New discovery shows a dead star eating shredded pieces of a Pluto-like world

Scientists identified the chemical composition of the doomed object by analyzing the material as it fell onto the white dwarf.
PUBLISHED SEP 19, 2025
This artist’s concept shows a white dwarf surrounded by a large debris disk. Debris from pieces of a captured, Pluto-like object is falling onto the white dwarf (Cover Image Source: NASA | Tim Pyle)
This artist’s concept shows a white dwarf surrounded by a large debris disk. Debris from pieces of a captured, Pluto-like object is falling onto the white dwarf (Cover Image Source: NASA | Tim Pyle)

A dead star in our cosmic neighborhood has been caught in the act of consuming fragments of an icy, Pluto-like object. NASA's Hubble Space Telescope, with its advanced ultraviolet capabilities, was the only instrument able to capture this celestial event, as per NASA Science



 

The star, a white dwarf with about half the mass of our Sun, is incredibly dense, packing its mass into a body the size of Earth. According to the findings published on September 18 in the Monthly Notices of the Royal Astronomical Society, the immense gravitational pull of this stellar remnant likely tore apart a dwarf planet from its own version of a Kuiper Belt, the icy ring of debris beyond Neptune in our own solar system.

These two multiple-exposure images from Hubble show Kuiper Belt Objects against a background of stars in the constellation Sagittarius (Image Source: NASA, ESA)
These two multiple-exposure images from Hubble show Kuiper Belt Objects against a background of stars in the constellation Sagittarius (Representative Image Source: NASA, ESA)

Scientists identified the chemical composition of the doomed object by analyzing the material as it fell onto the white dwarf. They discovered a significant amount of "volatiles," substances with low boiling points, including carbon, sulfur, nitrogen, and a high concentration of oxygen, which points to the presence of water. “We were surprised,” stated Snehalata Sahu of the University of Warwick, who led the data analysis for a Hubble survey of white dwarfs. “We did not expect to find water or other icy content. This is because the comets and Kuiper Belt-like objects are thrown out of their planetary systems early, as their stars evolve into white dwarfs.

Animation of Type Ia supernova from merging white dwarfs (Representative Image Source: NASA's Goddard Space Flight Center Conceptual Image Lab)
Animation of Type Ia supernova from merging white dwarfs (Representative Image Source: NASA's Goddard Space Flight Center Conceptual Image Lab)

Using the Hubble's Cosmic Origins Spectrograph, the research team determined that the fragments were composed of 64% water ice. The sheer amount of ice indicates the fragments came from a massive object that formed in the frigid outer reaches of its star system, an "exo-Pluto." They also detected the highest fraction of nitrogen ever found in debris around a white dwarf. “We know that Pluto's surface is covered with nitrogen ices,” Sahu explained. “We think that the white dwarf accreted fragments of the crust and mantle of a dwarf planet.”

This animation shows a burned-out star, called a white dwarf, accreting rocky debris left behind by the star's surviving planetary system (Image Source: NASA, ESA | G. Bacon)
This animation shows a burned-out star, called a white dwarf, accreting rocky debris left behind by the star's surviving planetary system (Image Source: NASA, ESA | G. Bacon)

Detecting these volatile-rich objects is extremely difficult in visible light, which is why Hubble's ultraviolet sensitivity was crucial. To an observer using a regular telescope, the white dwarf would appear completely normal. The star, located about 260 light-years away, is a relatively close cosmic neighbor and likely hosted planets and a Kuiper Belt analog before it collapsed, as mentioned by the space agency

This discovery offers a potential preview of our own solar system's fate. In billions of years, when our Sun becomes a white dwarf, its gravity will similarly pull in and destroy objects from our Kuiper Belt. “If an alien observer looks into our solar system in the far future, they might see the same kind of remains we see today around this white dwarf,” Sahu noted. The team plans to use the James Webb Space Telescope to further investigate the star in infrared light, hoping to detect molecular signatures of water vapor and carbonates. By studying these events, scientists hope to learn more about the formation of planets and how water is delivered to rocky worlds.

More on Starlust

Subaru Telescope discovers ancient ‘fossil’ object beyond Pluto, challenges the existence of Planet Nine

MORE STORIES

Previously, the most ancient supernova ever confirmed dated back to when the universe was 1.8 billion years old.
4 hours ago
NASA's Fermi telescope was the first to identify the highly unusual cosmic explosion.
9 hours ago
An international team of astronomers conducted a ten-day observation of the NGC 3783 black hole using mainly the XRISM space telescope.
1 day ago
A nova is a massive, temporary star explosion caused when a dense white dwarf star pulls material from a nearby star, setting off an uncontrolled nuclear reaction.
2 days ago
A team of computational astrophysicists has developed a simulation that explains the behavior of matter around black holes.
5 days ago
A study has also concluded that the interior of 3I/ATLAS is rich in metal, which could challenge our current understanding of comet formation.
5 days ago
The James Webb captures a more panoramic image of stars and galaxies, spectacular visuals that were missed by most other observatories.
6 days ago
The discovery comes as a surprise to scientists, as they believed the formation of such well-organized spiral galaxies took billions of years.
6 days ago
Scientists have found a nutrient crucial to the production of serotonin in the asteroid samples.
7 days ago
These giant radio quasars belong to a group of 369 that was recently discovered by the Giant Meterwave Radio Telescope near Pune, India.
Dec 2, 2025