Space Movie Reveals Shocking Secrets of the Crab Pulsar
This movie shows dynamic rings, wisps and jets of matter and antimatter
around the pulsar in the Crab Nebula as observed in X-ray light by
Chandra (left, blue) and optical light by Hubble (right, red).
(IMAGE CREDIT: NASA/CXC/HST/ASU/J. Hester et al)
(Click on image to start movie)
Just when it seemed the summer movie season had ended,
two of NASA's Great Observatories have produced their own
action movie. Multiple observations made over several months
with NASA's Chandra X-ray Observatory and the Hubble Space
Telescope captured the spectacle of matter and antimatter
propelled to nearly the speed of light by the Crab pulsar.
"Through this movie, the Crab Nebula has come to life," said
Jeff Hester of Arizona State University in Tempe, lead author
of a paper in the September 20 issue of The Astrophysical
Journal Letters. "We can see how this awesome cosmic
generator actually works."
The Crab was first observed by Chinese astronomers in 1054
A.D. and has since become one of the most studied objects in
the sky. By combining the power of Chandra and Hubble, the
movie reveals features never before seen in still images. By
understanding the Crab, astronomers hope to unlock the
secrets of how similar objects across the universe are
The movie provides a stunning view of the activity in the inner
region around the Crab Nebula pulsar, which is seen as a bright
white dot near the center of the images. Bright wisps can be
seen moving outward at half the speed of light to form an
expanding ring, visible in both X-ray and optical images.
These wisps appear to originate from a shock wave that shows
up as an inner X-ray ring.
The inner X-ray ring consists of about two dozen knots that form,
brighten and fade, jitter around, and occasionally undergo outbursts
that give rise to expanding clouds of particles, but remain in
roughly the same location. As a high-speed wind of matter and antimatter
particles from the pulsar plows into the surrounding nebula, it
creates a shock wave and forms the inner ring. Energetic shocked
particles move outward to brighten the outer ring and produce an
extended X-ray glow.
Enormous electrical voltages generated by the rotating, highly
magnetized neutron star accelerate particles outward along its
equator to produce the pulsar wind. These pulsar voltages also
produce the polar jets seen spewing X-ray emitting matter and
antimatter particles perpendicular to the rings.
"These data leave little doubt that the inner X-ray ring is
the location of the shock wave that turns the high-speed wind
from the pulsar into extremely energetic particles," said
Koji Mori of Penn State University in University Park, a
coauthor of the paper.
Another dramatic feature of the movie is a turbulent jet that
lies perpendicular to the inner and outer rings. Violent
internal motions are obvious, as is a slow motion outward
into the surrounding nebula of particles and magnetic field.
"The jet looks like steam from a high-pressure boiler," said
David Burrows of Penn State, another coauthor of the paper,
"except when you realize you are looking at a stream of
matter and anti-matter electrons moving at half the speed of
The inner region of the Crab Nebula around the pulsar was
observed with Hubble on 24 occasions between August 2000 and
April 2001 at 11-day intervals, and with Chandra on eight
occasions between November 2000 and April 2001. The Crab was
observed with Chandra's Advanced CCD Imaging Spectrometer and
Hubble's Wide-Field Planetary Camera.
More Images from the Crab Nebula Movie on
the Chandra (http://chandra.harvard.edu/photo/2002/0052/more.html)