn , M. Jakubik , K. Volk

By examining the absolute magnitude (H) distributions (hereafter HD) of the cold and hot populations in the Kuiper belt and of the Trojans of Jupiter, we find evidence that the Trojans have been captured from the outer part of the…

Earth and Planetary Astrophysics · Physics 2009-03-06 Morbidelli Alessandro , Harold F. Levison , William Bottke , Luke Dones , David Nesvorny

We conducted a two-night photometric survey of small Kuiper Belt objects (KBOs) near opposition using the wide-field Hyper Suprime-Cam instrument on the 8.2 m Subaru Telescope. The survey covered about 90 deg^2 of sky, with each field…

Earth and Planetary Astrophysics · Physics 2017-03-15 Ian Wong , Michael E. Brown

Abridged. We have performed an ecliptic survey of the Kuiper belt, with an areal coverage of 8.9 square degrees to a 50% limiting magnitude of r'=24.7, and have detected 88 Kuiper belt objects, roughly half of which received follow-up one…

Earth and Planetary Astrophysics · Physics 2015-05-19 Wesley C. Fraser , Michael E. Brown , Megan E. Schwamb

Using the absolute detection calibration and abundant detections of the OSSOS (Outer Solar System Origin Survey) project, we provide population measurements for the main Kuiper Belt. For absolute magnitude $H_r<8.3$, there are 30,000…

Earth and Planetary Astrophysics · Physics 2023-09-06 Jean-Marc Petit , Brett Gladman , J. J. Kavelaars , Michele T. Bannister , Mike Alexandersen , Kathryn Volk , Ying-Tung Chen

Color measurements and albedo distributions introduce non-intuitive observational biases in size-color relationships among Kuiper Belt Objects (KBOs) that cannot be disentangled without a well characterized sample population with systematic…

Earth and Planetary Astrophysics · Physics 2015-06-16 R. E. Pike , J. J. Kavelaars

We describe analytical and numerical collisional evolution calculations for the size distribution of icy bodies in the Kuiper Belt. For a wide range of bulk properties, initial masses, and orbital parameters, our results yield power-law…

Astrophysics · Physics 2009-11-10 Scott J. Kenyon , Benjamin C. Bromley

We present a new analysis of the currently available orbital elements for the known Kuiper belt objects. In the non-resonant, main Kuiper belt we find a statistically significant relationship between an object's absolute magnitude (H) and…

Astrophysics · Physics 2009-10-31 H. F. Levison , S. A. Stern

The Deep Ecliptic Survey (DES) discovered hundreds of Kuiper Belt objects from 1998-2005. Follow-up observations yielded 304 objects with good dynamical classifications (Classical, Scattered, Centaur, or 16 mean-motion resonances with…

Earth and Planetary Astrophysics · Physics 2015-06-17 E. R. Adams , A. A. S. Gulbis , J. L. Elliot , S. D. Benecchi , M. W. Buie , D. E. Trilling , L. H. Wasserman

The Hilda population of asteroids is located in a large orbital zone of long-term stability associated with the Jupiter J3/2 mean motion resonance. They are a sister population of the Jupiter Trojans, since both of them are likely made up…

Earth and Planetary Astrophysics · Physics 2025-03-07 David Vokrouhlický , David Nesvorný , Miroslav Brož , William F. Bottke , Rogerio Deienno , Carson D. Fuls , Frank C. Shelly

We present the results of a wide-field survey designed to measure the size, inclination, and radial distributions of Kuiper Belt Objects (KBOs). The survey found 86 KBOs in 73 square degrees observed to limiting red magnitude 23.7 using the…

Astrophysics · Physics 2009-11-06 Chadwick A. Trujillo , David C. Jewitt , Jane X. Luu

The cold main classical Kuiper Belt consists of those non-resonant small solar system bodies with low orbital inclinations and orbital semi-major axes between 42.4 and 47.7 au. These objects likely formed \textit{in situ} and the population…

We have performed a survey of the Kuiper belt covering ~ 1/3 a square degree of the sky using Suprime-cam on the Subaru telescope, to a limiting magnitude of m(R)~ 26.8 (50% threshold) and have found 36 new KBOs. We have confirmed that the…

Astrophysics · Physics 2009-11-13 W. C. Fraser , J. J. Kavelaars

This chapter reviews accretion models for Kuiper belt objects (KBOs), discussing in particular the compatibility of the observed properties of the KBO population with the streaming instability paradigm. Then it discusses how the dynamical…

Earth and Planetary Astrophysics · Physics 2020-01-22 Alessandro Morbidelli , David Nesvorny

The size distribution is determined directly from the current known Kuiper Belt Objects (KBOs). We found that there is a peak for the size distribution around 230 km in diameter. For the objects larger than 230 km, the KBOs populate as…

Astrophysics · Physics 2007-05-23 Cheng-Pin Chen , Ing-Guey Jiang

[Condensed] We search 0.02 deg^2 for trans-Neptunian objects (TNOs) with m<=29.2 (diameter ~15 km) using the ACS on HST. Three new objects are discovered, roughly 25 times fewer than expected from extrapolation of the differential sky…

Astrophysics · Physics 2009-11-10 G. M. Bernstein , D. E. Trilling , R. L. Allen , M. E. Brown , M. Holman , R. Malhotra

The classical Kuiper belt contains objects both from a low-inclination, presumably primordial, distribution and from a high-inclination dynamically excited population. Based on a sample of classical TNOs with observations at thermal…

We present observations of thermal emission from fifteen transneptunian objects (TNOs) made using the Spitzer Space Telescope. Thirteen of the targets are members of the Classical population: six dynamically hot Classicals, five dynamically…

Using data from the Deep Ecliptic Survey (DES), we investigate the inclination distributions of objects in the Kuiper Belt. We present a derivation for observational bias removal and use this procedure to generate unbiased inclination…

Earth and Planetary Astrophysics · Physics 2015-05-18 Amanda Gulbis , Jim Elliot , Elisabeth Adams , Susan Benecchi , Marc Buie , David Trilling , Larry Wasserman

Via joint analysis of a calibrated telescopic survey, which found scattering Kuiper Belt objects, and models of their expected orbital distribution, we measure the form of the scattering object's size distribution. Ruling out a single…

Earth and Planetary Astrophysics · Physics 2013-02-01 C. Shankman , B. Gladman , N. Kaib , J. J. Kavelaars , J. -M. Petit
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