enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. Earth's rotation - Wikipedia

    en.wikipedia.org/wiki/Earth's_rotation

    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 the modern day is longer by about 1.7 milliseconds than a century ago, [1] slowly increasing the rate at which UTC is adjusted by leap seconds.

  3. Tidal acceleration - Wikipedia

    en.wikipedia.org/wiki/Tidal_acceleration

    This process alone leads to an increase of the rotation rate (phenomenon of a spinning figure skater who spins ever faster as they retract their arms). From the observed change in the moment of inertia the acceleration of rotation can be computed: the average value over the historical period must have been about −0.6 ms/century.

  4. Inner core super-rotation - Wikipedia

    en.wikipedia.org/wiki/Inner_core_super-rotation

    Waves were observed to travel faster between north and south than along the equatorial plane. A model for the inner core with uniform anisotropy had a direction of fastest travel tilted at an angle 10° from the spin axis of the Earth. [15] Since then, the model for the anisotropy has become more complex. The top 100 kilometers are isotropic.

  5. Earth Is Spinning Faster Than Usual, Giving Us the Shortest ...

    www.aol.com/earth-spinning-faster-usual-giving...

    This minuscule change in time means we might need to consider a negative leap second. Earth Is Spinning Faster Than Usual, Giving Us the Shortest Day EVER Recorded Skip to main content

  6. Earth’s spin is believed to be speeding up - AOL

    www.aol.com/earth-spin-believed-speeding...

    Earth has reportedly reached its quickest spin speeds in the past half-century.

  7. We Know How Fast Earth Spins ... Don’t We? - AOL

    www.aol.com/lifestyle/know-fast-earth-spins-don...

    Earth rotates on its axis at about 1,000 miles per hour. That’s the short answer, but it’s not the whole story.

  8. Day length fluctuations - Wikipedia

    en.wikipedia.org/wiki/Day_length_fluctuations

    This implies a strong coupling between atmosphere and solid Earth due to surface friction with a time constant of about 7 days, the spin-down time of the Ekman layer. This spin-down time is the characteristic time for the transfer of atmospheric axial angular momentum to Earth's surface and vice versa. The zonal wind-component on the ground ...

  9. Axial precession - Wikipedia

    en.wikipedia.org/wiki/Axial_precession

    At present, the rate of precession corresponds to a period of 25,772 years, so tropical year is shorter than sidereal year by 1,224.5 seconds (20 min 24.5 sec ≈ (365.24219 × 86400) / 25772). The rate itself varies somewhat with time (see Values below), so one cannot say that in exactly 25,772 years the Earth's axis will be back to where it ...