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geologia: Earth
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9 zapisanych źródełEvidence: 94 • authority: 72
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 called the Geographic North Pole or Terrestrial North Pole, is the point in the Northern Hemisphere at which 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 at which 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 hour…
Otwórz źródło ↗Evidence: 42 • authority: 72
Sidereal time ("sidereal" pronounced sy-DEER-ee-əl, sə-) is a system of timekeeping used especially by astronomers. Using sidereal time and the celestial coordinate system, it is easy to locate the positions of celestial objects in the night sky. Sidereal time is a "time scale that is based on Earth's rate of rotation measured relative to the fixed stars". A sidereal day (also known as the sidereal rotation period) represents the time for one rotation about the planet axis relative to the stars. Viewed from the same location, a star seen at one position in the sky will be seen at the same position on another night at the same time of day (or night), if the day is defined as a sidereal day.…
Otwórz źródło ↗Evidence: 34 • authority: 80
Another System Wherein the Earth is Situated in the Center of the World and Moves About Its Own Axis in the Space of Twenty-Four Hours
Otwórz źródło ↗Evidence: 25 • authority: 72
A near-Earth object (NEO) is by definition any small Solar System body orbiting the Sun whose closest approach to the Sun (perihelion) is less than 1.3 times the Earth–Sun distance (astronomical unit, AU). This definition applies to the object's orbit around the Sun, rather than its current position, thus an object with such an orbit is considered a NEO even at times when it is far from making a close approach of Earth. If a NEO's orbit crosses the Earth's orbit, and the object is larger than 140 meters (460 ft) across, it is, by definition, considered a potentially hazardous object (PHO). Most known PHOs and NEOs are asteroids, but about a third of a percent are comets. There are over 37,0…
Otwórz źródło ↗Evidence: 25 • authority: 80
Observational Indications that the Velocity of the Wireless Wave around the Earth is about 10 percent less than that of Light
Otwórz źródło ↗Evidence: 25 • authority: 80
Curious Kids: What makes the Earth spin on its axis every day?
Otwórz źródło ↗Evidence: 25 • authority: 80
Earth “rotates” around parked plane by use of electronics
Otwórz źródło ↗Evidence: 25 • authority: 72
In astronomy, axial precession is a gravity-induced, slow, and continuous change in the orientation of an astronomical body's rotational axis. In the absence of precession, the astronomical body's orbit would show axial parallelism. In particular, Earth's axial precession is the gradual shift in the orientation of Earth's axis of rotation. It has a cycle of approximately 26,000 years, tracing out a double cone with a half-aperture of about 23.4°, an angle known as the obliquity of the ecliptic. This is similar to the precession of a spinning top. The term "precession" typically refers only to this largest part of the motion; other changes in the alignment of Earth's axis—nutation and polar…
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