A landmark episode packed with discoveries at the cutting edge of space and astronomy. Webb and Hubble redefine a category of stellar object, JWST delivers unprecedented chemistry data from an extreme exoplanet, a 21-year-old NASA observatory faces a daring robotic rescue, a multi-telescope image reveals an ancient galactic supernova, China's Tianwen-2 zeroes in on a possible fragment of our own Moon, and astronomers detect the chemical fingerprint of a planet swallowed by its star. Story 1: Webb & Hubble Rewrite History: Terzan 5 Is a 'Bulge Fossil Fragment' Using the James Webb Space Telescope and archival data from Hubble spanning 12 years, researchers have definitively reclassified Terzan 5 — a stellar system 22,000 light-years away in Sagittarius — from a globular cluster to an entirely new class of object: a 'bulge fossil fragment.' Four distinct generations of stars have been identified within Terzan 5, formed 12.5 billion, 4.7 billion, 3.8 billion, and 2.5 billion years ago. Unlike a typical globular cluster with a single ancient stellar population, Terzan 5 repeatedly formed new stars by retaining the gas and heavy elements expelled by its own supernovae. Astronomers believe Terzan 5 is a surviving relic of the primordial clumps that merged to form the Milky Way's central bulge billions of years ago — a living fossil of galaxy formation. Results were presented at the 248th American Astronomical Society meeting and published in Astronomy & Astrophysics. Source: NASA / ESA / STScI press release, 16–17 June 2026 Story 2: JWST Catches the 'Roasted Exoplanet' HD 80606 b in the Act Astronomers using the James Webb Space Telescope's MIRI instrument have observed the extreme exoplanet HD 80606 b experiencing a temperature increase of 1,100°F (600°C) during its close approach to its host star. HD 80606 b is a gas giant four times the mass of Jupiter on a highly elliptical 111-day orbit. The JWST study — led by Tiffany Kataria of NASA's Jet Propulsion Laboratory — also detected specific atmospheric chemical signatures including methane and carbon dioxide, enabling detailed study of how the planet's chemistry shifts under extreme heating. This is the most detailed look yet at an atmospheric response to a rapid, intense heating event. Results were presented at the 248th AAS meeting in Pasadena, California. Source: NASA / JPL press release, 16–17 June 2026 Story 3: Swift's Rescue Mission Cleared for Launch: LINK on the Pad NASA's Neil Gehrels Swift Observatory, which has studied gamma-ray bursts and other high-energy cosmic events since 2004, is facing re-entry as its orbit decays under increased solar activity. NASA contracted Katalyst Space Technologies in September 2025 to build and launch a robotic servicing spacecraft — called LINK — to boost Swift to a higher orbit. LINK is now encapsulated inside a Northrop Grumman Pegasus XL rocket, which has been attached to the Stargazer L-1011 carrier aircraft and is en route to Kwajalein Atoll in the Marshall Islands for launch later in June 2026. This will be the final flight of the Pegasus XL — the world's first privately developed orbital launch vehicle, which first flew in 1990. Its air-launch capability is uniquely suited to reaching Swift's unusual low-inclination orbit. Source: NASA press release and media teleconference, 17 June 2026 Story 4: Possible Supernova Remnant at the Galactic Centre A striking multi-telescope composite image released as NASA's Astronomy Picture of the Day on 18 June 2026 reveals a possible supernova remnant near the galactic centre — a blue X-ray-emitting structure whose light is estimated to have reached Earth approximately 1,700 years ago, in the third century CE. The image combines X-ray data from NASA's Chandra X-ray Observatory and ESA's XMM-Newton (the blue structure), radio data from the MeerKAT telescope in South Africa (the large red cloud), and optical background star data from the PanSTARRS telescopes in Hawaii. Source: NASA APOD, 18 June 2026. Image credit: NASA/CXC/UCLA/Z. Zhu et al.; ESA/XMM-Newton; MeerKAT; PanSTARRS Story 5: China's Tianwen-2 Closes In on Earth's 'Quasi-Moon' China's Tianwen-2 spacecraft — launched in May 2025 — performed its primary orbit insertion burn at asteroid 469219 Kamoʻoalewa on June 7, 2026, and has since been performing fine adjustment burns tracked by amateur radio astronomers in Germany and the Netherlands. China's space agency has released no official updates. Kamoʻoalewa is a 40–100 metre quasi-satellite of Earth, orbiting the Sun in a path that keeps it perpetually near our planet. Its reflectance spectrum resembles weathered lunar rock, fuelling a theory that it is a fragment blasted from the Moon by an ancient impact — though a competing theory holds that it is an ordinary inner asteroid belt migrant. Sample collection is scheduled to begin July 4, 2026. Tianwen-2 will depart Kamoʻoalewa in April 2027, with the sample return capsule landing in Inner Mongolia in late November 2027. A new paper in Nature Communications (June 2026) challenges the lunar-origin theory, suggesting Kamoʻoalewa may instead originate from the Flora asteroid family. Source: SpaceNews, Scientific American, Nature Communications, June 2026 Story 6: A Star That Ate a Planet: TOI-5882's Chemical Fingerprint Astronomers led by Brooke Kotten of the University of Michigan have identified a chemical imbalance between the two stars of binary system TOI-5882, located approximately 1,300 light-years away. One star is enriched in elements characteristic of rocky planetary material — including iron, silicon, and magnesium — while its companion is not. Because binary stars form from the same gas cloud and should have identical initial compositions, this difference is interpreted as evidence that one star subsequently ingested at least one planet. The amount of enrichment suggests the equivalent of several Earth masses of rocky material was consumed. Source: Phys.org / University of Michigan, June 15, 2026
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