Daylight Patterns — Latitude and Seasonal Effects Which statements about the length of daylight on Earth are correct?

Introduction / Context:
Daylight duration across Earth is controlled by axial tilt and latitude. Understanding these patterns explains phenomena such as equatorial day-length stability, mid-latitude seasonal swings, and polar day/night extremes (midnight sun and polar night).

Given Data / Assumptions:

• Earth’s axis is tilted about 23.5 degrees relative to its orbital plane.
• We consider typical annual behavior, not short-term weather effects.
• Polar “24-hour day” refers to continuous daylight within the Arctic/Antarctic Circles during respective summers.

Concept / Approach:
Near the equator, day length stays close to 12 hours year-round because the Sun’s apparent path crosses the sky at steep angles regardless of season. With increasing latitude, seasonal variation grows: longer days in summer, shorter in winter. Inside the polar circles, the Sun can remain above the horizon for 24 hours (midnight sun) in summer and remain below it in winter (polar night). Thus each individual statement is correct, making the inclusive choice appropriate.

Step-by-Step Solution:

Verification / Alternative check:
Globe-and-tilt diagrams and sunrise/sunset tables show near-constant ~12-hour days at the equator and 24-hour daylight spans above 66.5° latitude in their respective summers.

Why Other Options Are Wrong:

• Choosing only one or two statements ignores the full latitudinal pattern dictated by Earth’s axial tilt.

Common Pitfalls:
Assuming equatorial places have exactly 12:00 hours year-round; small deviations occur, but the key idea is “nearly constant,” which is correct.

Final Answer:
All of the above