What happens when a core's mass is less than 3 solar masses but greater than 1.44 solar masses?
a. Electron degeneracy pressure can no longer support the core and the electrons combine with the protons to generate neutrons and neutrinos, the neutrinos of which supply neutron degeneracy pressure to support the neutron star. b. Electron degeneracy pressure can no longer support the core and the electrons combine with the protons to generate neutrons and neutrinos, the neutrons of which supply neutron degeneracy pressure to support the neutron star.
c. Electron degeneracy pressure supports the core of the white dwarf. d. Electron degeneracy pressure can no longer support the core and the electrons combine with the protons to generate neutrons and neutrinos, the neutrinos of which supply neutron degeneracy pressure to support the black hole star.
Question 2
All radio telescopes are refracting telescopes.
a. True
b. False
Indicate whether the statement is true or false
Solar Energy Input Varies with Latitude
Solar Neutrino Experiment
The Core of the Rosette Nebula
Mass Exchange Between Close Binary Stars
An experimentally made Oldowan type core.
Climate models the flow of mass and energy