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Gold signet ring from Mycenae with similar celestial imagery, fifteenth century BC [61] A depiction of a sun and crescent moon similar to the Nebra disc appears on a gold signet ring from Mycenae in Greece, dating from the fifteenth century BC.
In its full form, a corona consists of several concentric, pastel-colored rings around the celestial object and a central bright area called an aureole. [ 2 ] [ 3 ] The aureole is often (especially in case of the Moon ) the only visible part of the corona and has the appearance of a bluish-white disk which fades to reddish-brown towards the edge.
In Greek antiquity the ideas of celestial spheres and rings first appeared in the cosmology of Anaximander in the early 6th century BC. [7] In his cosmology both the Sun and Moon are circular open vents in tubular rings of fire enclosed in tubes of condensed air; these rings constitute the rims of rotating chariot-like wheels pivoting on the Earth at their centre.
A halo (from Ancient Greek ἅλως (hálōs) 'threshing floor, disk') [1] is an optical phenomenon produced by light (typically from the Sun or Moon) interacting with ice crystals suspended in the atmosphere. Halos can have many forms, ranging from colored or white rings to arcs and spots in the sky.
Jost Bürgi and Antonius Eisenhoit: Armillary sphere with astronomical clock, made in 1585 in Kassel, now at Nordiska Museet in Stockholm. An armillary sphere (variations are known as spherical astrolabe, armilla, or armil) is a model of objects in the sky (on the celestial sphere), consisting of a spherical framework of rings, centered on Earth or the Sun, that represent lines of celestial ...
The ecliptic forms the center of the zodiac, a celestial belt about 20° wide in latitude through which the Sun, Moon, and planets always appear to move. [33] Traditionally, this region is divided into 12 signs of 30° longitude, each of which approximates the Sun's motion in one month. [ 34 ]
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