Image Source: NASA, ESA, CSA, and STScI | Image Description: An hourglass-shaped, multi-color cloud set against the black, starry background of space. This cloud of dust and gas is illuminated by light from a protostar, a star in the earliest stages of formation. The upper “bulb” of the hourglass is orange, while the lower “bulb” transitions from white to dark blue. Together, the two bulbs stretch out like butterfly wings turned 90 degrees to the side. Extending from the upper and lower bulbs are long, wispy filaments of color, looking almost like burning fire. In the center of the hourglass shape is a small, dark demarcation line. This line is an edge-on view of a protoplanetary disk, a disk of material being pulled into a star as it forms. End ID
The dark cloud L1527 within the Taurus star-forming region is only visible in infrared light, making it an ideal target for Webb’s Near-Infrared Camera (NIRCam). The protostar seen here is only about 100,000 years old, and is considered a Class 0 protostar - the earliest stage of star formation. It doesn't generate its own energy through nuclear fusion of hydrogen yet, and is still a small clump of hot puffy gas between 20 to 40% the mass of our Sun. As the protostar continues to gather mass, it gets closer to stable nuclear fusion. As material from the surrounding cloud falls into it, it spirals around the center and creates a dense disk of material called an accretion disk. The accretion disk is visible in this photo as a dark band in the center of the picture, and is about the size of our solar system.













