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Related papers: Trans-Neptunian objects and Centaurs at thermal wa…

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The trans-Neptunian objects (TNOs) are small Solar System bodies at large distances from the Sun. As such, their physical properties are difficult to measure. Accurate determination of their physical parameters is essential to model and…

Earth and Planetary Astrophysics · Physics 2018-09-05 C. Ayala-Loera , A. Alvarez-Candal , J. L. Ortiz , R. Duffard , E. Fernández-Valenzuela , P. Santos-Sanz , N. Morales

We report the rotational lightcurves of 21 trans-Neptunian objects (TNOs) in Neptune's 2:1 mean motion resonance obtained with the 6.5 m Magellan-Baade telescope and the 4.3 m Lowell Discovery Telescope. The main survey's goal is to find…

Earth and Planetary Astrophysics · Physics 2022-06-22 Audrey Thirouin , Scott S. Sheppard

The densities of mid-sized Kuiper belt objects are a key constraint into understanding the assembly of objects in the outer solar system. These objects are critical for understanding the currently unexplained transition from the smallest…

Earth and Planetary Astrophysics · Physics 2017-06-28 Michael E. Brown , Bryan J. Butler

A second large programme (LP) for the physical studies of TNOs and Centaurs, started at ESO Cerro Paranal on October 2006 to obtain high-quality data, has recently been concluded. In this paper we present the spectra of these pristine…

Earth and Planetary Astrophysics · Physics 2015-05-14 S. Fornasier , M. A. Barucci , C. de Bergh , A. Alvarez-Candal , F. DeMeo , F. Merlin , D. Perna , A. Guilbert , A. Delsanti , E. Dotto , A. Doressoundiram

Centaurs are objects whose orbits are found between those of the giant planets. They are supposed to originate mainly from the TransNeptunian objects, and they are among the sources of NearEarth Objects.TransNeptunian Objects (TNOs) cross…

Earth and Planetary Astrophysics · Physics 2016-11-18 Mattia Alvise Galiazzo , Paul Wiegert , Safwan Aljbaae

Asymmetric debris discs have been found around stars other than the Sun; asymmetries are sometimes attributed to perturbations induced by unseen planets. The presence or absence of asymmetries in our own trans-Neptunian belt remains…

Earth and Planetary Astrophysics · Physics 2022-03-01 C. de la Fuente Marcos , R. de la Fuente Marcos

The Trans-Neptunian Objects (TNOs) may preserve evidence of planet building in their orbital and size-distributions. While all populations show steep size-distributions for large objects, recently relative deficit of Neptunian Trojans and…

Earth and Planetary Astrophysics · Physics 2019-01-30 Mike Alexandersen , Brett Gladman , J. J. Kavelaars , Jean-Marc Petit , Stephen Gwyn , Cory Shankman

Recent observations (Burnes2002,Veillet2002,Margot2002a) have revealed an unexpectedly high binary fraction among the Trans-Neptunian Objects (TNOs) that populate the Kuiper Belt. The TNO binaries are strikingly different from asteroid…

Astrophysics · Physics 2007-05-23 Yoko Funato , Junichiro Makino , Piet Hut , Eiichiro Kokubo , Daisuke Kinoshita

Trans-Neptunian objects (TNOs) are among the most primitive remnants of the early Solar System, and constraining their sizes, shapes, albedos, and surface properties is essential for understanding their origin and evolution. Stellar…

Radio continuum observations trace thermal emission of ionized plasma in planetary nebulae and bring useful information on nebular geometries. A model of homogeneous sphere or shell cannot fit the nebular spectra and brightness…

We present a method to identify distant solar system objects in long-term wide-field asteroid survey data, and conduct a search for them in the Pan-STARRS1 (PS1) image data acquired from 2010 to mid-2015. We demonstrate that our method is…

Earth and Planetary Astrophysics · Physics 2016-07-19 R. J. Weryk , E. Lilly , S. Chastel , L. Denneau , R. Jedicke , E. Magnier , R. J. Wainscoat , K. Chambers , H. Flewelling , M. E. Huber , C. Waters , the PS1 Builders

The small solar-system bodies that reside between 30 and 50 AU are often referred to as the Trans Neptunian Objects, or TNOs. A far-infrared (FIR) mission with survey capabilities, like the prospective Cryogenic Aperture Large Infrared…

Earth and Planetary Astrophysics · Physics 2015-05-19 J. M. Bauer , P. F. Goldsmith , C. M. Bradford , A. J. Lovell

We present estimates of the basic physical properties -- including size and albedo -- of the extreme Centaur 2013 AZ60. These properties have been derived from optical and thermal infrared measurements. Our optical measurements revealed a…

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…

We describe the discovery circumstances and photometric properties of 2000 EB173, now one of the brightest trans-Neptunian objects (TNOs) with opposition magnitude m_R=18.9 and also one of the largest Plutinos, found with the drift-scanning…

Most known trans-Neptunian objects (TNOs) gravitationally scattering off the giant planets have orbital inclinations consistent with an origin from the classical Kuiper belt, but a small fraction of these "scattering TNOs" have inclinations…

Arcuate infrared nebulae are ubiquitous throughout the Galactic Plane and are candidates for partial shells, bubbles, or bowshocks produced by massive runaway stars. We tabulate infrared photometry for 709 such objects using images from the…

Both Centaurs and trans-Neptunian objects (TNOs) are minor bodies found in the outer Solar System. Centaurs are a transient population that moves between the orbits of Jupiter and Neptune, and they probably diffused out of the TNOs. TNOs…

Earth and Planetary Astrophysics · Physics 2016-06-06 Mattia Galiazzo , Carlos de la Fuente Marcos , Raul de la Fuente Marcos , Giovanni Carraro , Michele Maris , Marco Montalto

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…

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