Celestial hemisphere:  Northern  ·  Constellation: Perseus (Per)  ·  Contains:  B1  ·  HD21864  ·  HD22195  ·  HD22360  ·  HD22418
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Perseus Molecular Cloud, John Bozeman
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Perseus Molecular Cloud

Getting plate-solving status, please wait...
Perseus Molecular Cloud, John Bozeman
Powered byPixInsight

Perseus Molecular Cloud

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Description

The Perseus molecular cloud (Per MCld) is a nearby (~1000 ly) giant molecular cloud in the constellation of Perseus and contains over 10,000 solar masses of gas and dust covering an area of 6 by 2 degrees. Unlike the Orion molecular cloud it is almost invisible apart from two clusters, IC 348 and NGC 1333, where low-mass stars are formed. It is very bright at mid and far-infrared wavelengths and in the submillimeter originating in dust heated by the newly formed low-mass stars.

12 micron IR data from the WISE All Sky Survey. Processed with FITS Liberator, PixInsight and Photoshop 2023.

This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration.

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Perseus Molecular Cloud, John Bozeman