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相关论文: De-biased Populations of Kuiper Belt Objects from …

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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…

地球与行星天体物理 · 物理学 2015-05-18 Amanda Gulbis , Jim Elliot , Elisabeth Adams , Susan Benecchi , Marc Buie , David Trilling , Larry Wasserman

We numerically integrated the orbits of 1458 particles in the region of the classical Kuiper Belt (41 AU < a < 47 AU) to explore the role of dynamical instabilities in sculpting the inclination distribution of the classical Kuiper Belt…

天体物理学 · 物理学 2009-11-07 Marc J. Kuchner , Michael E. Brown , Matthew Holman

About 2500 square degrees of sky south of declination -25 degrees and/or near the galactic plane were surveyed for bright outer solar system objects. This survey is one of the first large scale southern sky and galactic plane surveys to…

In the outer solar system, the Kuiper Belt contains dynamical sub-populations sculpted by a combination of planet formation and migration and gravitational perturbations from the present-day giant planet configuration. The subdivision of…

地球与行星天体物理 · 物理学 2020-07-09 Rachel A. Smullen , Kathryn Volk

The DECam Ecliptic Exploration Project (DEEP) is a deep survey of the trans-Neptunian solar system being carried out on the 4-meter Blanco telescope at Cerro Tololo Inter-American Observatory in Chile using the Dark Energy Camera (DECam).…

We report the orbital distribution of the trans-neptunian objects (TNOs) discovered during the Canada-France Ecliptic Plane Survey, whose discovery phase ran from early 2003 until early 2007. The follow-up observations started just after…

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…

地球与行星天体物理 · 物理学 2015-05-19 Wesley C. Fraser , Michael E. Brown , Megan E. Schwamb

We present a survey for bright Kuiper Belt Objects (KBOs) and Centaurs, conducted at the Kitt Peak National Observatory (KPNO) 0.9 m telescope with the KPNO 8k Mosaic CCD. The survey imaged 164 sq deg near opposition to a limiting red…

天体物理学 · 物理学 2009-11-07 Chadwick A. Trujillo , Jane X. Luu , Amanda S. Bosh , James L. Elliot

We report the statistical detection (at the >99% confidence level) of a population of 28th magnitude objects exhibiting proper motions of ~1 arcsecond per hour at quadrature in deep HST/WFPC2 images. The drift directions imply a…

天体物理学 · 物理学 2009-10-28 Anita L. Cochran , Harold F. Levison , S. Alan Stern , Martin J. Duncan

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…

天体物理学 · 物理学 2009-11-06 Chadwick A. Trujillo , David C. Jewitt , Jane X. Luu

In this paper, we present the most comprehensive study to date on Neptune's mean-motion resonances (MMRs) in the distant Kuiper belt from 50 to 100 AU. Over 200 resonant Kuiper belt objects (KBOs) have been identified in this region,…

地球与行星天体物理 · 物理学 2026-01-22 Jian Li

We have started since 1997 the Meudon Multicolor Survey of Outer Solar System Objects with the aim of collecting a large and homogeneous set of color data for Trans-Neptunian and Centaurs objects [...] We have a combined sample of 52 B-R…

天体物理学 · 物理学 2009-11-07 A. Doressoundiram , N. Peixinho , C. de Bergh , S. Fornasier , Ph. Thebault , M. A. Barucci , C. Veillet

(Abridged) New optical colors of 58 objects in mean motion resonances with Neptune show the various resonant populations have significantly different color distributions. The 5:3 and 7:4 resonances have semi-major axes near the middle of…

地球与行星天体物理 · 物理学 2015-06-11 Scott S. Sheppard

The Kuiper belt includes tens of thousands of large bodies and millions of smaller objects. The main part of the belt objects is located in the annular zone between 39.4 au and 47.8 au from the Sun, the boundaries correspond to the average…

地球与行星天体物理 · 物理学 2018-10-24 E. V. Pitjeva , N. P. Pitjev

We numerically investigate the possibility that a close stellar encounter could account for the high inclinations of the Kuiper belt, as originally proposed by Ida, Larwood and Burkert, however we consider encounters with pericenters within…

天体物理学 · 物理学 2007-05-23 Alice C. Quillen , David E. Trilling , Eric G. Blackman

Here we measure the absolute magnitude distributions (H-distribution) of the dynamically excited and quiescent (hot and cold) Kuiper Belt objects (KBOs), and test if they share the same H-distribution as the Jupiter Trojans. From a…

地球与行星天体物理 · 物理学 2015-06-18 Wesley C. Fraser , Michael E. Brown , Alessandro Morbidelli , Alex Parker , Konstantin Batygin

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…

地球与行星天体物理 · 物理学 2013-02-01 C. Shankman , B. Gladman , N. Kaib , J. J. Kavelaars , J. -M. Petit

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…

天体物理学 · 物理学 2009-10-31 H. F. Levison , S. A. Stern

A modified Baker-Nunn camera was used to conduct a wide-field survey of 1428 square degrees of sky near the ecliptic in search of bright Kuiper Belt objects and Centaurs. This area is an order of magnitude larger than any previously…

天体物理学 · 物理学 2009-10-31 S. Sheppard , D. Jewitt , C. Trujillo , M. Brown , M. Ashley

We present the first set of trans-Neptunian objects (TNOs) observed on multiple nights in data taken from the DECam Ecliptic Exploration Project (DEEP). Of these 110 TNOs, 105 do not coincide with previously known TNOs and appear to be new…

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