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Last update: October 15, 2025

The Eagle Nebula: Stellar Nursery and Pillars of Creation

Eagle Nebula: M16

The Eagle Nebula

The Eagle Nebula (Messier 16, or M16) is an H II region located in the constellation Serpens, about 7,000 light-years from Earth. This nebula is famous for its Pillars of Creation, giant columns of gas and dust where new stars are born. Observations in visible and infrared light have revealed the complex structure of these pillars, which are sculpted by stellar winds and ultraviolet radiation from nearby massive stars.

Structure and Dynamics of the Pillars of Creation

Pillars of Creation in the Eagle Nebula

The pillars are several light-years long and are composed mainly of molecular gas and dust. The combined action of gravity and radiative pressures causes the fragmentation of clouds and the formation of dense clumps at their tips. Hydrodynamic models suggest that ionized fronts move at speeds of the order of 10 to 20 km/s, gradually eroding the columns.

Star Formation and Astrochemistry

Within M16, protostars form in the dense regions of the pillars. Intense UV radiation ionizes the surrounding gas, creating dense globules called EGGs that can eventually become full-fledged stars. Spectroscopic analysis reveals the presence of molecules such as CO, H2, and ions of sulfur and oxygen, essential for the chemistry of star-forming regions.

Comparative Table of Physical Properties

Here is a table comparing some physical characteristics of the Eagle Nebula and other famous H II regions:

Comparison of H II Regions
RegionSize (light-years)Temperature (K)Average Density (cm-3)Comments
Eagle Nebula (M16)~70 × 558,000500 to 2,000Pillars of Creation, EGGs, formation of open clusters
Orion Nebula (M42)~2410,0001,000 to 5,000Close, massive star formation, easy observation
Lagoon Nebula (M8)~1108,500300 to 1,500Complex of young stars, ionized gas

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