A chondritic meteorite dust shower in the early Ordovician. Proceedings of 50th Lunar and Planetary Science Conference

Schmitz, B., Tassinari, M. & Peucker-Ehrenbrink, B. A rain of ordinary chondritic meteorites in the early Ordovician. Earth is a planet. Sci. Lett. 194, 1–15 (2001).

Farley, K. A., Vokrouhlický, D., Bottke, W. F. & Nesvorný, D. A dust shower is caused by the break up of an asteroid. Nature 439, 295–297 (2006).

Kenkmann, T. The terrestrial impact crater record: A statistical analysis of morphologies, structures, ages and more It was a meteorite. Planet. Sci. 56, 1024–1070 (2021).

Greenwood, R. C., Burbine, T. H. & Franchi, I. A. Linking asteroids and meteorites to the primordial planetesimal population. There is a person who talks about a topic titled “geochim.” There was a person named Cosmochim. The Adherent’s 277, 377–406 was published in 2020.

Pieters, C. M. and Hiroi, T. RELAB (Reflectance Experiment Laboratory): A NASA Multiuser Spectroscopy Facility. In 35th Lunar and Planetary Science Conference, abstract no. 1720 (2004).

Marsset, M. et al. The global match between the near-Earth and main-belt asteroid populations and excess of D- type near-Earth objects is part of the debiased distribution of MIThnEOS. Astron. J. 163, 165 (2022).

Gaffey, M. J. & Fieber-Beyer, S. K., Is the (20) Massalia family the source of the L-chondrites? The 50th Lunar and Planetary Science Conference took place in 2019.

Nesvorn, D., Bottke, J., William, F., Dones, L. and Levison, H. F. The recent breakup of an asteroid in the main-belt region. Nature 417 was published in 2002.

There is evidence for a comet shower in the Late Eocene. Science 280 was published in 1998.

Kulik, L. A. Otet meteoritieskoj ekspedicii. po 29 Nojabrja 1922 g. Izv. Ross. The person is Akad. Nauk 16, 391–410 (1922).

Nesvorný, D. et al. Cometary origin of the zodiacal cloud and carbonaceous micrometeorites. Implications for hot disks. Astrophys. J. 713, article one, was published in 2010.

Rayner, J. T. et al. SpeX: a medium-resolution 0.8-5.5 micron spectrograph and imager for the NASA Infrared Telescope Facility. Publ. It is Astron. It’s soc. In the year 2003 the state of Pac. 115 was 362–382.

Estimation of the Gefion Asteroid Family: implications for L-chondrite link. It was Mon. Not. R. Astron. Soc. 515, 5211–5218 (2022).

Cloutis, E. A., Gaffey, M. J., Jackowski, T. L. & Reed, K. L. Calibrations of phase abundance, composition, and particle size distribution for olivine-orthopyroxene mixtures from reflectance spectra. J. Geophys. Res. 91 was published in 1986.

Orbital and physical characteristics of meter-scale impactors from airburst observations. I. The impact of the Hilda collisional family

THe delivery of meteorites to Earth after a big asteroid collision was fast. Nature 430, 323–325 (2004).

Vokrouhlick and D. Diurnal Yarkovsky had an effect on mobility of asteroidal fragments. I. Linear theory. Astron. Astrophys. 335, 1093–1100 (1998).

Brož, M., Vokrouhlický, D., Morbidelli, A., Nesvorný, D. & Bottke, W. F. Did the Hilda collisional family form during the late heavy bombardment? Mon. Not. R. Astron. Soc. 414, 2716–2727 (2011).

Brown, P., Wiegert, P., Clark, D. & Tagliaferri, E. Orbital and physical characteristics of meter-scale impactors from airburst observations. The journal Icarus published a 96–113 piece of work.

Interplanetary dust production from hypervelocity impact disruptions of Murchison meteorites: a possible scenario for early terrestrial planet formation by torque-driven planetary migration

Chladni, E. F. F. Über den Ursprung der von Pallas Gefundenen und anderer ihr ähnlicher Eisenmassen, und Über Einige Damit in Verbindung stehende Naturerscheinungen (Johan Friedrich Hartknoch, 1794).

Flynn, G. J., Durda, D. D., Sandel, L. E., Kreft, J. W. & Strait, M. M. Dust production from the hypervelocity impact disruption of the Murchison hydrous CM2 meteorite: implications for the disruption of hydrous asteroids and the production of interplanetary dust. Planet. Space Sci. 57, 119–126 (2009).

Campo Bagatin, A., Cellino, A., Davis, D. R., Farinella, P. & Paolicchi, P. Wavy size distributions for collisional systems with a small-size cutoff. It’s a planet. Space Sci. 42, 1079–1092 (1994).

The risk posed by potential Earth impacts was quantified. It was Icarus 159, 424–532 in 2002.

Chaotic transport and chronology of complex asteroid families are said to be related. There is a work day on Mon. Not. R. Astron. Soc. 402, 1263–1272 (2010).

Ševeček, P. et al. SPH/N-Body simulations of small (D = 10 km) asteroidal breakups and improved parametric relations for Monte-Carlo collisional models. It was Icarus 776, 241-258.

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).