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  2. Axial precession - Wikipedia

    en.wikipedia.org/wiki/Axial_precession

    The rotation axis of the Earth describes, over a period of 25,700 years, a small blue circle among the stars near the top of the diagram, centered on the ecliptic north pole (the blue letter E) and with an angular radius of about 23.4°, an angle known as the obliquity of the ecliptic. The direction of precession is opposite to the daily ...

  3. Earth's rotation - Wikipedia

    en.wikipedia.org/wiki/Earth's_rotation

    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 ).

  4. Diurnal motion - Wikipedia

    en.wikipedia.org/wiki/Diurnal_motion

    The daily arc path of an object on the celestial sphere, including the possible part below the horizon, has a length proportional to the cosine of the declination.Thus, the speed of the diurnal motion of a celestial object equals this cosine times 15° per hour, 15 arcminutes per minute, or 15 arcseconds per second.

  5. 10 Period Myths That You Definitely Should Not Believe (Like ...

    www.aol.com/lifestyle/10-period-myths-definitely...

    Here we debunk 10 period myths, including why it's ok (and safe) to swim on your period, why your period does not stop in water, and more.

  6. South Pole - Wikipedia

    en.wikipedia.org/wiki/South_Pole

    The South Pole is at an altitude of 9,200 feet (2,800 m) but feels like 11,000 feet (3,400 m). [34] Centripetal force from the spin of the planet throws the atmosphere toward the equator. The South Pole is colder than the North Pole primarily because of the elevation difference and for being in the middle of a continent. [35]

  7. What will happen when Earth's north and south poles flip

    www.aol.com/article/news/2019/02/05/what-will...

    Our compasses are just pointing to one pole at a time because there’s a dominant two-pole system. But sometimes, Earth doesn’t always just have a single magnetic North and South Pole.

  8. True polar wander - Wikipedia

    en.wikipedia.org/wiki/True_polar_wander

    This diagram of true polar wander shows the present-day Earth rotating with respect to its rotational axis. True polar wander is a solid-body rotation (or reorientation) of a planet or moon with respect to its spin axis, causing the geographic locations of the north and south poles to change, or "wander".

  9. Celestial pole - Wikipedia

    en.wikipedia.org/wiki/Celestial_pole

    The south celestial pole over the Very Large Telescope [3] Locating the south celestial pole. The south celestial pole is visible only from the Southern Hemisphere. It lies in the dim constellation Octans, the Octant. Sigma Octantis is identified as the south pole star, more than one degree away from the pole, but with a magnitude of 5.5 it is ...