The Hubble Space Telescope

The NASA and ESA observatory launched into low Earth orbit in 1990, whose repairs and discoveries — from the age of the universe to the first images of exoplanets — transformed astronomy and public engagement with science.

Events

Deep Fields and the Age of the Universe

Hubble's Deep Field images — long exposures of tiny "empty" patches of sky — revealed thousands of galaxies from the early universe. Combined with distance measurements of variable stars, Hubble data pinned the universe's age at roughly 13.8 billion years and pinned down the expansion rate debate.

Location: Space Telescope Science Institute, Baltimore, USA

Hubble and Webb Probe the Solar System's Smallest Relics

In the first coordinated Hubble-Webb study of trans-Neptunian objects, astronomers simultaneously observed a patch of sky in visible and infrared light and characterized 27 newly discovered bodies, including some of the smallest and faintest ever directly detected. The smallest measured about 5 kilometers across, and the survey found fewer tiny objects than some planet-formation models predicted; the similar colors of small and large objects suggested that many surfaces retained primordial compositions rather than being extensively altered by collisions. The result demonstrated how Hubble's visible-light sensitivity and Webb's infrared measurements could jointly probe objects that neither observatory could fully characterize alone.

Hubble Maps Thousands of Filaments in M82's Galactic Wind

Hubble Maps Thousands of Filaments in M82's Galactic Wind

A peer-reviewed study published September 15 reported that deep Hubble observations of the starburst galaxy Messier 82, or M82, resolved more than 2,000 narrow filaments in its southern galactic wind. A typical filament measured about 31 light-years long and 17 light-years wide. The team found that ultraviolet radiation from the central burst of star formation illuminated the bright filaments, while shocks and other heating processes became more important in the fainter, more diffuse gas. The observations provide a detailed benchmark for models of how gas survives, escapes galaxies, and carries newly formed elements into intergalactic space; the authors cautioned that smaller structures may be destroyed or too faint to detect, so the result constrains rather than settles the underlying physics.

Hubble Archive Yields First Candidate Second-generation Planet

Hubble Archive Yields First Candidate Second-generation Planet

On October 5, 2026, astronomers announced the first candidate second-generation planet ever identified: a Jupiter-sized world that may have formed not from a star's birth material but from the debris ejected when a star died. The study, published in Nature Astronomy, emerged from a reanalysis of Hubble archival observations of the white dwarf HS 0209+0832 first taken in 1999, which contained roughly 100 chemical features that went unidentified for more than a quarter of a century. Lead author Jamie Williams, a doctoral candidate at the University of Warwick, matched many of the mystery spectral lines to the element niobium using an updated chemical database, and the team confirmed the signature with data from NASA's retired FUSE observatory. Because niobium and other elements heavier than iron are forged only in the brief, extreme conditions inside dying stars rather than by ordinary fusion, the abundance points to a planet assembled from a star's cast-off innards rather than its birth disk. NASA's TESS satellite independently recorded periodic brightness variations over four months, indicating a gas giant orbiting about 6 million kilometers from the remnant and slowly losing its atmosphere to the still-hot star. Planets had been detected orbiting white dwarfs before, but the researchers described this as the first candidate bearing the chemical hallmarks of a planet born from stellar death, and cautioned that the interpretation still needs to be tested by further observations.