Results 71 to 80 of about 2,093,691 (201)
Formation and Migration of Trans-Neptunian Objects [PDF]
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.
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Advanced Techniques in Stability Analysis of Trans-Neptunian Objects
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
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
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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
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Water‐Ice Dominated Spectra of Saturn's Rings and Small Moons From JWST
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]
Chapter to be published in the book "The Transneptunian Solar System", Dina Prialnik, Maria Antonietta Barucci, Leslie Young Eds ...
Sicardy, Bruno +6 more
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LiDO: Discovery of a 10:1 Resonator with a Novel Libration State
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
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OSSOS. VII. 800+ Trans-Neptunian Objects—The Complete Data Release [PDF]
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
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
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THE INCLINATIONS OF FAINT TRANS-NEPTUNIAN OBJECTS
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
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