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March 3, 2025

Hubble captures new view of the Veil Nebula

This NASA/ESA Hubble Space Telescope image a supernova remnant called the Veil Nebula. Credit: ESA/Hubble & NASA, R. Sankrit
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This NASA/ESA Hubble Space Telescope image a supernova remnant called the Veil Nebula. Credit: ESA/Hubble & NASA, R. Sankrit

In this NASA/ESA Hubble Space Telescope image, Hubble once again lifts the veil on a famous—and frequently photographed—supernova remnant: the Veil Nebula. The remnant of a star roughly 20 times as massive as the sun that exploded about 10,000 years ago, the Veil Nebula is situated about 2,400 light-years away in the constellation Cygnus. Hubble images of this photogenic nebula were first taken in 1994 and 1997, and again in 2015.

This view combines images taken in three different filters by Hubble's Wide Field Camera 3, highlighting emissions from hydrogen, sulfur, and oxygen atoms. The image shows just a small fraction of the Veil Nebula; if you could see the entire nebula without the aid of a telescope, it would be as wide as six full moons placed side-by-side.

Although this image captures the Veil Nebula at a single point in time, it helps researchers understand how the supernova remnant evolves over decades. Combining this snapshot with Hubble observations from 1994 will reveal the motion of individual knots and filaments of gas over that span of time, enhancing our understanding of this stunning nebula.

Provided by NASA

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The Hubble Space Telescope captured a new image of the Veil Nebula, a supernova remnant from a star 20 times the mass of the sun that exploded 10,000 years ago. Located 2,400 light-years away in Cygnus, the image uses three filters to highlight emissions from hydrogen, sulfur, and oxygen. This snapshot, alongside past observations, aids in studying the nebula's evolution by tracking the movement of gas structures over time.

This summary was automatically generated using LLM.