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  2. Earth's rotation - Wikipedia

    en.wikipedia.org/wiki/Earth's_rotation

    Earth's rotation axis moves with respect to the fixed stars (inertial space); the components of this motion are precession and nutation. It also moves with respect to Earth's crust; this is called polar motion. Precession is a rotation of Earth's rotation axis, caused primarily by external torques from the gravity of the Sun, Moon and other bodies.

  3. Solarigraphy - Wikipedia

    en.wikipedia.org/wiki/Solarigraphy

    Solarigraphs are images that show real elements that cannot be seen with the naked eye, they represent the apparent trajectories of the sun in the sky due to the rotation of the Earth on its axis. They are mostly made with pinhole cameras and very long exposures, from one day to six months between the winter solstice and the summer solstice or ...

  4. Star trail - Wikipedia

    en.wikipedia.org/wiki/Star_trail

    A star trail is a type of photograph that uses long exposure times to capture diurnal circles, the apparent motion of stars in the night sky due to Earth's rotation. A star-trail photograph shows individual stars as streaks across the image, with longer exposures yielding longer arcs.

  5. Sidereal time - Wikipedia

    en.wikipedia.org/wiki/Sidereal_time

    Sidereal time is a "time scale that is based on Earth's rate of rotation measured relative to the fixed stars". [ 1 ] 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 (also known as the sidereal ...

  6. WorldWide Telescope - Wikipedia

    en.wikipedia.org/wiki/WorldWide_Telescope

    Images without AVM can be shown on the sky but the user must align the images in the sky by moving, scaling and rotating the images until star patterns align. Once the images are aligned they can be saved to collections for later viewing and sharing. The layer manager can be used to add vector or image data to planet surfaces or in orbit. [11]

  7. Earth - Wikipedia

    en.wikipedia.org/wiki/Earth

    Earth's rotation period relative to the Sun—its mean solar day—is 86,400 seconds of mean solar time (86,400.0025 SI seconds). [156] Because Earth's solar day is now slightly longer than it was during the 19th century due to tidal deceleration , each day varies between 0 and 2 ms longer than the mean solar day.

  8. AOL Mail

    mail.aol.com

    Get AOL Mail for FREE! Manage your email like never before with travel, photo & document views. Personalize your inbox with themes & tabs. You've Got Mail!

  9. Timeline of first images of Earth from space - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_first_images...

    First images and view of a sunset and sunrise over Earth at the same time, a solar eclipse by Earth (a celestial body other than the Moon), from the Moon's surface. [37] [38] April 30, 1967 First color image of Earth from another astronomical object's surface, the Moon's surface. [39] September 20, 1967 (released November 10th) [40] DODGE