A Star's Death Comes to Light (Forwarded)
- From: Andrew Yee <ayee@xxxxxxxxxxxxxxxxxxxxxx>
- Date: Thu, 11 Jan 2007 16:24:41 GMT
Steve Roy
Marshall Space Flight Center, Huntsville, Ala. January 9, 2007
(Phone: 256.544.0034)
Megan Watzke
Chandra X-ray Center, Cambridge, Mass.
(Phone: 617.496.7998)
News release: 07-004
A Star's Death Comes to Light
Using NASA's Chandra X-ray Observatory, scientists have created a stunning
new image of one of the youngest supernova remnants in the galaxy. This
new view of the debris of an exploded star helps astronomers solve a
long-standing mystery, with implications for understanding how a star's
life can end catastrophically and for gauging the expansion of the
universe.
Over 400 years ago, sky watchers -- including the famous astronomer
Johannes Kepler -- noticed a bright new object in the night sky. Since the
telescope had not yet been invented, only the unaided eye could be used to
watch as a new star that was initially brighter than Jupiter dimmed over
the following weeks.
Chandra's latest image marks a new phase in understanding the object now
known as Kepler's supernova remnant. By combining nearly nine days of
Chandra observations, astronomers have generated an X-ray image with
unprecedented detail of one of the brightest recorded supernovas in the
Milky Way galaxy.
The explosion of the star that created the Kepler remnant blasted the
stellar remains into space, heating the gases to millions of degrees and
generating highly energized particles. Copious X-ray light, like that
shining from many supernova remnants, was produced.
Astronomers have studied Kepler intensively over the past three decades
with radio, optical and X-ray telescopes, but its origin has remained a
puzzle. On the one hand, the presence of large amounts of iron and the
absence of a detectable neutron star points toward a so-called Type Ia
supernova. These events occur when a white dwarf star pulls material from
an orbiting companion until the white dwarf becomes unstable and is
destroyed by a thermonuclear explosion
On the other hand, when viewed in optical light, the supernova remnant
appears to be expanding into dense material that is rich in nitrogen. This
would suggest Kepler belongs to a different type of supernova (known as
"Type II") that is created from the collapse of a single massive star that
sheds material before exploding. Type Ia supernovas do not normally have
such surroundings.
A team of astronomers, led by Stephen Reynolds of North Carolina State
University in Raleigh, N.C., was able to use the Chandra dataset to
address this mystery. By comparing the relative amounts of oxygen and iron
atoms in the supernova, the scientists were able to determine that Kepler
resulted from a Type Ia supernova.
In solving the mystery of Kepler's identity, Reynolds and his team have
also given an explanation for the dense material in the remnant. Kepler
could be the nearest example of a relatively rare "prompt" Type Ia
explosion, which occur in more massive progenitors only about 100 million
years after the star formed rather than several billion years.
If that is the case, Kepler could teach astronomers more about all Type Ia
supernovas and the ways in which prompt explosions from massive stars
differ from their more common cousins associated with lower mass stars.
This information is essential to improve the reliability of the use of
Type Ia stars as "standard candles" for cosmological studies of dark
energy as well as to understand their role as the source of most of the
iron in the universe.
In the new Chandra Kepler image, red represents low-energy X-rays and
shows material around the star -- dominated by oxygen -- that has been
heated up by a blast wave from the star's explosion. The yellow color
shows slightly higher energy X-rays, mostly iron formed in the supernova,
while green (medium-energy X-rays) shows other elements from the exploded
star. The blue color represents the highest energy X-rays and shows a
shock front generated by the explosion.
NASA's Marshall Space Flight Center, Huntsville, Ala., manages the Chandra
program for the agency's Science Mission Directorate. The Smithsonian
Astrophysical Observatory controls science and flight operations from the
Chandra X-ray Center, Cambridge, Mass.
Additional information and images are available at:
http://chandra.harvard.edu
and
http://www.nasa.gov/mission_pages/chandra/news/07-004.html
.
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