Impact experiments on highly porous targets: Cavity morphology and disruption thresholds in the strength regime. (March 2015)
- Record Type:
- Journal Article
- Title:
- Impact experiments on highly porous targets: Cavity morphology and disruption thresholds in the strength regime. (March 2015)
- Main Title:
- Impact experiments on highly porous targets: Cavity morphology and disruption thresholds in the strength regime
- Authors:
- Okamoto, Takaya
Nakamura, Akiko M.
Hasegawa, Sunao - Abstract:
- Abstract: Small bodies were probably very porous during the formation of the solar system. To understand the evolution of such bodies, impact experiments on sintered glass-bead targets with porosities of 80%, 87%, and 94% were performed at velocities of 1.8–7.2 km s −1 using various projectiles with densities ranging from 1.1 g cm −3 to 4.5 g cm −3 . Here we report on the resulting cavity morphologies formed by these impacts, with particular attention paid to the depth from the cavity׳s entrance hole to its maximum diameter, the entrance-hole diameter, and the maximum diameter. We obtained empirical relations of the entrance-hole diameter and the maximum diameter using non-dimensional parameters for crater scaling. We also report on the targets׳ disruption thresholds, Q ⁎ . Each Q ⁎ value is on the order of kilojoules per kilogram, which is higher than the equivalent values for pure ice targets and basalt targets determined from high-velocity impact experiments. Non-dimensional disruption thresholds, ρ t Q ⁎ / Y, where ρ t and Y are the targets׳ bulk densities and compressive strengths, respectively, are calculated for various targets including those used in this study; they are shown to be within approximately one order of magnitude for a given porosity, although the impact velocities and target sizes range from 1 m s −1 to 7.2 km s −1 and from 2 cm to 14 cm, respectively. The previous proposed strength parameter for the catastrophic disruption threshold, Π s ⁎, is alsoAbstract: Small bodies were probably very porous during the formation of the solar system. To understand the evolution of such bodies, impact experiments on sintered glass-bead targets with porosities of 80%, 87%, and 94% were performed at velocities of 1.8–7.2 km s −1 using various projectiles with densities ranging from 1.1 g cm −3 to 4.5 g cm −3 . Here we report on the resulting cavity morphologies formed by these impacts, with particular attention paid to the depth from the cavity׳s entrance hole to its maximum diameter, the entrance-hole diameter, and the maximum diameter. We obtained empirical relations of the entrance-hole diameter and the maximum diameter using non-dimensional parameters for crater scaling. We also report on the targets׳ disruption thresholds, Q ⁎ . Each Q ⁎ value is on the order of kilojoules per kilogram, which is higher than the equivalent values for pure ice targets and basalt targets determined from high-velocity impact experiments. Non-dimensional disruption thresholds, ρ t Q ⁎ / Y, where ρ t and Y are the targets׳ bulk densities and compressive strengths, respectively, are calculated for various targets including those used in this study; they are shown to be within approximately one order of magnitude for a given porosity, although the impact velocities and target sizes range from 1 m s −1 to 7.2 km s −1 and from 2 cm to 14 cm, respectively. The previous proposed strength parameter for the catastrophic disruption threshold, Π s ⁎, is also calculated. It is shown to be roughly constant, irrespective of porosity if we assume that the scaling parameter μ decreases linearly with increasing porosity. Highlights: Impact experiments on targets with porosity of 80%, 87% and 94% were conducted. Empirical relations of cavity dimensions are obtained. Disruption thresholds are compiled using non-dimensional parameters. … (more)
- Is Part Of:
- Planetary and space science. Volume 107(2015)
- Journal:
- Planetary and space science
- Issue:
- Volume 107(2015)
- Issue Display:
- Volume 107, Issue 2015 (2015)
- Year:
- 2015
- Volume:
- 107
- Issue:
- 2015
- Issue Sort Value:
- 2015-0107-2015-0000
- Page Start:
- 36
- Page End:
- 44
- Publication Date:
- 2015-03
- Subjects:
- Impact experiments -- Small bodies -- Crater -- Catastrophic disruption -- Non-dimensional analysis
Space sciences -- Periodicals
Atmosphere, Upper -- Periodicals
Sciences spatiales -- Périodiques
Haute atmosphère -- Périodiques
523 - Journal URLs:
- http://www.sciencedirect.com/science/journal/00320633 ↗
http://www.elsevier.com/journals ↗ - DOI:
- 10.1016/j.pss.2014.08.008 ↗
- Languages:
- English
- ISSNs:
- 0032-0633
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 6508.320000
British Library DSC - BLDSS-3PM
British Library HMNTS - ELD Digital store - Ingest File:
- 6348.xml