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7 médias trouvés pour 'Supernova Type I'

Binary Star - Artist View - Binary star. Artist view - A white dwarf orbiting very close to her giant red companion tears him little by little from the material. This unstable couple will soon explode in supernova. Mass transfer between a red giant and a white dwarf star producing later a supernova explosion

Binary Star - Artist View - Binary star. Artist view - A white dwarf orbiting very close to her giant red companion tears him little by little from the material. This unstable couple will soon explode in supernova. Mass transfer between a red giant and a white dwarf star producing later a supernova explosion

P. Carril

PIX4572634

Binary Star - Artist View - Binary star. Artist view - Binary Star - mass exchange between a red giant a blue dwarf. When the material removed from the giant comes into contact with the accretion disc of the blue dwarf, it emits X-rays visible in the form of flashes by astronomers. This mass exchange process leads in a few thousand years to a nova explosion. Mass transfer between a red giant and a blue dwarf star producing X - ray emission and later a nova explosion

Binary Star - Artist View - Binary star. Artist view - Binary Star - mass exchange between a red giant a blue dwarf. When the material removed from the giant comes into contact with the accretion disc of the blue dwarf, it emits X-rays visible in the form of flashes by astronomers. This mass exchange process leads in a few thousand years to a nova explosion. Mass transfer between a red giant and a blue dwarf star producing X - ray emission and later a nova explosion

P. Carril

PIX4572585

Supernova Type I - Artist's View

Supernova Type I - Artist's View

P. Carril

PIX4583267

Supernova Type I - Artist's View

Supernova Type I - Artist's View

P. Carril

PIX4583269

Galaxies M95 and M96 in the Lion - Galaxies M95 and M96 in Leo - M95 (NGC 3351), on the left, is a barree spiral of type SBB, M96 (NGC 3368), on the right, is a spiral galaxy of type Sa. M96 is the brightest member of the Leo I galaxy group, which is also called the M96 group. It also contains M95, M105 and a number of weaker galaxies. Their distance to our Sun was measured with great precision thanks to the discovery of cepheides in these galaxies and the appearance of a supernova of type Ia in M96 in May 1998. These two galaxies are located 37 million light years away from Earth. M95 (NGC 3351, left), is a barred spiral galaxy, M96 (NGC 3368, right), is a spiral galaxy. With M105 (not pictured here), they are dominant members of the Leo I galactic group which also includes several fainter galaxies. Their distance from our Sun has been determinated with great precision thanks to the discovery of Cepheids stars in these galaxies and a type IA supernova in M96 appeared in May 1998. Their distance to our Sun is 37 million light - years — Galaxies M95 and M96 in the Lion - Galaxies M95 and M96 in Leo - M95 (NGC 3351), on the left, is a barree spiral of type SBB, M96 (NGC 3368), on the right, is a spiral galaxy of type Sa. M96 is the brightest member of the Leo I galaxy group, which is also called the M96 group. It also contains M95, M105 and a number of weaker galaxies. Their distance to our Sun was measured with great precision thanks to the discovery of cepheides in these galaxies and the appearance of a supernova of type Ia in M96 in May 1998. These two galaxies are located 37 million light years away from Earth. M95 (NGC 3351, left), is a barred spiral galaxy, M96 (NGC 3368, right), is a spiral galaxy. With M105 (not pictured here), they are dominant members of the Leo I galactic group which also includes several fainter galaxies. Their distance from our Sun has been determinated with great precision thanks to the discovery of Cepheids stars in these galaxies and a type IA supernova in M96 appeared in May 1998. Thei

Galaxies M95 and M96 in the Lion - Galaxies M95 and M96 in Leo - M95 (NGC 3351), on the left, is a barree spiral of type SBB, M96 (NGC 3368), on the right, is a spiral galaxy of type Sa. M96 is the brightest member of the Leo I galaxy group, which is also called the M96 group. It also contains M95, M105 and a number of weaker galaxies. Their distance to our Sun was measured with great precision thanks to the discovery of cepheides in these galaxies and the appearance of a supernova of type Ia in M96 in May 1998. These two galaxies are located 37 million light years away from Earth. M95 (NGC 3351, left), is a barred spiral galaxy, M96 (NGC 3368, right), is a spiral galaxy. With M105 (not pictured here), they are dominant members of the Leo I galactic group which also includes several fainter galaxies. Their distance from our Sun has been determinated with great precision thanks to the discovery of Cepheids stars in these galaxies and a type IA supernova in M96 appeared in May 1998. Thei

R. Gendler

PIX4610672

Supernova Explosion Type II - Artist's View 4/5 - 4 - All the material of the star is washed away; the shock wave reaches the surface, the supernova begins to shine

Supernova Explosion Type II - Artist's View 4/5 - 4 - All the material of the star is washed away; the shock wave reaches the surface, the supernova begins to shine

S. Numazawa

PIX4583224

Supernova Explosion Type II - Artist's View 5/5 - 5 - The outer layers of the star are blown by the shock wave, the star explodes

Supernova Explosion Type II - Artist's View 5/5 - 5 - The outer layers of the star are blown by the shock wave, the star explodes

S. Numazawa

PIX4583219

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