At least some of the mysterious particles are born
in supernova shock waves, satellite data confirm
In fact, just before posting this Top Pictures list, a NASA press release came out saying the Fermi satellite has seen gamma rays from this object, which is another very strong piece of evidence for this; gamma rays are the very highest energy form of light, and should be made when subatomic particles bounce around
in supernova shock waves.
Not exact matches
«Amateur astronomer captures rare first light from massive exploding star: First observation of optical light from
shock breakout
in a
supernova explosion.»
A ring of hot spots (
in images from the Hubble Space Telescope) gradually lit up as a
shock wave from
supernova 1987A plowed through a loop of gas that had been expelled by the star tens of thousands of years before the explosion.
The colors represent the relative amounts of short - lived radioactive isotopes, such as iron - 60, injected into a newly formed protoplanetary disk (seen face on with the protostar being the light purple blob
in the middle) by a
supernova shock wave.
«My findings indicate that a
supernova shock wave is still the most - plausible origin story for explaining the short lived radioactive isotopes
in our Solar System,» Boss said.
This effect becomes even more apparent as the
shock collides into the equatorial ring, as observed
in Hubble Space Telescope images of the
supernova.
While her research did not find a «smoking gun,» definitively proving that the radioactive isotopes were injected by a
shock wave, Telus did show that the amount of Fe - 60 present
in the early Solar System is consistent with a
supernova origin.
The team plans to look for evidence of similar reverse
shock waves
in other young
supernova remnants.
In the case of Tycho's
supernova remnant, astronomers have discovered that a reverse
shock wave racing inward at Mach 1000 (1000 times the speed of sound) is heating the remnant and causing it to emit X-ray light.
Both
shock breakout and «plateau» phases are shorter, bluer, and fainter for metal - poor
supernova in comparison with «metal - rich»
supernova.
A
shock wave from that collapse will speed outward, violently expelling the star's outer layers
in a massive explosion known as a
supernova.
Bersten and her colleagues analyzed the light from the
supernova and found that it matches models of the first phase of a
supernova called the
shock breakout phase,
in which a
shock wave from a massive star's collapse ricochets back from the star's core and pushes stellar material outward.
«He has constructed an experiment,
in which a hydraulic jump
in a circular water flow exhibits pulsational asymmetries
in close analogy to the
shock front
in the collapsing matter of the
supernova core.»
Writing
in Nature, the group says the discovery offers the first direct evidence for astrophysical models of
supernova shock waves that date to the 1970s.
The collision of the
supernova and the companion star
shocked the
supernova material, heating it to a blue glow heavy
in ultraviolet light.
Just over a decade ago, two teams used the
supernovae to show that the universe is accelerating
in its expansion due to the influence of dark energy, a
shocking discovery that thrust type Ia
supernovae into the astrophysical limelight.
Caption: The colors represent the relative amounts of short - lived radioactive isotopes, such as iron - 60, injected into a newly formed protoplanetary disk (seen face on with the protostar being the light purple blob
in the middle) by a
supernova shock wave.
Shocks in supernova explosions are thought to be the main source of cosmic rays — very high energy charged particles from space.
Shock waves
in plasmas form around planets, stars and
supernovas.
The orange - red filaments visible
in the image show the
shock fronts of a
supernova explosion (Credit: ESA / Hubble & NASA, < a href ="https://creativecommons.org/licenses/by/4.0/" rel="nofollow"> CC BY 4.0 )
Shock waves
in supernova remnants are thought to be responsible for accelerating many of these particles.
These
supernova blasts send material and
shock waves back into the nebular gas to create the Tarantula's glowing filaments also visible
in this Hubble Space Telescope Heritage image.
Scientists have attributed the patterns observed
in supernova explosions and ejecta from
shock - induced metal melt to RM instability.
HEFT will map the hard X-ray emission from
supernova remnants to investigate issues of stellar nucleosynthesis (through the mapping of radioactive Titanium) and study the origin and acceleration of cosmic - rays (through mapping the continuum hard X-rays produced
in the same
shocks that produce the cosmic - rays).
Although absorption
in ionized hydrogen suggests that the SNR is about 13,000 to 16,000 ly (4,000 to 5,000 pc) away (Schwarz et al, 1995), analysis of its optical proper motion and modelled
shock velocity provides a distance of about 7,500 ly (2,300 pc)(more at T. Joseph W. Lazio's Tycho's
Supernova Remnant).
For about two weeks the star could be seen
in daylight, but at the end of November it began to fade and change color, from bright white over yellow and orange to faint reddish light, finally fading away from visibility
in March, 1574, having been visible to the naked eye for almost 16 months (more about Brahe's «acid tongue and silver nose,» the cultural
shock of the «new star,» and how
supernovae create high - energy radiation from Wallace H. Tucker).
The
shock wave from the
supernova can initiate star formation
in other interstellar clouds.
NuSTAR, a high - energy X-ray observatory, has created the first map of radioactive material
in a
supernova remnant called Cassiopeia A, or Cas A, to reveal how
shock waves likely tear massive dying stars apart, the researchers said
in a study, published
in the Feb. 20 issue of Nature.
These
supernovae have a characteristic shockwave called the «
shock breakout,» which was captured for the first time
in optical light by Kepler.
NASA (
Shock rings around
Supernova 1987A)-- larger image While primordial
supernovas created much of the heavier elements such as iron found
in the Solar System, Sol orbits the galactic core without frequent crossings of the spiral arms where life - threatening
supernovas are more common.
Now, a research team led by the Kavli Institute for Particle Astrophysics and Cosmology (KIPAC) at Stanford University and SLAC has discovered evidence that cosmic rays are born
in the
shock waves of distant
supernovae.