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Tarantula Nebula Spitzer 3-Color Image (Annotated)
Ssc2020 06c

Credit: NASA/JPL-Caltech

Observation • January 27th, 2020 • ssc2020-06c

ssc2020-06c

This image shows the location of Supernova 1987A and the starburst region R136 where massive stars form at a significantly higher rate than anywhere else in the galaxy.

NASA's Spitzer Space Telescope shows the Tarantula Nebula in three wavelengths of infrared light, each represented by a different color. The magenta-colored regions are dust composed of molecules called polycyclic aromatic hydrocarbons (PAHs), which are also found in ash from coal, wood and oil fires on Earth. PAHs emit in multiple wavelengths. The PAHs emit in multiple wavelengths, so the magenta color is a combination of red (corresponding to an infrared wavelength of 8 micrometers) and blue (3.6 micrometers). The green color in this image shows the presence of particularly hot gas emitting infrared light at a wavelength of 4.5 micrometers. The stars in the image are mostly a combination of green and blue. White hues indicate regions that radiate in all three wavelengths.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology, also in Pasadena. Caltech manages JPL for NASA.

About the Object

Name
Tarantula NebulaSN 1987aR136
Type
Nebula > Type > Star Formation
Nebula > Type > Supernova Remnant
Star > Grouping > Cluster
Star > Spectral Type > O
Distance
160,000 Light Years

Color Mapping

Band Wavelength Telescope
Infrared 3.6 µm Spitzer IRAC
Infrared 4.5 µm Spitzer IRAC
Infrared 8.0 µm Spitzer IRAC

Astrometrics

Position (J2000)
RA =5h 37m 49.3s
Dec = -69° 16' 2.6"
Field of View
58.9 x 33.1 arcminutes
Orientation
North is 90.0° left of vertical