Please use this identifier to cite or link to this item:
Appears in Collections:Biological and Environmental Sciences Journal Articles
Peer Review Status: Refereed
Title: Oblique impact cratering experiments in brittle targets: Implications for elliptical craters on the Moon
Author(s): Michikami, Tatsuhiro
Hagermann, Axel
Morota, Tomokatsu
Haruyama, Junichi
Hasegawa, Sunao
Keywords: Oblique impact cratering process
Pit crater
Elliptical crater
Laboratory experiments
Issue Date: Jan-2017
Date Deposited: 12-Apr-2018
Citation: Michikami T, Hagermann A, Morota T, Haruyama J & Hasegawa S (2017) Oblique impact cratering experiments in brittle targets: Implications for elliptical craters on the Moon. Planetary and Space Science, 135, pp. 27-36.
Abstract: Most impact craters observed on planetary bodies are the results of oblique impacts of meteoroids. To date, however, there have only been very few laboratory oblique impact experiments for analogue targets relevant to the surfaces of extraterrestrial bodies. In particular, there is a lack of laboratory oblique impact experiments into brittle targets with a material strength on the order of 1 MPa, with the exception of ice. A strength on the order of 1 MPa is considered to be the corresponding material strength for the formation of craters in the 100 m size range on the Moon. Impact craters are elliptical if the meteoroid's trajectory is below a certain threshold angle of incidence, and it is known that the threshold angle depends largely on the material strength. Therefore, we examined the threshold angle required to produce elliptical craters in laboratory impact experiments into brittle targets. This work aims to constrain current interpretations of lunar elliptical craters and pit craters with sizes below a hundred meters. We produced mortar targets with compressive strength of 3.2 MPa. A spherical nylon projectile (diameter 7.14 mm) was shot into the target surface at a nominal velocity of 2.3 km/s, with an impact angle of 5°‐90° from horizontal. The threshold angle of this experiment ranges from 15° to 20°. We confirmed that our experimental data agree with previous empirical equations in terms of the cratering efficiency and the threshold impact angle. In addition, in order to simulate the relatively large lunar pit craters related to underground cavities, we conducted a second series of experiments under similar impact conditions using targets with an underground rectangular cavity. Size and outline of craters that created a hole are similar to those of craters without a hole. Moreover, when observed from an oblique angle, a crater with a hole has a topography that resembles the lunar pit craters. The relation between the impact velocity of meteoroids on the Moon and the probability of elliptical crater formation was investigated based on our experimental results and an existing empirical equation. The results suggest a distinct possibility that most craters in the 100 m size range on the Moon, given their elliptical shape, originated as secondary craters. © 2016 The Authors
DOI Link: 10.1016/j.pss.2016.11.004
Rights: © 2016 The Authors. Published by Elsevier Ltd. This is an open access article under the CC BY license (
Licence URL(s):

Files in This Item:
File Description SizeFormat 
1-s2.0-S003206331630157X-main.pdfFulltext - Published Version1.5 MBAdobe PDFView/Open

This item is protected by original copyright

A file in this item is licensed under a Creative Commons License Creative Commons

Items in the Repository are protected by copyright, with all rights reserved, unless otherwise indicated.

The metadata of the records in the Repository are available under the CC0 public domain dedication: No Rights Reserved

If you believe that any material held in STORRE infringes copyright, please contact providing details and we will remove the Work from public display in STORRE and investigate your claim.