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The Russian term Карта Мира or in transcription Karta Mira is now commonly used to describe this series, even outside the Soviet Union or Russia. The Karta Mira consists of a total of 224 (#1–17 & 28–234) main sheets and 38 overlap sheets (although at least 10 were dropped [clarification needed] [when?]). They depict the entire ...
During the interwar period, the Soviet project Bolshoi Sovietskii Atlas Mira, was produced. This was intended to be the most comprehensive atlas of modern times, remained, however, incomplete due to The Second World War; only two out of three planned volumes were published in 1937 and 1939.
A high-profile has been gained worldwide by map series published as a collaborative effort by several countries, especially the International Map of the World (1:1,000,000) (IMW) and the World Map / Karta Mira (1:2.500,000). The IMW was developed from 1913.
The Karta Mira or World Map was an atlas that was begun by Radó in July 1964. [120] The Soviet Union had used the 1-2,500,000 scale for their cartography since the 1930s and were familiar with its use. [ 121 ]
Early world maps cover depictions of the world from the Iron Age to the Age of Discovery and the emergence of modern geography during the early modern period.Old maps provide information about places that were known in past times, as well as the philosophical and cultural basis of the map, which were often much different from modern cartography.
Rock-cut tombs in Myra Rock-cut tombs in Myra. Although some scholars equate Myra with the town, of Mira, in Arzawa, there is no proof for the connection. [citation needed] There is no substantiated written reference for Myra before it was listed as a member of the Lycian League (168 BC–AD 43); according to Strabo (14:665), it was one of the largest towns of the alliance.
Krasnoyarsk [a] is the largest city and administrative center of Krasnoyarsk Krai, Russia.It is situated along the Yenisey River, and is the second-largest city in Siberia after Novosibirsk, with a population of over 1.1 million. [21]
Mira as seen by the Hubble Space Telescope in August 1997. Mira A is a variable star, specifically the prototypical Mira variable. The 6,000 to 7,000 known stars of this class [24] are all red giants whose surfaces pulsate in such a way as to increase and decrease in brightness over periods ranging from about 80 to more than 1,000 days.