19 trillion kilometres!
The Boomerang Nebula is a cloud of gas and dust blown off by a dying star, about 5,000 light-years from Earth in the constellation Centaurus. A light-year is the distance light travels in one year, about 9.46 trillion kilometers. The nebula's two lobes stretch about 2 light-years, or 19 trillion kilometers, from end to end. As of 2026 it is the coldest known natural object in the universe.
Seen through the Hubble Space Telescope, the nebula has two nearly matching lobes on opposite sides of its central star, giving it the shape of an hourglass. NASA estimates that each lobe is nearly 1 light-year long, which makes the whole nebula about 2 light-years long.
That figure depends on the nebula's distance, which is uncertain. NASA gives about 5,000 light-years, and the team that studied it with the ALMA radio observatory uses a similar figure, about 4,900. The team also calculated that it can be no more than about 13,000 light-years away. If it is farther than 5,000 light-years, it is also larger.
The visible lobes are only part of the nebula. ALMA's observations traced very cold gas flowing out from the star to at least 120,000 astronomical units, where 1 astronomical unit (au) is the average distance from Earth to the Sun. That makes this cold outflow at least 3.8 light-years across, nearly twice the length of the visible nebula. Astronomers think the lobes are the parts of it lit by starlight escaping from the center.
Radio measurements made in 1995 showed that gas in the nebula is only about 1 kelvin, one degree above absolute zero. That is about −272 degrees Celsius (−458 degrees Fahrenheit). It is even colder than the cosmic microwave background, the oldest light in the universe, which reaches Earth from the whole sky at about 2.7 kelvins.
The gas has cooled by expanding very fast. It streams away from the star at about 164 kilometers per second (590,000 kilometers per hour). ALMA observations show that the cold outflow holds at least 3.3 times the mass of the Sun.
The Boomerang is a pre-planetary nebula. That is a short stage, lasting about 1,000 years, between an old, swollen red giant star and a planetary nebula, the glowing shell of gas a dying star leaves behind. The gas is the red giant's outer layers.
The star has lost mass unusually fast. Astronomers studying it with ALMA argue that a companion star spiraled into the red giant and merged with its core, flinging off the giant's outer layers. Keith Taylor and Mike Scarrott named the nebula in 1980, after its shape as seen through a large telescope in Australia.