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Young asteroid families are the primary source of meteorites

Nature: https://www.nature.com/articles/s41586-024-08007-6

The origin of the asteroid regolithic dust shower. Iscar 218, 78 and 84. The Chelyabinsk LL5 chondrite

Kohout, T. et al. Insight into the impact of shock on asteroid regoliths can be gleaned from the information contained in the Chelyabinsk LL5 chondrite. Iscar 218, 78–84.

K. A., Vokrouhick, D., W. F., and Nesvorn, D. A dust shower came from the break up of an asteroid in the main belt. Nature 439, 295–297 (2006).

The record of impact craters on the ground. A statistical analysis of morphologies, structures, ages, lithologies, and more. Meteorit. Planet. The following issues ofSci. 56, 1070, are available through the internet.

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Milliken, Hiroi, and T. are from The NASA Reflectance Experiment Laboratory. In 47th Lunar and Planetary Science Conference, the contribution No. 1903 was published.

Marsset, M. The global match between near-Earth and main-belt asteroid populations and excess of D type near-Earth objects are the debiased composition of MITHNEOS. Astron. J. 163, 165 (2022).

The Massalia family is thought to be the source of the L-chondrites. In 50th Lunar and Planetary Science Conference, no. 2132, id. 1441 (2019).

Nesvorný, D., Bottke, J., William, F., Dones, L. & Levison, H. F. The asteroid broke up in the main-belt region. Nature 417, 720–771 (2002).

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Nesvorný, D. et al. It is said that the zodiacal cloud and carbonaceous micrometeorites were the beginnings of the universe. The implications for hot debris disks. There are astrophys. J. 912, 850, and 8610 were published in the year 2010.

Rayner, J. T. and their colleagues developed a spectrograph and imager for theInfrared Telescope Facility. Publ. Astron. Soc. Pac. 115, 362–382 (2003).

The implications for L-chondriTE link are discussed in Spectroscopic characterization of the Gefion Asteroid Family. Mon. Not. R. Astron. Soc. 515, 5211–5218 (2022).

A., Gaffey, M J., Jackowski, T.L. and Reed collaborated on a project on calibrating phase abundance, composition, and particle size distributions. J. Geophys. Res. 92, 11641–31165.

Theory of D. Diurnal Yarkovsky effect for collisional families of asteroid fragments and observation of airburst impactors

After a large asteroid hit the earth, meteorites were fast delivered. Nature 430, 323–3325 was published in 2004.

D. Diurnal Yarkovsky effect has a source of mobility for asteroidal fragments. There is a linear theory. Astron. Astrophys. 335, 1093–1100 (1998).

Did the collisional family form in the middle of the bombardment? Mon. Not. R. Astron. The results of the Soc. 409, 2716 and 2760 are from 2011.

Brown, P., Wiegert, P., Clark, D. & Tagliaferri, E. Orbital and physical characteristics of meter-scale impactors from airburst observations. The Icarus series of books were published in the year 2016

CM2 dust disruption and possible planet formation in collisions with a small-size cutoff. I. SpaceSci. 42

ber den Urprung von Pallas Gefundenen und anderer ihr hnlicher Eisenmassen.

The disruption of the hydrous CM2 meteorite is related to the dust production from the hypervelocity impact. A planet. SpaceSci. 57 was published in 2009.

Campo Bagatin, A., Cellino, A., Davis, D. R., Farinella, P. & Paolicchi, P. Wavy size distributions for collisional systems with a small-size cutoff. There is a planet. SpaceSci. 42 was published in 1994.

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Chaotic transport and historiographical information of complex asteroid families. Mon. Not. R. Astron. 409, 1263–1272 were published in 2010.

Eveek, P. SPH/N-Body simulations of small (D = 10 km) asteroidal breakups and improved parametric relations for Monte-Carlo collisional models. Icarus 295, 241, 251, 251, 251

Brož, M., Chrenko, O., Nesvorný, D. & Dauphas, N. Early terrestrial planet formation by torque-driven convergent migration of planetary embryos. Nat. Astron. 5, 898–902 (2021).

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