Observing in infrared light, Hubble pierced through the obscuring gas and dust of M16’s Pillars of Creation. This ethereal image reveals the young stars that are being formed within the pillars. It also uncovers a myriad of background stars that were hidden at visible wavelengths.
Credits: NASA, ESA and the Hubble Heritage Team (STScI/AURA)
These towering tendrils of cosmic dust and gas sit at the heart of M16, or the Eagle Nebula. The aptly named Pillars of Creation, featured in this stunning Hubble image, are part of an active star-forming region within the nebula and hide newborn stars in their wispy columns.
Although this is not Hubble’s first image of this iconic feature of the Eagle Nebula, it is the most detailed. The blue colors in the image represent oxygen, red is sulfur, and green represents both nitrogen and hydrogen. The pillars are bathed in the scorching ultraviolet light from a cluster of young stars located just outside the frame. The winds from these stars are slowly eroding the towers of gas and dust.
Stretching roughly 4 to 5 light-years, the Pillars of Creation are a fascinating but relatively small feature of the entire Eagle Nebula, which spans 70 by 55 light-years. The nebula, discovered in 1745 by the Swiss astronomer Jean-Philippe Loys de Chéseaux, is located 7,000 light-years from Earth in the constellation Serpens. With an apparent magnitude of 6, the Eagle Nebula can be spotted through a small telescope and is best viewed during July. A large telescope and optimal viewing conditions are necessary to resolve the Pillars of Creation.
Although the Pillars of Creation are a prominent feature of M16, they are relatively small compared to the entire nebula. This video begins with a ground-based image of the sky near Serpens and zooms into Hubble’s iconic image.
Credits: NASA, ESA, G. Bacon (STScI); Acknowledgment: NASA, ESA, Hubble Heritage Team (STScI/AURA), Digitized Sky Survey ((DSS), STScI/AURA, Palomar/Caltech, UKSTU/AAO), T.A. Rector (NRAO/AUI/NSF, NOAO/AURA/NSF), B.A. Wolpa (NOAO/AURA/NSF), A. Fujii
This haunting spire, captured by Hubble in visible and infrared light, is composed of cold gas and dust within M16. Stretching 9.5 light-years, this tower spans more than twice the distance from our sun to its nearest star. Radiation from the hot young stars in the top half of the image are illuminating and eroding the structure.
Credits: NASA, ESA and the Hubble Heritage Team (STScI/AURA)
For more information about Hubble’s observations of M16, see:
This star chart for M16 represents the view from mid-northern latitudes for the given month and time.
Credits: Image courtesy of Stellarium
Last Updated: Oct. 19, 2017
Editor: Rob Garner
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