The National Aeronautics and Space Administration (NASA) regularly captures stunning images of our universe, leaving space lovers mesmerized.
This complex cluster of emission nebulae was discovered by American astronomer and NASA astronaut Karl Gordon in 1956.
The picture was captured by the space agency’s Hubble Space Telescope.
According to the space agency, the N11 complex consists of a group of emission nebulae – formations made up of light-emitting clouds of gas and dust.
As per NASA, N11 is one of the largest and most energetic regions in the LMC.
Scientists are using Hubble to better understand the types of stars within N11 and how they’re distributed.
Their stellar winds and supernovae carved the surrounding area into shells of gas and dust,” NASA explained.
A nebula is a giant cloud of dust and gas in space.
Space enthusiasts are enthralled by the breathtaking images of our universe that the National Aeronautics and Space Administration (NASA) regularly obtains. For people who enjoy watching informative videos and eye-catching pictures of Earth and space, the US Space Agency’s social media accounts are a veritable gold mine. Presently, NASA has released an amazing photo of the N11 nebula cluster, which is located in the constellation Dorado and is roughly 160 000 light-years away. Karl Gordon, an American astronomer and NASA astronaut, made the discovery of this intricate cluster of emission nebulae in 1956. The space agency’s Hubble Space Telescope took the image.
A “bubbling region of stars” was how NASA referred to the ethereal image in a statement. NASA described N11’s sprawling filaments as “about 1,000 light-years across, weaving stellar matter in and out of each other like sparkling candy floss.”. “The complex appears cherry-pink due to the ionization of these cotton-spun clouds of gas by a burgeoning host of young, massive stars,” the statement went on.
The space agency claims that the N11 complex is composed of a collection of emission nebulae, which are formations composed of gas and dust clouds that emit light. Situated in the vicinity of our Milky Way, the Large Magellanic Cloud (LMC) is a dwarf galaxy.
Within the LMC, N11 is one of the biggest and most active regions. This dwarf galaxy orbits the Milky Way, making it a satellite galaxy as well. Despite being a small galaxy, star formation is active in this region. One of the biggest and most active regions in the LMC is N11, according to NASA. Through Hubble, scientists are able to gain a better understanding of the different types and distributions of stars within N11.
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Massive chasms emerged from the fog all across N11. The rapidly emerging and dying stars inside the nebulae are what caused these bubbles to form. The surrounding region was formed into shells of gas and dust by their stellar winds and supernovae, according to NASA.
A nebula is an enormous gas and dust cloud in space. A supernova, or the explosion of a dying star, can release gas and dust, which can result in multiple nebulae. Where new stars are starting to form is where other nebulae are located.
Astronomically stunning, nebulae can provide insights into the birth, life, and demise of stars. Approximately 4 Point 6 Billion Years ago, our sun formed in a nebula.
