Astronomers captured an image of a dying star that appears as a glowing, milky-white "crystal ball" in the constellation Taurus [1].
The discovery provides a rare glimpse into the final stages of stellar evolution. By studying the unique shape of the nebula, researchers can better understand how stars shed their outer layers before they die.
The image was released on May 22, 2026 [2]. It was captured by the Gemini North Telescope, located on Mauna Kea, Hawaii [3]. The effort included teams from the U.S. National Science Foundation's NOIRLab [3].
The dying star is located approximately 1,500 light-years from Earth [1]. Its distinct appearance is not accidental. Astronomers said the crystal-ball shape was sculpted by the gravitational influence of a hidden binary star system [3].
Binary systems consist of two stars orbiting a common center of mass. In this case, the interaction between the two stars likely shaped the outflow of gas and dust as the primary star began to die [3]. This process creates the symmetrical, glowing shell seen in the images.
Such observations allow scientists to map the transition from a red giant to a planetary nebula. This phase is relatively brief in cosmic terms, making high-resolution captures of these structures essential for astrophysical modeling [3].
“A dying star whose nebula appears as a glowing, milky‑white "Crystal Ball"”
The identification of a binary system as the architect of this nebula confirms that stellar death is often a collaborative process. When a dying star has a companion, the resulting nebula is rarely a simple sphere; instead, the companion's gravity twists and shapes the ejecta. This specific observation helps astronomers refine the mathematical models used to predict how different types of stars will end their life cycles.
