Extraterrestrial cause for the Cretaceous-Tertiary extinction. (Record no. 51988)

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fixed length control field 02178nam a2200217Ia 4500
003 - CONTROL NUMBER IDENTIFIER
control field MX-MdCICY
005 - DATE AND TIME OF LATEST TRANSACTION
control field 20250625160218.0
040 ## - CATALOGING SOURCE
Transcribing agency CICY
090 ## - LOCALLY ASSIGNED LC-TYPE CALL NUMBER (OCLC); LOCAL CALL NUMBER (RLIN)
Classification number (OCLC) (R) ; Classification number, CALL (RLIN) (NR) B-17827
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245 10 - TITLE STATEMENT
Title Extraterrestrial cause for the Cretaceous-Tertiary extinction.
490 0# - SERIES STATEMENT
Volume/sequential designation Science, 208(4448), p.1095-1108, 1980
520 3# - SUMMARY, ETC.
Summary, etc. Platinum metals are depleted in the earth's crust relative to their cosmic abundance; concentrations of these elements in deep-sea sediments may thus indicate influxes of extraterrestrial material. Deep-sea limestones exposed in Italy, Denmark, and New Zealand show iridium increases of about 30, 160, and 20 times, respectively, above the background level at precisely the time of the Cretaceous-Tertiary extinctions, 65 million years ago. Reasons are given to indicate that this iridium is of extraterrestrial origin, but did not come from a nearby supernova. A hypothesis is suggested which accounts for the extinctions and the iridium observations. Impact of a large earth-crossing asteroid would inject about 60 times the object's mass into the atmosphere as pulverized rock; a fraction of this dust would stay in the stratosphere for several years and be distributed worldwide. The resulting darkness would suppress photosynthesis, and the expected biological consequences match quite closely the extinctions observed in the paleontological record. One prediction of this hypothesis has been verified: the chemical composition of the boundary clay, which is thought to come from the stratospheric dust, is markedly different from that of clay mixed with the Cretaceous and Tertiary limestones, which are chemically similar to each other. Four different independent estimates of the diameter of the asteroid give values that lie in the range 10 ± 4 kilometers.
650 14 - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element THE CRETACEOUS-TERTIARY EXTINCTION
700 12 - ADDED ENTRY--PERSONAL NAME
Personal name Alvarez, L.W.
700 12 - ADDED ENTRY--PERSONAL NAME
Personal name Alvarez,W.
700 12 - ADDED ENTRY--PERSONAL NAME
Personal name Asaro, F.
700 12 - ADDED ENTRY--PERSONAL NAME
Personal name Michel, H. V.
856 40 - ELECTRONIC LOCATION AND ACCESS
Uniform Resource Identifier <a href="https://drive.google.com/file/d/1x8BTNkdaK5NPR5FvYXSmA0X_EmdELehM/view?usp=drivesdk">https://drive.google.com/file/d/1x8BTNkdaK5NPR5FvYXSmA0X_EmdELehM/view?usp=drivesdk</a>
Public note Para ver el documento ingresa a Google con tu cuenta: @cicy.edu.mx
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Source of classification or shelving scheme Clasificación local
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  Clasificación local     Ref1 CICY CICY Documento préstamo interbibliotecario 25.06.2025   B-17827 25.06.2025 25.06.2025 Documentos solicitados