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Related papers: Pencil-Beam Surveys for Trans-Neptunian Objects: L…

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The census of solar neighbours is still complemented by new discoveries, mainly of very low-mass, faint dwarfs, close to or within the substellar domain. These discoveries contribute to a better understanding of the field population; its…

Solar and Stellar Astrophysics · Physics 2016-04-13 G. Bihain , R. -D. Scholz

Trans-Neptunian objects (TNOs) with large perihelion distances ($q > 60$ au) and semi-major axes ($a > 200$ au) provide insights into the early evolution of the solar system and the existence of a hypothetical distant planet. These objects…

We present observations of 32 primarily bright, newly discovered Transneptunian objects observable from the Southern Hemisphere during 39 nights of observation with the 2.5-m telescope at Las Campanas Observatory. Our dataset includes…

Earth and Planetary Astrophysics · Physics 2015-06-12 Susan D. Benecchi , Scott S. Sheppard

The recently discovered population of interstellar objects presents us with the opportunity to characterize material from extrasolar planetary and stellar systems up close. The forthcoming Vera C. Rubin Observatory Legacy Survey of Space…

Earth and Planetary Astrophysics · Physics 2022-02-01 Devin J. Hoover , Darryl Z. Seligman , Matthew J. Payne

We have discovered a large number of circular and elliptical shells at 24 microns around luminous central sources with the MIPS instrument on-board the Spitzer Space Telescope. Our archival follow-up effort has revealed 90% of these…

Astrophysics of Galaxies · Physics 2015-05-18 S. Wachter , J. C. Mauerhan , S. D. Van Dyk , D. W. Hoard , S. Kafka , P. W. Morris

Through a semi-analytic approach of the Kozai resonance inside an MMR, we show phase diagrams (e,{\omega}) that suggest the possibility of a scattered particle, after being captured in an MMR with Neptune, to become a detached object. We…

Earth and Planetary Astrophysics · Physics 2014-05-14 P. I. O. Brasil , R. S. Gomes , J. S. Soares

Determining the distribution and spectral signature of volatile ices and organics exposed on icy body surfaces can provide crucial clues for deciphering how the outer solar system formed and evolved. Over the past few decades, ground- and…

Earth and Planetary Astrophysics · Physics 2019-03-20 Richard J. Cartwright , Bryan Holler , Susan Benecchi , Roser Juanola-Parramon , Giada Arney , Aki Roberge , Heidi Hammel

The accumulating, but small, set of large semi-major axis trans-Neptunian objects (TNOs) shows an apparent clustering in the orientations of their orbits. This clustering must either be representative of the intrinsic distribution of these…

Due to the effects of gravitational lensing, the magnification distribution of high redshift supenovae can be a powerful discriminator between smooth dark matter and dark matter consisting of compact objects. We use high resolution N-body…

Astrophysics · Physics 2007-05-23 Uros Seljak , Daniel E. Holz

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…

(Abridged) Thirty-three objects with possible origins beyond the Kuiper Belt edge, very high inclinations, very large semi-major axes or large perihelion distances were observed to determine their surface colors. All three objects that have…

Earth and Planetary Astrophysics · Physics 2015-05-18 Scott S. Sheppard

The Neptune Trojans are the most recently discovered population of small bodies in the Solar System. To date, only eight have been discovered, though it is thought likely that the total population at least rivals that of the asteroid belt.…

Earth and Planetary Astrophysics · Physics 2012-03-02 Jonathan Horner , Patryk Sofia Lykawka

We discuss two new observational techniques that use observations of the Cosmic Microwave Background (CMB) to place constraints upon the mass, distance, and size distribution of small objects in the Kuiper Belt and inner Oort Cloud,…

Astrophysics · Physics 2009-11-13 Daniel Babich , Cullen H. Blake , Charles Steinhardt

Trans-Neptunian objects (TNOs) are remnants of a collisionally and dynamically evolved planetesimal disk in the outer solar system. This complex structure, known as the trans-Neptunian belt (or Edgeworth-Kuiper belt), can reveal important…

Astrophysics · Physics 2010-11-11 Patryk Sofia Lykawka , Tadashi Mukai

New data on the distribution of distant trans-Neptunian objects and on the properties of comets indicate the importance of dynamical processes in the outer part of the protoplanetary disk in the formation of the observed structure of the…

Earth and Planetary Astrophysics · Physics 2020-04-08 V. V. Emel'yanenko

The spiral structure in the Solar neighborhood is an important issue in astronomy. In the past few years, there is significant progress in observation. The distances for a large number of good spiral tracers, i.e. giant molecular clouds,…

Astrophysics of Galaxies · Physics 2021-10-12 L. G. Hou

The solar system's distant reaches exhibit a wealth of anomalous dynamical structure, hinting at the presence of a yet-undetected, massive trans-Neptunian body - Planet 9. Previous analyses have shown how orbital evolution induced by this…

Earth and Planetary Astrophysics · Physics 2024-04-18 Konstantin Batygin , Alessandro Morbidelli , Michael E. Brown , David Nesvorny

The study of planets beyond the solar system and the search for other habitable planets and life is just beginning. Ground-based (radial velocity and transits) and space-based surveys (transits and astrometry) will identify planets spanning…

The inverse square law of gravity is poorly probed by experimental tests at distances of ~ 10 AUs. Recent analysis of the trajectory of the Pioneer 10 and 11 spacecraft have shown an unmodeled acceleration directed toward the Sun which was…

Astrophysics · Physics 2009-06-23 John F. Wallin , David S. Dixon , Gary L. Page

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…