eem to be outstandingly brigtle more tating buffoon.” A fitness buff, en drop to teco demonstrate y to anyone it. oriously aggressive, ually becoming so intimidating t collaborator, a gentle man named alter Baade, refused to be left alone . Onat least one occasion Zened to kill Baade, ilson Observatory, if ech campus.
But Zartling brilliance. In turned tention to a question t roubled astronomers: ts of ligars. Improbably ron—tomic particle t been discovered in England by JamesC be at t of toccurred to if a star collapsed to t of densities found in toms, t ed core. Atoms erally be crusogetrons forced into trons. You ar.
Imagine a million really ill not even close. tron star is so dense t a single spoonfulof matter from it after tar t of energy leftover—enougo make t bang in tant explosionssupernovae. t events in creation.
On January 15, 1934, tract of apresentation t ed by Z StanfordUniversity. Despite its extreme brevity—one paragrapy-four lines—tractcontained an enormous amount of ne provided t reference to supernovaeand to neutron stars; convincingly explained tion; correctly calculatedted supernovaexplosions to tion of a mysterious neionary to say t. Neutron stars be confirmed for ty-four years. tion,t been verified yet. Altogetract ecrop Kip S. t prescient documents in tory of pronomy.”
Interestingly, Zanding of whis would happen.
According to t understand to be able tosubstantiate alent ly—to do tical sweeping up.
Z to recognize t t nearly enougo oget t be some otational influence—ter. One to see if a neutron star s even lig escape its immense gravitationalpull. You ely, Zracted almost no notice. er, tRobert Oppenurned tention to neutron stars in a landmark paper, asingle reference to any of Z doions concerning dark matter attract serious attention for nearly four decades. e can only assume t of pushis period.
Surprisingly little of to us 6,000 stars are visible to t 2,000 can be seenfrom any one spot.