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neutron star
the part of the star’s core that survives after a Type II supernova explosion; is as dense as an atomic nucleus and is very small
rotation and magnetic field
the other important properties of neutron stars besides mass and size
pulsars
rapidly spinning neutron stars that radiate their energy quickly; the first one was discovered in 1967
millisecond pulsar
a type of pulsar that has a period less than 0.01 seconds; was first discovered in the early 1980s
merging neutron stars and a hypernova
the two models that have been proposed as the source of gamma-ray bursts
black hole
a remant that has a gravitational force so intense that even light can’t escape
Schwarzchild radius
the radius at which the escape speed from the black hole equals the speed of light
event horizon
an area in a black hole where nothing can escape; happens after the black hole has collapsed
Einstein’s Special Relativity Theory
states that the speed of light is the maximum possible speed, and it is always measured to have the same value by all observers, and there is no absolute frame of reference and no absolute state of rest
spacetime
the term used to express the unification of space and time; is explained in Einstein’s Special Relativity Theory
Einstein’s General Relativity Theory
states that it is impossible to tell from within a closed system whether one is accelerating or in a gravitational field; was tested in Einstein’s Elevator Experiment
gravitational redshift
occurs when a probe nears the event horizon of a black hole; observers will see it as experiencing a dramatic redshift as it gets closer, so that time appears to be going more slowly as it approaches
Cygnus X-1
a strong X-ray emitter that is thought to be a black hole; its visible partner is about 25 solar masses, and the total system is 35 solar masses
LIGO (Laser Interferometric Gravity-wave Observatory) and LISA (Laser Interferometer Space Antenna)
two space detectors that were designed to detect gravitational waves