Results 101 to 110 of about 216,519 (217)

Long-term Dynamical Stability in the Outer Solar System. II. Detailed Secular Evolution of Four Large Regular and Resonant Trans-Neptunian Objects

The Astronomical Journal
The long-term evolution of the outer solar system is subject to the influence of the giant planets, however, perturbations from other massive bodies located in the region imprint secular signatures, which are discernible in long-term simulations. In this
Marco A. Muñoz-Gutiérrez, Antonio Peimbert, Angeles Pérez-Villegas   +2 more
doaj   +1 more source

88th Annual Meeting of the Meteoritical Society 2026: Abstracts

Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley   +1 more source

LiDO: Exploring the Stable Plutino Parameter Space

The Planetary Science Journal
We present a publicly available, high-resolution, filled-parameter-space synthetic distribution of the plutinos, trans-Neptunian objects (TNOs) librating in the 3:2 mean-motion resonance with Neptune, with particular focus on the plutinos simultaneously ...
Samantha M. Lawler, Mark Comte, Rosemary E. Pike, Mike Alexandersen, Ying-Tung Chen, Cameron Collyer, Matthew Holman, J. J. Kavelaars, Lowell Peltier, Cameron Semenchuck   +9 more
doaj   +1 more source

Geochemical Modeling from the Asteroid Belt to the Kuiper Belt: Systematic Review

Encyclopedia
The high costs and time-consuming nature of space exploration missions are among the major barriers to studying deep space. The lack of samples and limited information make such studies challenging, highlighting the need for innovative solutions ...
Arash Yoosefdoost, Rafael M. Santos
doaj   +1 more source

THE SURFACE COMPOSITION OF LARGE KUIPER BELT OBJECT 2007 OR10

, 2011
We present photometry and spectra of the large Kuiper belt object 2007 OR10. The data show significant near-infrared absorption features due to water ice.
Brown, M. E., Fraser, W. C., M. E. Brown, Burgasser, Adam J., W. C. Fraser, A. J. Burgasser   +5 more
core   +1 more source

The Edges of Planetary Systems: Falling Off the Kuiper Cliff in a Dissipating Gas Disk

The Astrophysical Journal
Probably the last planetesimals to have formed from dust in the solar nebula are cold classical Kuiper Belt Objects (CCKBOs). To the extent that they are isolated and unchanged since birth, CCKBOs offer direct insights into nebular processes.
Rixin Li, Eugene Chiang
doaj   +1 more source

Faint moons orbiting Kuiper Belt objects

, 2010
The Kuiper Belt is a Belt of ice and rocks located beyond the orbit of Neptune; Pluto is considered part of the Kuiper Belt. We used photometric data taken from the Magellan Clay telescope located in the Las Campanas Observatory in Chile.
Michael Ryan
core  

Col-OSSOS: Investigating the Origins of Different Surfaces in the Primordial Kuiper Belt

The Planetary Science Journal
The Colours of the Outer Solar System Origins Survey (Col-OSSOS) measured the optical/near-IR colors of a brightness-complete sample of trans-Neptunian objects (TNOs).
Laura E. Buchanan, Megan E. Schwamb, Wesley C. Fraser, Michele T. Bannister, J. J. Kavelaars, Michaël Marsset, Rosemary E. Pike, David Nesvorný, Samantha M. Lawler, Susan D. Benecchi, Nuno Peixinho, Nicole J. Tan, Kathryn Volk, Mike Alexandersen, Jean-Marc Petit   +14 more
doaj   +1 more source

The Effect of Massive Trans-Neptunian Objects in the Long-term Evolution and Leakage Rates of Neptune’s 3:2 and 2:1 Mean Motion Resonances

The Astronomical Journal
The current populations trapped in Neptune’s main mean motion resonances in the Kuiper Belt, Plutinos in the 3:2 and Twotinos in the 2:1, contain some of the best-characterized minor objects in the solar system, given their dynamical importance.
Marco A. Muñoz-Gutiérrez, Sebastián Ramírez-Vargas, Antonio Peimbert, Angeles Pérez-Villegas, Cristobal Petrovich   +4 more
doaj   +1 more source

Other Kuiper Belts

The Astrophysical Journal, 2004
When a main sequence star evolves into a red giant and its Kuiper Belt Object's (KBO's) reach a temperature of about 170 K, the dust released during the rapid ice-sublimation of these cometary bodies may lead to a detectable infrared excess at 25 microns, depending upon the mass of the KBO's.
openaire   +2 more sources