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Supernova dealt deaths on earth? Stellar blasts may have killed ancient marine life. (This Week).


A group of young, hot stars in and near the constellation Scorpius shine brightly, making a memorable sight in the southern night sky. But if Narciso Benitez of Johns Hopkins University Johns Hopkins University, mainly at Baltimore, Md. Johns Hopkins in 1867 had a group of his associates incorporated as the trustees of a university and a hospital, endowing each with $3.5 million. Daniel C.  in Baltimore and his colleagues are correct, this collection of stars could have a lot to answer for. One of its members may have exploded in the solar system's neighborhood 2 million years ago, causing the widespread destruction of a variety of marine species here on Earth.

About 35 of the thousands of stars in this group, known as the Scorpius-Centaurus (Sco-Cen) OB association, weigh several times as much as the sun. These heavyweights--the group's brightest stars--tend to end their relatively brief lives with a powerful bang called a supernova. Other astronomers have determined that previous supernovas within the Sco-Cen association carved out the Local Bubble The Local Bubble is a cavity in the interstellar medium (ISM) of the Orion Arm of the Milky Way. It is at least 300 light years across and has a neutral hydrogen density approximately one tenth of the 0.5 atoms per cubic centimetre average for the ISM in the Milky Way. , a low-density cavity of interstellar in·ter·stel·lar  
adj.
Between or among the stars: interstellar gases.


interstellar
Adjective

between or among stars

Adj. 1.
 gas that extends about 150 light-years around the sun (SN: 4/20/96, p. 248).

The Sco-Cen stars now lie some 450 light-years from Earth, too far away for a supernova explosion to harm our solar system solar system, the sun and the surrounding planets, natural satellites, dwarf planets, asteroids, meteoroids, and comets that are bound by its gravity. The sun is by far the most massive part of the solar system, containing almost 99.9% of the system's total mass. . But by using data from the Hipparcos satellite to measure the current positions and velocities of stars in the association, Benitez' team traced the stars' paths back in time. The researchers found that the Sco-Cen members were quite a bit closer a few million years ago. Some could have passed within 130 light-years of Earth.

That's near enough that if one of the stars went supernova, cosmic rays cosmic rays, charged particles moving at nearly the speed of light reaching the earth from outer space. Primary cosmic rays consist mostly of protons (nuclei of hydrogen atoms), some alpha particles (helium nuclei), and lesser amounts of nuclei of carbon, nitrogen,  from the explosion would have destroyed much of Earth's ozone layer. Then, the sun's harmful ultraviolet radiation would have penetrated the atmosphere and could have led to the destruction of plankton plankton: see marine biology.
plankton

Marine and freshwater organisms that, because they are unable to move or are too small or too weak to swim against water currents, exist in a drifting, floating state.
, mollusks, and other marine life at the so-called Pliocene-Pleistocene boundary 2 million years ago, the team suggests.

Benitez and his colleagues Jesus Maiz-Apellaniz of the Space Telescope Science Institute The Space Telescope Science Institute (STScI) is the science operations center for the Hubble Space Telescope (HST; in orbit since 1990) and for the James Webb Space Telescope (JWST; scheduled to be launched in 2013).  in Baltimore and biologist Matilde Canelles of Silver Spring, Md., describe their analysis in an upcoming Physical Review Letters Physical Review Letters is one of the most prestigious journals in physics.[1] Since 1958, it has been published by the American Physical Society as an outgrowth of The Physical Review. .

Two key pieces of evidence support their proposal, the researchers note. A study by Maiz-Apellaniz indicates that the Sco-Cen association has had 20 supernova explosions over the past 11 million years. Further, an analysis of deep-ocean crusts by other teams shows an excess of iron-60 in samples that date roughly from the time of the Pliocene-Pleistocene extinction. Iron-60, an isotope produced by supernovas, could have become incorporated into ocean sediment if dust from a stellar explosion bombarded Earth.

The extinction at the Pliocene-Pleistocene boundary is considered a modest one. Several researchers over the past 25 years have proposed that nearby supernova explosions could have caused one or more of the most massive extinctions, such as the dinosaur die-off. However, the new analysis shows that unless a supernova came within a few light-years of Earth, its radiation wouldn't be intense enough to cause such an extinction.

Geologist Luann Becker of the University of California, Santa Barbara History
The predecessor to UCSB, Santa Barbara State College, focused on teacher training, industrial arts, home economics, and foreign languages. Intense lobbying by an interest group in the City of Santa Barbara led by Thomas Storke and Pearl Chase persuaded the State
 concurs with Benitez' team that a supernova is indeed a plausible but unproven candidate for the marine extinction. She notes that supernova dust isn't the only type of iron-rich space debris to pelt pelt

the undressed, raw skin of a wild animal with the fur in place. If from a sheep or goat there is a short growth of wool or mohair on the skin.
 Earth. Analyzing more samples of ocean sediment to pinpoint the amount and timing of the iron-60 excess could provide a more rigorous test of the supernova model, Becker adds.
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Author:Cowen, R
Publication:Science News
Article Type:Brief Article
Date:Feb 2, 2002
Words:543
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