ROYAL ASTRONOMICAL SOCIETY PRESS INFORMATION NOTE EMBARGOED UNTIL 0001 BST, 1 April 2008 Date: 28 March 2008 Ref.: PN 08/17 (NAM 08) Issued by RAS Press Officers: Dr Robert Massey Tel: +44 (0)20 7734 3307 / 4582 Mobile: +44 (0)794 124 8035 E-mail: rm@ras.org.uk Anita Heward Tel: +44 (0)1483 420904 Mobile: +44 (0)7756 034243 E-mail: anitaheward@btinternet.com NATIONAL ASTRONOMY MEETING PRESS ROOM (31 MARCH - 4 APRIL ONLY): Tel: +44 (0)2890 975262 975263 975264 NAM 2008 http://nam2008.qub.ac.uk Royal Astronomical Society http://www.ras.org.uk < http://www.ras.org.uk/> CONTACT DETAILS ARE LISTED AT THE END OF THIS RELEASE RAS PN 08/17 (NAM 08) (EMBARGOED): THE (SUPER)WASP FACTORY FINDS 10 NEW PLANETS IN THE LAST 6 MONTHS In the last 6 months an international team of astronomers have used two batteries of cameras, one in the Canary Islands and one in South Africa, to discover 10 new planets in orbit around other stars (commonly known as extrasolar planets). The results from the Wide Area Search for Planets (SuperWASP) will be announced by team member Dr Don Pollacco of Queen’s University Belfast, in his talk at the RAS National Astronomy Meeting (NAM 2008) on Tuesday 1 April. Scientists have found more than 270 extrasolar planets since the first one was discovered in the early 1990s. Most of these are detected through their gravitational influence on the star they orbit – as it moves the planet pulls on the star, tugging it back and forth. However, making these discoveries depends on looking at each star over a period of weeks or months and so the pace of discovery is fairly slow. SuperWASP uses a different method. The two sets of cameras watch for events known as transits, where a planet passes directly in front of a star and blocks out some of the star’s light, so from the Earth the star temporarily appears a little fainter. The SuperWASP cameras work as robots, surveying a large area of the sky at once and each night astronomers have data from millions of stars that they can check for transits and hence planets. The transit method also allows scientists to deduce the size and mass of each planet. Each possible planet found using SuperWASP is then observed by astronomers working at the Nordic Optical Telescope on La Palma, the Swiss Euler Telescope in Chile and the Observatoire de Haute Provence in southern France, who use precision instruments to confirm or reject the discovery. 45 planets have now been discovered using the transit method, and since they started operation in 2004 the SuperWASP cameras have found 15 of them – making them by far the most successful discovery instruments in the world. The SuperWASP planets have masses between a middleweight 0.5 and a huge 8.3 times that of Jupiter, the largest planet in our Solar System. A number of these new worlds are quite exotic. For example, a year on WASP-12B (its orbital period) is just 1.1 days. The planet is so close to its star that its daytime temperature could reach a searing 2300 degrees Celsius. Dr Pollacco is delighted with the results. “SuperWASP is now a planet-finding production line and will revolutionise the detection of large planets and our understanding of how they were formed. It’s a great triumph for European astronomers.” FURTHER INFORMATION (INCLUDING IMAGES): SuperWASP Project website http://www.superwasp.org < http://www.superwasp.org/> Images of the SuperWASP Cameras 1) http://star.pst.qub.ac.uk/~dlp/SWASP_1.jpg - a close up of the 8 SuperWASP-North cameras. 2) http://star.pst.qub.ac.uk/~dlp/SWASP_2.jpg - an aerial view of the SuperWASP-North cameras (courtesy of Damon Hart-Davis, http://d.hd.org/). 3) http://star.pst.qub.ac.uk/~dlp/SWASP_3.jpg - the SuperWASP-South instrument. Image of the Euler (Swiss) Telescope dome http://www.cosmograil.org/images/euler-dome.jpg Image of the SOPHIE spectrograph at the Observatoire de Haute Provence http://www.obs-hp.fr/www/guide/sophie/sophie.html RAS National Astronomy Meeting http://nam2008.qub.ac.uk RAS home page http://www.ras.org.uk NOTES FOR EDITORS The SuperWASP cameras are operated by a consortium including the Isaac Newton Group on La Palma, the Instituto Astrofisica Canarias, the University of Keele, the University of Leicester, the Open University, Queen’s University Belfast and St Andrew’s University. Follow up [observations] of SuperWASP exoplanet candidates are obtained at the Nordic Optical Telescope on La Palma, the Swiss Euler Telescope at La Silla, Chile (in collaboration with colleagues at Geneva Obs