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JAN. 2015

Hubble Revisits Famous Pillars for 25th Anniversary

New image of the Pillars of Creation in Eagle Nebula
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Revisiting a space icon
A sharper and wider view

In celebration of its 25th anniversary, the Hubble Space Telescope has revisited the famous "Pillars of Creation" in the Eagle Nebula, providing astronomers with a sharper and wider view of the giant structures where young stars are being born.

The original Hubble photo, taken in 1995, revealed never-before-seen details of three giant pillars of cold gas bathed in the ultraviolet light from a cluster of young, massive stars.

The brilliant glow of massive stars

In fact, that bright star cluster was the first object discovered almost 370 years ago in what is now the Eagle Nebula. The discoverer, Philippe Loys de Chéseaux, could only see the glow of the stellar grouping when he recorded his finding in 1745-1746.

While studying the cluster 20 years later, Charles Messier wrote that the stars were surrounded by a faint glow and looked like a nebula. He catalogued the cluster as Messier 16, or M16. Astronomer Edward Emerson Barnard was the first to photograph the nebula in the late 1800s at the Lick Observatory in California. The image revealed a large area of glowing gas. In 1908, the nebula, along with the M16 star cluster, was added to a catalogue of nebulas, galaxies, and star clusters, and was named IC 4703. Astronomers later named the region the "Eagle Nebula" because it looked like an eagle with outstretched wings.

Giant pillars of star birth

Ground-based view of the Eagle Nebula
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Ground-based view
The pillars within a wider view of the nebula

Almost 100 years later, the Hubble image of the tall pillars of gas, taken in visible light, made the Eagle Nebula famous. When the Hubble observations were taken in 1995, astronomers had seen the pillar-like structures in ground-based images, but not in detail. They knew that the physical processes are not unique to the Eagle Nebula because star birth takes place across the universe. Its location near Earth, however, makes the Eagle Nebula the most dramatic example of those star-making pillars.

Looking at the Hubble image, the first features that jumped out at the astronomers were the streamers of gas seemingly floating away from the pillars. These features were evidence that ultraviolet radiation from the cluster of hefty stars was eating away at the gaseous structures. The Hubble picture provided the first view of this process.

A sharper look at the Pillars of Creation

In 2014, Hubble again observed the Eagle Nebula, this time with one of its new cameras, the Wide Field Camera 3. Astronauts installed the camera during the last Servicing Mission in 2009, allowing Hubble to take sharper pictures. The versatile camera took images of the pillars in visible light and in near-infrared light.

Near-infrared view of the pillars
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Near-infrared view
Cutting through the dust, revealing stars

The near-infrared view reveals the pillars as wispy silhouettes seen against a background of stars. That is because near-infrared light can penetrate much of the gas and dust, revealing stars behind the nebula as well as hidden away inside the pillars. Some of the gas and dust clouds are so dense that even near-infrared light cannot penetrate them. By using both types of light, astronomers can get a more complete picture of where and how stars are forming in the nebula.

Creation and destruction in one view

Visible light view versus near-infrared light view
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Side-by-side comparison
Visible versus near-infrared

Although the original image was dubbed the Pillars of Creation, the new image hints that they are also pillars of destruction. The near-infrared image reveals that the pillars are slowly disappearing before our very eyes. The ghostly bluish haze around the dense edges of the pillars is material getting heated up and evaporating away into space. Astronomers say they have caught the pillars at a very unique and short-lived moment in their evolution.

The promise of a future telescope

More infrared images like this one await us in the future with NASA's James Webb Space Telescope, scheduled to launch in 2018. Astronomers hope that Webb will help yield more information on how stars form and on the chaotic environment in which stars are born.

 

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