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Dark patches on the sun's surface, known as sunspots, are areas of reduced temperature caused by magnetic activity inhibiting heat transfer. They are temporary phenomena that appear darker than their surroundings due to their cooler temperatures. Sunspots are associated with increased solar activity and can impact Earth's space weather.
Dark patches on the sun's surface are known as sunspots. They appear darker because they are cooler regions on the sun's surface where magnetic activity inhibits the flow of heat. Sunspots can be large and can last for days or weeks before dissipating.
Dark areas on the surface of the sun are called sunspots. They appear darker because they are cooler areas compared to their surroundings due to strong magnetic activity. Sunspots are temporary phenomena that can last from days to weeks.
The dark patches on the moon are known as lunar maria, which are ancient basaltic plains formed by volcanic activity. The light patches are highlands, which are older and more heavily cratered. The contrast between these two types of terrain creates the distinctive pattern of dark and light patches seen on the moon's surface.
The dark area is known as a sunspot on the Sun's surface. Sunspots appear darker because they are cooler than their surroundings. They are caused by strong magnetic activity that inhibits convection and reduces temperature.
The flat areas on the moon are called lunar maria. They are dark plains formed by ancient volcanic activity and are visible from Earth as dark patches on the moon's surface.