Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.3 4.3bsd-beta 6/6/85; site ucbvax.BERKELEY.EDU Path: utzoo!watmath!clyde!burl!ulysses!ucbvax!space From: barnes@INFINET.UUCP (Jim Barnes) Newsgroups: net.space Subject: Re: nearby supernovas etc. Message-ID: <8603061510.AA04282@infinet.UUCP> Date: Thu, 6-Mar-86 10:10:05 EST Article-I.D.: infinet.8603061510.AA04282 Posted: Thu Mar 6 10:10:05 1986 Date-Received: Sat, 8-Mar-86 05:01:46 EST References: <8603020306.AA00249@s1-b.arpa> Sender: daemon@ucbvax.BERKELEY.EDU Organization: Infinet, Inc. Lines: 23 In article <8603020306.AA00249@s1-b.arpa> you write: >By the way, in latest Sky&Telescope there's a note on Sirius being >reddish in recorded history (in fact about 600 AD), because at that >time its white-dwarf companion was in the red giant stage. It's hard >to believe the conversion from red giant to white dwarf could occur so >quickly, although with Sirius gobbling most of the loose hydrogen as >fast as it is shed, and ionizing & light-pressure-shoving the rest of >the emitted hydrogen, I could imagine it within the realm of >possibility. Any news since S&T publishing date on that topic that you >know of? > I recently (two months ago?) read an article in the Boston Globe that said roughly the same thing - Sirius was reddish within recorded history. I posted the same question to net.astro. The general response received was that the redness was due to the time of day when the observations were made. ie. Sirius sets near the sun during the dog days of the summer, hence the reddish color is due to the sunset, not the color of the star. Current theories of stellar evolution do not allow for a star to evolve that rapidly. ------------------------- decvax!wanginst!infinet!barnes Jim Barnes