noirlab_noao-ic239kempton February 19th, 2014
Credit: KPNO/NOIRLab/NSF/AURA/Sharon Kempton and Karen Brister/Adam Block
At a distance of 30-40 million light years IC 239 is not terribly distant. However, its low (surface) brightness may indicate that this galaxy isn't as massive as many others of the same type (M101 for example). The bright foreground stars of our own galaxy make detecting the delicate structure of this face-on spiral a difficult venture. There are hints of bluish spiral arms with a myriad of pink nebulae (star forming regions). If we lived in this galaxy, our sun would orbit the galactic center at a speed of 280km/s. This is a bit faster than our speed in the Milky Way at around 220km/s. This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.
Provider: NOIRLab
Image Source: https://noirlab.edu/public/images/noao-ic239kempton/
Curator: NSF's NOIRLab, Tucson, AZ, USA
Image Use Policy: Creative Commons Attribution 4.0 International License
Detailed color mapping information coming soon...
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