File:PIA22568-CatsPawNebula-Spitzer-20181023.jpg
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| DescriptionPIA22568-CatsPawNebula-Spitzer-20181023.jpg |
English: PIA22568: Cat's Paw Image 1
https://www.spitzer.caltech.edu/image/ssc2018-14a-the-cats-paw-nebula-mips-irac RELATED IMAGE => https://photojournal.jpl.nasa.gov/catalog/PIA22567 The Cat's Paw Nebula, imaged here by NASA's Spitzer Space Telescope, lies inside the Milky Way Galaxy and is located in the constellation Scorpius. Its distance from Earth is estimated to be between 1.3 kiloparsecs (about 4,200 light years) to 1.7 kiloparsecs (about 5,500 light years). The bright, cloudlike band running left to right across the image shows the presence of gas and dust that can collapse to form new stars. The black filaments running through the nebula are particularly dense regions of gas and dust. The entire star-forming region is thought to be between 24 and 27 parsecs (80-90 light years) across. The stars that form inside the nebula heat up the pressurized gas surrounding them, such that the gas may expand and form "bubbles", which appear red in this image. Asymmetric bubbles may "burst," creating U-shaped features. The green areas show regions where radiation from hot stars collided with large molecules and small dust grains called "polycyclic aromatic hydocarbons" (PAHs), causing them to fluoresce. This image was compiled using data from two Spitzer instruments, the Infrared Array Camera (IRAC) and the Multiband Imaging Photometer (MIPS). The colors correspond with wavelengths of 3.6 microns (blue), 4.5 microns (cyan), 8 microns (green) and 24 microns (red). NASA's Jet Propulsion Laboratory, Pasadena, California, manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at Caltech in Pasadena, California. Spacecraft operations are based at Lockheed Martin Space Systems Company, Littleton, Colorado. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech. Caltech manages JPL for NASA. For more information about the Spitzer mission, visit http://www.nasa.gov/spitzer and http://spitzer.caltech.edu. Photojournal Note: Also available is the full resolution TIFF file PIA22568_full.tif. This file may be too large to view from a browser; it can be downloaded onto your desktop by right-clicking on the previous link and viewed with image viewing software. |
| Date | |
| Source | https://photojournal.jpl.nasa.gov/jpeg/PIA22568.jpg |
| Author | NASA/JPL-Caltech |
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23 October 2018
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 21:39, 24 August 2024 | 11,402 × 4,215 (9.23 MB) | Fabian RRRR | full resolution, source https://www.spitzer.caltech.edu/system/avm_images/binaries/6551/jpg_original/ssc2018-14a.jpg |
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| Date and time of data generation | 23 October 2018 |
| Contact information |
http://www.spitzer.caltech.edu 1200 E. California Blvd. Pasadena, CA, 91125 USA |
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| Credit/Provider | NASA/JPL-Caltech |
| Headline | The Cat's Paw Nebula, imaged here by NASA's Spitzer Space Telescope using the MIPS and IRAC instruments, is a star-forming region that lies inside the Milky Way Galaxy. New stars may heat up the surrounding gas, which can expand to form"bubbles." |
| Source | Spitzer Space Telescope |
| JPEG file comment | The Cat's Paw Nebula, imaged here by NASA's Spitzer Space Telescope using the MIPS and IRAC instruments, is a star-forming region that lies inside the Milky Way Galaxy. New stars may heat up the surrounding gas, which can expand to form "bubbles." |