Keplers Supernova Remnant in X Rays
Explanation:
What caused this mess?
Some type of star exploded to create the unusually shaped nebula known as
Kepler's supernova remnant,
but which type?
Light from the stellar explosion that
created this energized cosmic cloud was first seen on planet
Earth in October 1604, a mere
four hundred years
ago.
The supernova produced a bright
new star
in early 17th century skies within the constellation
Ophiuchus.
It was studied by astronomer
Johannes Kepler
and his contemporaries, with out the benefit of a telescope, as they
searched for an explanation of the heavenly apparition.
Armed with a
modern
understanding of stellar evolution, early 21st century
astronomers continue to explore the expanding debris cloud, but can now use
orbiting space telescopes to survey Kepler's supernova remnant (SNR)
across the spectrum.
Recent X-ray data and
images
of Kepler's supernova remnant taken by the orbiting
Chandra X-ray Observatory has shown relative elemental abundances more typical
of a
Type Ia supernova, indicating that the progenitor was a
white dwarf star that exploded
when it accreted too much material and went over
Chandrasekhar's limit.
About 13,000 light years away,
Kepler's supernova
represents the most recent stellar explosion seen to
occur
within
our Milky Way galaxy.
Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official: Jay Norris.
Specific
rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
