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.
Specifically, the NuStar will map radioactive
material in supernovae remnants in an attempt to study the origins of cosmic rays and extreme physics surrounding collapsed stars.
Not exact matches
Supernova 1987A appears to be creating a lot of this dust, suggesting that stellar explosions play a crucial role
in seeding the cosmos with planet - building
material.
The object is located
in the center of a colorful cloud of
material consisting of the remains of an ancient star that exploded as a massive
supernova.
This calcium and other heavy elements could have been created
in supernova explosions, and then incorporated into new stars, but the clusters as they are today are too small to keep hold of the
material violently thrown out by
supernovae.
Jon Mauerhan at the Steward Observatory
in Tucson, Arizona, cites brightening on 26 September and
material shooting out at 13,000 kilometres per second as sure - fire signs that SN 2009ip truly went
supernova (arxiv.org/abs/1209.6320).
But if the
supernova came from two white dwarfs colliding, its debris would have shot out unevenly, with some
material flying faster
in one direction than another.
Such stars end their lives
in huge
supernova explosions, ejecting their stellar
materials outwards into space and leaving behind an extremely dense and compact object; this could either be a white dwarf, a neutron star or a black hole.
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.
The instruments are expected to reveal details about gases trapped
in galaxy clusters and wafting through
supernova remnants as well as the turbulent streams of
material spiraling away from black holes.
When they die, stars explode
in supernovae, leaving behind a cloud of ejected
material called a
supernova remnant.
The collision of the
supernova and the companion star shocked the
supernova material, heating it to a blue glow heavy
in ultraviolet light.
New supercomputer simulations of the crusts of neutron stars — the rapidly spinning ashes left over from
supernova explosions — reveal that they contain the densest and strongest
material in the universe.
The top candidates, the astronomers suggested, are a neutron star, possibly a highly - magnetic magnetar, surrounded by either
material ejected by a
supernova explosion or
material ejected by a resulting pulsar, or an active nucleus
in the galaxy, with radio emission coming from jets of
material emitted from the region surrounding a supermassive black hole.
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.
As the white dwarf pulls
material from a companion star, the temperature increases, eventually triggering a runaway reaction that detonates
in a violent
supernova that destroys the white dwarf.
Qingzhu Yin et al., «Diverse
Supernova Sources of Pre-Solar
Material Inferred from Molybdenum Isotopes
in Meteorites,» Nature, Vol.
Most of the energy from the
supernova turns into light when it hits this previously ejected
material, resulting
in a short, but brilliant burst of radiation.
Chandra had seen hot elements like iron and silicon and magnesium
in the
supernova cloud, and the shape of some of the
material seemed to support the double - jets theory, vaguely following where the beams would be.
So the scientists set out to test two main theories: whether the
supernova was caused
in part by two narrow jets of
material streaming out of either end of a rotating star, or whether it was the result of stuff «sloshing» around inside, leaving behind a lumpy shape.
Making their debut
in Strange Attractor, Haroon Mirza's Cosmos (2016) and
Supernova (2016) were created through a process of placing live peyote (Lophophora williamsii) on blank PCBs (
material usually used to make circuit boards) and running electrical current through them.
Thus the interior of the Sun consists mostly of Fe, O, Ni, Si, S, Mg and Ca from the deep interior of the
supernova — the same elements that comprise > 99 % of the
material in ordinary meteorites.