Not exact matches
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.
Thanks to new detectors that can pick up neutrino signals and even gravitational waves, scientists will be ready when the next
nearby star explodes, Emily Conover reported
in «Waiting for a
supernova» (SN: 2/18/17, p. 24).
«Caught
in the act: Astronomers find a rare
supernova «impostor»
in a
nearby galaxy.»
A new influx of metalrich dust to the solar system, perhaps from a
nearby supernova, would have augmented isotopes
in the outer asteroids but not the inner ones.
«Massive fails» like this one
in a
nearby galaxy could explain why astronomers rarely see
supernovae from the most massive stars, said Christopher Kochanek, professor of astronomy at The Ohio State University and the Ohio Eminent Scholar
in Observational Cosmology.
Pulsars form when stars at least 1.4 times larger than our sun blow up
in supernovas; these powerful explosions usually knock
nearby stars out
The savannahs early hominins occupied might have appeared thanks to a spate of wildfires 8 million years ago — which might
in turn be linked to a
nearby supernova
Using elaborate computer simulations, a team of researchers from RIKEN
in Japan and the Max Planck Institute for Astrophysics (MPA) were able to explain the recently measured spatial distributions of radioactive titanium and nickel
in Cassiopeia A, a roughly 340 year old gas remnant of a
nearby supernova.
The process could be used to detect
supernovas as well — if a
supernova explodes
nearby, scientists could spot its neutrinos scattering off nuclei
in their detectors.
In the early 2000s, when looking for other objects in a nearby galaxy, he and his colleagues captured an image filled with the echoing light of three known supernova
In the early 2000s, when looking for other objects
in a nearby galaxy, he and his colleagues captured an image filled with the echoing light of three known supernova
in a
nearby galaxy, he and his colleagues captured an image filled with the echoing light of three known
supernovas.
Shortly after a burst of neutrinos from a
nearby supernova, the detector could direct astronomers to zero
in on a few degrees of sky.
In that case, faraway
supernovas (which we see as they were billions of years ago, when the growth was more rapid) would have accumulated redshift more quickly relative to their distance than
nearby ones.
Rob Beswick, a co-author of the research paper from the University of Manchester's Jodrell Bank Centre for Astrophysics added: «The explosion of a Type Ia
supernova is a rare event
in the
nearby Universe.
Supernova explosions
in older,
nearby galaxies, says Lee, may have fertilized the nascent Milky Way — and
in particular its center — with some of the heavy elements we now find here.
Nearby, large stars erupt
in cataclysmic
supernova explosions, sparking additional emissions from gas heated to millions of degrees.
Two previously undetected molecules, formylium (HCO +) and sulphur monoxide (SO), were found
in the cooling aftermath of
Supernova 1987A, located 163,000 light years away
in a
nearby neighbour of our own Milky Way galaxy.
Earlier this year, astronomers
in London detected a spectacular, once -
in - a-century
supernova (dubbed SN2014J)
in a relatively
nearby galaxy known as Messier 82 (M82), or the Cigar Galaxy, 12 million light - years away.
But the
supernovae that go off a few million years later could be hazardous to life
in solar systems unfortunate enough to be
nearby, Lockman says.
Measurements based on the cosmic microwave background, the earliest light
in the universe, suggest one rate of expansion, while measurements of
nearby supernovas suggest a faster one.
At his proposed distance, the 1181 explosion was roughly a fifth as luminous as the 1987
supernova in the Large Magellanic Cloud, a
nearby galaxy, that also emitted less light than the norm.
A newfound star
in a
nearby galaxy appears to have cheated death by blowing up at least twice as a
supernova.
By measuring about 2,400 Cepheid stars
in 19
nearby galaxies and comparing the apparent brightness of both types of stars, they accurately determined the true brightness of the Type Ia
supernovae.
«We have found a remarkably large dust mass concentrated
in the central part of the ejecta from a relatively young and
nearby supernova,» said Remy Indebetouw, an astronomer at the National Radio Astronomy Observatory (NRAO) and the University of Virginia, both
in Charlottesville, USA.
Other discoveries
in the Milky Way detailed
in the special edition include the sharpest image yet of a gamma ray source — a
nearby supernova remnant — which will enable researchers to study this object at finer scale than before — and three new «gamma ray shells» that are possibly examples of a new type of
supernova remnant.
Type Ia
supernovae are fairly rare
in the
nearby Universe and represent the explosion of at least one white dwarf star
in a binary system.
They made their best measurement to date
in a recent study of a
supernova first seen 27 years ago
in a
nearby galaxy.
In any case, any developing carbon - based life on a developing Earth - type planet would be subject to tremendous heat on a newly formed planet that is under intense asteroidal and cometary bombardment, in addition to the intense and deadly radiation produced by nearby supernovae and other massive young star
In any case, any developing carbon - based life on a developing Earth - type planet would be subject to tremendous heat on a newly formed planet that is under intense asteroidal and cometary bombardment,
in addition to the intense and deadly radiation produced by nearby supernovae and other massive young star
in addition to the intense and deadly radiation produced by
nearby supernovae and other massive young stars.
(iii) Far - infrared spectroscopy of dust and ice features will address uncertainties
in the mass and composition of dust
in galaxies, and the contributions of
supernovae to the interstellar dust budget will be quantified by photometry and monitoring of
supernova remnants
in nearby galaxies.
For example, Helfand pointed out that there are cases
in which astronomers concluded that a pulsar and
supernova remnant, while
nearby, are not related because the pulsar's «characteristic age» was much younger than the age calculated for the
supernova remnant.
On that «super» day, the All Sky Automated Survey for SuperNovae (ASASSN) reported a
supernova in the same
nearby galaxy Kepler was monitoring.
By comparing the observed brightness of both types of stars
in those
nearby galaxies, the astronomers could then accurately measure their true brightness and therefore calculate distances to roughly 300 Type Ia
supernovae in far - flung galaxies.
The youngest stars
in the galactic region surrounding around the Solar Neighborhood are associated with «subgroup B1» of the Pleiades (M 45) stellar moving group, and astronomers hypothesize that the more massive stars born
in this group may have already exploded as 20 or so
supernovae over the past 10 to 20 million years as the entire group of stars moved through a
nearby region of the Local Bubble (Berghoefer and Breitschwerdt, 2002).
As he puts it: «Today the Royal Astronomical Society
in London publishes (online) Henrik Svensmark's latest paper entitled «Evidence of
nearby supernovae affecting life on Earth».
GCRs are modulated by both solar magnetic field, which is largely unpredictable
in strength except for generalities associated with 11 - year sunspot cycle and is also modulated by unpredictable events like
nearby supernovas, and by more predictable very very long slow changes
in intensity due to the solar system traversing spiral arms of our galaxy and wandering above and below the galactic plane
in cycles lasting tens and hundreds of millions of years.