Results 71 to 80 of about 2,093,691 (201)

Formation and Migration of Trans-Neptunian Objects [PDF]

open access: yesAIP Conference Proceedings, 2004
Trans-Neptunian objects (TNOs) with diameter d>100 km moving now in not very eccentric orbits could be formed directly by the compression of large rarefied dust condensations (with semi-major axes a>30 AU), but not by the accretion of smaller solid planetesimals.
openaire   +3 more sources

Advanced Techniques in Stability Analysis of Trans-Neptunian Objects

open access: yesUniverse
The trans-Neptunian region (30–50 AU) is a dynamically structured reservoir of icy planetesimals whose orbital architecture reflects resonant dynamics, chaotic transport, and long-term gravitational sculpting by the giant planets. This review synthesizes
Tamás Kovács
doaj   +1 more source

A Spiral Structure in the Inner Oort Cloud

open access: yesThe Astrophysical Journal
As the Galactic tide acts to decouple bodies from the scattered disk it creates a spiral structure in physical space that is roughly 15,000 au in length. The spiral is long-lived and persists in the inner Oort cloud to the present time.
David Nesvorný   +7 more
doaj   +1 more source

Photometry of Outer Solar System Objects from the Dark Energy Survey. I. Photometric Methods, Light-curve Distributions, and Trans-Neptunian Binaries

open access: yesThe Astrophysical Journal Supplement Series, 2023
We report the methods of and initial scientific inferences from the extraction of precision photometric information for the >800 trans-Neptunian objects (TNOs) discovered in the images of the Dark Energy Survey (DES). Scene-modeling photometry is used to
Pedro H. Bernardinelli   +53 more
doaj   +1 more source

Water‐Ice Dominated Spectra of Saturn's Rings and Small Moons From JWST

open access: yesJournal of Geophysical Research: Planets, Volume 129, Issue 3, March 2024.
Abstract JWST measured the infrared spectra of Saturn's rings and several of its small moons (Epimetheus, Pandora, Telesto, and Pallene) as part of Guaranteed Time Observation program 1247. The NIRSpec instrument obtained near‐infrared spectra of the small moons between 0.6 and 5.3 microns, which are all dominated by water‐ice absorption bands.
M. M. Hedman   +13 more
wiley   +1 more source

The dynamics of rings around Centaurs and Trans-Neptunian objects [PDF]

open access: yes, 2020
Chapter to be published in the book "The Transneptunian Solar System", Dina Prialnik, Maria Antonietta Barucci, Leslie Young Eds ...
Sicardy, Bruno   +6 more
openaire   +4 more sources

LiDO: Discovery of a 10:1 Resonator with a Novel Libration State

open access: yesThe Planetary Science Journal
The Large inclination Distant Objects (L i DO) survey has discovered the first securely classified object in the 10:1 mean motion resonance of Neptune.
Rosemary E. Pike   +11 more
doaj   +1 more source

OSSOS. VII. 800+ Trans-Neptunian Objects—The Complete Data Release [PDF]

open access: yes, 2018
The Outer Solar System Origins Survey (OSSOS), a wide-field imaging program in 2013–2017 with the Canada–France–Hawaii Telescope, surveyed 155 deg2 of sky to depths of m r = 24.1–25.2.
Susan D. Benecchi   +91 more
core   +1 more source

OSSOS. XXIX. The Population and Perihelion Distribution of the Detached Kuiper Belt

open access: yesThe Planetary Science Journal, 2023
The detached trans-Neptunian objects (TNOs) are those with semimajor axes beyond the 2:1 resonance with Neptune that are neither resonant nor scattering.
Matthew Beaudoin   +6 more
doaj   +1 more source

THE INCLINATIONS OF FAINT TRANS-NEPTUNIAN OBJECTS

open access: yesThe Astrophysical Journal, 2010
Bernstein et al. found that the population of faint (R> 26) trans-Neptunian objects (TNOs) known at that time was dominated by "Classical" objects, which have low inclinations (i < 5°) and distances of 40-45 AU. Since those observations, the number of faint TNOs whose orbits are sufficiently well known to be classified as "Classical" or "Excited" has ...
D. E. Trilling   +2 more
openaire   +1 more source

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