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FWD: [UASR] Lunar Sodium Tail Discovered

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  • Frits Westra
    Posted by : [UASR] Perry van den BrinkBoston UniversityContact: Shauna LaFauci, 617/353-2399, slafauci@bu.eduFor Immediate
    Message 1 of 1 , Jun 5, 1999
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      Posted by : "[UASR]> Perry van den Brink" <owner-uasr@...>

      Boston University

      Contact: Shauna LaFauci, 617/353-2399, slafauci@...

      For Immediate Release: June 2, 1999

      BOSTON UNIVERSITY CENTER FOR SPACE PHYSICS DISCOVERS LUNAR SODIUM TAIL

      Boston, Mass. -- Boston University astronomers announced today the
      discovery of an enormous tail of sodium gas stretching to great
      distances >from the moon. The observations were made at the McDonald
      Observatory in Fort Davis, Texas, on nights following the Leonid
      meteor shower of November 1998. The tail of sodium gas was seen to
      distances of at least 500,000 miles >from the moon, changing its
      appearances over three consecutive nights. These results were
      presented on Tuesday, June 1st, at the Annual Spring Meeting of the
      American Geophysical Union (AGU) in Boston. Complete papers will
      appear in the AGU journal Geophysical Research Letters in its June
      15th edition.

      Since the days of NASA's Apollo Program of lunar, scientists have
      known that the moon has a very thin atmosphere. "It is one
      continuously being produced by evaporation of surface materials, and
      then continuously being lost by escape or impact back onto the
      surface," said Michael Mendillo, professor of astronomy. Such
      processes act daily, and so while there is always some atmosphere
      present, the various gases are being cycled through it. It is a
      "transient atmosphere" similar to the ones found in comets.

      Ten years ago, groundbased telescopes revealed that sodium gas (Na)
      was in the lunar atmosphere, an element that can be used to trace the
      shape and behavior of such a thin atmosphere. Sodium reflects sunlight
      very efficiently and so has become a standard way for space scientists
      to study gases that are otherwise difficult to see.

      "There are less than 50 atoms of sodium per cubic centimeter in the
      atmosphere just above the surface of the moon," says Jeffrey
      Baumgardner, Senior Research Associate in the University's Center for
      Space Physics. "But the most modern camera systems built in our lab
      can photograph such a thin environment out to distances that are
      several times the radius of the moon," Baumgardner added. In contrast
      to the tenuousness the moon's atmosphere -- only 50 atoms per cubic
      centimeter -- there are 10**19 molecules per cubic centimeters in
      earth's atmosphere at the surface.

      During the November observations, the BU team pointed their sensitive
      camera in the opposite direction from the moon and recorded, just by
      chance, images of the tail in an otherwise moonless sky. "At the time
      of the Leonid meteor shower on November 17, 1998, the moon was in
      'new' phase, impossible to see at its location between the Earth and
      the Sun," described Dr. Steven Smith, research associate in the center
      for space physics. "Our team was operating on the nightside of the
      earth, essentially looking away from the sun and moon, searching for
      meteor effects in our atmosphere." After one night of uneventful
      observations, on November 18th our imaging system detected a small
      patch of sodium emission in the dark skies above west Texas. "It grew
      to be larger and brighter on November 19th, and then faded slightly on
      November 20th," Smith said.

      The BU team considered several theories that could explain these
      unusual features, ruling out a comet, the impact of Leonid meteors
      upon dust in the solar system, and even possible instrumentation
      problems. Dr. Jody Wilson, research associate in the BU space physics
      group suggested that the mysterious sodium gas might come from the
      moon, and set out to model it using computer simulation and
      visualization techniques. "We found out that when the moon is new, it
      takes two days or so for Sodium atoms leaving the surface to reach the
      vicinity of the earth. They are pushed away from the moon by the
      pressure of sunlight and, as they sweep past us, the earth's gravity
      pulls on them, focusing them into a long narrow tail," Wilson
      explained.

      "The pieces of the puzzle fit together rather well," Mendillo added.
      "While some of the Leonid meteors burned up in their streaks through
      the earth's atmosphere on the night of November 17th -- producing
      spectacular showers in some locations -- others crashed into the
      moon's dusty soil liberating sodium gas. These atoms, speeding away
      from the earth-moon system, were then captured in photographs from our
      instrument in Texas several days later, looking down the length of the
      tail."

      "If it were bright enough for the human eye to see, perhaps a thousand
      times brighter," Baumgardner added, "it would be a glowing orange
      cloud dominating the nighttime, moonless sky."

      In trying to determine if this comet-like appearance of the moon
      occurred only on nights following a strong meteor shower, as happened
      with the Leonids, the BU team examined some earlier data taken at
      their site in Texas. During the previous August, similar observations
      were made, fortuitously on the nights following the new moon of August
      21, 1998. "It was there," Dr. Smith said, "several times fainter, but
      with the same shapes over the same three nights spanning the new moon,
      just as occurred in November."

      Taken together, the August observations without meteors and the
      November observations with meteors imply that the daily flux of
      micrometeors that strikes the moon's surface creates an extended tail
      at all times; it was just so enhanced during the strong Leonid storm
      that it was observed rather easily.

      "What we do not know yet is whether the entire atmosphere of the moon
      is produced by meteors, or just the small component of fast sodium
      atoms that can escape from it," Mendillo said.

      For visual information http://vega.bu.edu/moontail .
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