Space Zone:
- Far-infrared observations
- Gamma-ray observations
- X-ray observations
- Far-ultraviolet observations
Surface Zone:
- Visible observations
- Radio observations
You may be most familiar with the light that your eyes can perceive. This corresponds to the visible, or optical, part of the electromagnetic spectrum. As shown in the figure, the visible part of the EM spectrum is but a small part of the overall spectrum of wavelengths that is emitted by astronomical sources. To understand the nature of many astronomical sources, astronomers endeavor to obtain observations at multiple wavelengths throughout the EM spectrum. A fair bit of the radio and infrared parts make it through Earth’s atmosphere to be collected and detected by ground-based observing facilities.
However, Earth’s atmosphere is essentially opaque to the cosmic radiation at ultraviolet, X-ray, and gamma-ray wavelengths. To perceive astronomical sources at these wavelengths, it is necessary to loft telescopes above the bulk of Earth’s light-absorbing atmosphere. Collectively, observations of celestial sources at different wavelengths help astronomers to understand the universe, similar to how we use all of our five senses to help us to understand our immediate environment.