Young Stars across Each Formation Stage in Orion | James Webb Space Telescope
Behind the stars, gas, and dust of M42 is a long, massive filament of cold gas and dust called (somewhat confusingly) the Orion Molecular Clouds, divided into four parts, OMC-1 through OMC-4. OMC-1 sits immediately behind M42, to the north are OMC-2 and OMC-3, and OMC-4 lies to the south.
This image shows just a small, northern portion of OMC-2, located 1280 light-years from Earth and a little north of the Orion Nebula. Every stage of star formation—from the youngest stellar embryos, to protoplanetary discs, to newly-minted pre-main sequence stars—is contained within just this scene, stretching 150 light-years across. The intense star-forming activity has produced an impressive display of billowing outflows and sparkling stars atop swirling layers of gas and dark, obscuring clouds.
Molecular clouds, such as OMC-2, are vast clumps of gas much more dense than the rest of interstellar space. This density allows complex molecules to form, protected from the radiation given off by other stars, and it means that gravity can cause the cloud to collapse and form stars. The earliest stage of this process is a protostar—a growing star that is being fed gas from the surrounding cloud through a spinning disc of gas. As gas falls onto the protostar, it heats up, powering the glow of the protostar. The immense amount of energy acquired during this process is unleashed in fierce jets of gas from the poles of the star, frequently seen as twin glowing outflows that mark the location of a protostar.
The abundance of protostars forming here in OMC-2 has created many spectacular outflows, large and small. Jets emitted from the young stars form high-speed shockwaves that sweep through the dense material around them; where the shockwaves are impacting the gas, it heats up and glows brightly, creating sharp ridges. Zoom in to observe the fine details in these shockwaves, as well as spot the smaller outflows from younger protostars. See if you can spot the location of hidden protostars, still so deeply obscured by their dusty cradles that they cannot be seen directly, by following outflows. Compare these very young protostars to the most evolved examples: the large, bright stars have cleared away the clouds that surrounded them and now illuminate OMC-2.
Webb’s Near-Infrared Camera (NIRCam) was used to capture this view of OMC-2. The thick gas and dust in and around the Orion Nebula blocks any light coming from OMC-2 at visible wavelengths, and the clouds in OMC-2 itself obscure the protostars that astronomers really want to find. Only in the infrared do we see these protostars begin to shine out from their cocoons of dust. In many places, the cold dust is so dense that it absorbs all or almost all light, creating dark globules. Orange, brown and some of the red colors mark warmer dust that absorbs light and emits its own. The yellow to green gradient is largely emission from polycyclic aromatic hydrocarbons (PAHs), while light from stars and protostars scattered by dust grains is seen here primarily as blue and cyan hazes. Gas heated by the outflows creates the detailed, glowing red ridges.
The data was collected in observing program #5804. It aims to study the star formation in OMC-2 and its immediate neighbor, OMC-3. Since these molecular clouds are so near to Earth, they are excellent laboratories to learn about the earliest stages of stellar evolution. Astronomers will use the data from Webb to investigate how the many outflows affect star formation in the two regions, how the ultraviolet emission from the young stars impacts chemistry in the circumstellar discs that one day will form planets, and how gas and dust accretes onto the tens of protostars in the region.
Image Description: An area inside a star-forming molecular cloud. The background is covered with layers of gas and dust in blue, green, and yellowish colors. Thicker clumps of cold dust, dark brown to black, block out light completely. Stars lie among and atop the clouds, from small orange ones to large white or blue ones. Waves and streams of glowing whitish gas are created by jets from protostars colliding with the surrounding material.
Acknowledgement: M. H. Özsaraç
Release Date: June 5, 2026
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