Neutron star density. a typical neutron star has a mass of about 1.5m☉ and a radius of 10 kilometers. calculate the average density of a neutron star, in kilograms per cubic centimeter. compare the mass of 1 cm3 of neutron star material to the mass of mount everest ( 5 1010 kg).

explanation:

earth's surface is mainly heated by the absorption of infrared radiation from the sun.

evaporation occurs because molecules in liquid water are warmed ( usually by the sun) and vibrate quicker, becoming less dense and rise.

condensation occurs because molecules in water vapor are cooled and therefore vibrate more slowly thus becoming more dense and eventually fall to earth.

lines of equal barometric pressure on a weather map are called: isobars : lines of equal temp on a weather map are called: isotherms.​

radiation warms things up temp rises convection currents air circ windy weather