Hubble Space Telescope “Catches” Boomerang Nebula
Hubble has revealed the intricate details of the Boomerang Nebula, a near-absolute zero temperature nebula 5,000 light-years away, showcasing significant matter ejection over millennia.
The Hubble Space Telescope has “caught” the Boomerang Nebula in these spectacular images taken with the Advanced Camera for Surveys. This reflecting cloud of dust and gas has two nearly symmetric lobes (or cones) of matter that are being ejected from a central star. Over the last 1,500 years, nearly one and a half times the mass of our Sun has been lost by the central star of the Boomerang Nebula in an ejection process known as a bipolar outflow.
The nebula’s catchy name is derived from its symmetric structure as seen from ground-based telescopes. Hubble’s sharp view is able to resolve patterns and ripples in the nebula very close to the central star that are not visible from the ground.
Often touted for its unique and symmetric appearance, the Boomerang Nebula has garnered significant attention in the astronomical community and has become an iconic subject for telescopic studies. At its heart, the nebula boasts a central star that has undergone dramatic changes, ejecting almost one and a half times the mass of our Sun in a process known as a bipolar outflow over the last 1,500 years. This has resulted in two almost symmetric lobes of matter radiating outwards.
One of the most intriguing characteristics of the Boomerang Nebula is its temperature. The nebula is chillingly cold, registering at just about one degree Kelvin above absolute zero, translating to nearly -460 degrees Fahrenheit. This makes it one of the coldest known regions in the universe, even colder than the background temperature of space. The nebula’s near-absolute zero temperature, combined with its unique structure and the mysteries surrounding its central star, make the Boomerang Nebula a compelling subject of study and a testament to the universe’s endless wonders.
