red giants

Two nearly symmetrical swirling loops of gas and dust mark the dying flickers of an ancient red giant star. Credit: International Gemini Observatory/NOIRLab/NSF/AURA, TA Rector (University of Alaska Anchorage/NSF's NOIRLab), J. Miller (Gemini Observatory/NSF's NOIRLab), M. Rodriguez (Gemini Observatory/NSF's NOIRLab), M. Zamani ( NSF's NOIRLab)

An overflowing cosmic "urn" - a telescope captures the spectacular end-of-life display of a red giant

This end-of-life phase of red giant stars is relatively short, and the celestial structures that form around them are rare, so the Tobi Pitcher Nebula is an excellent example of a case study in the evolution of a star
Abell 39, object number 39 in the catalog of large nebulae discovered by George Abell in 1966 is of a large nebula discovered by George Abell in 1966, is a fine example of a planetary nebula. This photograph was taken in 1997 from the Kite Peak National Observatory in Arizona through a blue-green filter that isolates the light emitted by the oxygen atoms in the nebula at a wavelength of 500.7 nm. The diameter of the nebula is about five light years, and the thickness of the spherical shell is about a third of a light year. The nebula itself is about 7,000 light-years from Earth in the constellation Hercules. Credit: TARector (NRAO/AUI/NSF and NOAO/AURA/NSF) and BAWolpa (NOAO/AURA/NSF) WIYN

What will happen when our sun dies?

A red giant (and a planet next to it). Illustration: shutterstock

A hybrid star - a neutron star inside a red supergiant

U Cam - an exploding star in the Giraffe group (not far from the North Star from our perspective on Earth). Photo: Hubble Space Telescope

The last outburst of a dying star was captured by Hubble

Cosmic scene with DNA, stars, solvents and atomic circles in oral flow.

A giant star or the water world?