New research from the Niels Bohr Institute at the University of Copenhagen and Aarhus University shows that not only can
grains of dust form in gigantic supernova explosions, they can also survive the subsequent shockwaves they are exposed to.
Not exact matches
«The problem has been that even though
dust grains composed
of heavy elements would
form in supernovae, the supernova explosion is so violent that the
grains of dust may not survive.
Within these clouds, on the surfaces
of tiny
dust grains, hydrogen atoms link with oxygen to
form water.
These saturated organic molecules are
formed in interstellar space and are preserved on the surfaces
of dust grains.
The
dust in the gas cloud that
formed comets and the rest
of the solar system is thought to consist
of amorphous glass - like
grains instead.
Looking at Comet ISON's chemical fingerprints — its ratio
of carbon dioxide to water, its mix
of different kinds
of hydrogen atoms, the kind
of dust grains it contains — will indicate where it
formed 4.56 billion years ago, and thus put the wandering - Jupiter theory to the test.
The
dust grains that float through our solar system contain the ingredients to make water, which
forms when the
dust is zapped by a blast
of charged wind from the sun.
New work from a team
of Carnegie cosmochemists published by Science Advances reports analyses
of carbon - rich
dust grains extracted from meteorites that show that these
grains formed in the outflows from one or more type II supernovae more than two years after the progenitor stars exploded.
For this study, the team set out to investigate the timing
of supernova
dust formation by measuring isotopes — versions
of elements with the same number
of protons but different numbers
of neutrons — in rare presolar silicon carbide
grains with compositions indicating that they
formed in type II supernovae.
Rather, they analyzed microscopic silicon carbide, SiC,
dust grains that
formed in supernovae more than 4.6 billion years ago and were trapped in meteorites as our Solar System
formed from the ashes
of the galaxy's previous generations
of stars.
Silvia is optimistic, noting that most
of the
dust is in the
form of large, robust
grains.
Its centre ignited to make the sun, while farther out
grains of dust slowly coalesced to
form larger and larger solid bodies.
Simulations by Nora de Leeuw
of University College London and colleagues suggest that the
dust grains from which Earth
formed had such a tenacious grip on water that they could have held onto the molecules despite the high temperatures.
Weaver's models also demonstrate that once the temperature in the
dust cloud reaches about — 280ºF, most
of the molecules evaporate from the ice on
dust grains and enter a gas phase, allowing them to react a lot more quickly and to
form complex molecules.
In the prevailing theory
of planet formation, called core accretion,
dust grains stick together to
form rocky worlds, and some
of these rocky bodies then grow massive enough to attract surrounding gas, becoming gas giants like Jupiter.
Applying aperture photometry on the azimuthally averaged deconvolved PACS images and using a modified blackbody
of the
form Bν · λ − β, as expected for a
grain emissivity Qabs ~ λ − β with β equal to 1.2 (representing amorphous carbon, Mennella et al. 1998), we derived a
dust temperature between 108 ± 5 K at 20 ′ ′ and 40 ± 5 K at 180 ′ ′.
[2] The ejected shell
formed around AGB stars is composed
of gas and
dust grains.
I apply numerical models to investigate the physical and chemical evolution
of planetary materials, ranging from the small
dust grains suspended in protoplanetary disks to the many kilometer - scale objects which accrete together to
form planets.
While other species detected in space are
formed by gas - phase chemistry alone, or by a combination
of both gas and solid - phase generation, methanol is a complex organic compound which is
formed solely in the ice phase via surface reactions on
dust grains.
Each
of those holes had
formed when a
grain of cosmic
dust smacked into the surface
of the moon.
The impinging photons warm
dust grains, resulting in a lower probability
of forming and maintaining complex organic molecules.
After six months
of work, the team
formed by CSIC staff and the LuzLux production company, among others, has completed the documentary «Nanocosmos, a journey to the origins
of dust grains, a road movie which talks about the technological and human challenge that lies behind the development
of instruments in the area
of Laboratory Astrophysics.
Astronomers believe that planets
form like snowballs over millions
of years, as small
dust grains clump together to
form larger bodies.
It was a detailed portrait
of a so - called protoplanetary disk, made up
of gas and
dust grains, associated with a young star — the kind
of structure out
of which planets could be expected to
form.