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Inizio > THE LUNAR EXPLORER ARCHIVES > Original Nasa Apollo Frames: from Apollo 4 to Apollo 17
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AS 16-107-17483 - Station 4 Crater (ejecta crater)
Station 4 crater. Note that there is very little debris on the Western (right) side of the Crater. As John Young recognized in the field, this crater was almost certainly formed by a large piece of highly-shocked ejecta from South Ray Crater which plowed into the side of Stone Mountain at relatively low velocity and came apart. 

Hence, this is a Secondary Crater.

Notes (from "Glossary of Geology", 2nd Edition, American Geological Inst., Falls Church (VA) - 1980)

Ejecta — The material thrown out of an impact crater by the shock pressures generated during the impact event. Ejecta generally covers the surface around an impact crater to a distance of at least one crater diameter, with individual streamers of material extending well beyond this distance ("rays"). The ejecta blanket of a crater becomes less visible with increasing age of the crater.

Secondary craters — Craters produced by the impact of debris thrown out by a large impact event. Many secondary craters occur in clusters or lines where groups of ejecta blocks impacted almost simultaneously.
Parole chiave: Lunar Surface - Station 4 Crater

AS 16-107-17483 - Station 4 Crater (ejecta crater)

Station 4 crater. Note that there is very little debris on the Western (right) side of the Crater. As John Young recognized in the field, this crater was almost certainly formed by a large piece of highly-shocked ejecta from South Ray Crater which plowed into the side of Stone Mountain at relatively low velocity and came apart.

Hence, this is a Secondary Crater.

Notes (from "Glossary of Geology", 2nd Edition, American Geological Inst., Falls Church (VA) - 1980)

Ejecta — The material thrown out of an impact crater by the shock pressures generated during the impact event. Ejecta generally covers the surface around an impact crater to a distance of at least one crater diameter, with individual streamers of material extending well beyond this distance ("rays"). The ejecta blanket of a crater becomes less visible with increasing age of the crater.

Secondary craters — Craters produced by the impact of debris thrown out by a large impact event. Many secondary craters occur in clusters or lines where groups of ejecta blocks impacted almost simultaneously.

as16-107-17476.JPG as16-107-17477.JPG as16-107-17483.JPG as16-107-17510.JPG as16-107-17537.JPG
Informazioni sul file
Nome del file:as16-107-17483.JPG
Nome album:MareKromium / Original Nasa Apollo Frames: from Apollo 4 to Apollo 17
Valutazione (1 voti):55555(Mostra dettagli)
Parole chiave:Lunar / Surface / - / Station / 4 / Crater
Copyright:NASA - Apollo Programme - Apollo 16 e Lunar Explorer Italia per l'ulteriore processing del frame
Dimensione del file:2135 KiB
Data di inserimento:Dic 15, 2007
Dimensioni:4400 x 4600 pixels
Visualizzato:55 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=18927
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