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Nearby Spiral Galaxy NGC 4945

Beautiful Red Spider!

stunning view from the James Webb Telescope ✨

This image captures the planetary nebula NGC 6537, also known as the Red Spider Nebula. Its exact distance is unknown; various sources cite figures ranging from 2,000 to 8,000 light-years.

Objects like this represent the future that awaits our Sun. Once it exhausts its hydrogen fuel, it will begin to expand, transforming into a red giant. Eventually, it will shed its outer layers, leaving behind only a bare core. Radiation from the core will ionize the surrounding material, causing it to glow and form a visible nebula—much like NGC 6537. This phase will not last long; in a few tens of thousands of years, the core will cool, and the nebula will dissipate.

In the case of NGC 6537, there is a possibility that its center harbors two stars rather than one. Hourglass-shaped nebulae of this kind often originate in binary star systems, though the existence of a companion star has not yet been confirmed.

Wellcome Young Stars! ✨🌟✨⭐

The active star-forming region LH 95, captured by the Hubble Telescope!

The object is located in the Large Magellanic Cloud.

The image shows bright blue and white stars set against red hydrogen clouds, along with dark streaks formed by dense dust clouds.

❕ Scientists have discovered approximately 2,500 young stars in the LH 95 region.

The Antennae Galaxies in Collision