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Recent photometric surveys of Trans-Neptunian Objects (TNOs) have revealed that the cold classical TNOs have distinct z-band color characteristics, and occupy their own distinct surface class. This suggested the presence of an absorption…

Earth and Planetary Astrophysics · Physics 2021-02-18 Tom Seccull , Wesley C. Fraser , Thomas H. Puzia

Using data from the Infrared Array Camera on the Spitzer Space Telescope, we present photometric observations of a sample of 100 trans-Neptunian objects (TNOs) beyond 2.2 {\mu}m. These observations, collected with two broad-band filters…

Near-Earth objects (NEOs) are excellent laboratories for testing processes that affect airless bodies, as well as informing us about Solar System history. Though most NEOs are nominally anhydrous because they formed inside the Solar System…

Earth and Planetary Astrophysics · Physics 2026-02-03 Lauren McGraw , Cristina Thomas , Josh Emery , Andy Rivkin

We report complete near-infrared (0.9-2.4 $\mu$m) spectral observations of trans-neptunian objects (TNOs) 2000 EB173 and 2000 WR106 collected using the new Near Infrared Camera Spectrometer (NICS) attached to the 3.56m Telescopio Nazionale…

Astrophysics · Physics 2009-11-06 J. Licandro , E. Oliva , M. Di MArtino

The recent discovery of two large trans-Neptunian objects (TNOs) 2003 UB313 and 2005 FY9, with surface properties similar to those of Pluto, provides an exciting new laboratory for the study of processes considered for Pluto and Triton:…

Astrophysics · Physics 2009-11-11 J. Licandro , W. M. Grundy , N. Pinilla-Alonso , J. de Leon

We present the first photometric observations of trans-Neptunian objects (TNOs) taken with the Kepler space telescope, obtained in the course of the K2 ecliptic survey. Two faint objects have been monitored in specifically designed pixel…

Earth and Planetary Astrophysics · Physics 2015-05-27 A. Pál , R. Szabó , Gy. M. Szabó , L. L. Kiss , L. Molnár , K. Sárneczky , Cs. Kiss

The thermal emission of transneptunian objects (TNO) and Centaurs has been observed at mid- and far-infrared wavelengths - with the biggest contributions coming from the Spitzer and Herschel space observatories-, and the brightest ones also…

Earth and Planetary Astrophysics · Physics 2020-01-22 Thomas Müller , Emmanuel Lellouch , Sonia Fornasier

We introduce a novel search technique that can identify trans-neptunian objects in three to five exposures of a pointing within a single Hubble Space Telescope orbit. The process is fast enough to allow the discovery of candidates soon…

Earth and Planetary Astrophysics · Physics 2015-05-19 Cesar I. Fuentes , Matthew J. Holman , David E. Trilling , Pavlos Protopapas

Trans-Neptunian objects (TNOs) contain the most primitive and thermally least-processed materials from the early accretional phase of the solar system. They allow us to study interrelations between various classes of small bodies, their…

Astrophysics · Physics 2009-11-13 S. Bagnulo , I. Belskaya , K. Muinonen , G. P. Tozzi , M. A. Barucci , L. Kolokolova , S. Fornasier

Trans-Neptunian objects (TNO) represent the leftovers of the formation of the Solar System. Their physical properties provide constraints to the models of formation and evolution of the various dynamical classes of objects in the outer…

We present a pipeline for searching for trans-Neptunian objects (TNOs) using data from the TESS mission, that includes a novel optimization-based framework for subtracting the effects of scattered light and pointing jitter. The background…

Earth and Planetary Astrophysics · Physics 2022-09-21 Varun Ganapathi

Models of the Solar System's dynamical evolution predict the dispersal of primitive planetesimals from their formative regions amongst the gas-giant planets due to the early phases of planetary migration. Consequently, carbonaceous objects…

Earth and Planetary Astrophysics · Physics 2018-03-28 Tom Seccull , Wesley C. Fraser , Thomas H. Puzia , Michael E. Brown , Frederik Schoenebeck

Reflection spectroscopy in the Near Infrared (NIR) is used to investigate the surface composition of Trans-Neptunian objects (TNOs). In general, these spectra are difficult to interpret due to the low apparent brightness of the TNOs,…

Earth and Planetary Astrophysics · Physics 2018-07-11 Ana Carolina Souza-Feliciano , Alvaro Alvarez-Candal , Yolanda Jiménez-Teja

Physical characterization of Trans-Neptunian objects, a primitive population of the outer solar system, may provide constraints on their formation and evolution. The goal of this work is to characterize a set of 15 scattered disk (SDOs) and…

We present a measurement of H2O ice crystallinity on the surface of trans-neptunian objects (TNOs) with near-infrared narrow-band imaging. The newly developed photometric technique allows us to efficiently determine the strength of an…

Earth and Planetary Astrophysics · Physics 2016-08-17 Tsuyoshi Terai , Yoichi Itoh , Yumiko Oasa , Reiko Furusho , Junichi Watanabe

We present our latest results about the short-term variability of trans-Neptunian objects (TNOs). We performed broad-band CCD photometric observations using several telescopes in Spain and Chile. We present results based on three years of…

Earth and Planetary Astrophysics · Physics 2015-06-05 A. Thirouin , J. L. Ortiz , A. Campo Bagatin , P. Pravec , N. Morales , O. Hainaut , R. Duffard

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…

Trans-Neptunian objects (TNOs) in the outer Solar System are predominantly small, icy worlds long presumed to be atmosphereless except for the largest bodies. Until now, Pluto has been unique among TNOs in exhibiting a substantial…

Earth and Planetary Astrophysics · Physics 2026-05-05 Ko Arimatsu , Fumi Yoshida , Tsutomu Hayamizu , Satoshi Takita , Katsumasa Hosoi , Takafumi Ootsubo , Jun-ichi Watanabe

Context: The recent discovery of a group of trans-neptunian objects (TNOs) in a narrow region of the orbital parameter space and with surfaces composed of almost pure water ice, being 2003 EL61 its largest member, promises new and…

Astrophysics · Physics 2009-11-13 N. Pinilla-Alonso , J. Licandro , V. Lorenzi
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