Saturn Nebula Caldwell 55 (NGC 7009)
Garden-variety stars like the Sun live fairly placid lives in their galactic neighborhoods, steadily churning out heat and light for billions of years. When these stars reach retirement age, however, they transform into unique and often psychedelic works of art. This Hubble Space Telescope image of Caldwell 55, also known as the Saturn Nebula and NGC 7009, shows the result, called a planetary nebula. While it looks like a piece of wrapped cosmic candy, what we see is actually the outer gaseous layers of a dying star.
Stars are powered by nuclear fusion, but each one comes with a limited supply of fuel. When a medium-mass star exhausts its nuclear fuel, it will swell up and shrug off its outer layers until only a small, hot core remains. The leftover core, called a white dwarf, is a lot like a hot coal that glows after a barbecue — eventually it will fade out. Until then, the cast-off gaseous debris fluoresces as it expands out into the cosmos, possibly destined to be recycled into later generations of stars and planets.
The Saturn Nebula is only about 1,400 light-years away in the direction of the Aquarius constellation. Its proximity has made it a popular target for study by telescopes all around the world. Hubble took this image in visible light using the Wide Field and Planetary Camera 2 in 1996. Using Hubble’s observations, scientists have characterized the nebula’s composition, structure, temperature, and the way it interacts with surrounding material. Studying planetary nebulae is particularly interesting since our Sun will experience a similar fate around five billion years down the road.
The Saturn Nebula has been known since 1782 when it was discovered by astronomer William Herschel. Late summer skies will provide ideal viewing of this kaleidoscopic structure for Northern Hemisphere observers (late winter for those in the Southern Hemisphere). This magnitude-8 nebula will look like a star in smaller telescopes, but larger telescopes will reveal more detail, including two extended lobes on either side of the nebula that resemble the rings of Saturn, lending the nebula its nickname. Using high magnification along with averted vision (looking away from the center of the object) will provide the best views of the fainter exterior regions of the nebula.
For more information about Hubble’s observations of Caldwell 55, see: hubblesite.org/image/575
For Hubble's Caldwell catalog website and information on how to find these objects in the night sky, visit: www.nasa.gov/content/goddard/hubble-s-caldwell-catalog
Credits: Bruce Balick (University of Washington), Jason Alexander (University of Washington), Arsen Hajian (U.S. Naval Observatory), Yervant Terzian (Cornell University), Mario Perinotto (University of Florence, Italy), Patrizio Patriarchi (Arcetri Observatory, Italy), NASA/ESA