Ulysses sees Galactic Dust on the rise

From: Amara Graps (amara@amara.com)
Date: Tue Aug 05 2003 - 02:46:11 MDT

  • Next message: Wei Dai: "Re: Inside-out MBrains [was Re: Fermi "Paradox"]"

    ESA Science News
    http://sci.esa.int

    01 Aug 2003

    Ulysses sees Galactic Dust on the rise

    Since early 1992 Ulysses has been monitoring the stream of stardust flowing
    through our Solar System. The stardust is embedded in the local galactic cloud
    through which the Sun is moving at a speed of 26 kilometres every second. As a
    result of this relative motion, a single dust grain takes twenty years to
    traverse the Solar System. Observations by the DUST experiment on board Ulysses
    have shown that the stream of stardust is highly affected by the Suns magnetic
    field.

    In the 1990s, this field, which is drawn out deep into space by the out-flowing
    solar wind, kept most of the stardust out. The most recent data,
    collected up to
    the end of 2002, shows that this magnetic shield has lost its protective power
    during the recent solar maximum. In an upcoming publication in the Journal of
    Geophysical Research ESA scientist Markus Landgraf and his co-workers from the
    Max-Planck-Institute in Heidelberg report that about three times more stardust
    is now able to enter the Solar System.

    The reason for the weakening of the Suns magnetic shield is the increased solar
    activity, which leads to a highly disordered field configuration. In the
    mid-1990s, during the last solar minimum, the Suns magnetic field resembled a
    dipole field with well-defined magnetic poles (North positive, South negative),
    very much like the Earth. Unlike Earth, however, the Sun reverses its magnetic
    polarity every 11 years. The reversal always occurs during solar maximum. Thats
    when the magnetic field is highly disordered, allowing more
    interstellar dust to
    enter the Solar System. It is interesting to note that in the reversed
    configuration after the recent solar maximum (North negative, South positive),
    the interstellar dust is even channelled more efficiently towards the inner
    Solar System. So we can expect even more interstellar dust from 2005 onwards,
    once the changes become fully effective.

    While grains of stardust are very small, about one hundredth the diameter of a
    human hair, they do not directly influence the planets of the Solar System.
    However, the dust particles move very fast, and produce large numbers of
    fragments when they impact asteroids or comets. It is therefore
    conceivable that
    an increase in the amount of interstellar dust in the Solar System will create
    more cosmic dust by collisions with asteroids and comets. We know from the
    measurements by high-flying aircraft that 40,000 tonnes dust from asteroids and
    comets enters the Earths atmosphere each year. It is possible that the increase
    of stardust in the Solar System will influence the amount of extraterrestrial
    material that rains down to Earth.

    For further information please contact:
           SciTech.editorial@esa.int

    IMAGE CAPTIONS:

    [Image 1:
    http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33620]
    The Sun and the nearest stars move through filaments of galactic clouds.
    Copyright: P. C. Frisch, University of Chicago

    [Image 2:
    http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33619]
    The pictures above show cut-aways of where interstellar dust is concentrated in
    the Solar System -- high concentration: red/yellow, low concentration:
    blue/green (the planets are not shown). During solar minimum (top picture) most
    interstellar dust can be found above or below the Sun, while at the solar
    maximum (bottom picture) the dust is concentrated close to the Sun in the plane
    of the planets' orbits. Copyright: ESA

    [Image 3:
    http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=33482]
    SWOOPS image of solar wind at solar minimum and solar maximum.
    Copyright: D. McComas

    -- 
    ***********************************************************************
    Amara Graps, PhD
    Istituto di Fisica dello Spazio Interplanetario, INAF - ARTOV,
    Via del Fosso del Cavaliere, 100, I-00133 Roma, ITALIA
    tel: +39-06-4993-4384       |fax:  +39-06-4993-4383
    Amara.Graps@ifsi.rm.cnr.it  | http://www.mpi-hd.mpg.de/dustgroup/~graps
    ************************************************************************
    I'M SIGNIFICANT!...screamed the dust speck. -- Calvin
    


    This archive was generated by hypermail 2.1.5 : Tue Aug 05 2003 - 02:54:46 MDT