Not exact matches
As far our atomic composition, we are made up of «stardust» from exploding supernovas (as noted by Lawrence Krauss, an American theoretical physicist, and Robert Kirshner, Harvard College Professor of Astronomy
As far our atomic composition, we are made up
of «stardust» from exploding
supernovas (
as noted by Lawrence Krauss, an American theoretical physicist, and Robert Kirshner, Harvard College Professor of Astronomy
as noted by Lawrence Krauss, an American theoretical physicist, and Robert Kirshner, Harvard College Professor
of Astronomy).
The universe itself,
as described by science, may be seen
as our Mother but it can also be a capricious Tyrant who could destroy all
of us in the blink
of an eye and with less effort at any moment (
supernova, asteroid, etc).
Then light was liberated, and then gravity created the first stars and galaxies, then billions
of years later, a local star went
supernova and seeded the local nebula with heavier elements, elements necessary for life, elements that were not created during the Big Bang, then the sun was born, then the planets coalesced, and billions
of years later some primate wrote a story about how the Earth was created at the same time
as the rest
of the universe, getting it wrong because that primate did not have the science nor technology to really understand what happened, so he gave it his best guess, most likely an iteration
of an older story told prior to the advent
of the Judeo Christian religion.
Supernovae: For distances between galaxies, scientists measure the brightness of supernovae based on the mathematical formulae used to determine brightness as measured by distance, called «The Standard Cand
Supernovae: For distances between galaxies, scientists measure the brightness
of supernovae based on the mathematical formulae used to determine brightness as measured by distance, called «The Standard Cand
supernovae based on the mathematical formulae used to determine brightness
as measured by distance, called «The Standard Candle».
I'm reminded
of some dude named Icarus... and
of the term «hubris» and the phrase «pride before the fall»... McGregor was a
supernova flash in the pan, and
as I've said before, he's probably going to go out just
as quickly.
Cristiano Ronaldo went
supernova, Wayne Rooney solidified his claim
as one
of the greatest Premier League players
of all time, and Carlos Tevez played a leading man who was disguised
as a character actor.
She estimated Buso's chances
of such a discovery, his first
supernova, at one in 10 million or perhaps even
as low
as one in 100 million.
They turned to a type
of supernova created by the death
of stars
of about the same mass
as our sun.
SHINE BRIGHT
Supernova 1987A shone
as a brilliant point
of light near the Tarantula Nebula (pink cloud) in the Large Magellanic Cloud,
as pictured from an observatory in Chile.
The
supernova, known
as SN1987A, was first seen by observers in the Southern Hemisphere in 1987 when a giant star suddenly exploded at the edge
of a nearby dwarf galaxy called the Large Magellanic Cloud.
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.
As technology advances, new facilities keep providing fresh looks at the remains
of the
supernova.
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.
After a star explodes
as a
supernova, it usually leaves behind either a black hole or what's called a neutron star — the collapsed, high - density core
of the former star.
Riess has since hunted down
supernovae that exploded more than 7 billion years ago, filling in gaps: The universe first slowed down
as the inward pull
of matter dominated over the relatively mild outward push
of dark energy.
«By introducing asymmetry into the explosion and adjusting the gas properties
of the surrounding environment, we were able to reproduce a number
of observed features from the real
supernova such
as the persistent one - sidedness in the radio images,» said Dr Toby Potter.
This should lead to tremendous advances in time - domain astronomy: studying fast - changing phenomena
as they occur — black holes being born,
supernovas exploding —
as well
as locating potentially Earth - threatening asteroids and mapping the little - understood population
of objects orbiting out beyond Neptune.
This effect becomes even more apparent
as the shock collides into the equatorial ring,
as observed in Hubble Space Telescope images
of the
supernova.
But,
as what's now called Tycho's
supernova remnant demonstrates, something still fuels the radiation fire hundreds
of years after its energy should have been drained.
At first, astronomers suspected that 1987A was a class
of supernova known
as type 1a — the detonation
of a stellar core left behind after a star like the sun quietly sheds gas at the end
of its life.
After shining for many millions
of years, stars end their lives, mainly, in two ways: very high mass stars die very violently
as supernovae, while low mass stars end
as planetary nebulae.
A neutron star is the crushed core
of a massive star that ran out
of fuel, collapsed under its own weight, and exploded
as a
supernova.
Lower velocity runaway stars can be produced when one half
of a binary pair explodes
as a
supernova, blasting its partner away.
If they are jettisoned out
of the galaxy and then explode
as supernovae, the heavy elements they contain could be released into this medium.
The increased sensitivity and improved resolution
of the EVLA will let scientists peer deep into star - forming clouds and spy on protoplanetary disks
of dense gas surrounding young stars
as well
as track
supernovae, fast - moving neutron stars and black holes, McKinnon says.
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.
As many as 30 percent of such stars, it seems, may quietly collapse into black holes — no supernova require
As many
as 30 percent of such stars, it seems, may quietly collapse into black holes — no supernova require
as 30 percent
of such stars, it seems, may quietly collapse into black holes — no
supernova required.
Measuring gravitational waves would allow astronomers to probe phenomena such
as the heart
of supernovas and could provide insight into the Big Bang.
During this period, six normal
supernovae have occurred within the galaxies we've been monitoring, suggesting that 10 to 30 percent
of massive stars die
as failed
supernovae,» he said.
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.
Strangely, though, none
of those stars was bigger than about 17 solar masses, even though much more massive stars abound and should also be dying
as supernovae.
As it floats in an area
of the LMC racked by the explosions
of numerous
supernovae in recent cosmic history, one theory was that the pattern might be caused by a set
of localised ripples created when clumps
of debris from an ancient
supernova were hit by a blast wave from a relatively recent one.
In the failed
supernova of a red supergiant, the envelope
of the star is ejected and expands, producing a cold, red transient source surrounding the newly formed black hole,
as illustrated by the expanding shell (left to right).
Metals (elements heavier than hydrogen and helium) are created in the interiors
of stars
as they evolve and then released into surrounding gas through
supernova explosions or stellar winds (often referred to
as chemical evolution).
A particular class
of supernovae known
as type Ia are well suited to the task.
Stars exploding
as supernovae are the main sources
of heavy chemical elements in the Universe.
• What do we know about the nature
of the death
of massive stars — signaled by Type II
supernovae — that fashion crucial elements such
as calcium and oxygen?
Given the redshift
of the light from this stellar explosion — which occurred about 10 billion years ago, when the universe was one third its current size — the object appeared much brighter than it would have been if [dust filling intergalactic space simply made the
supernovae appear dim,
as some researchers had proposed].
And just
as stars,
supernova explosions, and the Big Bang's fading glow all give off different frequencies
of light, they also send out different frequencies
of gravitational waves.
The vast distances to the galaxies and thick shrouds
of dust blocked a view
of the inevitable climax:
supernovas exploding in rapid succession
as each generation
of giant stars dies out.
Collectively, the findings support the notion that type Ia
supernovas suffer from «stellar amnesia,» meaning that they «forget» the specifics
of their earlier selves and become largely identical once they go off — just
as astronomers hoped.
Gas and dust in space can have an impact on the brightness
of standard candles — objects with known brightness such
as type 1a
supernovas and some variable stars
DAZZLING in its brightness, a rare type
of star's first outburst in 2009 was soon dismissed
as the tantrum
of a
supernova impostor.
For example the filaments to the right
of the image are the remnants
of an ancient
supernova (SNR G332.4 - 00.4, also known
as RCW 103), and the glowing red filaments at the lower left surround an unusual and very hot star (RCW 104, surrounding the Wolf - Rayet star WR 75).
When the bubbling
of the gas becomes sufficiently powerful, the
supernova explosion sets in
as if the lid
of the pot were blown off.
Cassiopeia A Just before it explodes
as a
supernova, a massive star is like an onion, with layers
of different chemical compositions atop one another.
Because this class
of explosion was distinct from the far more frequent and far less bright stellar outburst known
as a nova, they said, it deserved a classification all its own:
supernova.
Stars that are eight or more times the mass
of the sun explode
as supernovae at the end
of their lives.
As for the fate of these huge stars, he adds, «They could explode as spectacular supernovas and leave no remnants behind.&raqu
As for the fate
of these huge stars, he adds, «They could explode
as spectacular supernovas and leave no remnants behind.&raqu
as spectacular
supernovas and leave no remnants behind.»
FLASH
OF LIGHT Type 1a
supernovas, such
as the one seen in this Hubble Space Telescope image, can be triggered in at least two different ways, new research shows.