Awash with Infrared Light

Mwplane-herschel

Creator: NASA Herschel Science Center

Image Source: http://www.herschel.caltech.edu/index.php?SiteSection=ImageGallery&ViewImage=nhsc2009-020a

Some of the coldest and darkest dust in space shines brightly in this infrared image from the Herschel Observatory, a European Space Agency mission with important participation from NASA. The image is a composite of light captured simultaneously by two of Herschel's three instruments -- the photodetector array camera and spectrometer, and its spectral and photometric imaging receiver.

The image reveals a cold and turbulent region where material is just beginning to condense into new stars. It is located in the plane of our Milky Way galaxy, 60 degrees from the center. Blue shows warmer material, red the coolest, while green represents intermediate temperatures. The red filaments are made up of the coldest material pictured here -- material that is slightly warmer than the coldest temperature theoretically attainable in the universe.

Light captured by the photodetector array camera and spectrometer is colored blue and green (blue represents 70-micron light, and green, 160-micron light). The light detected by the spectral and photometric imaging receiver is colored red (and shows the combined wavelengths of 250, 350 and 500 microns). The image spans a region 2.1 by 2.2 degrees.

View Options

Image Details

Image Type
Observation
Object Name
Milky Way

Color Mapping

  Telescope Spectral Band Wavelength
Arrow_left_blue Herschel (PACS) Infrared (Far-IR) 70.0 µm
Arrow_left_green Herschel (PACS) Infrared (Far-IR) 160.0 µm
Arrow_left_red Herschel (SPIRE) Infrared (Far-IR) 250.0 µm
Arrow_left_red Herschel (SPIRE) Infrared (Far-IR) 350.0 µm
Arrow_left_red Herschel (SPIRE) Infrared (Far-IR) 500.0 µm
Spectrum_ir1
Arrow_top_blue
Arrow_top_green
Arrow_top_red
Arrow_top_red
Arrow_top_red