Andromeda’s coat of many colours


 
Andromeda in multiple wavelengths
 
27 April 2011
 
ESA’s fleet of space telescopes has captured the nearby Andromeda Galaxy, also known as M31, in different wavelengths. Most of these wavelengths are invisible to the eye and each shows a different aspect of the galaxy’s nature.
 
Visible light, as seen by optical ground-based telescopes and our eyes, reveals the various stars that shine in the Andromeda Galaxy, yet it is just one small part of the full spectrum of electromagnetic radiation. There are many different wavelengths that are invisible to us but which are revealed by ESA’s orbiting telescopes.

Starting at the long wavelength end, the Planck spacecraft collects microwaves. These show up particles of incredibly cold dust, at just a few tens of degrees above absolute zero. Slightly higher temperature dust is revealed by the shorter, infrared wavelengths observed by the Herschel space telescope. This dust traces locations in the spiral arms of the Andromeda Galaxy where new stars are being born today.

The XMM-Newton telescope detects wavelengths shorter than visible light, collecting ultraviolet and X-rays. These show older stars, many nearing the end of their lives and others that have already exploded, sending shockwaves rolling through space. By monitoring the core of Andromeda since 2002, XMM-Newton has revealed many variable stars, some of which have undergone large stellar detonations known as novae.

Ultraviolet wavelengths also display the light from extremely massive stars. These are young stars that will not live long. They exhaust their nuclear fuel and explode as supernovae typically within a few tens of millions of years after they are born. The ultraviolet light is usually absorbed by dust and re-emitted as infrared, so the areas where ultraviolet light is seen directly correspond to relatively clear, dust-free parts of Andromeda.

By putting all of these observations together, and seeing Andromeda in its many different colours, astronomers are able to follow the life cycle of the stars.
 
 


More information

 •  Planck overview (http://www.esa.int/SPECIALS/Planck/index.html#a)
 •  Herschel overview (http://www.esa.int/SPECIALS/Herschel/index.html)
 •  XMM-Newton overview (http://www.esa.int/esaSC/120385_index_0_m.html)
 •  Online Showcase of Herschel Images OSHI (http://oshi.esa.int/)

ESA on YouTube

 •  Inside Herschel (http://www.youtube.com/watch?v=j9_VBKn8Jq4 &feature=PlayList &p=CD471914889C152B &index=1)
 •  XMM-Newton mission (http://www.youtube.com/watch?v=8n0ziDKsV0Y)
 •  Planck mission (http://www.youtube.com/watch?v=Ijl_N-Vz5Vg &feature=channel_video_title)

Related articles

 •  Andromeda’s once and future stars (http://www.esa.int/esaCP/SEMY1K0SDIG_index_0.html)
 •  Recipe for water: just add starlight (http://www.esa.int/esaCP/SEMW76EODDG_index_0.html)
 •  Herschel and Planck win the French Grand Prix (http://www.esa.int/esaCP/SEMARKPK2AG_index_0.html)
 •  Herschel finds a hole in space (http://www.esa.int/esaCP/SEMFEAKPO8G_index_0.html)
 •  XMM-Newton uncovers a celestial Rosetta stone (http://www.esa.int/esaCP/SEM4F8LW3ZF_index_0.html)
 •  XMM-Newton discovers a new class of black holes (http://www.esa.int/esaCP/SEMZGM1P0WF_index_0.html)
 •  Giant eruption reveals 'dead' star (http://www.esa.int/esaCP/SEMLEDQORVF_index_0.html)
 •  XMM-Newton exclusive photo: Messier 82 (http://www.esa.int/esaSC/SEMC5IEH1TF_index_0.html)
 •  Planck’s new view of the cosmic theatre (http://www.esa.int/esaCP/SEMK4D3SNIG_index_0.html)
 •  Planck unveils the Universe – now and then (http://www.esa.int/esaCP/SEMF2FRZ5BG_index_0.html)
 •  Planck highlights the complexity of star formation (http://www.esa.int/esaCP/SEM0FVF098G_index_0.html)

Read more

 •  Herschel in depth (http://sci.esa.int/science-e/www/area/index.cfm?fareaid=16)
 •  XMM-Newton in-depth (http://sci.esa.int/science-e/www/area/index.cfm?fareaid=23)
 •  Planck in depth (http://sci.esa.int/science-e/www/area/index.cfm?fareaid=17)