equality of the rotation angles - translation to ρωσικά
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equality of the rotation angles - translation to ρωσικά

ROTATION OF EARTH AROUND ITS AXIS
Rotation of Earth; Earth rotation; Rotation of the Earth; Rotation of the earth; Earths rotation; Slowing of Earth; Slowing of the Earth; Slowing of Earth's rotation; Slowing of the Earth's rotation; Stellar day; Earth's rotation period; Earth's rotation speed
  • 000-year}} cycle and is currently decreasing.
  • Deviation of day length from SI-based day
  • apparent paths]] of the stars as Earth rotates.
  • Earth's rotation imaged by [[Deep Space Climate Observatory]], showing axis tilt
  • solar day]]. At time 1, the Sun and a certain distant star are both overhead. At time 2, the planet has rotated 360° and the distant star is overhead again but the Sun is not (1→2 = one stellar day). It is not until a little later, at time 3, that the Sun is overhead again (1→3 = one solar day).
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equality of the rotation angles      

строительное дело

равенство углов поворота (сечений)

equality of the rotation angles      
равенство углов поворота (сечений)
equal terms         
  • Sir George Arthur]] to [[Indigenous Tasmanians]], purporting to show the equality of white and black before the law
  • Statue of Equality in Paris as an allegory of equality
PRINCIPLE THAT EACH INDIVIDUAL MUST BE TREATED EQUALLY BY THE LAW WITHOUT DISCRIMINATION OR PRIVILEGES BY THE GOVERNMENT
Democratic egalitarianism; One law for all; Equality under the law; Equality under law; Legal egalitarianism; Equal before the law; Equality of all citizens before the law; Legal equality; Right to equality before the law; Equality before law; Equal terms; Equality in the eyes of the law; All are equal in the eyes of the law; All are equal in the eyes of law; Right to equality; Judicial equality; Equal rights before the law; Equality of rights
одинаковые условия

Ορισμός

БИБЛИОТЕКА КОНГРЕССА
национальная библиотека США, в Вашингтоне. Основана в 1800. В 1993 св. 86 млн. ед. хр., фонд почти универсален (кроме иностранной, сельскохозяйственной и медицинской литературы). Редкие американские издания, коллекции инкунабул, китайской, японской и других литерар; собрание русских изданий (св. 300 тыс. названий, в т. ч. библиотека Г. Юдина). Ведет информационное обслуживание конгресса США, специалистов и других читателей.

Βικιπαίδεια

Earth's rotation

Earth's rotation or Earth's spin is the rotation of planet Earth around its own axis, as well as changes in the orientation of the rotation axis in space. Earth rotates eastward, in prograde motion. As viewed from the northern polar star Polaris, Earth turns counterclockwise.

The North Pole, also known as the Geographic North Pole or Terrestrial North Pole, is the point in the Northern Hemisphere where Earth's axis of rotation meets its surface. This point is distinct from Earth's North Magnetic Pole. The South Pole is the other point where Earth's axis of rotation intersects its surface, in Antarctica.

Earth rotates once in about 24 hours with respect to the Sun, but once every 23 hours, 56 minutes and 4 seconds with respect to other distant stars (see below). Earth's rotation is slowing slightly with time; thus, a day was shorter in the past. This is due to the tidal effects the Moon has on Earth's rotation. Atomic clocks show that a modern day is longer by about 1.7 milliseconds than a century ago, slowly increasing the rate at which UTC is adjusted by leap seconds. Analysis of historical astronomical records shows a slowing trend; the length of a day increased about 2.3 milliseconds per century since the 8th century BCE.

Scientists reported that in 2020 Earth had started spinning faster, after consistently spinning slower than 86,400 seconds per day in the decades before. On June 29, 2022, Earth's spin was completed in 1.59 milliseconds under 24 hours, setting a new record. Because of that trend, engineers worldwide are discussing a 'negative leap second' and other possible timekeeping measures.

This increase in speed is thought to be due to various factors, including the complex motion of its molten core, oceans, and atmosphere, the effect of celestial bodies such as the Moon, and possibly climate change, which is causing the ice at Earth's poles to melt. The masses of ice account for the Earth's shape being that of an oblate spheroid, bulging around the equator. When these masses are reduced, the poles rebound from the loss of weight, and Earth becomes more spherical, which has the effect of bringing mass closer to its centre of gravity. Conservation of angular momentum dictates that a mass distributed more closely around its centre of gravity spins faster.

Μετάφραση του &#39equality of the rotation angles&#39 σε Ρωσικά