Difficulty: Easy
Correct Answer: Equator
Explanation:
Introduction / Context:
The length of day and night changes with latitude and season due to the tilt of the Earth's axis and its revolution around the Sun. However, there is one special line on the Earth where days and nights are always very close to equal throughout the year. This question tests fundamental understanding of how latitude affects day length, a topic commonly covered in school geography and competitive exams.
Given Data / Assumptions:
Concept / Approach:
The key concept is that the Equator is the line of zero latitude that lies halfway between the North and South Poles. Because of the geometry of the Earth Sun relationship, the Equator receives almost equal amounts of daylight and darkness throughout the year. While slight variations can occur due to atmospheric refraction and the definition of sunrise and sunset, in school level geography the equatorial region is treated as the place where day and night remain nearly 12 hours each every day. In contrast, the poles experience extreme variations, including continuous day or night for months.
Step-by-Step Solution:
Step 1: Recall that at the Equator, the Sun is overhead at noon on the equinoxes, and the path of the Sun across the sky gives roughly 12 hours of daylight and 12 hours of darkness daily.Step 2: Remember that at higher latitudes, day length varies with seasons, becoming longer in summer and shorter in winter.Step 3: Note that at the poles, extremes occur, with polar day and polar night lasting for long periods, so day and night are not always equal there.Step 4: Understand that the Prime Meridian is a line of longitude, not latitude, and does not control day length in the way latitude does.Step 5: Conclude that the Equator is the place where day and night remain approximately equal throughout the year.
Verification / Alternative check:
To verify, consider the definition of equinoxes, which are the dates when day and night are equal everywhere on Earth. At the Equator, this near equality extends throughout the year, because the Sun's apparent movement is symmetrical about the equator. Geography textbooks usually illustrate this with diagrams showing the circle of illumination and explaining that, at the Equator, the day night division always cuts the globe in such a way that the equatorial regions receive equal halves of light and darkness.
Why Other Options Are Wrong:
Prime Meridian: This is the zero degree longitude line that passes through Greenwich. It is important for time zones but does not guarantee equal day and night length.
Poles: The North and South Poles experience extreme seasonal variation with six months of continuous daylight and six months of continuous night, so they do not have equal days and nights all year.
Nowhere: This is incorrect because the Equator clearly provides a well known example where days and nights stay nearly equal in length throughout the year.
Common Pitfalls:
Some candidates confuse meridians with parallels and may think that the Prime Meridian has special effects on day length. Others might underestimate how extreme conditions at the poles are and mistakenly guess poles as the answer. To avoid such mistakes, always remember that latitude primarily controls climate and daylight variation, and the Equator is the special latitude where the seasonal variation in day length is minimal.
Final Answer:
Days and nights are always of equal length at the Equator.
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