Mar 4, 2024
MASSIVE STAR
the 2nd design from my new collection, coming soon!
The massive star will feature pearl with glitter and glow in the dark!
Life and Death of a star HERE
seen from Mexico
seen from Uruguay
seen from Kazakhstan
seen from United Kingdom
seen from Canada
seen from Germany
seen from China
seen from Yemen
seen from Malaysia
seen from Germany
seen from China
seen from China
seen from Mexico
seen from China
seen from Singapore
seen from Yemen
seen from United States
seen from United States
seen from Lithuania
seen from United States
MASSIVE STAR
the 2nd design from my new collection, coming soon!
The massive star will feature pearl with glitter and glow in the dark!
Life and Death of a star HERE
album cover OOooOOo
Beyond the Stars
[ collab with @snavian who did the sketch/lines ]
5 Ways To Have A ‘Failed Supernova’ Instead Of A Real One
“1.) Mass thievery. The outer, lighter-element layers are required for massive supernovae. Mass-siphoning binary companions can “abort” otherwise inevitable explosions, creating exotic white dwarf remnants.”
Just because you’re born, as a star, with eight or more solar masses worth of material, doesn’t mean you’re destined to go supernova. There’s a whole lot that can happen in your evolution to alter your fate, and prevent you from going supernova initially. (Although, in some cases, these stars will still get a second chance!)
Learn what the five ways are to have a failed supernova instead of a real one, and learn what else these massive stars can create!
Kurzgesagt on Neutron Stars – The most extreme things that are not black holes
Forming from cosmic clouds, massive stars create heavy elements in their cores. After a few million years, the enriched material is blasted back into interstellar space where star formation can begin once again. Light from the explosion which created this supernova remnant, Cassiopeia A, would have been first seen in planet Earth's sky about 350 years ago, although it took that light about 11,000 years to reach us.
This false-color image, composed of X-ray and optical image data from the Chandra X-ray Observatory and Hubble Space Telescope, shows the still hot filaments and knots in the remnant. High-energy X-ray emission from specific elements has been color coded, silicon in red, sulfur in yellow, calcium in green and iron in purple, to help astronomers explore the recycling of our galaxy's star stuff. Still expanding, the outer blast wave is seen in blue hues. The bright speck near the center is a neutron star, the incredibly dense, collapsed remains of the massive stellar core.
Image Credit: X-ray - NASA, CXC, SAO; Optical - NASA,STScI
Passing a rare, extremely bright Wolf-Rayet star
Birth Of A Massive Star