"We used a trick called earthshine observation to look at the Earth as if it were an exoplanet," says Michael Sterzik (ESO), lead author of the paper . "The Sun shines on the Earth and this light is reflected back to the surface of the Moon. The lunar surface acts as a giant mirror and reflects the Earth's light back to us -- and this is what we have observed with the VLT."
The astronomers analyse the faint earthshine light to look for indicators, such as certain combinations of gases in the Earth's atmosphere , that are the telltale signs of organic life. This method establishes the Earth as a benchmark for the future search for life on planets beyond our Solar System.
The fingerprints of life, or biosignatures, are hard to find with conventional methods, but the team has pioneered a new approach that is more sensitive. Rather than just looking at how bright the reflected light is in different colours, they also look at the polarisation of the light , an approach called spectropolarimetry. By applying this technique to earthshine observed with the VLT, the biosignatures in the reflected light from Earth show up very strongly.
Co-author of the study Stefano Bagnulo (Armagh Observatory, Northern Ireland, United Kingdom) explains the advantages: "The light from a distant exoplanet is overwhelmed by the glare of the host star, so it's very difficult to analyse -- a bit like trying to study a grain of dust beside a powerful light bulb. But the light reflected by a planet is polarised, while the light from the host star is not. So polarimetric techniques help us to pick out the faint reflected light of an exoplanet from the dazzling starlight."
The team studied both the colour and the degree of polarisation of light from the Earth after reflection from the Moon, as if the light was coming from an exoplanet. They managed to deduce that the Earth's atmosphere is partly cloudy, that part of its surface is covered by oceans and -- crucially -- that there is vegetation present. They could even detect changes in the cloud cover and amount of vegetation at different times as different parts of the Earth reflected light towards the Moon.
"Finding life outside the Solar System depends on two things: whether this life exists in the first place, and having the technical capability to detect it," adds co-author Enric Palle (Instituto de Astrofisica de Canarias, Tenerife, Spain). "This work is an important step towards reaching that capability."
"Spectropolarimetry may ultimately tell us if simple plant life -- based on photosynthetic processes -- has emerged elsewhere in the Universe," concludes Sterzik. "But we are certainly not looking for little green men or evidence of intelligent life."
The next generation of telescopes, such as the E-ELT (the European Extremely Large Telescope), may well be able to bring us the extraordinary news that the Earth is not alone as a bearer of life in the vastness of space.
 Earthshine, sometimes called the old Moon in the new Moon's arms, can easily be seen with the unaided eye and is spectacular in binoculars. It is best seen when the Moon is a thin crescent, about three days before or after new Moon. As well as the bright crescent the rest of the lunar disc is visible, dimly illuminated by the bright Earth in the lunar sky.
 In the Earth's atmosphere, the main biologically produced gases are oxygen, ozone, methane and carbon dioxide. But these can all occur naturally in a planet's atmosphere without the presence of life. What constitutes a biosignature is the simultaneous presence of these gases in quantities that are only compatible with the presence of life. If life were suddenly to disappear and no longer continuously replenish these gases they would react and recombine. Some would quickly disappear and the characteristic biosignatures would disappear with them.
 When light is polarised, its component electric and magnetic fields have a specific orientation. In unpolarised light the orientation of the fields is random and has no preferred direction. The trick used in some 3D cinemas involves polarised light: separate images made with differently polarised light are sent to our left and right eyes by polarising filters in the glasses. The team measured the polarisation using a special mode of the FORS2 instrument on the VLT.
This research was presented in a paper, "Biosignatures as revealed by spectropolarimetry of Earthshine", by M. Sterzik et al. to appear in the journal Nature on 1st March 2012.
The team is composed of Michael F. Sterzik (ESO, Chile), Stefano Bagnulo (Armagh Observatory, Northern Ireland, UK) and Enric Palle (Instituto de Astrofisica de Canarias, Tenerife, Spain).
The year 2012 marks the 50th anniversary of the founding of the European Southern Observatory (ESO). ESO is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 15 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the world's largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 40-metre-class European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".
- Research paper: Nature paper: http://www.
- Photos of the VLT: http://www.
Tel: +56 55 43 5216
Cell: +56 9 8819 3424
Tel: +44 2837 522928
Instituto de Astrofisica de Canarias
Tel: +34 922 60 + Ext. 5268
ESO, La Silla, Paranal, E-ELT & Survey Telescopes Press Officer
Garching bei München, Germany
Tel: +49 89 3200 6655
Cell: +49 151 1537 3591