Zobrazit minimální záznam

dc.contributor.authorWeyburne, Kyle
dc.date.accessioned2021-08-31T08:04:03Z
dc.date.available2021-08-31T08:04:03Z
dc.date.issued2021
dc.identifier.urihttp://hdl.handle.net/20.500.11956/136485
dc.language.isoencs
dc.publisherUniverzita Karlova, Filozofická fakultacs
dc.subjectchimneycs
dc.subjectSnefrucs
dc.subjectBent Pyramidcs
dc.subjectsolar elevationscs
dc.subjectRhind Papyruscs
dc.titleUsing the so‑called chimney in the Bent Pyramid to measure solar elevations in summercs
dc.typeVědecký článekcs
dcterms.accessRightsopenAccess
dcterms.licensehttp://creativecommons.org/licenses/by-nc-nd/2.0/
uk.abstract.enThe so called “chimney” is a deep, vertical shaft located in the centre of the Bent Pyramid that starts at ground level and descends for over 15 metres into the earth. While the purpose of this chimney is disputed in scholarly literature, this paper offers the speculative hypothesis that it served as a tool for solar obser vations. For a period of time (before the pyramid was built above it), the shaft would have been open to the elements, allowing the sun’s light to reach the bottom corner at the summer solstice, and thereby dividing this structure into two equal, but inverse triangles: one filled with light, the other dark. This precision sug gests that the chimney may have been specifically designed to enable this phenomenon to occur. Moreover, further investigation shows that, for a period of 47 days centred around the solstice, the sun created a line of light on the floor of the chimney that would have made it possible to accurately measure solar elevations.cs
dc.publisher.publicationPlacePrahacs
uk.internal-typeuk_publication
dc.description.startPage126cs
dc.description.endPage138cs
dcterms.isPartOf.namePražské egyptologické studiecs
dcterms.isPartOf.journalYear2021
dcterms.isPartOf.journalVolume2021
dcterms.isPartOf.journalIssue26
dcterms.isPartOf.issn1801-3899
dc.relation.isPartOfUrlhttps://pes.ff.cuni.cz


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Zobrazit minimální záznam


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