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Roman plate; 1st–2nd century AD; height: 0.1 cm, diameter: 12.7 cm; Metropolitan Museum of Art Roman bust of Serapis ; 2nd century; 15.6×9.5 cm; Metropolitan Museum of Art Auricular basin with scenes from the story of Diana and Actaeon; 1613; length: 50 cm, height: 6 cm, width: 40 cm; Rijksmuseum ( Amsterdam , the Netherlands )
1929: Under the Series of 1928, all U.S. currency was changed to its current size and began to carry a standardized design. All variations of the $100 bill would carry the same portrait of Benjamin Franklin, same border design on the obverse, and the same reverse with a vignette of Independence Hall.
An alternative is to consider the depth of field given by the same lens in conjunction with different sized sensors (changing the angle of view). The change in depth of field is brought about by the requirement for a different degree of enlargement to achieve the same final image size. In this case the ratio of depths of field becomes
A temporal dimension is one way to measure physical change. It is perceived differently from the three spatial dimensions in that there is only one of it, and that we cannot move freely in time but subjectively move in one direction. The equations used in physics to model reality do not treat time in the same way that humans commonly perceive it.
They are coated with a shallow layer of magnetic material typically 10–20 nm in depth, with an outer layer of carbon for protection. [ 47 ] [ 48 ] [ 49 ] For reference, a standard piece of copy paper is 0.07–0.18 mm (70,000–180,000 nm) [ 50 ] thick.
Size comparison of Earth and Uranus. Uranus's mass is roughly 14.5 times that of Earth, making it the least massive of the giant planets. Its diameter is slightly larger than Neptune's at roughly four times that of Earth. A resulting density of 1.27 g/cm 3 makes Uranus the second least dense planet, after Saturn.
Comparison of a 10 km radius neutron star (top left corner) and a 6000 km radius white dwarf, the latter roughly the size of Earth. Neutron stars have overall densities of 3.7 × 10 17 to 5.9 × 10 17 kg/m 3 ( 2.6 × 10 14 to 4.1 × 10 14 times the density of the Sun), [ a ] which is comparable to the approximate density of an atomic nucleus of ...
Drag coefficients in fluids with Reynolds number approximately 10 4 [1] [2] Shapes are depicted with the same projected frontal area. In fluid dynamics, the drag coefficient (commonly denoted as: , or ) is a dimensionless quantity that is used to quantify the drag or resistance of an object in a fluid environment, such as air or water.
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