Pillars of Creation

Pillars of Creation

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Pillars of Creation transparent
M16 · Eagle Nebula
VIS · 500–700 nm
RA 18h 18m 48s DEC −13°49′
6,500 LY
Select a wavelength band to see how each telescope reveals the pillars differently
InstrumentHubble HST
Dust Penetration0%
Stars Revealed~0
Gas Temperature10–50 K
Key FeatureDust Opacity
Visible Light // Hubble Space Telescope
Opaque Pillars of Cosmic Dust

In visible light, the Pillars of Creation appear as towering, opaque columns of cold molecular hydrogen and interstellar dust. These dense clouds block virtually all background starlight. Ultraviolet radiation from nearby massive stars slowly erodes the pillar surfaces through photoevaporation — the glowing finger-like tips mark where ionized gas streams away into space.

First Imaged 1995
Hubble HST

What Are the Pillars of Creation?

Everything you need to know — optimized for quick answers and deep dives alike.

What are the Pillars of Creation?

The Pillars of Creation are towering columns of interstellar gas and dust located in the Eagle Nebula (Messier 16), approximately 6,500 light-years from Earth in the constellation Serpens. They measure roughly 4–5 light-years tall — about 40 trillion kilometres — and are famous for being active stellar nurseries where new stars are currently forming inside their dense, opaque cores. First photographed in detail by the Hubble Space Telescope in 1995, they became one of the most iconic astronomical images ever taken. The James Webb Space Telescope captured new near-infrared and mid-infrared views in 2022, revealing thousands of previously hidden stars within and around the pillars.

Pillars of Creation — Key Facts

At-a-glance data points sourced from NASA, ESA, and peer-reviewed astronomy literature.

📍 Location Eagle Nebula

Messier 16 (M16), in the constellation Serpens Cauda

📏 Distance from Earth 6,500 Light-Years

Approximately 61.5 quadrillion kilometres (38.2 quadrillion miles)

🔭 Height (Tallest Pillar) ~5 Light-Years

Roughly 47 trillion km — about 11× the distance to the nearest star

Stars Forming Inside Hundreds

Young stellar objects (YSOs) detected by Webb NIRCam in 2022

🌡️ Dust Temperature 10 – 50 K

Extremely cold interior; surface heated to ~30,000 K by UV radiation

Remaining Lifespan ~3 Million Years

Photoevaporation by hot Trapezium stars will eventually dissolve the pillars

🪐 Composition H₂ + Dust

Molecular hydrogen gas (70%) and interstellar silicate/carbon dust grains

📸 First Famous Image April 1, 1995

Captured by Hubble’s Wide Field and Planetary Camera 2 (WFPC2)

🌌 Parent Region Eagle Nebula

The pillars occupy only a small corner of M16, a 70 light-year wide H II region

Discovery Timeline

From a blurry 19th-century sketch to Webb’s stunning 2022 infrared portraits — drag to scroll.

1745 First observed Swiss astronomer Jean-Philippe de Chéseaux catalogs the Eagle Nebula star cluster
1833 Messier designation M16 added to Messier’s catalog; the nebula’s extent becomes better appreciated
1995 Hubble iconic photo Jeff Hester & Paul Scowen photograph the pillars with WFPC2. Image becomes a cultural phenomenon.
2007 Chandra X-ray data NASA’s Chandra Observatory reveals hundreds of X-ray emitting young stars embedded in the nebula
2007 “Already destroyed?” Spitzer infrared data suggests a supernova shockwave may have vaporized the pillars 6,000 years ago — we’d see it in ~1,000 years
2015 Hubble 20th anniversary Hubble re-images the pillars with upgraded WFC3, producing a sharper visible and near-IR mosaic
2022 Webb NIRCam image JWST’s near-infrared camera pierces the dust, revealing thousands of newborn stars never seen before
2022 Webb MIRI image Mid-infrared view from MIRI maps warm dust thermal emission and PAH molecules across the nebula
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How Big Are They, Really?

The numbers are staggering. Here’s how the Pillars of Creation compare to other cosmic and human-scale distances.

The tallest pillar is approximately 5 light-years (47 trillion km) tall. To put that in context:

Light takes 8 minutes to travel from the Sun to Earth. It would take light 5 years to travel the full height of a single pillar — meaning if you shone a flashlight from the base, your great-grandchildren might not live to see it exit the top.

6 Remarkable Things About the Pillars

Beyond the iconic image, the science is even more astonishing.

01

They May Already Be Gone

Because the pillars are 6,500 light-years away, we’re seeing them as they were 6,500 years ago. Spitzer telescope data hints a supernova shockwave may have already vaporized them — but we won’t know for another ~1,000 years when the light from that event finally reaches us.

02

Stars Are Born in the Dark

The pillar interiors are so dense that visible light cannot escape — which is precisely why star formation happens inside them. The dust shields collapsing gas from the disruptive radiation of nearby stars, creating protected pockets where gravity can win. Webb’s infrared eyes can finally see inside.

03

They’re Being Eroded Right Now

Massive O-type stars in the Trapezium Cluster bombard the pillar surfaces with ultraviolet radiation, boiling off gas and dust in a process called photoevaporation. The wispy “fingers” at the pillar tips are streams of evaporating material being driven away at thousands of kilometres per hour.

04

Webb Revealed 8,000 New Stars

The 1995 Hubble image showed almost no stars — the dust blocked everything. When JWST turned its NIRCam on the same region in 2022, astronomers counted approximately 8,000 previously unknown stars, many still swaddled in protoplanetary disks and actively accreting material.

05

The EGGs Are Stellar Embryos

The dark fingertip “claws” visible at the top of each pillar are called Evaporating Gaseous Globules — EGGs. Each one is a dense knot of gas being sculpted by radiation, and many contain a protostar at their core. The pillars are essentially incubators for a generation of new solar systems.

06

A Snapshot Frozen in Time

Every telescope image is a time machine. The light we received in 1995 left the pillars in 4505 BCE — when ancient Egypt was in its early dynastic period. Webb’s 2022 images show the pillars as they looked around 4478 BCE. We are watching a stellar nursery that predates written human civilization.

Hubble vs. James Webb: Same Pillars, Different Universe

Both telescopes have imaged the Pillars — but what each reveals is radically different.

Hubble Space Telescope vs. James Webb Space Telescope
FeatureHubble (1995 / 2015)Webb (2022)
Primary wavelengthVisible light (380–700 nm)Near + Mid Infrared (0.6–28 µm)
Dust penetrationNear zero — pillars fully opaque80–99% — reveals interior stars
Stars detected~0 (obscured by dust)~8,000 (NIRCam) / ~25,000 (MIRI)
Pillar appearanceSolid, dramatic blue-green columnsSemi-transparent amber-gold pillars
Key instrumentsWFPC2 (1995), WFC3 (2015)NIRCam, MIRI
What it showsDust structure, pillar morphology, ionized gas surfacesProtostars, protoplanetary disks, warm dust chemistry
Mirror diameter2.4 metres6.5 metres (7× collecting area)
Operating temperature~15 °C (room temperature mirrors)−233 °C (cooled to near absolute zero)

Frequently Asked Questions

The most-searched questions about the Pillars of Creation, answered clearly.

Are the Pillars of Creation still there? +

Almost certainly yes — but we can’t be completely sure. Because the pillars are 6,500 light-years away, we see them as they were 6,500 years ago. NASA’s Spitzer Space Telescope detected infrared evidence in 2007 suggesting that a supernova shockwave (from a stellar explosion roughly 8,000–9,000 years ago in our timeline) may have already reached and destroyed the pillars. If so, we won’t see that destruction for another ~1,000 years. Most astronomers consider this scenario possible but not confirmed.

Why are they called the Pillars of Creation? +

The name was coined by astronomers Jeff Hester and Paul Scowen when they published their 1995 Hubble image. The “creation” refers to star formation — new stars are actively being born inside the dense interior of these pillars. The name was also evocative enough to capture public imagination, and it stuck. The phrase originally appeared in a 19th-century sermon by Charles Spurgeon (“pillars of creation”), which Hester and Scowen may have drawn from.

How far away are the Pillars of Creation? +

The Pillars of Creation are located approximately 6,500 light-years from Earth (about 61.5 quadrillion kilometres, or 38.2 quadrillion miles). They are part of the Eagle Nebula (Messier 16) in the constellation Serpens Cauda. Some measurements place them slightly closer at about 5,700 light-years; the value of 6,500 light-years is the most widely cited in NASA literature.

What is happening inside the Pillars of Creation? +

Inside the pillars, dense pockets of cold molecular hydrogen gas are slowly collapsing under gravity, heating up, and eventually igniting as new protostars and young stars. The pillars’ extreme density (they are opaque even to most UV light) shields the forming stars from the harsh radiation environment around them. Webb’s 2022 NIRCam image revealed hundreds of these young stellar objects — some still surrounded by protoplanetary disks that may one day form planetary systems.

Can you see the Pillars of Creation with a telescope? +

You can see the Eagle Nebula (M16) with a modest amateur telescope — it appears as a faint nebulous patch around a star cluster. However, the Pillars of Creation themselves are too small and too faint to be resolved by anything other than a very large professional telescope or space telescope. They span only a few arcminutes in the sky. Even in photographs from amateur telescopes, the pillars require significant image processing and a large aperture (12 inches or more) to hint at their structure.

What do the Pillars of Creation look like in infrared? +

In near-infrared (Webb NIRCam), the solid blue-green pillars become semi-transparent amber and brown structures — like frosted glass — filled with thousands of glittering stars that were completely invisible in optical light. In mid-infrared (Webb MIRI), the pillars practically vanish into a ghostly translucent haze, while the surrounding region blazes with warm dust emission and the chemical fingerprints of complex carbon molecules (PAHs). The two views look so different it can be hard to believe they show the same object.

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