Euclid and Hubble's view of Cat's Eye Nebula

For this month’s ESA/Hubble Picture of the Month, we turn our gaze to one of the most visually intricate remnants of a dying star: the Cat’s Eye Nebula, also known as NGC 6543. This extraordinary planetary nebula lies roughly 4 400 light-years away in the constellation Draco, and has captivated astronomers for decades with its elaborate and multilayered structure.

Planetary nebulae, so-called because of their round shape when viewed through early telescopes, are in fact expanding gas thrown off by stars in their final stages of evolution. It was the Cat’s Eye Nebula itself where this fact was first discovered in 1864 — examining the spectrum of its light reveals the emission from individual molecules that’s characteristic of a gas, distinguishing planetary nebulae from stars and galaxies.

The NASA/ESA Hubble Space Telescope also revolutionised our understanding of planetary nebulae; its detailed images showed that the simple, circular appearance of a planetary nebula seen from the ground belies a very complex morphology. This was particularly true of the Cat’s Eye Nebula, where Hubble’s images in 1995 revealed never-before-seen structures that broadened our understanding of how planetary nebulae come to be.

This time, Hubble is joined by ESA’s Euclid space telescope to create a new image of NGC 6543. The nebula is showcased through the combined eyes of Hubble and Euclid, revealing the remarkable complexity of stellar death in this object. Though primarily designed to map the distant Universe, Euclid captures the Cat’s Eye Nebula as part of its deep imaging surveys, resulting in this broad view that situates the nebula against the deep space beyond.

In Euclid’s wide, near-infrared and visible light view, the arcs and filaments of the nebula’s bright central region are situated within a halo of colourful fragments of gas zooming away from the star. This ring was ejected from the star at an earlier stage, before the main nebula at the centre formed. Hubble captures the very core of the billowing gas with high-resolution visible-light images, adding extra detail in the centre of this image. The whole nebula stands out against a backdrop teeming with distant galaxies, demonstrating how local astrophysical beauty and the farthest reaches of the cosmos can be seen together in modern astronomical surveys.

Together, these missions provide a rich and complementary view of NGC 6543 — revealing the delicate interplay between stellar end-of-life processes and the vast cosmic tapestry beyond.

[Image Description: A planetary nebula in space. The star in the very centre is surrounded by white bubbles and loops of gas, all shining with a powerful blue light. Farther away a broken ring of red and blue gas clouds surrounds the nebula. A multitude of golden and white stars, wisps of gas and distant galaxies of various sizes surround the nebula on the black background.]

Links

Credit:

ESA/Hubble & NASA, ESA Euclid/Euclid Consortium/NASA/Q1-2025, J.-C. Cuillandre & E. Bertin (CEA Paris-Saclay), Z. Tsvetanov

About the Image

Id:potm2602c
Type:Observation
Release date:3 March 2026, 15:00
Size:13212 x 7250 px

About the Object

Name:NGC 6543
Distance:4400 light years
Constellation:Draco
Category:Nebulae

Image Formats

r.titleLarge JPEG
41.3 MB
r.titleScreensize JPEG
289.9 KB

Zoomable


Classic Wallpapers

r.title1024x768
401.3 KB
r.title1280x1024
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r.title1600x1200
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r.title1920x1200
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r.title2048x1536
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Desktop Wallpapers

r.title1280x720 (HD)
431.6 KB
r.title1920x1080 (FHD)
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Mobile Wallpapers


Coordinates

Position (RA):17 58 33.73
Position (Dec):66° 37' 46.67"
Field of view:22.02 x 12.08 arcminutes
Orientation:North is 0.4° left of vertical


Colours & filters

BandWavelengthTelescope
Infrared
I
700 nmEuclid
VIS
Infrared
Y
1.1 μmEuclid
NISP
Infrared
J
1.259 μmEuclid
NISP
Infrared
H
1.7 μmEuclid
NISP
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