Cocoons for Young Stars

The initial collapse phase of star formation before fusion reactions are initiated is termed the protostar phase. When collapsing protostars form inside nebulae, they are surrounded initially by the gas and dust cloud from which they condensed. These "cocoons" of gas and dust are opaque to visible light, but we can see evidence for the protostars hiding inside in IR light.
The Eagle Nebula
The visible-light image adjacent right shows starbirth regions in the Eagle Nebula (M16), which is about 7000 light years away in the constellation Serpens. The yellow rectangle in the inset indicates the region of the nebula blown up in the main part of the image. The clouds are columns of cool molecular hydrogen and dust that that serve as incubators for new stars. The tallest is almost a light year in length!

Erosion in Astronomy and Geology

The process producing EGGs by "erosion" with UV photons is similar to the water and wind erosion that produces many striking landscapes in the Western United States. For example, a feature like Ship Rock in New Mexico represents the throat of an old volcano that contained much harder rock than the surrounding region. Thus, when the surrounding softer rock has been eroded away, Ship Rock remains. EGGs are similar; they remain after the surrounding "soft" gas has been eroded away.

The Eagle's EGGs
Nearby hot stars (approximately 100 young stars can be counted in this part of the nebula) are emitting a flood of UV photons. The strong flux of photons is heating the gas of the nebula and causing it to be driven off in a process called photoevaporation.

This photoevaporation uncovers small globules of dense gas buried within the cloud that are less susceptible to evaporation. These are termed EGGs ("Evaporating Gaseous Globules"). They are evaporating too, but much more slowly than the surrounding lower-density gas (see the adjacent box). The finger-like structures at the tops of the clouds are larger than the Solar System and hide embryonic stars that are forming within them. They are produced by the shadows of the EGGs, which protect the gas behind them from the intense UV flux.

Starbirth in the Trifid
The image adjacent left shows a region of star birth in the Trifid Nebula, which is approximately 9000 light years away in the constellation Sagittarius. There is a hot, young star above and to the right of this image. When it formed, its radiation and stellar wind swept away much of the gas in this region and only low-mass stars are presently forming here.

The pillars visible in the image were more dense than their surroundings and thus have survived, though they too are being eroded by the radiation and wind from hot stars. The unusual jet of material that can be seen in the upper left is not well understood, though its source presumably lies hidden in the large left pillar. The red dots are newly formed low-mass stars.