![]() Given its age and its brightness in far-infrared light as observed by missions like the Infrared Astronomical Satellite, L1527 is considered a class 0 protostar, the earliest stage of star formation. As a result, the protostar dominates the space, taking much of the material for itself.ĭespite the chaos that L1527 causes, it’s only about 100,000 years old – a relatively young body. Shocks and turbulence inhibit the formation of new stars, which would otherwise form all throughout the cloud. Webb also reveals filaments of molecular hydrogen that have been shocked as the protostar ejects material away from it. The thicker the layer of dust, the less blue light is able to escape, creating pockets of orange. ![]() The blue areas are where the dust is thinnest. The colors themselves are due to layers of dust between Webb and the clouds. ![]() The region’s most prevalent features, the clouds colored blue and orange in this representative-color infrared image, outline cavities created as material shoots away from the protostar and collides with surrounding matter. Koekemoer (STScI)ĭownload the full-resolution image from the Space Telescope Science Institute. ![]()
0 Comments
Leave a Reply. |
AuthorWrite something about yourself. No need to be fancy, just an overview. ArchivesCategories |