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  • Extrasolar Planets Detection Fractal Map

    Paper number

    IAC-09.A4.1.10

    Author

    Mr. Karan Molaverdikhani, United States

    Year

    2009

    Abstract
    “Are we alone?” This is a mankind question for a long time. Galilei saw the Jupiter’s
    moons 400 years ago and now we know about the multiplanetary stellar systems and till
    now have found more than 340 extrasolar planets that shown we are close to find answer.
    KEPLER will launch soon to survey a wide region of the Cygnus-Lyra constellations in
    the northern sky, to find earth-size planets beyond our solar system. Some ground and
    space missions also work together for detecting new worlds. But countries can not
    continue their researches without managing and optimizing their investigations.
    One of the most important ways to reducing costs is detection of those regions of sky that
    have more chance to finding earth-like planets. Our scientific and technical capability is
    of course important in the detection of such planets; but technological readiness is not the
    overall concern of this project. The primary goal of this work is to provide a map
    showing detection probability of stars throughout the Milky Way that fall in the Galactic
    Habitable Zone and could potentially host planets conducive to live. We suggested this
    map on microlensing method previously, and now we propose a new way to
    measurement this map independent to exoplanets detection methods, such as
    microlensing, transit or radial velocity.
    Today, fractals roles are so critical, especially for modeling or analyzing complex
    systems and fractals structures and also fractals dimension(s) can help us to find type(s),
    pattern(s) or physic(s) of the systems. Ever since the first planet outside the solar system
    was found in the early 1990s, a number of questions have been existed, such as “Is there
    any stellar systems like ours or the solar planetary system is unique?” Fractals are tools
    for answering this question.
    In this way, we surveyed thousands of sun-like stars and any stars which had potential to
    making an earth-like planet in a habitable zone. This analyzing had shown the first fractal
    structure of new worlds that help us to calculate dimensions of fractal and then predict
    our chance to find them. Type of stars, metallicity and distance from Galactic center are
    some important parameters to measuring star fractal dimension. These results provide a
    new 2-D map of earth-like planet existing probability in the Milky Way disc.
    Abstract document

    IAC-09.A4.1.10.pdf

    Manuscript document

    (absent)