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The Sun is 1.4 million kilometers (4.643 light-seconds) wide, about 109 times wider than Earth, or four times the Lunar distance, and contains 99.86% of all Solar System mass. The Sun is a G-type main-sequence star that makes up about 99.86% of the mass of the Solar System. [26]
According to many researchers, dolmens and cromlechs known in Azerbaijan are also associated with the cult of the Sun. [3] Ethnographers of the mythological school of the 18-19th centuries gave exaggerated significance to solar myths, declaring various cult heroes and mythological characters as personifications of the Sun, who in fact have no ...
If the Sun–Neptune distance is scaled to 100 metres (330 ft), then the Sun would be about 3 cm (1.2 in) in diameter (roughly two-thirds the diameter of a golf ball), the giant planets would be all smaller than about 3 mm (0.12 in), and Earth's diameter along with that of the other terrestrial planets would be smaller than a flea (0.3 mm or 0. ...
For example, a fact could be "The Earth orbits the sun." You can usually verify such facts through scientific methods or observation. Opinions, on the other hand, are personal views or ...
Ace trivia night with these cool and random fun facts for adults and kids. This list of interesting facts is the perfect way to learn something new about life. 105 Fun Facts About Science, History ...
And the Instagram page ‘Unbelievable Facts’ is one of the best places to do just that. Every day, they share fascinating trivia, building a collection that now includes over 10,000 unique facts.
In the Sun, the region between the solar core at 0.2 of the Sun's radius and the outer convection zone at 0.71 of the Sun's radius is referred to as the radiation zone, although the core is also a radiative region. [1] The convection zone and the radiative zone are divided by the tachocline, another part of the Sun.
The solar transition region is a region of the Sun's atmosphere between the upper chromosphere and corona. [1] [2] It is important because it is the site of several unrelated but important transitions in the physics of the solar atmosphere: