Celestial hemisphere:  Northern  ·  Constellation: Auriga (Aur)  ·  Contains:  B25  ·  LBN 737  ·  LBN 742  ·  LBN 744  ·  LBN 745  ·  LBN 747  ·  LBN 754  ·  LBN 755  ·  LBN 759  ·  LDN 1465  ·  LDN 1475  ·  Sh2-216  ·  Sh2-217  ·  Sh2-219  ·  Sh2-221
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Fraternal Twins - Sh2-216 & 221 - SHO, Timothy Martin
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Fraternal Twins - Sh2-216 & 221 - SHO

Getting plate-solving status, please wait...
Fraternal Twins - Sh2-216 & 221 - SHO, Timothy Martin
Powered byPixInsight

Fraternal Twins - Sh2-216 & 221 - SHO

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Description

This image depicts many phases of stellar birth and death.

Sh2-221 (on the left) is a supernova remnant about 2,600 light years distant that came from a star that exploded approximately 6,000 years ago. It's roughly 130 light years in diameter. The star, which was once much like our sun, that created the planetary nebula Sh2-216 (on the right) started dying its slow death a half million years ago, which makes it ancient by planetary-nebula standards. Sh2-216 is much closer at around 400 light years and is much smaller, at 11 light years in diameter. It's the second-closest known planetary nebula--also the largest and the oldest. 

The yellow-orange blob above Sh2-221 is Sh2-217. It's part of a larger star-forming region and contains around 4,100 solar masses of material. The aforementioned star-forming region is very young for such things at only 4 million years old. Sh2-217 is about 13,700 light years away and about 35 light years across at its widest point. Looking like it sits atop Sh2-221's right shoulder, the smaller Sh2-219 is part of the same star-forming region as Sh2-217 and is about the same distance from us. The emission nebula BFS 44/LBN 755 at the bottom of the frame between the two large objects is also part of the same star-forming region.

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