Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.1 6/24/83; site ecsvax.UUCP Path: utzoo!watmath!clyde!bonnie!akgua!mcnc!ecsvax!mullen From: mullen@ecsvax.UUCP (Mike McMullen) Newsgroups: net.physics Subject: Re:Color of Neutron Stars Message-ID: <957@ecsvax.UUCP> Date: Thu, 4-Apr-85 09:16:37 EST Article-I.D.: ecsvax.957 Posted: Thu Apr 4 09:16:37 1985 Date-Received: Sun, 7-Apr-85 03:44:36 EST Organization: NC Educational Computing Service Lines: 12 I don't pretend to be an astrophysicist. The answer I present here was given to me by a friend who is one , however. "Neutron stars have typical surface temperatures of a million degrees K, so they are the "color" of X-ray photons (i.e., way past the ultra- violet side of the visible color spectrum). That assumes they radiate somewhat like blackbody emitters, which is about what the sun does. But at any rate, the X-ray astronomers have measured their surface emission and they generally fit a blackbody spectrum at 1 million degrees. You wouldn't want to observe them from up close with your own eyeballs." Makes sense if you think about it for a minute.