PIA03031: Amazing Andromeda in Red
Target Name: M31
Mission: Spitzer Space Telescope
Instrument: MIPS
Product Size: 8193 x 2410 pixels (width x height)
Produced By: California Institute of Technology
Full-Res TIFF: PIA03031.tif (19.75 MB)
Full-Res JPEG: PIA03031.jpg (3.247 MB)

Click on the image above to download a moderately sized image in JPEG format (possibly reduced in size from original)

Original Caption Released with Image:

figure 1 for PIA03031 Dust in Andromeda Galaxy (M31)
Figure 1
Dust in Andromeda Galaxy (M31)

figure 2 for PIA03031 Infrared (24, 70, 160 microns)figure 3 for PIA03031 Visible
Figure 2
Infrared (24, 70, 160 microns)
Figure 3

NASA's Spitzer Space Telescope has captured this stunning infrared view of the famous galaxy Messier 31, also known as Andromeda. Spitzer's 24-micron mosaic (main image) is the sharpest image ever taken of the dust in a spiral galaxy, other than our Milky Way. Asymmetrical features are seen in the prominent ring of star formation, which appears to be split into two pieces, forming the hole to the lower right. These features may have been caused by interactions with satellite galaxies around Andromeda as they plunged through its disk.

At optical wavelengths, the center of the galaxy is dominated by a large bulge. This bulge is far less pronounced in the Spitzer 24-micron infrared image, allowing us to see the delicate tracings of spiral arms in the inner region that reach into the center of the galaxy. One sees the scattering of stars within Andromeda, but only select stars that are wrapped in envelopes of dust light up at infrared wavelengths.

The multi-wavelength view of Andromeda (figure 2) combines images taken at 24 microns (blue), 70 microns (green), and 160 microns (red). Use of all three bands from the multiband imaging photometer allows the astronomers to measure the temperature of the dust by its color. The warmest dust is brightest at 24 microns, while the coolest is most evident at 160 microns. The blue/white areas have the hottest dust, as seen in the bulge and in the star-forming areas along the arms. The cooler dust floating in the ring and arms are the redder regions.

This is a dramatic contrast to the traditional view at visible wavelengths (figure 3), which shows the starlight instead of the dust. The center of the galaxy in this optical view is dominated by a large bulge that overwhelms the inner spirals seen in dust. The dust lanes are faintly visible in places, but only where they can be seen in silhouette against background stars.

The data were taken on August 25, 2004, the one-year anniversary of the launch of the space telescope. The observations have been transformed into this remarkable gift from Spitzer the most detailed infrared image of the spectacular galaxy to date.

Image Credit:
NASA/JPL-Caltech/Univ. of Ariz.

Image Addition Date: