Übersetzung für 'axial tilt' von Englisch nach Deutsch

axial tilt

Achsneigung {f}astron.tech.

Achsenneigung {f}astron.tech.

• The most striking involve Jupiter, which has four large moons and a low axial tilt, making eclipses more frequent as these bodies pass through the shadow of the larger planet.
• Paleontological evidence and computer simulations show that Earth's axial tilt is stabilized by tidal interactions with the Moon.
• Earth's axial tilt varies over a 41,000 year period from 22.1 to 24.5 degrees and currently resides at about 23.4 degrees.
• Likewise, they approximate the angle of the Earth's axial tilt.
• For planets and other rotating celestial bodies, the angle of the equatorial plane relative to the orbital plane – such as the tilt of the Earth's poles toward or away from the Sun – is sometimes also called inclination, but less ambiguous terms are axial tilt or obliquity.

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• This gives an axial tilt of 29°.
• He was also the first to calculate Earth's axial tilt, which has also proved to have remarkable accuracy.
• This impact hypothesis is also used in some attempts to explain the planet's axial tilt.
• The axial tilt of Jupiter is relatively small, only 3.13°, so its seasons are insignificant compared to those of Earth and Mars.
• The evaluation is controversial Herschel measured the axial tilt of Mars and in the process, took a measurement just beyond the red end of the visible spectrum.

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• Given its axial tilt of 97.77°, with its polar regions exposed to sunlight or darkness for long periods, scientists were not sure what to expect at Uranus.
• Owing to Earth's axial tilt of 23.439281°, winter in the Northern Hemisphere lasts from the December solstice (typically December 21 UTC) to the March equinox (typically March 20 UTC), while summer lasts from the June solstice through to the September equinox (typically on 23 September UTC).
• Nutation subtly changes the axial tilt of Earth with respect to the ecliptic plane, shifting the major circles of latitude that are defined by the Earth's tilt (the tropical circles and the polar circles).
• Mercury's axial tilt is almost zero, with the best measured value as low as 0.027 degrees.
• A further improvement defines a fictitious mean Sun that moves with constant speed along the celestial equator; the speed is the same as the average speed of the real Sun, but this removes the variation over a year as the Earth moves along its orbit around the Sun (due to both its velocity and its axial tilt).

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