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Alicia Costa Fresneda 1ºB
Neutron Stars
• What is a neutron stars?
Are extremely dense collapsed stars sometimes left
behind after a core –collapse supernova explosion.

• When is a neutron stars created?
Neutron stars are created when giant stars die in
supernovas and their cores collapse, with the protons
and electrons essentially melting into each other to form
neutrons.
CORTEZA:
Núcleos de Hierro
Neutrones

Neutron Stars
• Fluid core: neutron stars
pack their mass inside.
• 20-kilometer (12.4 miles)
diameter.
• 1,5 suns of mass.
• Massive core : 1,7kilometer of thickness.
• Stars 1.4 to 3 times as
massive as the SUN.
Superfluido de Neutrones.
Protones superconductores.
Neutron stars and white dwarfs

Recommended for you

NEUTRON STARS AND WHITE DWARFS
NEUTRON STARS AND WHITE DWARFSNEUTRON STARS AND WHITE DWARFS
NEUTRON STARS AND WHITE DWARFS

White dwarfs are the burned-out cores of stars that have collapsed into an extremely dense state with no empty space between atoms. They have a mass similar to the sun's but are very small, around the size of Earth. Neutron stars are created during supernova explosions from the central core of a star that collapsed under gravity. They are an extremely compact ball of neutrons that are very hot, small, dense, and have masses higher than the sun's. Both white dwarfs and neutron stars achieve extreme density through electron or quantum degeneracy pressure preventing further gravitational collapse.

THE LIFE CYCLE OF A STAR!
THE LIFE CYCLE OF A STAR!THE LIFE CYCLE OF A STAR!
THE LIFE CYCLE OF A STAR!

All stars begin as clouds of dust and gas called nebulae. When gravity causes the nebula to collapse, a protostar forms at the center. The protostar grows in size and temperature through nuclear fusion reactions until it becomes a stable main sequence star. Small stars like our Sun will eventually expand into red giants and shed their outer layers, leaving behind dense white dwarf cores. Larger stars may explode as supernovae, collapsing into neutron stars or black holes. The life cycle of a star depends on its initial mass, with smaller stars ending as white dwarfs and more massive stars ending as black holes or neutron stars.

startuplife cycle of stardeath of star
life cycle of a star
life cycle of a starlife cycle of a star
life cycle of a star

The life cycle of stars depends on their mass. Lower mass stars like our Sun will eventually become red giants then white dwarfs. Higher mass stars live shorter lives and end as supernovas, leaving behind neutron stars or black holes. All stars begin as nebulae of dust and gas that collapse under gravity into protostars and main sequence stars fueled by nuclear fusion.

astronomyastrobiology
White Dwarf
• What is a white dwarf?
Is a stella remnant composed mostly of electrondegenerate matter. They are very dense; a white dwarf’s
mass is comparable to that of the Sun, and its volume is
comparable to that of the Earth.
White Dwarf
• What will happen?
The sun will expand into a red giant star, in 5 billion years
from now, its outer layers engulfing the planets Mercury,
Venus and possibly the Earth, it will shrink into a hot and
dense White dwarf.

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Neutron stars and white dwarfs

  • 2. Neutron Stars • What is a neutron stars? Are extremely dense collapsed stars sometimes left behind after a core –collapse supernova explosion. • When is a neutron stars created? Neutron stars are created when giant stars die in supernovas and their cores collapse, with the protons and electrons essentially melting into each other to form neutrons.
  • 3. CORTEZA: Núcleos de Hierro Neutrones Neutron Stars • Fluid core: neutron stars pack their mass inside. • 20-kilometer (12.4 miles) diameter. • 1,5 suns of mass. • Massive core : 1,7kilometer of thickness. • Stars 1.4 to 3 times as massive as the SUN. Superfluido de Neutrones. Protones superconductores.
  • 5. White Dwarf • What is a white dwarf? Is a stella remnant composed mostly of electrondegenerate matter. They are very dense; a white dwarf’s mass is comparable to that of the Sun, and its volume is comparable to that of the Earth.
  • 6. White Dwarf • What will happen? The sun will expand into a red giant star, in 5 billion years from now, its outer layers engulfing the planets Mercury, Venus and possibly the Earth, it will shrink into a hot and dense White dwarf.