Understanding Sunspots — Passage

Grades
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2
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5
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This learning resource is available in interactive and printable formats. The interactive worksshet can be played online and assigned to students. The Printable PDF version can be downloaded and printed for completion by hand.
ABOUT THIS READER
Sunspots are fascinating dark patches on the Sun's surface caused by intense magnetic activity that lowers the temperature in these regions. Despite appearing dark, sunspots are extremely hot, with temperatures of around 4,000°C (7,232°F), compared to the surrounding areas that reach 5,500°C (9,932°F). Sunspots often occur in pairs or groups and are closely linked to the Sun’s 11-year solar cycle. During the solar maximum, the number of sunspots increases, while during the solar minimum, they become less frequent. These magnetic phenomena can influence Earth by causing minor disruptions in radio signals and navigation systems. They are also responsible for creating stunning auroras, like the Northern and Southern Lights, near Earth’s poles. Understanding sunspots not only helps us learn about solar activity but also allows scientists to predict its effects on technology and the environment. This topic aligns with Common Core standards by integrating scientific knowledge and Earth-space concepts, encouraging students to explore connections between celestial phenomena and everyday life.
Publisher: Workybooks
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Written by:Neha Goel Tripathi
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Illustrated by:
Sunspots,Magnetic activity, Solar maximum, Solar minimum, Auroras

Sunspots are dark areas on the Sun’s surface that appear as spots. They are caused by strong magnetic activity, which reduces the temperature in those areas compared to the surrounding regions. Sunspots are usually found in pairs or groups and can last for a few days to a few months.

 

Sunspots are cooler than the rest of the Sun’s surface, with temperatures around 4,000°C (7,232°F), while the surrounding areas can reach 5,500°C (9,932°F). Although sunspots appear dark, they are still very bright and hot compared to Earth’s standards.

 

The number of sunspots varies over an 11-year cycle, known as the solar cycle. During the peak of this cycle, called the solar maximum, the number of sunspots increases. Conversely, during the solar minimum, the number of sunspots decreases.

 

Sunspots can have effects on Earth. They can cause minor disruptions in radio communications and navigation systems when they are particularly active. However, they can also produce beautiful auroras, known as the Northern and Southern Lights, near Earth’s poles.

What causes sunspots on the Sun’s surface?

Increased solar radiationStrong magnetic activityHigh temperaturesGravitational forces

How long can sunspots last?

A few hoursSeveral yearsA few days to a few monthsThey are permanent features

What is the temperature of sunspots compared to the surrounding areas?

Cooler, around 4,000°C (7,232°F)Hotter, around 7,000°C (12,632°F)The same temperatureCooler, around 2,000°C (3,632°F)

What is the term for the peak of the 11-year solar cycle?

Solar minimumSolar maximumSolar eclipseSolar flare

During which phase of the solar cycle are there more sunspots?

Solar minimumSolar equinoxSolar eclipseSolar maximum

What natural phenomenon can sunspots produce near Earth's poles?

EarthquakesAuroras (Northern and Southern Lights)TsunamisVolcanic eruptions

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