Results 61 to 70 of about 256 (139)
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source
The decade-long debate over the existence of apsidal clustering in the outer solar system is poised for reignition given the plethora of distant trans-Neptunian object (TNO) discoveries expected from the forthcoming Vera C.
Amir Siraj +2 more
doaj +1 more source
The Formation of Bilobate Comet Shapes through Sublimative Torques. [PDF]
Safrit TK +6 more
europepmc +1 more source
The Luminosity Function of Ultrafaint Trans-Neptunian Objects Detected by JWST
We present a definitive discovery of 27 trans-Neptunian objects (TNOs) using the Near-Infrared Camera aboard the James Webb Space Telescope (JWST). By employing a shift-and-stack technique and a machine learning network geared specifically to identifying
Marielle R. Eduardo +10 more
doaj +1 more source
Organic Matter in the Asteroid Ryugu: What We Know So Far. [PDF]
Potiszil C +8 more
europepmc +1 more source
A Near-infrared Survey of Candidate Haumea Family Members
The Haumea family is the only known dynamical family in the trans-Neptunian region. To date, 10 family members have been unambiguously identified using near-infrared (NIR) spectral or photometric data in combination with their strong dynamical proximity ...
Benjamin C. N. Proudfoot +7 more
doaj +1 more source
The formation of Haumea and its family via binary merging. [PDF]
Proudfoot B, Ragozzine D.
europepmc +1 more source
The Inner Kernel of the Classical Kuiper Belt
The “kernel” of the classical Kuiper Belt was discovered by Petit et al. as a visual overdensity of objects with low ecliptic inclinations and eccentricities at semimajor axes near ∼44 au.
Amir Siraj +2 more
doaj +1 more source
Sedna-like objects (a.k.a. sednoids) are trans-Neptunian objects (TNOs) characterized by large semimajor axes and exceptionally high perihelia. Their high- q orbits are detached from the influence of the four giant planets and need extra perturbation to ...
Qingru Hu +3 more
doaj +1 more source
Observation of the most H2-dense filled ice under high pressure. [PDF]
Ranieri U +9 more
europepmc +1 more source

