Impact spallation experiments: Fracture patterns and spall velocities
Spall velocities were measured for nine experimental impacts into San Marcos gabbro targets. Impact velocities ranged from 1 to 6.5 km/sec. Projectiles were iron, aluminum, lead, and basalt of varying sizes. The projectile masses ranged from a 4-g lead bullet to a 0.04-g aluminum sphere. The velocit...
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description | Spall velocities were measured for nine experimental impacts into San Marcos gabbro targets. Impact velocities ranged from 1 to 6.5 km/sec. Projectiles were iron, aluminum, lead, and basalt of varying sizes. The projectile masses ranged from a 4-g lead bullet to a 0.04-g aluminum sphere. The velocities of fragments were measured from high-speed films taken of the events. The maximum spall velocity observed was 30 m/sec, or 0.56 percent of the 5.4 km/sec impact velocity. The measured velocities were compared to the spall velocities predicted by the spallation model of
Melosh (1984). The compatibility between the spallation model for large planetary impacts and the results of these small-scale experiments is considered in detail. The targets were also bisected to observe the pattern of internal fractures. The series of fractures was observed, whose location coincided with the boundary between rock subjected to the peak shock compression and a theoretical “near-surface zone” predicted by the spallation model. According to the model, between this boundary and the free surface, the target material is expected to have received reduced levels of compressive stress as compared to the more highly shocked region below. |
doi_str_mv | 10.1016/0019-1035(90)90025-5 |
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Melosh (1984). The compatibility between the spallation model for large planetary impacts and the results of these small-scale experiments is considered in detail. The targets were also bisected to observe the pattern of internal fractures. The series of fractures was observed, whose location coincided with the boundary between rock subjected to the peak shock compression and a theoretical “near-surface zone” predicted by the spallation model. According to the model, between this boundary and the free surface, the target material is expected to have received reduced levels of compressive stress as compared to the more highly shocked region below.</description><identifier>ISSN: 0019-1035</identifier><identifier>EISSN: 1090-2643</identifier><identifier>DOI: 10.1016/0019-1035(90)90025-5</identifier><identifier>CODEN: ICRSA5</identifier><language>eng</language><publisher>Legacy CDMS: Elsevier Inc</publisher><subject>640107 - Astrophysics & Cosmology- Planetary Phenomena ; ASTEROIDS ; CAVITIES ; CHEMICAL COMPOSITION ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; COLLISIONS ; COMPARATIVE EVALUATIONS ; Cosmochemistry. Extraterrestrial geology ; CRATERS ; DAMAGE ; Earth sciences ; Earth, ocean, space ; Exact sciences and technology ; Extraterrestrial geology ; Lunar And Planetary Exploration ; METEORITES ; NUCLEAR REACTIONS ; PLANETARY EVOLUTION ; PLANETS ; SOLAR SYSTEM EVOLUTION ; SPALLATION</subject><ispartof>Icarus (New York, N.Y. 1962), 1990-09, Vol.87 (1), p.140-155</ispartof><rights>1990</rights><rights>1991 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a438t-4d90267212be75071d390af6c297a2aaffb72bf5af4627c4e846fae2883628ec3</citedby><cites>FETCH-LOGICAL-a438t-4d90267212be75071d390af6c297a2aaffb72bf5af4627c4e846fae2883628ec3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/0019-1035(90)90025-5$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>230,314,780,784,885,3550,27924,27925,45995</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=19458138$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/6479303$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Polanskey, Carol A.</creatorcontrib><creatorcontrib>Ahrens, Thomas J.</creatorcontrib><title>Impact spallation experiments: Fracture patterns and spall velocities</title><title>Icarus (New York, N.Y. 1962)</title><description>Spall velocities were measured for nine experimental impacts into San Marcos gabbro targets. Impact velocities ranged from 1 to 6.5 km/sec. Projectiles were iron, aluminum, lead, and basalt of varying sizes. The projectile masses ranged from a 4-g lead bullet to a 0.04-g aluminum sphere. The velocities of fragments were measured from high-speed films taken of the events. The maximum spall velocity observed was 30 m/sec, or 0.56 percent of the 5.4 km/sec impact velocity. The measured velocities were compared to the spall velocities predicted by the spallation model of
Melosh (1984). The compatibility between the spallation model for large planetary impacts and the results of these small-scale experiments is considered in detail. The targets were also bisected to observe the pattern of internal fractures. The series of fractures was observed, whose location coincided with the boundary between rock subjected to the peak shock compression and a theoretical “near-surface zone” predicted by the spallation model. According to the model, between this boundary and the free surface, the target material is expected to have received reduced levels of compressive stress as compared to the more highly shocked region below.</description><subject>640107 - Astrophysics & Cosmology- Planetary Phenomena</subject><subject>ASTEROIDS</subject><subject>CAVITIES</subject><subject>CHEMICAL COMPOSITION</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>COLLISIONS</subject><subject>COMPARATIVE EVALUATIONS</subject><subject>Cosmochemistry. 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Extraterrestrial geology</topic><topic>CRATERS</topic><topic>DAMAGE</topic><topic>Earth sciences</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Extraterrestrial geology</topic><topic>Lunar And Planetary Exploration</topic><topic>METEORITES</topic><topic>NUCLEAR REACTIONS</topic><topic>PLANETARY EVOLUTION</topic><topic>PLANETS</topic><topic>SOLAR SYSTEM EVOLUTION</topic><topic>SPALLATION</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Polanskey, Carol A.</creatorcontrib><creatorcontrib>Ahrens, Thomas J.</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>Icarus (New York, N.Y. 1962)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Polanskey, Carol A.</au><au>Ahrens, Thomas J.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Impact spallation experiments: Fracture patterns and spall velocities</atitle><jtitle>Icarus (New York, N.Y. 1962)</jtitle><date>1990-09-01</date><risdate>1990</risdate><volume>87</volume><issue>1</issue><spage>140</spage><epage>155</epage><pages>140-155</pages><issn>0019-1035</issn><eissn>1090-2643</eissn><coden>ICRSA5</coden><abstract>Spall velocities were measured for nine experimental impacts into San Marcos gabbro targets. Impact velocities ranged from 1 to 6.5 km/sec. Projectiles were iron, aluminum, lead, and basalt of varying sizes. The projectile masses ranged from a 4-g lead bullet to a 0.04-g aluminum sphere. The velocities of fragments were measured from high-speed films taken of the events. The maximum spall velocity observed was 30 m/sec, or 0.56 percent of the 5.4 km/sec impact velocity. The measured velocities were compared to the spall velocities predicted by the spallation model of
Melosh (1984). The compatibility between the spallation model for large planetary impacts and the results of these small-scale experiments is considered in detail. The targets were also bisected to observe the pattern of internal fractures. The series of fractures was observed, whose location coincided with the boundary between rock subjected to the peak shock compression and a theoretical “near-surface zone” predicted by the spallation model. According to the model, between this boundary and the free surface, the target material is expected to have received reduced levels of compressive stress as compared to the more highly shocked region below.</abstract><cop>Legacy CDMS</cop><pub>Elsevier Inc</pub><doi>10.1016/0019-1035(90)90025-5</doi><tpages>16</tpages></addata></record> |
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subjects | 640107 - Astrophysics & Cosmology- Planetary Phenomena ASTEROIDS CAVITIES CHEMICAL COMPOSITION CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COLLISIONS COMPARATIVE EVALUATIONS Cosmochemistry. Extraterrestrial geology CRATERS DAMAGE Earth sciences Earth, ocean, space Exact sciences and technology Extraterrestrial geology Lunar And Planetary Exploration METEORITES NUCLEAR REACTIONS PLANETARY EVOLUTION PLANETS SOLAR SYSTEM EVOLUTION SPALLATION |
title | Impact spallation experiments: Fracture patterns and spall velocities |
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