After 50 years, NASA finally found the answer. For centuries, astronomers have studied the final acts of dying stars with a mix of fascination and restraint. Planetary nebulae—once mistaken for cloudy planets—offered a glimpse into stellar death throes. In 1790, William Herschel stumbled upon one so odd it forced him to rethink his assumptions. He wrote of “a most singular phenomenon,” noting a star “surrounded with a faintly luminous atmosphere,” unlike anything he had cataloged before.
Cosmic enigma from 1970 finally took shape in 2010: the story was far from over
The last few decades have offered tantalizing clues, but left the true nature of this object elusive. Infrared observations in 2010 revealed ghostly rings invisible to the naked eye, hinting at a complex structure beyond simple spherical shells. Still, without sharper sight or deeper insight, the mystery endured—its full form hidden in cosmic dust.
Now, technology has caught up to the question. Mid-infrared data brings new clarity—fuzzy clumps, tangled patterns, pinprick holes through glowing clouds, and hints of sculpting forces at work. That buildup of detail is guiding us toward an answer—but more remains to unfold. And that brings us to the new discovery by NASA while using the James Webb in April 2025.
New images reveal the tangled heart of NGC 1514 after thousands of years in the making
NASA’s James Webb Space Telescope has given astronomers their clearest view yet of the gas and dust surrounding the dying star system at the heart of NGC 1514. Mid-infrared findings showed tangled clumps of material punctuated by clear gaps, where faster stellar winds have punched through the surrounding cloud. This slow-motion spectacle has been evolving for at least four millennia and will continue to shift for thousands of years to come.
At the center lies a close-knit binary system — two stars that, in NASA’s images, blur into what appears to be a single point of light crowned by sharp diffraction spikes. They orbit each other once every nine years, tracing an elongated path, and are enveloped by an arc of dust that glows in orange tones.
One of the pair, once several times more massive than the Sun, expelled much of its outer layers as it aged. David Jones of the Institute of Astrophysics in the Canary Islands, who confirmed the binary nature of the system in 2017, has explained that the primary star expanded during its final stages, releasing gas and dust in a slow, dense wind. Now reduced to a white dwarf, it produces faster but weaker outflows that may have sculpted the surrounding material into delicate shells.
NASA’s James Webb team reveals unexpected secrets behind the star’s mysterious mass loss
Webb’s perspective shows the nebula tilted at roughly 60 degrees, a view that can give the illusion of liquid pouring from a container. In reality, the structure is more like an hourglass with truncated ends, its narrow waist visible where orange dust tapers into shallow V-shaped forms.
NASA suggest that, at the height of the primary star’s mass loss, its companion may have approached closely enough to distort the outflow, shaping rings rather than a perfect sphere. The effect is three-dimensional, with dim, semi-transparent clouds filling the space between the rings, giving the nebula a layered appearance.
NASA found Earth common element in the center of the phenomenon
Alongside the dust, Webb’s instruments detected oxygen concentrated in the pink-hued central regions, especially along the edges of the cavities carved into the nebula’s heart. This process can continue for thousands of years, with the area of the nebula expanding as long as the dust can hold together. After that, the oxygen will become free in space and should be incorporated by other cosmic objects.