108.9K
SCDo you know the difference between a Nova, Supernova , Hypernova and Kilonova? #physics #nasa #universe #kilonova #hypernova
@scienceluxe
#Hypernova Vs Supernova
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INThe sun explodes into a supernova CAUGHT ON CAMERA #VFX
@insanepatient2
1.2M
GASupernova 1987A erupted 39 years ago, becoming the brightest naked-eye supernova since Kepler’s time. Exploding in the Large Magellanic Cloud, it gave astronomers an unprecedented close-up view of a massive star’s death and expanding shockwave.
@galaxies
1.7K
SUSupernova 😨 VS Hypernova 🥶 #shorts #spacevideos #reels #viral #space #earth #nova #jwst #hypernova #sun #supernova #kilonova #bigbang #moon #universe #galaxy #star #milkyway #planet #exoplanet #solarsystem #cosmos #science #cosmic #astrophysics #astronomy #cosmology
@surojit_banerjee_2004
9.3K
SPA hypernova is a cosmic phenomenon that is a supernova that occurs in a very giant star whose age stars are 100 times larger than the sun
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#hypernova #cosmos #univers #stars #supernova
@spi6t
300.0K
PUA supernova is one of the most powerful and dramatic events in the universe, marking the explosive death or transformation of a star. For a brief period, a single star undergoing a supernova can shine brighter than an entire galaxy. These explosions occur in two main ways.
In a core-collapse supernova, a massive star, typically more than eight times the mass of the Sun, runs out of nuclear fuel, causing its core to collapse under gravity in a matter of seconds. This collapse generates an enormous shockwave that blasts the outer layers of the star into space, often leaving behind a dense neutron star or a black hole.
A typical supernova releases an astonishing amount of energy, around 10⁴⁴ joules, which is comparable to the total energy the Sun will emit over its entire 10-billion-year lifetime. Interestingly, most of this energy is not emitted as visible light but as nearly undetectable particles called neutrinos.
@pulsareducation
104.8K
UNIn the year 1054…
Something appeared in the sky so bright—
that it was visible even during the day.
Ancient Chinese astronomers recorded it
as a “guest star.”
But it wasn’t a star being born…
💥 It was a star dying.
A massive explosion known as a supernova.
The remains of that explosion still exist today—
forming what we now call the
Crab Nebula 🌌
What you’re looking at isn’t just space…
👉 It’s history frozen in time
A cosmic event that happened nearly 1,000 years ago—
and is still expanding even now.
The Universe doesn’t forget.
💥 It leaves behind evidence…
for those who know where to look.
#Supernova #Space #Universe
#Cosmos #Astronomy
@universe_bytes
8.3K
MAA hypernova, sometimes called a collapsar, is a particularly energetic core-collapse supernova. Scientists think a hypernova occurs when stars more than 30 times the mass of the Sun quickly collapse into a black hole. The resulting explosion is 10 to 100 times more powerful than a supernova. They have also been referred to as superluminous supernovae.
[Space, Universe, Cosmos, Science, Astronomy, Cosmology, Supernova, Hypernova, Kilonova, Neutron star, Blackhole, Astronaut, Solar System]
@macrooocosm
847.8K
MIA supernova is one of the most powerful events in the universe.
It occurs when a massive star exhausts its nuclear fuel and can no longer resist its own gravity. The core collapses in a fraction of a second, triggering a colossal explosion that releases more energy than our Sun will emit in its entire lifetime.
For a brief period, a single supernova can shine brighter than an entire galaxy 🌌.
These explosions are not just endings — they are cosmic creators. Supernovae forge heavy elements like iron, gold, and uranium, scattering them across space. These elements later form new stars, planets, and even life.
Every atom of calcium in your bones and iron in your blood was once created inside a star… and spread through the universe by a supernova 💫
In short, supernovae are how the universe recycles matter and continues evolving.
#supernova
#astronomy
#space
#universe
#cosmos
#astrophysics
#spacefacts
#sciencefacts
#stars
#galaxy
#milkyway
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@mindshift.ai18
4.1M
ASA new video shows the evolution of Kepler’s Supernova Remnant using data from NASA’s Chandra X-ray Observatory captured over more than two and a half decades.
Kepler’s Supernova Remnant, named after the German astronomer Johannes Kepler, was first spotted in the night sky in 1604. Today, astronomers know that a white dwarf star exploded when it exceeded a critical mass, after pulling material from a companion star, or merging with another white dwarf. This kind of supernova is known as a Type Ia, and scientists use it to measure the expansion of the universe.
Supernova remnants, the debris fields left behind after a stellar explosion, often glow strongly in X-ray light because the material has been heated to millions of degrees from the blast. The remnant is located in our galaxy, about 17,000 light-years from Earth, allowing Chandra to make detailed images of the debris and how it changes with time. This latest video includes its X-ray data from 2000, 2004, 2006, 2014, and 2025. This makes it the longest-spanning video that Chandra has ever released, enabled by Chandra’s longevity.
“The plot of Kepler’s story is just now beginning to unfold,” said Jessye Gassel, a graduate student at George Mason University in Virginia, who led the work. “It’s remarkable that we can watch as these remains from this shattered star crash into material already thrown out into space.” Gassel presented the new Chandra video and the associated research at the 247th meeting of the American Astronomical Society in Phoenix.
The researchers used the video to show that the fastest parts of the remnant are traveling at about 13.8 million miles per hour (2% of the speed of light), moving toward the bottom of the image. Meanwhile, the slowest parts are traveling toward the top at about 4 million miles per hour (0.5% of the speed of light). This large difference in speed is because the gas that the remnant is plowing into toward the top of the image is denser than the gas toward the bottom. This gives scientists information about the environments into which this star exploded.
#supernova #space #star #explosion #fast
@astrovise
896.0K
_SThis video shows the evolution of Kepler's Supernova Remnant using data from NASA's Chandra X-ray Observatory captured over more than two and a half decades.
Kepler's Supernova Remnant, named after the German astronomer Johannes Kepler, was first spotted in the night sky in 1604. Today, astronomers know that a white dwarf star exploded when it exceeded a critical mass, after pulling material from a companion star, or merging with another white dwarf. This kind of supernova is known as a Type la, and scientists use it to measure the expansion of the universe.
Supernova remnants, the debris fields left behind after a stellar explosion, often glow strongly in X-ray light because the material has been heated to millions of degrees from the blast. The remnant is located in our galaxy, about 17,000 light-years from Earth, allowing Chandra to make detailed images of the debris and how it changes with time. This latest video includes its X-ray data from 2000, 2004, 2006, 2014, and 2025. This makes it the longest-spanning video that Chandra has ever released, enabled by Chandra's longevity.
"The plot of Kepler's story is just now beginning to unfold," said Jessye Gassel, a graduate student at George Mason University in Virginia, who led the work. "It's remarkable that we can watch as these remains from this shattered star crash into material already thrown out into space." Gassel presented the new Chandra video and the associated research at the 247th meeting of the American Astronomical Society in Phoenix.
The researchers used the video to show that the fastest parts of the remnant are traveling at about 13.8 million miles per hour (2% of the speed of light), moving toward the bottom of the image. Meanwhile, the slowest parts are traveling toward the top at about 4 million miles per hour (0.5% of the speed of light). This large difference in speed is because the gas that the remnant is plowing into toward the top of the image is denser than the gas toward the bottom. This gives scientists information about the environments into which this star exploded.
Follow @_stellarzone for more Space content
@_stellarzone
115.4K
NAA star's last breath is still rewriting space.🌟💥
This new video shows changes in Kepler's Supernova Remnant using data from @NASA's Chandra X-ray Observatory captured over more than two and a half decades. Located about 17,000 light-years from Earth, parts of the remnant are still traveling at roughly 13.8 million miles (22.2 million kilometers) per hour — or about 2% of the speed of light. More in the comments!
Video Description:
This is a silent video of Kepler's expanding Supernova Remnant. The video was created using X-ray data gathered in 2000, 2004, 2006, 2014, and 2025. Those distinct datasets were turned into highly-detailed visuals, creating a 25-year timelapse-style video of the growing remnant.
Kepler's Supernova Remnant was once a white dwarf star that exploded when it exceeded its critical mass. In X-ray light, the remnant resembles a cloudy neon blue ring with a diagonal cross line stretching from our upper right down to our lower left. The ring appears thinner and wispier at the bottom, with a band of white arching across the top.
As the video plays, cycling through the datasets, the ring subtly, but clearly, expands, like a slowly inflating balloon. The bottom of the remnant is expanding fastest and the top of the ring is expanding the slowest. The large difference in speed is because the gas that the remnant is plowing into towards the top of the image is denser than the gas towards the bottom.
#AAS247 #space #supernova #new #astronomy
@nasachandraxray
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