The Neutron Star

GPTKB entity

Statements (57)
Predicate Object
gptkbp:instance_of gptkb:physicist
gptkbp:bfsLayer 4
gptkbp:bfsParent gptkb:Larry_Niven
gptkbp:area about 10 kilometers
gptkbp:can_be quark matter
gptkbp:can_create gptkb:observatory
gptkbp:capacity about 4 x 10^17 kg/m^3
gptkbp:discovered_by gptkb:1967
gptkbp:emissions_standard gptkb:X-rays
gptkbp:field up to 10^11 to 10^15 T
gptkbp:formed gptkb:Type_II_supernovae
gptkb:core-collapse_supernovae
the collapse of a massive star
massive stars with initial masses greater than 8 solar masses
gptkbp:has_ability magnetic field
https://www.w3.org/2000/01/rdf-schema#label The Neutron Star
gptkbp:is_a_source_of pulsars
gravitational wave signals
gptkbp:is_accessible_by pulsar timing
gptkbp:is_analyzed_in magnetic field dynamics
extreme physical conditions
gptkbp:is_associated_with supernova explosions
gptkbp:is_characterized_by rapid rotation
gptkbp:is_observed_in gamma-ray bursts
gptkbp:is_often_associated_with gptkb:magnetars
gptkbp:is_often_compared_to black holes
gptkbp:is_often_depicted_as star clusters
the remnants of supernovae
gptkbp:is_part_of gptkb:Ninjutsu
gptkb:neutron_star_merger
life cycle of stars
neutron star merger event
neutron star-black hole binary
gptkbp:is_studied_in astrophysics
equation of state
gravitational wave astronomy
gptkbp:key nuclear physics research
the universe's evolution
the study of dense matter physics
gptkbp:key_people the synthesis of heavy elements.
gptkbp:mass 1.4 to 2.16 solar masses
gptkbp:max_speed up to 700 times per second
gptkbp:notable_inductees exotic states of matter
gptkbp:recognizes X-ray emissions
radio telescopes
gptkbp:religion a crust made of neutron-rich matter
a superfluid interior
gptkbp:research_focus astrophysical phenomena
gptkbp:serving_temperature up to 1 billion Kelvin shortly after formation
gptkbp:subject gptkb:spacecraft
high-energy astrophysics
gptkbp:supports neutron degeneracy pressure
gptkbp:surface about 1 million Kelvin
about 10^11 m/s^2
gptkbp:theory binary systems
gptkbp:torque up to 10^53 ergs
gptkbp:type_of gptkb:nebula