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The Earth and Its Motion
Bawal matulog kapag nanonoood
Rotation of The Earth
Earth's rotation period relative to the Sun (true noon to true noon) is its true solar day or apparent
solar day. It depends on the Earth's orbital motion and is thus affected by changes in
the eccentricity and inclination of Earth's orbit. Both vary over thousands of years so the annual
variation of the true solar day also varies. Generally, it is longer than the mean solar day during two
periods of the year and shorter during another two.[n 1] The true solar day tends to be longer
near perihelion when the Sun apparently moves along the ecliptic through a greater angle than
usual, taking about 10 seconds longer to do so. Conversely, it is about 10 seconds shorter
near aphelion. It is about 20 seconds longer near a solstice when the projection of the Sun's
apparent movement along the ecliptic onto the celestial equator causes the Sun to move through a
greater angle than usual. Conversely, near an equinox the projection onto the equator is shorter by
about 20 seconds. Currently, the perihelion and solstice effects combine to lengthen the true solar
day near December 22 by 30 mean solar seconds, but the solstice effect is partially cancelled by the
aphelion effect near June 19 when it is only 13 seconds longer. The effects of the equinoxes shorten
it near March 26 and September 16 by 18 seconds and 21 seconds, respectively.[1][2][3]
Revolution of The Earth
Throughout the year, as our small blue planet orbits the Sun,
many parts of the Earth experience changing seasons. The warm
Spring brings new flowers, and young animals. This is followed
by a hot Summer, filled with vacations, hikes, and outdoor
swimming. Following Summer is another warm season known as
Autumn, where leaves turn beautiful shades of reds and browns
before falling off of their trees. Finally after all of these warmer
seasons comes one that is cold, wet, and dry, known as Winter.
Thank You for the Watching!
The Awesome Group of Saint
Ildephonsus
Yumi Takada
Nic Agnote
Kelly Basilan
Our Adviser: Ms. Kathrene
Asuncion

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The Earth and Its Motion

  • 1. The Earth and Its Motion
  • 4. Earth's rotation period relative to the Sun (true noon to true noon) is its true solar day or apparent solar day. It depends on the Earth's orbital motion and is thus affected by changes in the eccentricity and inclination of Earth's orbit. Both vary over thousands of years so the annual variation of the true solar day also varies. Generally, it is longer than the mean solar day during two periods of the year and shorter during another two.[n 1] The true solar day tends to be longer near perihelion when the Sun apparently moves along the ecliptic through a greater angle than usual, taking about 10 seconds longer to do so. Conversely, it is about 10 seconds shorter near aphelion. It is about 20 seconds longer near a solstice when the projection of the Sun's apparent movement along the ecliptic onto the celestial equator causes the Sun to move through a greater angle than usual. Conversely, near an equinox the projection onto the equator is shorter by about 20 seconds. Currently, the perihelion and solstice effects combine to lengthen the true solar day near December 22 by 30 mean solar seconds, but the solstice effect is partially cancelled by the aphelion effect near June 19 when it is only 13 seconds longer. The effects of the equinoxes shorten it near March 26 and September 16 by 18 seconds and 21 seconds, respectively.[1][2][3]
  • 6. Throughout the year, as our small blue planet orbits the Sun, many parts of the Earth experience changing seasons. The warm Spring brings new flowers, and young animals. This is followed by a hot Summer, filled with vacations, hikes, and outdoor swimming. Following Summer is another warm season known as Autumn, where leaves turn beautiful shades of reds and browns before falling off of their trees. Finally after all of these warmer seasons comes one that is cold, wet, and dry, known as Winter.
  • 7. Thank You for the Watching!
  • 8. The Awesome Group of Saint Ildephonsus
  • 12. Our Adviser: Ms. Kathrene Asuncion