Results 61 to 70 of about 307 (159)
The Largest Kuiper Belt Objects
While for the first decade of the study of the Kuiper belt, a gap existed between the sizes of the relatively small and faint Kuiper belt objects (KBOs) that were being studied and the largest known KBO.
Brown, Michael E.
core
Spectral Characterization of the Organic- and Methanol-rich Cliff-type Trans-Neptunian Objects
Trans-Neptunian objects (TNOs) harbor pristine materials from the early solar system. The James Webb Space Telescope offers major insights into the spectral classification of these small bodies.
Lucas T. McClure +18 more
doaj +1 more source
By revisiting three decades of molecular data, we retraced the evolution and mapped the diversity of Pelophylax water frogs, a famous group of Eurasian amphibians. The results highlight the Paratethys Paleo‐sea as a major driver of diversification, implement a new timetree validation approach, emphasize the rare ability of lineages to hybridize despite
Christophe Dufresnes +9 more
wiley +1 more source
Cosmic Ray Mantle Visibility on Kuiper Belt Objects
Optically red objects constitute the dynamically cold, old component of the Classical Kuiper Belt (40 - 47 AU) with heliocentric orbits of low eccentricity and inclination.
Sturner, S. J. +3 more
core
Rotational Study of 5:3 and 7:4 Resonant Objects within the Main Classical Trans-Neptunian Belt
The 5:3 and 7:4 mean motion resonances of Neptune are at 42.3 and 43.7 au, respectively, and overlap with objects in the classical trans-Neptunian belt (Kuiper Belt).
Audrey Thirouin, Scott S. Sheppard
doaj +1 more source
A Correlation between Inclination and Color in the Classical Kuiper Belt [PDF]
We have measured broadband optical BVR photometry of 24 classical and scattered Kuiper belt objects (KBOs), approximately doubling the published sample of colors for these classes of objects. We find a statistically significant correlation between object
Trujillo, Chadwick A., Brown, Michael E.
core
There are currently close to 3000 known Kuiper Belt Objects. Their orbits show that the Kuiper Belt contains rich dynamical structures. By carefully recording telescope pointings, tracking biases, and detection biases, as has been done for a handful of
Lawler, Samantha (5588618) +1 more
core +1 more source
The Hapke bidirectional reflectance model is widely used to analyze photometric observations of planetary surfaces. When fitting disk-integrated data, nonuniqueness concerns arise if observations lack sufficient phase angle coverage to constrain the ...
Paul Helfenstein, Anne J. Verbiscer
doaj +1 more source
Retention of a Primordial Cold Classical Kuiper Belt in an Instability-Driven Model of Solar System Formation [PDF]
The cold classical population of the Kuiper Belt exhibits a wide variety of unique physical characteristics, which collectively suggest that its dynamical coherence has been maintained throughout the solar system's lifetime. Simultaneously, the retention
Batygin, Konstantin +2 more
core
In 2019, NASA’s New Horizons mission, using the Long Range Reconnaissance Imager, revealed Arrokoth’s bilobated shape and a large impact-crater-like region (“Sky”) on the small lobe, which is ∼7 km wide and ∼1 km deep. Given that this depression takes up
Yaeji Kim +2 more
doaj +1 more source

