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Visual Timeline of the Universe

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Protoplanetary Disks

Circumstellar Debris Disk - Forming planetary systems may appear as dark or luminous disks silhouetted against a glowing nebula.

Circumstellar Debris Disk - Forming planetary systems may appear as dark or luminous disks silhouetted against a glowing nebula.

NASA, ESA, and P. Kalas (University of California, Berkeley)
Forming planetary systems may appear as dark or luminous disks silhouetted against a glowing nebula. Others, deeply embedded in their natal clouds, can be seen only in infrared light. Still others show knots of material with long, comet-like streamers formed as an interstellar wind blows the area clear.

These protoplanetary regions are up to 20 times the diameters of our solar system. All the material in a protoplanetary disk spins in the same direction around the star. The disk includes the complex molecules found in the original nebula, plus others that may form as the density and temperature change in the dense regions of the nebula surrounding the star.

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