Pretražite po imenu i prezimenu autora, mentora, urednika, prevoditelja

Napredna pretraga

Pregled bibliografske jedinice broj: 324226

Searching for extrasolar planets by microlensing ; Discovery of a 5.5 Earth mass planet OGLE-2005-BLG-390Lb


Dominis Prester, Dijana
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:

Avatar Url Dijana Dominis Prester (autor)


Citiraj ovu publikaciju:

Dominis Prester, Dijana
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)
Dominis Prester, D. (2007) Searching for extrasolar planets by microlensing ; Discovery of a 5.5 Earth mass planet OGLE-2005-BLG-390Lb. U: The first summer school in astronomy and geophysics.
@article{article, author = {Dominis Prester, Dijana}, year = {2007}, keywords = {Extrasolar planets, microlensing}, title = {Searching for extrasolar planets by microlensing ; Discovery of a 5.5 Earth mass planet OGLE-2005-BLG-390Lb}, keyword = {Extrasolar planets, microlensing}, publisherplace = {Beograd, Srbija} }
@article{article, author = {Dominis Prester, Dijana}, year = {2007}, keywords = {Extrasolar planets, microlensing}, title = {"Searching for extrasolar planets by microlensing ; Discovery of a 5.5 Earth mass planet OGLE-2005-BLG-390Lb"}, keyword = {Extrasolar planets, microlensing}, publisherplace = {Beograd, Srbija} }




Contrast
Increase Font
Decrease Font
Dyslexic Font