The Manne Siegbahn Memorial Lecture presents recent breakthroughs and developments in experimental physics. The lecture series was instituted in 1993 to the memory of Manne Siegbahn, and it is supported by the Royal Swedish Academy of Sciences through its Nobel Institute for Physics.
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Abstract
In 2008, the photometric monitoring during 5 months by the French-European satellite CoRoT of thousands of stars,
revealed for one of them 176 very shallow (ΔF/F = 3x10-4) but significant periodic decreases of
brightness, every 0.854 day, with a duration of 1.3 h each. If the possible interpretation of those events as
partial eclipses of the target, a solar-like star, by a transiting planet was correct, the planet should have a
radius as small as 1.7 REarth, making it the smallest transiting planet discovered to date. However,
before publishing such an outstanding result, the team had to accomplish a thorough task of complementary
observations from ground to assess this interpretation. Indeed, several alternative interpretations were possible,
such as a background system of mutually eclipsing stars. Many techniques were used, on several among the most
powerful telescopes: high resolution visible and infrared spectroscopy, on/off transit photometric observations,
high resolution imaging with adaptive optics, colours of the transit, etc. None of them succeeded in invalidating
the small planet hypothesis and the announcement of the discovery of Corot-7b was released in February 2009. A
firm confirmation came a few months later with the analysis of a long series of radial velocity measurements using
HARPS, the best instrument in the world in this respect. The planet was there in the data, with a firm evaluation
of its mass: 4.8 MEarth. The derived density, precisely equal to the Earth one, suggests a similar
type - a rocky one - and a similar composition, dominated by silicates. In addition, it was shown that a second
planet, of only twice the mass of the first one was present on a slightly larger orbit, but still extremely close
from the star. The discovery of the Corot-7 system is obviously an important milestone on the pathway to habitable
planets and I will discuss several questions that have been worked out since then: Is there a third planet? What
is the structure of Corot-7b? Its physical conditions? Are there clues on its formation? Etc.
| 1993 | Gerald Gabrielse | One Antiproton Radio: Precision Comparisons of a Single Trapped Antiproton and Proton |
| 1994 | Till Kirsten | GALLEX Solar Neutrino Results and their Implications |
| 1995 | Hiroyuki Sakaki | Quantum Engineering of Nanostructures: Novel Physics and New Concepts for Electronic Devices |
| 1996 | Eric Cornell | Bose-Einstein Condensation in a Dilute Atomic Vapor |
| 1996 | Geoffrey W. Marcy | Discovery of Planets Orbiting Sun-like Stars |
| 1997 | Alain Blondel | Elementary Particles from the Z to the Higgs. Loops, Tides and Trains. |
| 1998 | Rainer Weiss | The Prospects for the Detection of Gravitational Waves |
| 1999 | Yuri Oganessian | The Long Way to the Island of Stability of Superheavy Elements close to Z=114 |
| 2000 | Serge Haroche | Seeing a Single Photon without Destroying it and Manipulating Entaglement in Atom-Cavity Experiments |
| 2001 | Andrew E. Lange | Imaging the Embryonic Universe: First Resolved Images of the Cosmic Microwave Background |
| 2002 | Lene Vestergaard Hau | Light at Bicycle Speed — and Slower Yet! |
| 2003 | Andreas Eckart | A Massive Accreting Black Hole at the Center of the Milky Way! |
| 2004 | Michel H. Devoret | Towards a Solid State Quantum Information Processor: Manipulation and Control of the Quantum State of an Electrical Circuit |
| 2005 | Arthur B. McDonald | Neutrino and Astrophysics Measurements with the Sudbury Neutrino Observatory |
| 2006 | Ferenc Krausz | Attosecond Physics |
| 2007 | Sidney R. Nagel | Topological Transitions and Singularities in Fluids: The Life and Death of a Drop |
| 2008 | Alan Watson | Is the search for the origin of the highest-energy cosmic rays over? |
| 2009 | Fritz Bosch | Experiments on the beta decay of highly-ionized atoms with challenging and puzzling results |
| webmaster@msl.se | 2010-09-01 |