Neutron Star Flashcards
Prediction and Discovery
Walter Baade and Fritz Zwicky predicted the existence of neutron stars in 1934.
Jocelyn Bell first discovered a Pulsar (a type of neutron star) in 1967.
Nuclear fusion
Stars exist because of the balance between the mass of trillions of tons of hot plasma and gravity.
Gravity squeezes the material together with so much force that nuclear fusion occurs: hydrogen fuses into helium
Death of a Medium Star
Medium stars, like our Sun, go through a giant phase, where they burn helium into carbon and oxygen before they eventually turn into white dwarfs
Medium Star–> Subgiant–>Red Giant–>White Dwarf
Death of a Massive Star
When the helium fuel is exhausted the balance between pressure and radiation tips and gravity wins which squeezes the star tighter than before
The core burns hotter and faster while the outer layers swell, fusing heavier and heavier elements
Core Collapse
The iron in the core is ”nuclear ash”, meaning, it has no energy to give and cannot be fused.
The pressure is so great electrons and protons fuse into neutrons which then get squeezed together as an atomic nuclei in an event called electron capture.
An iron ball the size of Earth is squeezed into a ball of pure nuclear matter the size of a city.
Supernova
Gravity pulls the outer layers in at 25% the speed of light, the implosion bounces off the iron core which produces a shockwave outwards and catapults the rest of the material into space
Neutron Star
What remains after the supernova is a neutron star. It has a 1-2 solar masses but is compressed to an object 25 km (15.5 miles) wide
Structure
Atmosphere: Carbon atmosphere
Crust–> Outermost layers: Extremely hard and made of iron leftover from the supernova that is squeezed together in a crystal lattice with a sea of electrons flowing through them
Core: Not sure of the properties of matter when they are squeezed this hard
Nuclear Pasta in the Crust
Gnocchi phase
Spaghetti phase
Lasagna phase
Pulsar
Pulsars are rotating neutron stars observed to have pulses of radiation at very regular intervals that typically range from milliseconds to seconds
Magnetar
In a typical neutron star the magnetic field is trillions of times that of Earth’s but in a magnetar the magnetic field is another 1,000 times stronger