Astronomers have discovered a new ground-based technique to study the atmospheres of planets outside our Solar System, accelerating our search for Earth-like planets with life-related molecules. Their work is reported today (3 Feb. 2010) in the journal Nature.
The scientists developed the new technique by using NASA's relatively small Earth-based infrared telescope to identify an organic molecule in the atmosphere of a Jupiter-sized planet nearly 63 light-years away. Using a novel calibration method to remove systematic observation errors, they obtained a measurement revealing details of the exoplanet's atmospheric composition and conditions, an unprecedented achievement from an Earth-based observatory.
Dr. Giovanna Tinetti from University College London (UCL), whose work on the project was funded by the Science and Technology Facilities Council (STFC), said, "The final goal is to observe the atmosphere of a planet with the capability to support life. We're not there yet, but the possibility to use ground-based telescopes in combination with space-based observatories, will speed up the work of studying exoplanet atmospheres."
Lead author Mark Swain, an astronomer at NASA's Jet Propulsion Laboratory, added, "The fact that we have used a relatively small, ground-based telescope is exciting because it implies that the largest telescopes on the ground, using this technique, may be able to characterize terrestrial exoplanet targets."
Currently, more than 400 exoplanets are known. Most are gaseous like Jupiter, but some "super-Earths" are thought to be large terrestrial, or rocky, worlds. A true Earth-like planet the same size as our planet and distance from its star has yet to be discovered. NASA's Kepler mission is searching from space now, and is expected to find several of these earthly worlds.
On Aug. 11, 2007, Swain and his team turned the infrared telescope to the hot, Jupiter-size planet HD 189733b in the constellation Vulpecula. Every 2.2 days, the planet orbits a K-type main sequence star slightly cooler and smaller than our Sun. HD 189733b had already yielded breakthrough advances in exoplanet science, including detections of water vapor, methane and carbon dioxide using space telescopes. Using the new technique, the astronomers successfully detected carbon dioxide and methane in the atmosphere of HD 189733b with a spectrograph, which splits light into its components to reveal the distinctive spectral signatures of different chemicals. Their key work was development of the novel calibration method to remove systematic observation errors caused by the variability of Earth's atmosphere and instability due to the movement of the telescope system as it tracks its target.
"As a consequence of this work, we now have the exciting prospect that other suitably equipped yet relatively small ground-based telescopes should be capable of characterizing exoplanets," said John Rayner, the NASA Infrared Telescope Facility support scientist who built the SpeX spectrograph used for these measurements. "On some days we can't even see the Sun with the telescope, and the fact that on other days we can now obtain a spectrum of an exoplanet 63 light-years away is astonishing."
In the course of their observations, the team found unexpected bright infrared emission from methane that stands out on the day side of HD 189733b. This could indicate some kind of activity in the planet's atmosphere which could be related to the effect of ultraviolet radiation from the planet's parent star hitting the planet's upper atmosphere, but more detailed study is needed.
"An immediate goal for using this technique is to more fully characterize the atmosphere of this and other exoplanets, including detection of organic and possibly prebiotic molecules" like those that preceded the evolution of life on Earth, said Swain. "We're ready to undertake that task." Some early targets will be the super-Earths. Used in synergy with observations from NASA's Hubble, Spitzer and the future James Webb Space Telescope, the new technique "will give us an absolutely brilliant way to characterize super-Earths," Swain said
Nature Paper
Other authors of the Nature paper are Pieter Deroo, Gautam Vasisht and Pin Chen of JPL; Caitlin A. Griffith of the University of Arizona, Tuscon; Ian J. Crossfield of UCLA; Azam Thatte of the George Institute of Technology, Atlanta; Jeroen Bouwman, Cristina Afonso and Thomas Henning of Max-Planck Institute for Astronomy, Heidelberg, Germany; and Daniel Angerhausen of the German SOFIA Institute, Stuttgart, Germany.
Dr. Giovanna Tinetti
Dr. Tinetti graduated from the University of Turin in Italy in theoretical physics and also obtained her doctorate there in the same subject. She then carried out post-doctoral work at the Jet Propulsion Laboratory and California Institute of Technology in the United States and worked for the headquarters of the European Space Agency in Paris before undertaking her current position at University College London. Awarded an Aurora fellowship in 2006 she is now continuing her work at UCL as a Royal Society Fellow.
For the Aurora fellowship Giovanna`s research continued her interests in the detection of biosignatures, i.e., indicators of biological life, on extrasolar planets, more than 300 of which have so far been detected. Her work focused on planetary and atmospheric modeling of the environments of Earth-like planets to assist in interpretation of spectral observations of exoplanets. In 2007 she published the first finding of water vapor in the atmosphere of a giant exoplanet in the science journal Nature. In 2008 she and her co-workers reported the detection of the organic molecule methane and later in the same year also carbon dioxide in the atmosphere of the same exoplanet.
Image are available from the STFC press office.
Media Contact:
Julia Short
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Science and Technology Facilities Council
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Science Contact:
Dr. Giovanna Tinetti
University College London
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g.tinetti@ucl.ac.uk
Science and Technology Facilities Council (STFC)
The Science and Technology Facilities Council ensures the UK retains its leading place on the world stage by delivering world-class science; accessing and hosting international facilities; developing innovative technologies; and increasing the socio-economic impact of its research through effective knowledge exchange.
The Council has a broad science portfolio including Astronomy, Particle Physics, Particle Astrophysics, Nuclear Physics, Space Science, Synchrotron Radiation, Neutron Sources and High Power Lasers. In addition the Council manages and operates three internationally renowned laboratories:
* The Rutherford Appleton Laboratory, Oxfordshire
* The Daresbury Laboratory, Cheshire
* The UK Astronomy Technology Centre, Edinburgh
The Council gives researchers access to world-class facilities and funds the UK membership of international bodies such as the European Laboratory for Particle Physics (CERN), the Institute Laue Langevin (ILL), European Synchrotron Radiation Facility (ESRF), the European organization for Astronomical Research in the Southern Hemisphere (ESO) and the European Space Agency (ESA). It also funds UK telescopes overseas on La Palma, Hawaii, Australia and in Chile, and the MERLIN/VLBI National Facility, which includes the Lovell Telescope at Jodrell Bank Observatory. The Council distributes public money from the Government to support scientific research.
The Council is a partner in the UK space program, coordinated by the British National Space Centre.
