It's 1,000 times brighter than a nova (when a white dwarf erupts) but not as
bright as a supernova.
The future of science writing is as
bright as a supernova!
Not exact matches
Eta Carinae is sometimes called a «
supernova impostor» because its eruptions are so violent they can be nearly
as bright as exploding stars.
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 star, which was 25 times
as massive
as our sun, should have exploded in a very
bright supernova.
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].
A type Ia
supernova that exploded when the universe was half its present size is about one ten - billionth
as bright as Sirius, the
brightest star in the sky.
The resulting explosion can be up to a million times
as bright as the sun, but unlike
supernovas, classical novas don't destroy the star.
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.
Depending on its chemistry, the star might then explode
as an exceptionally
bright supernova or collapse into a smaller, faster - spinning millisecond pulsar, an event that has not been witnessed before (arxiv.org/abs/1302.4634).
The Compton Gamma Ray Observatory (CGRO), designed to detect gamma rays from distant astrophysical objects such
as neutron stars and
supernova remnants, had also begun recording
bright, millisecond - long bursts of gamma rays coming not from outer space but from Earth below.
But some astronomers wonder if distant
supernovae appear dimmer than expected because
supernovae in the past were not
as bright as they are now.
At its
brightest,
Supernova 1987A glowed
as intensely
as the stars in the Big Dipper constellation.
But this one, called KSN 2015K, was just about
as bright as a regular
supernova, so the team thinks it may have started out dim and then received an extra boost.
Type Iax
supernovae are fainter than their type Ia relatives, which are so reliably
bright that we use them
as «standard candles» to estimate cosmic distances.
This is about a hundred times
as much energy
as that released in the
brightest supernova explosion, and is many times more than the amount needed to explain the origin of the bursts of gamma rays.
Remarkably, these
supernovae were spotted
as close
as 600 light years from the
bright nuclear regions of these galaxies — despite being at least 150 million light years from the Earth.
Core collapse
supernova (CCSN) rates suffer from large uncertainties
as many CCSNe exploding in regions of
bright background emission and significant dust extinction remain unobserved.
«We're surprised that Lofar can see
as many
as 16
bright supernova remnants in M 82.
The Crab Nebula, one of the most famous nebulae and seen here by the Hubble Space Telescope, is actually the expanding explosion of a core collapse
supernova, the light of which was
bright enough to be seen here on Earth in the year 1054 CE,
as documented by Chinese astronomers at the time.
As such, this was the first
bright supernova to be observed with modern scientific instruments.
Those first stars led hard and fast lives, burning
bright and dying quickly
as supernovas.
Tycho found it at first
as bright as Jupiter, but the
supernova soon grew
as brilliant
as Venus (around -4 magnitude).
In x-ray emission, SN 3006gy was also nearly
as bright as the core of host galaxy NGC 1260, but not
bright enough for a Type - Ia
supernova (more).
On September 18, 2006, astronomer Robert M. Quimby detected the
brightest and largest
supernova ever recorded by contemporary astronomers, using the ROTSE - IIIb telescope at McDonald Observatory (Robert M. Quimby, 2006; and Katie Humphrey, Austin - American Statesman, May 9, 2007)-- but became second brightest on October 10, 2007 after twice - as - bright Supernova 2005ap (see APOD; and Quimby et a
supernova ever recorded by contemporary astronomers, using the ROTSE - IIIb telescope at McDonald Observatory (Robert M. Quimby, 2006; and Katie Humphrey, Austin - American Statesman, May 9, 2007)-- but became second
brightest on October 10, 2007 after twice -
as -
bright Supernova 2005ap (see APOD; and Quimby et a
Supernova 2005ap (see APOD; and Quimby et al, 2007).
The Florida Project loses the jagged iPhone imagery of that big breakthrough, but the colors (and characters) shine just
as supernova -
bright on 35 mm.