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Published in 2019 at "Icarus"
DOI: 10.1016/j.icarus.2019.113417
Abstract: Abstract The dynamically hot and cold populations of the Kuiper Belt probably formed from two distinct regions of the Solar System. The former originated from a massive planetesimal disk extending from the primordial position of…
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Keywords:
planetesimal disk;
disk;
positions secular;
kuiper belt ... See more keywords
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Published in 2020 at "Icarus"
DOI: 10.1016/j.icarus.2020.113834
Abstract: Abstract The dominant topographic features on two-lobed Kuiper Belt object (486958) Arrokoth (provisionally designated 2014 MU69) are scattered, small, circular depressions or pits up to ~1.0 km across and curvilinear troughs observed near the terminator during…
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Keywords:
topography;
new horizons;
486958 arrokoth;
kuiper belt ... See more keywords
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Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz1069
Abstract: We perform N-body simulations of the early phases of open cluster evolution including a large population of planetesimals, initially arranged in Kuiper-belt like discs around each star. Using a new, fourth-order, and time-reversible N-body code…
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Keywords:
fate planetesimal;
planetesimal discs;
kuiper belt;
discs young ... See more keywords
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Published in 2023 at "Science advances"
DOI: 10.1126/sciadv.adg6936
Abstract: Kuiper Belt objects exhibit a wider color range than any other solar system population. The origin of this color diversity is unknown, but likely the result of the prolonged irradiation of organic materials by galactic…
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Keywords:
belt objects;
color diversity;
cosmic rays;
belt ... See more keywords
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Published in 2019 at "Science"
DOI: 10.1126/science.aaw9771
Abstract: New Horizons flies past MU69 After flying past Pluto in 2015, the New Horizons spacecraft shifted course to encounter (486958) 2014 MU69, a much smaller body about 30 kilometers in diameter. MU69 is part of…
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Keywords:
new horizons;
kuiper belt;
mu69;
belt object ... See more keywords