---
title: "Observing with Light Waves"
description: "Describe the electromagnetic spectrum from radio waves to gamma rays. Give examples of what radio, microwave, infrared, visible, ultraviolet and X-ray observations reveal. Explain atmospheric limits, "
canonical: https://lightmysky.com/learn/science/observing-with-light-waves-mt_rbY77m8_s1
source: https://lightmysky.com/learn/science/observing-with-light-waves-mt_rbY77m8_s1.md
retrieved: 2026-10-19
---

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# Observing with Light Waves

Describe the electromagnetic spectrum from radio waves to gamma rays. Give examples of what radio, microwave, infrared, visible, ultraviolet and X-ray observations reveal. Explain atmospheric limits, direct and indirect gamma-ray observations, and the wavelength choices of Hubble and Webb.

Subject: Science · Area: Space Exploration · Ages 11 to 13
Page: https://lightmysky.com/learn/science/observing-with-light-waves-mt_rbY77m8_s1

## Ready when they can

- Lists at least four regions of the EM spectrum and gives a specific astronomical object or phenomenon observed in each
- Explains why direct astronomical X-ray and gamma-ray detectors operate above the absorbing atmosphere, and why space provides access to infrared bands blocked from the ground
- Describes the James Webb Space Telescope or Hubble and explains which part of the spectrum each primarily observes and why that was chosen

## Lesson: Observing with Light Waves

Astronomers use starlight to find planets. They also study light our eyes cannot detect. The electromagnetic spectrum includes all these kinds of light. Radio waves have the longest wavelengths; gamma rays have the shortest. Wavelength is the distance between neighbouring wave crests. Frequency counts cycles passing each second. In a vacuum, all electromagnetic waves have the same speed, so higher frequency goes with shorter wavelength.

*(drawing: Moving right means shorter wavelength and higher frequency. The boxes show order, not the relative widths of the regions.)*

Radio observations can map cold gas clouds where stars may form. Microwaves reveal the cosmic microwave background: light released in the early universe and stretched during expansion. X-rays reveal extremely hot gas, including gas near black holes. Infrared reveals warm dust and forming stars. Visible light shows stars and galaxies. Ultraviolet helps trace hot young stars.

Visible light and some radio and infrared wavelengths pass through Earth's air. It absorbs incoming astronomical X-rays and gamma rays. Direct detectors for those rays operate above the absorbing air. Ground gamma-ray observatories instead detect secondary signals made when gamma rays interact with air. Space also provides access to infrared bands blocked from the ground.

Hubble observes ultraviolet, visible and some near-infrared light. Being in space lets it collect ultraviolet wavelengths blocked by air and avoid atmospheric blurring. Images can use assigned colours to display measurements, so they need not match what your eyes would see.

Webb observes infrared. Some infrared wavelengths pass through dust more readily than visible light, revealing forming stars. Expansion stretches light from very distant galaxies to longer wavelengths. Light emitted as visible light can reach us in the infrared. Webb uses infrared measurements to study early galaxies.

**Recap.** Different wavelengths reveal different objects and processes. Earth's air passes some bands and blocks others, so astronomers use both ground and space observatories.

## Practice

8 questions on this page, each with its working shown.

## Needs first

- [The Electromagnetic Spectrum](https://lightmysky.com/learn/science/the-electromagnetic-spectrum-mt_XSp-S0wter)
