Results 111 to 120 of about 14,134 (215)
Geochemical Modeling from the Asteroid Belt to the Kuiper Belt: Systematic Review
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
Col-OSSOS: Investigating the Origins of Different Surfaces in the Primordial Kuiper Belt
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 +14 more
doaj +1 more source
Formation of Kuiper Belt Binaries
It appears that at least several percent of large Kuiper belt objects are members of wide binaries. Physical collisions are too infrequent to account for their formation. Collisionless gravitational interactions are more promising. These provide two channels for binary formation. In each, the initial step is the formation of a transient binary when two
Goldreich, Peter +2 more
openaire +2 more sources
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 +4 more
doaj +1 more source
Binaries have played a crucial role many times in the history of modern astronomy and are doing so again in the rapidly evolving exploration of the Kuiper Belt. The large fraction of transneptunian objects that are binary or multiple, 48 such systems are now known, has been an unanticipated windfall.
Noll, Keith S +4 more
openaire +3 more sources
Index of Authors and Co‐Authors
United European Gastroenterology Journal, Volume 13, Issue S8, Page 1559-1604, October 2025.
wiley +1 more source
In Situ Formation of the Cold Classical Kuiper Belt
Cold classical Kuiper Belt objects (CCKBOs) are considered first-generation planetesimals that formed 42–47 au from the Sun and have remained untouched since. Formation is thought to proceed by clumping of dust particles in protoplanetary disk gas by the
Rixin Li, Eugene Chiang
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The DECam Ecliptic Exploration Project (DEEP). III. Survey Characterization and Simulation Methods
We present a detailed study of the observational biases of the DECam Ecliptic Exploration Project’s B1 data release and survey simulation software that enables direct statistical comparisons between models and our data.
Pedro H. Bernardinelli +26 more
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We present the first set of trans-Neptunian objects (TNOs) observed on multiple nights in data taken from the DECam Ecliptic Exploration Project. Of these 110 TNOs, 105 do not coincide with previously known TNOs and appear to be new discoveries.
Hayden Smotherman +27 more
doaj +1 more source
Not a simple relationship between Neptune's migration speed and Kuiper belt inclination excitation. [PDF]
Volk K, Malhotra R.
europepmc +1 more source

