Pregled bibliografske jedinice broj: 324226
Searching for extrasolar planets by microlensing ; Discovery of a 5.5 Earth mass planet OGLE-2005-BLG-390Lb
Searching for extrasolar planets by microlensing ; Discovery of a 5.5 Earth mass planet OGLE-2005-BLG-390Lb // The first summer school in astronomy and geophysics
Beograd, Srbija, 2007. (pozvano predavanje, nije recenziran, sažetak, znanstveni)
CROSBI ID: 324226 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Searching for extrasolar planets by microlensing ; Discovery of a 5.5 Earth mass planet OGLE-2005-BLG-390Lb
("Searching for extrasolar planets by microlensing ; Discovery of a 5.5 Earth mass planet OGLE-2005-BLG-390Lb")
Autori
Dominis Prester, Dijana
Vrsta, podvrsta i kategorija rada
Sažeci sa skupova, sažetak, znanstveni
Skup
The first summer school in astronomy and geophysics
Mjesto i datum
Beograd, Srbija, 06.08.2007. - 10.08.2007
Vrsta sudjelovanja
Pozvano predavanje
Vrsta recenzije
Nije recenziran
Ključne riječi
Extrasolar planets; microlensing
Sažetak
Gravitational microlensing can reveal extrasolar planets orbiting the foreground lens stars if the light curves are measured frequently enough to characterize planetary light curves with features lasting a few hours. Microlensing is most sensitive to planets in Earth-to Jupiter-like orbits with semi-major axis in the range 1-5 AU. We (PLANET, OGLE and MOA collaborations) have detected a 5.5 Earth mass planet named OGLE-2005-BLG-390Lb orbiting a 2.2 solar mass M-dwarf host star at a separation of 2.6 AU, at a distance of 6.6kpc. This is the lowest-mass and the coolest extrasolar planet, out of more than 200 planets discovered up to date. Our detection, together with a latter detection of OGLE-2005-BLG-169Lb, suggests that cool, sub-Neptune-mass may be more common than gas giant planets, as predicted by the core accretion theory. The basics of microlensing will be explained, and microlensing surveys towards the Galactic Bulge searching for extrasolar planets presented, with special emphasis on the role of binary stars as lenses and sources. Numerical optimization methods for light curve modeling and breaking ambiuguitis in light curve solutions will be discussed, explained using the example of OGLE-2005-BLG-390Lb planet discovery. Some new ideas and methods for improving planet detection by microlensing will be presented.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
316-0000000-2824 - Dijagnostika i fizička svojstva cirkumstelarne tvari (Kotnik-Karuza, Dubravka, MZOS ) ( CroRIS)
Ustanove:
Sveučilište u Rijeci - Odjel za fiziku
Profili:
Dijana Dominis Prester
(autor)