How Incoming Solar Radiation Changes with Latitude — Reading Comprehension
Rate this
Premium Resource
Present
Present in classroom. No work saved
Assign
Classroom with student accounts, Track progress
Quick Play
No student accounts, assign with a link
Grades
3
4
5
6
7
Standards
MS-ESS1-1
PRINT+DIGITAL RESOURCE
This learning resource is available in interactive and printable formats. The interactive worksheet can be played online and assigned to students. The Printable PDF version can be downloaded and printed for completion by hand.
This NGSS-aligned science reading passage helps middle school students understand how solar radiation, or insolation, changes with latitude. It explains why areas near the equator receive more direct sunlight while regions near the poles receive less, due to the angle of the Sun’s rays. The passage also explores how Earth's tilt causes seasonal differences in sunlight and temperature. These variations help explain climate zones and the differences in weather and ecosystems across the globe. The passage supports science reading comprehension and includes essential vocabulary like latitude, insolation, equator, and greenhouse effect. It is ideal for lessons on Earth’s energy system, seasons, and climate under NGSS Earth and Space Science standards.
CONTENT PREVIEW
Expand content preview
Incoming solar radiation, also known as insolation, is the sunlight that reaches Earth’s surface. The amount of solar radiation a place receives depends on its latitude, or distance from the equator. Latitude plays a major role in shaping Earth’s climates, temperatures, and seasons.
At the equator (0° latitude), the Sun’s rays hit Earth almost directly throughout the year. This means sunlight is more concentrated and delivers more energy to the surface. That’s why tropical regions near the equator are typically warm and receive consistent sunlight all year long.
As you move toward the poles (higher latitudes like 60° or 90°), the Sun’s rays strike Earth at a lower angle. This spreads the energy over a larger area and reduces its intensity. Because of this, regions near the poles receive less solar radiation and are much colder. The Sun also rises lower in the sky and may not appear at all during some parts of winter in polar areas.
Latitude also affects seasonal changes in solar radiation. For example, during summer in the Northern Hemisphere, the North Pole tilts toward the Sun, so places like the United States get longer days and more sunlight. In winter, the North Pole tilts away from the Sun, leading to shorter days and less incoming solar energy.
This variation in solar radiation with latitude helps explain Earth’s climate zones—tropical, temperate, and polar. It also influences ecosystems, agriculture, and how people adapt to their environments.
Fun Fact: During summer, the Arctic Circle can have up to 24 hours of sunlight a day—this is called the
!
What is solar radiation also called?
Light speedInsolationReflectionRotation
Which part of Earth gets the most direct sunlight?
The polesThe equatorThe oceansThe mountains
Why do areas near the poles receive less solar radiation?
They are farther from the MoonThey reflect more lightThe Sun's rays hit at a lower angleThere are more clouds
What happens to sunlight at higher latitudes?
It becomes strongerIt covers a smaller areaIt is more concentratedIt spreads out more
What causes seasonal changes in solar radiation?
Earth’s distance from the SunEarth’s rotationEarth’s tilted axisThe shape of Earth
What is the climate like at the equator?
Cold and icyWindy and dryWarm and consistentCloudy all year
What is the main idea of the passage?
The Sun only shines near the equatorSolar radiation changes due to weatherLatitude affects how much solar radiation places receiveSunlight always hits Earth equally
If a place gets very little sunlight in winter, what can you guess about its latitude?
It is close to the equatorIt is in the Southern HemisphereIt is near a desertIt is closer to the poles
Perfect For:
👩🏫 Teachers
• Reading comprehension practice
• Auto-graded assessments
• Literacy skill development
👨👩👧👦 Parents
• Reading practice at home
• Comprehension improvement
• Educational reading time
🏠 Homeschoolers
• Reading curriculum support
• Independent reading practice
• Progress monitoring
Reading Features:
📖
Reading Passage
Engaging fiction or nonfiction text
❓
Comprehension Quiz
Auto-graded questions
📊
Instant Feedback
Immediate results and scoring
📄
Printable Version
Download for offline reading
🔊
Read Aloud
Voice-over with word highlighting
Reviews & Ratings
No reviews yet. Be the first to share your experience!
Related Content
What is Solar Radiation
This NGSS-aligned science reading passage for middle school students explores the concept of solar radiation. Solar radi...
MS-ESS1-1
Tides and Tidal Forces
This middle school science passage explores the mechanisms of tides and tidal forces, aligning with NGSS standards MS-ES...
MS-ESS1-1MS-ESS1-2
The Night Sky
This comprehensive science reading passage for grades 6-8 aligns with NGSS standard MS-ESS1-1 and explores the systems a...
MS-ESS1-1
Ancient Astronomy
This engaging passage for grades 6-8 explores the history of astronomy through the lens of ancient observations. Student...
MS-ESS1-1
Tools of Modern Astronomy
This passage introduces middle school students to modern astronomy, aligning with NGSS standard MS-ESS1-1. It explains h...
MS-ESS1-1
How Astronomy Became a Science
This passage explores the transformative period known as the Scientific Revolution, with a special focus on the history ...
MS-ESS1-1
Earth's Rotation
This middle school science passage, aligned with NGSS standard MS-ESS1-1, focuses on Earth's rotation—how Earth spins on...
MS-ESS1-1
Earth's Revolution
This middle school science passage explores the science behind Earth's revolution around the Sun, closely aligned with N...
MS-ESS1-1
Why We Have Seasons
This comprehensive middle school science reading passage explains the mechanisms behind Earth's seasons, directly addres...
MS-ESS1-1
Earth's Seasons
This comprehensive reading passage for grades 6-8 explains why Earth has seasons, revealing the scientific mechanisms be...
MS-ESS1-1
Phases of the Moon
This comprehensive middle school science passage explains the phases of the Moon, focusing on the mechanisms behind the ...
MS-ESS1-1
Tides
This comprehensive middle school science reading passage explores the phenomenon of ocean tides, aligned to NGSS standar...
MS-ESS1-1MS-ESS1-2
Eclipses
This comprehensive passage for grades 6-8 explores the science behind eclipses, including solar and lunar eclipses, thei...
MS-ESS1-1
The Moon's Characteristics
This comprehensive science reading passage for grades 6-8 examines the Moon's physical characteristics, including its si...
MS-ESS1-1MS-ESS1-2
Lunar Eclipses
This passage introduces middle school students to the phenomenon of lunar eclipses, connecting observable events to the ...
MS-ESS1-1
The Sun's Characteristics
This engaging science passage introduces middle school students to the Sun’s key characteristics, such as its classifica...
MS-ESS1-1MS-ESS1-2
What Is a Galaxy?
This comprehensive middle school science passage answers the question: What is a galaxy? Aligned to NGSS standard MS-ESS...
MS-ESS1-1
The Milky Way: Our Home Galaxy
This comprehensive science passage introduces middle school students to the Milky Way, the barred spiral galaxy that is ...
MS-ESS1-1
Types of Galaxies
This comprehensive middle school science passage introduces students to the classification and characteristics of galaxi...