Neutron stars are the densest objects known (because politicians aren’t technically “objects”).  Every star’s lifespan is mediated by an astral tug-of-war between its outwardly propulsive fusion furnace and the compressive force of gravity, and how each star dies depends on its size.  If a star is massive enough, when it runs out of nuclear fuel gravity does its victory dance.  The star collapses on itself at up to one-fourth the speed of light, to a size as small as 30 kilometers (19 miles).  All that’s left is an ultra-condensed core, 100 million million million times as There are so many considerations that you need to follow when you are using these tablets. kamagra tablets does not protect against STDs (sexual transmitted diseases) like HIV. icks.org purchase levitra online In short, due to shortage supply of blood towards the penis may fall short to obtain an enough levitra online no prescription erection. The medical term for sales uk viagra having a gallbladder removed is not a new thing. Massage assists in building sildenafil india wholesale healthy and productive lifestyle naturally. hard as a diamond.  At that point, the star’s atomic nuclei are so crushed together that quantum mechanics shouts “no mas,” and like a cosmic Superball the star’s stellar matter rebounds, producing the most violent explosion we know of, a supernova.  The resulting shock wave produces the highest temperatures in the universe, at over 100 billion degrees Kelvin.  Even though neutron stars can be as small as 30 kilometers in diameter, they’re more massive than the Sun.  According to NASA’s Goddard Space Flight Center, one teaspoonful of neutron star, on Earth, would weigh a billion tons.