Hubble Space Telescope
The Hubble Space Telescope is a joint NASA–European Space Agency observatory in low Earth orbit. Launched in 1990, it observes ultraviolet, visible and near-infrared light from above Earth's atmosphere, producing high-resolution images and spectra. Designed for astronaut servicing, it underwent five shuttle servicing missions, including the 1993 correction of an optical flaw and a major 2009 upgrade. Its observations and public archive support research across astronomy.
Purpose and design
The Hubble Space Telescope (HST) is a space-based astronomical observatory operated through a partnership between the United States National Aeronautics and Space Administration (NASA) and the European Space Agency (ESA). Named for astronomer Edwin Hubble, it was developed as a long-lived observatory rather than a single-purpose probe. Its 2.4-metre reflecting telescope was deployed in low Earth orbit, about 600 kilometres above the planet.
Hubble's position above most of Earth's atmosphere is central to its work. The atmosphere blurs some astronomical images and blocks much ultraviolet light, while also adding background in parts of the infrared spectrum. Hubble's instruments observe ultraviolet, visible and near-infrared wavelengths, allowing astronomers to examine objects from the Solar System to very distant galaxies. Cameras record images, while spectrographs separate light by wavelength to reveal information about astronomical objects.
A serviceable observatory
Hubble's modular design included handholds and grapple fixtures so astronauts could reach, repair and upgrade the observatory during space-shuttle visits. This feature proved crucial soon after launch, when engineers found that the primary mirror had a shape error called spherical aberration. The flaw caused early images to appear blurred, but it did not make the telescope unusable.
During the first servicing mission in December 1993, astronauts installed corrective optics and new instruments, bringing the incoming light into sharper focus. Four further servicing missions replaced or repaired equipment and added more capable instruments. On the final mission, in 2009, astronauts installed the Wide Field Camera 3 and Cosmic Origins Spectrograph and repaired two instruments that had stopped working. The upgrades extended the observatory's capabilities without returning it to Earth.
Observations and scientific use
Hubble collects observations selected through a competitive process in which astronomers propose investigations for peer review. The Space Telescope Science Institute (STScI) coordinates the observatory's science operations, calibrates and distributes observation data, and maintains an archive. Researchers can use archived observations to pursue questions beyond the original purpose of a program.
Hubble's long-running observations have contributed to work on many subjects, including stars and planetary systems, galaxies, and the history and expansion of the universe. For example, ESA describes Hubble observations of discs of gas and dust around young stars and measurements of exoplanet atmospheres. Its ultraviolet access and detailed imaging complement other observatories, including the James Webb Space Telescope, which works in tandem with Hubble on astronomical research.
Key facts
- Partners
- NASA and the European Space Agency.
- Type
- A 2.4-metre reflecting space telescope in low Earth orbit.
- Launch
- 24 April 1990; deployed from Space Shuttle Discovery the following day.
- Wavelengths
- Ultraviolet, visible and near-infrared light.
- Servicing
- Five shuttle servicing missions, from 1993 to 2009.
- Science operations
- Coordinated by the Space Telescope Science Institute, which also maintains Hubble's data archive.
Timeline
1946
Astronomer Lyman Spitzer proposed an observatory in Earth orbit, an idea that helped establish the case for space-based astronomy.
24–25 April 1990
Hubble launched aboard the space shuttle Discovery on 24 April and was deployed in orbit on 25 April.
December 1993
Astronauts carried out the first servicing mission and installed corrective optics for the primary mirror's spherical aberration.
May 2009
The fifth and final shuttle servicing mission installed new scientific instruments and repaired existing ones.
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Answers use only “Hubble Space Telescope” and its references, with citations.
References
- 1.Our History
Space Telescope Science Institute · other · reliability: high · retrieved 17 October 2026
Supports: Lyman Spitzer's 1946 space-observatory proposal and the development of Hubble and its science institute.
- 2.About the Mission
Space Telescope Science Institute · other · reliability: high · retrieved 17 October 2026
Supports: HST's design, orbit, mission partnership, instruments, science operations and data archive.
- 3.Hubble Space Telescope
Space Telescope Science Institute · other · reliability: high · retrieved 17 October 2026
Supports: Observatory wavelength coverage, high-resolution imaging and spectroscopy, and its coordinated work with the James Webb Space Telescope.
- 4.Hubble overview
European Space Agency · other · reliability: high · retrieved 17 October 2026
Supports: Mission overview, partnership, launch date, telescope design, wavelength coverage and examples of scientific work.
- 5.Astronaut Missions to Hubble
NASA Science · other · reliability: high · retrieved 17 October 2026
Supports: The five servicing missions and the correction of Hubble's primary-mirror aberration.
- 6.Servicing Mission 1 (SM1)
NASA Science · other · reliability: high · retrieved 17 October 2026
Supports: The 1993 servicing mission, the mirror problem and the installation of corrective optics and instruments.
- 7.Servicing Mission 4 (SM4)
NASA Science · other · reliability: high · retrieved 17 October 2026
Supports: The May 2009 final servicing mission, which installed two instruments and repaired two others.
- 8.Hubble's Mirror Flaw
NASA Science · other · reliability: high · retrieved 17 October 2026
Supports: Explains how spherical aberration affected early images and how servicing enabled corrective optics.
References are suggested by the research engine and may be incomplete. Unverified URLs are omitted rather than guessed.
Article history
- Version 117 October 2026 · EditorCreated by Zapia