Morning Dew

950 Words2 Pages

Science NCEA Level 1
AS90954 (Science 1.15)
Demonstrate comprehensive understanding of astronomical cycles and their affects on earth.

What are Astronomical Cycles (and their relevance to the effects they have on Earth)?
Astronomical Cycles:
Astronomical cycles are mainly associated with orbits of a primary body (in this case the Sun) by a satellite (the earth). Astronomical cycles can also refer to the systems specific to a satellite (the spin and tilt of the earth). Astronomical cycle’s specific to earth serve as a reference for our measurement of time and play an important role in the earth’s climate and ecology. Things such as seasons, temperature increase and decrease, and weather cycles are all caused by the astronomical cycles relevant to earth; to be specific, the spin of the earth and the tilt of the earth.

Identification of Astronomical Cycles Specific to Earth:
The Cycles:
- The Spin of The Earth:
The spin of the earth refers to the rotation of the earth on its axis. The earth spins anti-clockwise on an axis which runs from the North Pole (the arctic) to the South Pole (Antarctic). It takes exactly 23 hours 56 minutes and 4 seconds at a rate of 1,670 kph (at the equator) for the earth to complete a full rotation in context with the sun. This spin is caused by the conservation of angular momentum. Since space is a vacuum, the earth will continue with this momentum for as long as no significant forces disrupt the momentum.
- Effects It Causes:
Day and Night:
The spin of the Earth is the reason we have day and night. The logic is simple, when one side of the Earth is facing the sun we call that day and when one side of the Earth is facing away from the sun we call that night. Around half of the Earth experiences day an...

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... sun) affects the temperature we feel as well as how visible it is during the day. Days in the southern hemisphere during summer seem longer and generally have warmer and brighter days. As shown on the diagram to the right, the north hemisphere (during the summer) tilts towards the sun, therefore it has more exposure. The north hemisphere has a wedge of sunlight that sits in between the orbital axis and the rotational axis, When this is compared to the southern hemisphere which has a wedge of darkness (night), it shows that the north hemisphere has longer days than the south hemisphere. This is especially apparent when we take into consideration that the equator, which experiences equal length days and nights, sits on the intersection between the orbital axis (where day and night meet) and the rotational axis (the white line). This next diagram shows this perfectly.

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