MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIFORNIA 91109. TELEPHONE (818) 354-5011
http://www.jpl.nasa.gov
Contact: Jane Platt/JPL 818-354-0880
Ray Villard/Space Telescope Science Institute 410-338-4514
IMAGE ADVISORY
February 1, 2001
INSECT-LIKE SPACE STRUCTURE PREVIEWS OUR SUN'S DEATH
A new Hubble Space Telescope image of a celestial object
called the Ant Nebula may shed new light on the future demise
of our Sun. The image is available at
http://www.jpl.nasa.gov/pictures/wfpc .
The nebula, imaged on July 20, 1997, and June 30, 1998,
by Hubble's Wide Field and Planetary Camera 2, was observed by
Drs. Raghvendra Sahai and John Trauger of NASA's Jet
Propulsion Laboratory, Pasadena, Calif.; Bruce Balick of the
University of Washington in Seattle; and Vincent Icke of
Leiden University in the Netherlands. JPL designed and built
the camera.
The Ant Nebula, whose technical name is Mz3, resembles
the head and thorax of an ant when observed with ground-based
telescopes. The new Hubble image, with 10 times the
resolution revealing 100 times more detail, shows the "ant's"
body as a pair of fiery lobes protruding from a dying, Sun-
like star. The Ant Nebula is located between 3,000 and 6,000
light years from Earth in the southern constellation Norma.
The image challenges old ideas about what happens to
dying stars. This observation, along with other pictures of
various remnants of dying stars called planetary nebulae,
shows that our Sun's fate will probably be much more
interesting, complex and dramatic than astronomers previously
believed.
Although the ejection of gas from the dying star in the
Ant Nebula is violent, it does not show the chaos one might
expect from an ordinary explosion, but instead shows
symmetrical patterns. One possibility is that the central
star has a closely orbiting companion whose gravitational
tidal forces shape the outflowing gas. A second possibility
is that as the dying star spins, its strong magnetic fields
are wound up into complex shapes like spaghetti in an
eggbeater. Electrically charged winds, much like those in our
Sun's solar wind but millions of times denser and moving at
speeds up to 1,000 kilometers per second (more than 600 miles
per second) from the star, follow the twisted field lines on
their way out into space.
The Space Telescope Science Institute, Baltimore, Md.,
manages space operations for the Hubble Space Telescope for
NASA's Office of Space Science, Washington, D.C. The
Institute is operated by the Association of Universities for
Research in Astronomy, Inc., for NASA under contract with
NASA's Goddard Space Flight Center, Greenbelt, Md. The Hubble
Space Telescope is a project of international cooperation
between NASA and the European Space Agency. JPL is a division
of the California Institute of Technology in Pasadena.
Additional information about the Hubble Space Telescope
is available at http://www.stsci.edu . More information about
the Wide Field and Planetary Camera 2 is available at
http://wfpc2.jpl.nasa.gov .
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01/31/01 JP
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