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Meteoritics &Planetary Science, Volume 61, Issue 6, Page 953-954, June 2026.
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Computational study of the separation of regular sphere clusters in high-Mach-number flow. [PDF]

J Fluid Mech
Whalen T, Deiterding R, Laurence SJ.
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Meteoritics &Planetary Science, Volume 61, Issue 6, June 2026.
wiley   +1 more source

Deep microbial colonization during impact-generated hydrothermal circulation at the Lappajärvi impact structure, Finland. [PDF]

Nat Commun
Gustafsson J, Osinski GR, Roberts NMW, Quade J, Wang Z, Whitehouse MJ, Jeon H, Karlsson A, Hietala S, Drake H.   +9 more
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Automated Lunar Crater Identification with Chandrayaan-2 TMC-2 Images using Deep Convolutional Neural Networks. [PDF]

Sci Rep
Sinha M, Paul S, Ghosh M, Mohanty SN, Pattanayak RM.   +4 more
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Prediction of meteoroid stream structure based on meteoroid fragmentation

Journal of Astrophysics and Astronomy, 2020
Every day, large number of meteoroids enter the Earth’s atmosphere and deposit their mass either in atomic form or in ionic form depending on whether it has undergone ablation or fragmentation. The heavier meteoroids undergo fragmentation while the lighter ones are more prone to ablate.
K. SANJEEV KUMAR, N. RAKESH CHANDRA, G. YELLAIAH, B. PREM KUMAR   +3 more
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Meteoroid ablation models

Earth, Moon, and Planets, 2004
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
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RADAR MEASUREMENTS OF METEOROID DECELERATIONS

Earth, Moon, and Planets, 2004
Measurements of meteoroid velocities and decelerations have been obtained from post-t 0 diffraction patterns present in echo signatures obtained from the multi-site AMOR radar operated at the University of Canterbury’s research facility. The system allows the sampling of a meteoroid’s velocity at separated points along the body’s trajectory to yield ...
W. J. Baggaley, J. Grant
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Meteoroid Storms Detected on the Moon

Science, 1976
Seismometers on the moon have detected several brief periods of enhanced meteoroid-impact activity, believed to represent encounters of the moon with "clouds" of objects in the kilogram range. The latest and most active encounter, in June 1975, is interpreted as a meteoroid cloud of diameter 0.1 astronomical unit and total mass 10
F K, Duennebier, Y, Nakamura, G V, Latham, H J, Dorman   +3 more
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Meteoroid Streams

Symposium - International Astronomical Union, 1994
Meteoroid streams, producing meteor showers if some part of the stream has a node near 1 AU, have complex structures which are only just beginning to be understood. The old simplistic idea of a narrow loop being formed about the orbit of a parent comet with one, or possibly two, terrestrial intersection(s) is now being replaced by the recognition that ...
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