noirlab_noao-ic417 June 30th, 2020
Credit: T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOIRLab/NSF/AURA)
This image was obtained with the wide-field view of the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory. Informally known as the spider, IC 417 is an emission nebula that is energized by embedded hot, massive blue stars. The bluish clouds of gas at the top of the image are locations of new star formation. The image was generated with observations in the B (blue), I (orange) and Hydrogen-Alpha (red) filters. In this image, North is left, East is down.
Provider: NOIRLab
Image Source: https://noirlab.edu/public/images/noao-ic417/
Curator: NSF's NOIRLab, Tucson, AZ, USA
Image Use Policy: Creative Commons Attribution 4.0 International License
| Telescope | Spectral Band | Wavelength | |
|---|---|---|---|
|
KPNO-4m (Mosaic I) | Optical (Olll) | 502.0 nm |
|
KPNO-4m (Mosaic I) | Optical (Sll) | 673.0 nm |
|
KPNO-4m (Mosaic I) | Optical (R) | 651.0 nm |
|
KPNO-4m (Mosaic I) | Optical (V) | 538.0 nm |
|
KPNO-4m (Mosaic I) | Optical (U) | 355.0 nm |
|
KPNO-4m (Mosaic I) | Optical (Ha) | 656.0 nm |
|
KPNO-4m (Mosaic I) | Optical (I) | 805.0 nm |
|
KPNO-4m (Mosaic I) | Optical (B) | 436.0 nm |
Detailed color mapping information coming soon...
Providers | Sign In