Carbon Monoxide

Basic Information

What is this?

A map of carbon monoxide in our Galaxy

Where is it in the sky?

Carbon monoxide tends to be located in the plane of our Galaxy, but has now been found in more locations

How big is it?

The image above shows the entire sky, with the disc of our Galaxy across the centre

How far away is it?

Most of the carbon monoxide is thousands of light years away, though some of the closer regions are probably much closer

What do the colours represent?

The brighter colours show a higher density of carbon monoxide. The faint stripes across the image are due to the way in which Planck scans the sky, combined with the map is made.
Carbon monoxide detected by Planck, compared with a previous survey
Planck detections of carbon monoxide (blue), combined with the results of the "Dame survey" from 2001 (red). The region that the Dame survey covered is outlined. Image credit: ESA/Planck collaboration/T. Dame et al. (2001)

Clouds of cold gas are mostly made of molecules of hydrogen. This molecular hydrogen is very hard to detect as it doesn't emit much light. However, the gas clouds also contain smaller amounts of other molecules which emit light more readily. One such molecule, carbon monoxide, emits light at frequencies which are measured by Planck's High Frequency Instrument. These cold gas clouds mark locations where stars are likely to be forming. The way in which Planck surveys the sky, combined with the process of extraction of the carbon monoxide emission, leaves stripes across the map, which are visible in the image above.

Carbon monoxide has been detected by previous ground-based experiments, but such experiments are very time consuming and only cover limited areas of the sky, primarily in the plane of our Galaxy. Planck, meanwhile, surveys the whole sky, and so can pick out carbon monoxide in previously unknown locations. A comparison of the Planck carbon monoxide map with that from a previous survey is shown on the right.

While Planck has seen more detail in some known location, such as in the constellations of Cepheus and Taurus, it has also picked out small clouds in locations such as the constellation of Pegasus, shown below. These regions can now be investigated in much more detail by other telescope, both on the ground and in space.

Cepheus
Planck & Dame survey
Taurus
Planck & Dame survey
Pegasus
Planck only
CO in Cepheus
CO in Taurus
CO in Pegasus

Detailed Information

Object Name: 
Carbon Monoxide
Type of Object: 
Foreground component
Image Scale: 
The image covers the entire sky
Instrument: 
HFI
Date of Release: 
13/02/2012