Hubble Space Telescope
The Hubble Space Telescope (HST) is a joint NASA and ESA observatory launched on April 24, 1990, aboard the Space Shuttle Discovery (STS‑31). Positioned in low Earth orbit at about 547 kilometers altitude, Hubble avoids atmospheric distortion and captures high-resolution observations in ultraviolet, visible, and near-infrared light.
Named after American astronomer Edwin Hubble, the telescope was inspired by Lyman Spitzer’s 1946 proposal to place telescopes in space. Hubble features a 2.4-meter primary mirror and a suite of scientific instruments designed to be upgraded during space servicing missions.
Soon after deployment, a flaw was discovered in the shape of its primary mirror, which was corrected by astronauts during the first servicing mission in 1993. Over its lifetime, Hubble received five servicing missions, which not only fixed technical issues but also significantly upgraded its capabilities.
Hubble has transformed our understanding of the universe. It helped determine the age of the universe (~13.8 billion years), provided evidence for the acceleration of cosmic expansion due to dark energy, revealed the presence of supermassive black holes in galaxies, and observed planets outside our solar system.
Iconic images captured by Hubble—such as the Pillars of Creation and the Hubble Deep Field—have expanded public engagement with space and allowed astronomers to peer billions of years into the past, studying galaxy formation and cosmic evolution.
Now operating alongside the James Webb Space Telescope, Hubble continues to provide critical observations despite aging hardware, including issues with gyroscopes. Its contributions to astronomy remain unparalleled, offering a legacy of scientific discovery and technological achievement.
Sources
APODs including "Hubble Space Telescope"
M82: Galaxy with a Supergalactic Wind
29 June 2026
Why is the Cigar Galaxy billowing red smoke? M82, as this starburst galaxy is also known, was stirred up by a recent pass near large spiral galaxy M81. This doesn't fully explain the source of the red-glowing outwardly expanding gas and dust, however. Evidence indicates that this gas and dust is being driven out by the combined emerging particle winds of many stars, together creating a galactic superwind. The dust particles are thought to originate in M82's interstellar medium and are actually similar in size to particles in cigar smoke. The featured photographic mosaic combines images taken in visible light from the Hubble Space Telescope and images taken in infrared light from James Webb Space Telescope. It shows the light-colored central galaxy nearly edge on across the image center with tremendous orange and red colored filaments of gas and dust extending both up and down. The filaments extend for over 10,000 light years. The 12-million light-year distant Cigar Galaxy is the brightest galaxy in the sky in infrared light and can be seen in visible light with a small telescope towards the constellation of the Great Bear (Ursa Major).