Download Image
- TIFF
About the Image
- Date
- 2003-11-24
- ID
- ssc2003-06e
- Type
- Observation
- Credit
- NASA/JPL-Caltech/K. Gordon (University of Arizona)
- Observers
- Karl D. Gordon, Principal Investigator (University of Arizona) Steven P. Willner, Principal Investigator (Harvard-Smithsonian Center for Astrophysics) Almudena Alonso-Herroro (University of Arizona) Philip Appleton (SSC/Caltech) Matthew L. N. Ashby (Harvard-Smithsonian Center for Astrophysics) Pauline Barmby (Harvard-Smithsonian Center for Astrophysics) Chad Engelbracht (University of Arizona) Giovanni G. Fazio (Harvard-Smithsonian Center for Astrophysics) David Frayer (SSC/Caltech) George Helou (SSC/Caltech) Joannah Hinz (University of Arizona) Robert Kennicutt (University of Arizona) Karl Misselt (University of Arizona) Michael A. Pahre (Harvard-Smithsonian Center for Astrophysics) Pablo Perez-Gonzalez (University of Arizona) George Rieke (University of Arizona) Marcia Rieke (University of Arizona) Susan Stolovy (SSC/Caltech) Lisa Storrie-Lombardi (SSC/Caltech)
About the Object
- Name
- Bode's Galaxy • Messier 81 • M81 • NGC 3031 • UGC 5318
- Type
- Galaxy > Type > Spiral
- Distance
- 12,000,000 Light Years
- Redshift
- -0.000113
Color Mapping
| Band | Wavelength | Telescope |
| Infrared | 24.0 µm | Spitzer MIPS |
| Infrared | 70.0 µm | Spitzer MIPS |
| Infrared | 160.0 µm | Spitzer MIPS |
Astrometrics
- Position (J2000)
- RA = 9h 55m 34.0s
- Dec = 69° 3' 54.9"
- Field of View
- 23.5 x 17.9 arcminutes
- Orientation
- North is 268.7° left of vertical
- Constellation
- Ursa Major
Messier 81
The magnificent and dusty spiral arms of the nearby galaxy Messier 81 are highlighted in these NASA Spitzer Space Telescope images. Located in the northern constellation of Ursa Major (which also includes the Big Dipper), this galaxy is easily visible through binoculars or a small telescope. M81 is located at a distance of 12 million light-years.
The three-panel mosaic is a series of images obtained with the multiband imaging photometer. Thermal infrared emission at 24 microns (top), 70 microns (center) and 160 microns (bottom) is shown in the images. Note that the effective spatial resolution degrades as ones moves to longer wavelengths.
At these wavelengths, Spitzer sees the dust, rather than the stars, within the disc of silicates and carbonaceous grains. It is well-mixed with gas, which is best seen at radio wavelengths, to form the essential ingredients for future star formation.
Related Media
|
News Release NASA Releases Dazzling Images from New Space Telescope ssc2003-06 |
|
|
Image Dark Globule in IC 1396 ssc2003-06a |
|
|
Image Dark Globule in IC 1396 ssc2003-06b |
|
|
Image Spiral Galaxy Messier 81 ssc2003-06c |
|
|
Image Spiral Galaxy Messier 81 ssc2003-06d |
|
|
Image Messier 81 ssc2003-06e |
|
|
Image Embedded Outflow in HH 46/47 ssc2003-06f |
|
|
Image Embedded Outflow in HH 46/47 ssc2003-06g |
|
|
Image Galaxy IRAS F00183-7111 ssc2003-06h |
|
|
Image Fomalhaut Circumstellar Disk ssc2003-06i |
|
|
Image Comet Schwassmann-Wachmann 1 ssc2003-06j |























