If you’ve ever pointed a large-aperture telescope toward the dense star fields of Sagittarius in June, July or August, you know the region is absolutely packed with planetary nebulae masquerading as faint, bluish-green disks. But there is one target in particular that just received a massive scientific update, and it completely changes how we look at it through the eyepiece: NGC 6563.
Discovered way back in 1826 by James Dunlop, this planetary nebula (often designated PN G358.5-07.3) is well known to deep-sky observers for its distinct, slightly asymmetrical, egg-like shape. But a brand-new study published in June 2026 by a team of international astronomers has peeled back the layers of this celestial egg using high-resolution 3D morphokinematic modeling.
The results? This isn't just a simple bubble of gas—it’s a dynamic, time-delayed playground of ancient stellar jets.
The full article is availble over at Eadsy Astronomy. Please head over and take a look and join our community there.
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