• Astronomers discover how long-lived Pete

    From ScienceDaily@1337:3/111 to All on Thu Jun 11 21:30:24 2020
    Astronomers discover how long-lived Peter Pan discs evolve

    Date:
    June 11, 2020
    Source:
    Queen Mary University of London
    Summary:
    New research has revealed how long-lived Peter Pan discs form,
    which could provide new insights into how planets arise.



    FULL STORY ==========================================================================
    New research from scientists at Queen Mary University of London has
    revealed how long-lived Peter Pan discs form, which could provide new
    insights into how planets arise.


    ========================================================================== Planet-forming, or protoplanetary, discs are giant discs of gas and
    dust found circling young stars. The recently discovered Peter Pan discs received their name as like their fictional counterpart they are thought
    to "never grow up," living around 5-10 times longer than other typical protoplanetary discs.

    Whilst astronomers have been aware of the existence of Peter Pan discs
    since 2016, questions around how and why these discs live so long and
    the implications for how planets form, have been left unanswered.

    In this study, the scientists used computer simulations to look at a range
    of possible starting configurations and ways in which the disc evolves
    to reveal the combination of conditions needed to form Peter Pan discs,
    which they termed 'Neverland's parameters'. They found these discs only
    form in lonely environments, away from other stars, and that they need
    to start out much larger than normal discs.

    Dr Gavin Coleman, first author of the study and postdoctoral researcher
    at Queen Mary, said: "Most stars form in big groups containing around
    100,000 stars however it seems that Peter Pan discs can't form in these environments.

    They need to be much more isolated from their stellar neighbours as the radiation from other stars would blow these discs away. They also need
    to start out massive, so they have more gas to lose and are therefore
    able to live for much longer." Until the discovery of long-lived Peter
    Pan discs, scientists thought that all discs had a lifetime of a few
    million years and faded away by 10 million years, suggesting that the
    planets within them must form quickly.

    Dr Thomas Haworth, a Dorothy Hodgkin Fellow at Queen Mary, said: "The
    existence of these long-lived discs was really surprising, and finding
    out why these discs can survive longer than expected could be critical
    for helping us understand more about disc evolution and planet formation
    in general. A particularly interesting point is that Peter Pan discs have
    so far only been found around low mass stars, and these low mass stars are generally being found to host lots of planets. The large disc masses that
    we need to end up with Peter Pan discs could be an important ingredient
    that allows these planets to exist." Due to the specific environment
    needed for the formation of these discs it is expected that they are
    very rare. So far, seven Peter Pan discs have been discovered as the
    result of a citizen science collaboration between NASA and Zooniverse,
    known as the Disk Detective project.

    Dr Coleman, said: "It's great that the findings of a citizen science
    project are now fuelling novel scientific research into these unique
    discs, and could even help us to better understand planet formation,
    one of the key problems in astrophysics."

    ========================================================================== Story Source: Materials provided by Queen_Mary_University_of_London. Note: Content may be edited for style and length.


    ========================================================================== Journal Reference:
    1. Thomas J Haworth, Gavin A L Coleman. Peter Pan discs: finding
    Neverland's
    parameters. Monthly Notices of the Royal Astronomical Society:
    Letters, 2020; 496 (1): L111 DOI: 10.1093/mnrasl/slaa098 ==========================================================================

    Link to news story: https://www.sciencedaily.com/releases/2020/06/200611094206.htm

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