#Supernova 1006

[bedroom-kingdom]

You’ll find me in the end Go line reality Look around You’ll see these doors Buy one way ticket to alienation Where you get off the train on the final station They lie to you You leave them They lie to you You leave this way They lie to you Let me go there They lie to you You forget them all They lie to you You take the sky They lie to you You kill them all They lie to you Let me go there Ah, ah Ah, ah Ah, ah Ah, ah In this place you’ll lose your mind And forget who you are Stop dreaming, you’ll see they lie Stop dreaming, you’ll see they kill Stop dreaming, you’ll see they lie Stop dreaming, stop lying to yourself You’ll find me in the end Go line reality Look around You’ll see these doors Buy one way ticket to alienation Where you get off the train on the final station

No More Sorry Supernova 1006 Ministry

2016 • Russia

[inthewindtunnel]

Supernova 1006

How I Need You

(Blind Seagull remix)

(Casket Cassette remix)

(Giirls remix)

(Culttastic remix)

-original-

[z428]

Music for nights. This is where we try to keep distance to the day.

https://video.mecp.de/embed/Ax7Zz5mkTBM

https://video.mecp.de/watch?v=Ax7Zz5mkTBM

#music for nights #synthwave #supernova 1006 #post punk

[planetaryalphabet]

SN 1006 was a supernova that appeared in the year 1006, in the constellation of Lupus. It was observed across China, Japan, modern-day Iraq, Egypt, and Europe. It exceeded roughly sixteen times the brightness of Venus. Modern astronomers consider its distance from Earth to be about 7,200 light-years

This ribbon is part of SN 1006’s expanding supernova remnant.

[netmassimo]

An article published in the journal "Astronomy & Astrophysics" reports a study of the supernova remnant cataloged as SN 1006 which led to the identification of an ejecta fragment of the progenitor star. A team of researchers led by Roberta Giuffrida of the University of Palermo and the Italian National Institute of Astrophysics used observations conducted with various telescopes exploiting X-ray emissions and compared them with theoretical models. The conclusion is that this iron-rich fragment is moving at a very high speed within the debris cloud generated by the supernova. This discovery is useful in the study of supernovae like this one, generated by explosions of white dwarfs.

[2001honda-civic]

i need to stop looking at the wikipedia page for the history of supernova observation. what do you mean that out of the 8 supernovae visible to the human eye the two brightest both happened in the same century. why not my century. asshole.

[silvereyedowl]

[source]

SN 1006: Pieces of the Cosmic Ray Puzzle - October 16th, 1996.

"Research balloon flights conducted in 1912 by Austrian physicist Victor Hess revealed that the Earth was constantly bombarded by high energy radiation from space - which came to be called "cosmic rays." What are cosmic rays and where do they come from? They are known to be mostly subatomic particles - predominantly protons and electrons - but their origin is a long standing mystery. After almost a century of study, this cosmic puzzle was at least partially solved by X-ray images and spectra from the ASCA satellite observatory. Pieced together to show the region around a star observed to go supernova in 1006 AD, the overlapping X-ray snapshots above (seen in false colour) revealed the bright rims of the exploded star's still expanding blast wave. These ASCA observations showed, for the first time, that the energy spectrum of the bright regions is like that produced by extremely high energy electrons streaming through a magnetic field at nearly the speed of light. If (as expected) high energy protons are associated with these energetic electrons, then supernova remnants like SN 1006 are sources of Hess' puzzling cosmic rays."

[darsispazio]

Srotolando nastri nello spazio

Cosa è mai questo nastro che si va srotolando negli spazi cosmici? A cosa è dovuto? Per la cronaca, ad una delle esplosioni più violente cui abbiano mai assistito i nostri antenati. SN 1006, un lungo nastro osservato da Hubble Credit: NASA, ESA, Hubble Heritage (STScI/AURA); Acknowledgement: W. Blair et al. (JHU) Per capire, dobbiamo tornare indietro fino al 1006 DC. In quel lontano anno la…

[androgynousbirdtale]

SN 1006: A Supernova Ribbon from Hubble

What created this unusual space ribbon? The answer: one of the most violent explosions ever witnessed by ancient humans. Back in the year 1006 AD, light reached Earth from a stellar explosion in the constellation of the Wolf (Lupus), creating a "guest star" in the sky that appeared brighter than Venus and lasted for over two years. The supernova, now cataloged at SN 1006, occurred about 7,000 light years away and has left a large remnant that continues to expand and fade today. Pictured here is a small part of that expanding supernova remnant dominated by a thin and outwardly moving shock front that heats and ionizes surrounding ambient gas. The supernova remnant SN 1006 now has a diameter of nearly 60 light years.

Image Copyright: Credit: NASA, ESA, Hubble Heritage (STScI/AURA); Acknowledgement: W. Blair et al. (JHU)

[inthewindtunnel]

Supernova 1006

Tell Your Name

[the-wolf-and-moon]

SN 1006, Supernova Streams

[thespacewirednews]

A supernova glowing in the dark 🌟⁣

When supernova remnant SN 1006 first appeared in the sky in 1006 C.E., it was far brighter than Venus and visible during the daytime for weeks. From that moment on, it occupied the hearts of astronomers all over the world; it has been studied from the ground and from space many times.⁣ ⁣ In this image, visible, radio, and X-ray data combine to give us that blue (and red) view of the remnant’s full shell – the debris field that was created when a white dwarf star exploded and sent material hurtling into space.⁣ ⁣ Scientists believe SN 1006 is a Type Ia supernova. This class of supernova is caused when a white dwarf never lets another star go: either it pulls too much mass from a companion star and explodes, or it merges with another white dwarf and explodes. Understanding Type Ia supernovas is especially important because astronomers use observations of these explosions in distant galaxies as mileposts to mark the expansion of the universe.⁣ ⁣ Image description: This supernova remnant looks like a bubble filled with blue and red clouds of dust and gas, floating amid a million stars. These stars are visible all around the bubble and even can be seen peeking through it.⁣ ⁣

[seasoflife]

When supernova remnant SN 1006 first appeared in the sky in 1006 C.E., it was far brighter than Venus and visible during the daytime for weeks. From that moment on, it occupied the hearts of astronomers all over the world; it has been studied from the ground and from space many times.

In this image, visible, radio, and X-ray data combine to give us that blue (and red) view of the remnant's full shell - the debris field that was created when a white dwarf star exploded and sent material hurtling into space.

Scientists believe SN 1006 is a Type la supernova.

This class of supernova is caused when a white dwarf never lets another star go: either it pulls too much mass from a companion star and explodes, or it merges with another white dwarf and explodes.

Understanding Type la supernovas is especially important because astronomers use observations of these explosions in distant galaxies as mileposts to mark the expansion of the universe.

Image description: This supernova remnant looks like a bubble filled with blue and red clouds of dust and gas, floating amid a million stars. These stars are visible all around the bubble and even can be seen peeking through it.

Credit: NASA, ESA, and Z. Levay (STScl)

seasoflife