* Spread out energy: When sunlight hits Earth at a more direct angle (closer to 90 degrees), the energy is concentrated over a smaller area. This results in a higher temperature.

* Less energy per unit area: As the angle becomes more oblique (closer to 0 degrees), the sunlight spreads out over a larger area. This means each unit of area receives less energy, leading to a lower temperature.

Think of it like this:

Imagine shining a flashlight directly onto a wall. The light is concentrated and bright. Now angle the flashlight. The light spreads out, becoming dimmer. The same principle applies to sunlight and Earth's temperature.

Examples:

* Equator: The equator receives sunlight at a near-perpendicular angle year-round, resulting in higher temperatures.

* Poles: The poles receive sunlight at a very oblique angle, leading to much lower temperatures.

* Seasons: During summer in the Northern Hemisphere, the sun's rays are more direct, while in winter, the rays are more oblique, resulting in colder temperatures.

In summary: The angle at which sunlight strikes Earth's surface directly impacts the amount of energy received per unit area, which in turn determines the temperature.