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Martian cratering 11. Utilizing decameter scale crater populations to study Martian history
DOI: 10.1111/maps.12807 Bibcode: 2017M&PS...52..493H

Daubar, I. J.; Hartmann, W. K.

New information has been obtained in recent years regarding formation rates and the production size-frequency distribution (PSFD) of decameter-scale primary Martian craters formed during recent orbiter missions. Here we compare the PSFD of the currently forming small primaries (P) with new data on the PSFD of the total small crater population that…

2017 Meteoritics and Planetary Science
MEx 62
Investigating target versus impactor influences on Martian crater morphology at the simple-complex transition
DOI: 10.1111/maps.12884 Bibcode: 2017M&PS...52.1722H

Hynek, Brian M.; Herrick, Robert R.

Comparing craters of identical diameter on a planet is an empirical method of studying the effects of different target and impactor properties while holding total impact energy nearly constant. We have analyzed the Martian crater population within a narrow diameter range (7 km < crater diameter < 9 km) at the simple-complex crater transition…

2017 Meteoritics and Planetary Science
MEx 12
Snow carrots after the Chelyabinsk event and model implications for highly porous solar system objects
DOI: 10.1111/maps.12831 Bibcode: 2017M&PS...52..979L

Luther, Robert; Wünnemann, Kai; Artemieva, Natalia +2 more

After the catastrophic disruption of the Chelyabinsk meteoroid, small fragments formed funnels in the snow layer covering the ground. We constrain the pre-impact characteristics of the fragments by simulating their atmospheric descent with the atmospheric entry model. Fragments resulting from catastrophic breakup may lose about 90% of their initia…

2017 Meteoritics and Planetary Science
Rosetta 7