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Cosmic Question Mark (NGC 7822), Harold Soto
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Cosmic Question Mark (NGC 7822)

Getting plate-solving status, please wait...
Cosmic Question Mark (NGC 7822), Harold Soto
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Cosmic Question Mark (NGC 7822)

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Description

What Do You See?

Meet NGC 7822, a giant molecular cloud and star-forming region in Cepheus. This is the brightest portion of the "Question Mark Nebula", an enormous emission nebula that you will probably need to capture via a mosaic.

It may look like a huge cosmic question mark, but the big question really is how does the bright gas and dark dust tell this nebula's history of star formation. At the edge of a giant molecular cloud toward the northern constellation Cepheus, the glowing star forming region NGC 7822 lies about 3,000 light-years away. Within the nebula, bright edges and dark shapes stand out in this colorful and detailed skyscape. The emission line and color combination has become well-known as the Hubble palette. The atomic emission is powered by energetic radiation from the central hot stars. Their powerful winds and radiation sculpt and erode the denser pillar shapes and clear out a characteristic cavity light-years across the center of the natal cloud. Stars could still be forming inside the pillars by gravitational collapse but as the pillars are eroded away, any forming stars will ultimately be cut off from their reservoir of star stuff. This field of view spans over 40 light-years across at the estimated distance of NGC 7822.

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Cosmic Question Mark (NGC 7822), Harold Soto