Hubble Space Telescope Learning Path

Concept, design, and scientific aim

The “Concept, design and aim” of the Hubble Space Telescope traces its origins to early ideas about the scientific advantages of observing from space. In 1946, Lyman Spitzer argued that an extraterrestrial observatory would overcome atmospheric turbulence (improving angular resolution) and could observe ultraviolet and infrared wavelengths that Earth’s atmosphere absorbs. These ideas were reinforced by later small-scale space astronomy missions (e.g., Orbiting Solar Observatory and Orbiting Astronomical Observatory), which demonstrated the value of space-based observations and helped build momentum for a large, long-lived telescope. Hubble’s design concept also emphasized that the telescope should be maintainable in orbit, enabling upgrades and repairs over a long operational lifetime. Nancy Grace Roman played a major role in shaping the scientific objectives and advocating for the project, including organizing astronomer input and lobbying for sustained funding. NASA then established committees to define engineering and scientific goals, but the program faced major budget challenges, including congressional cuts and a period when funding was removed, followed by a coordinated lobbying effort by astronomers to restore support. Finally, the topic explains how Hubble’s scientific aims depended on its optical performance and how the mission’s initial design was compromised by a flawed primary mirror. The mirror was polished to an incorrect shape, producing severe spherical aberration that greatly reduced image quality for faint or high-contrast targets. The resulting problem led to the development of corrective optics (planned within the servicing-mission framework) and a major repair effort, demonstrating that Hubble’s intended maintainability was essential to achieving its scientific goals.

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Proposals and precursors to Hubble

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