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Monoceros R1 Nebular Complex containing NGC 2264, Jeff McClure

Monoceros R1 Nebular Complex containing NGC 2264

Getting plate-solving status, please wait...
Monoceros R1 Nebular Complex containing NGC 2264, Jeff McClure

Monoceros R1 Nebular Complex containing NGC 2264

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Description

Capturing and creating this image was one of the most difficult and time-consuming projects I have done in my 14 years of astrophotography. It comprises 12.5 hours of exposures captured on December 9, 10, and 11, in H-alpha, S-II, and O-III, plus several hours of calibration images. It took me about 40 hours to convert this from the resulting gigabyte of data into the finished product you see here. To reveal the structure of the sculpted surface of the nebula, I have shrunk the stars between us and the Monoceros R1 Nebula Complex (Mon R1 DNC), a mass of interstellar molecular cloud with a diameter of about 531 light years, with its boundaries at the left and right edges of this image. It is only a small portion of the unimaginably large band of clouds that wrap around the central portion of our galaxy and serve to shield us from what would otherwise be the deadly gamma ray radiation emitted by Sagittarius A, the supermassive black hole at our galaxy’s center.The image is of a fluorescing, star-sculpted area of that nebula (cloud) identified generally as NGC 2264 at the center of the Mon R1 Complex and is about 3,000 to 5,500 light-years from us. The structure of the cloud has been carved out by the white supergiant binary star S Monocerotis (S Mon) and the associated Christmas Tree star cluster. S Mon has 35 times the mass of our sun, is 217,000 times brighter, and is expelling a significant part of its mass each year, creating one of the most powerful stellar winds in our galaxy.

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Monoceros R1 Nebular Complex containing NGC 2264, Jeff McClure