Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.1 6/24/83; site utastro.UUCP Path: utzoo!watmath!clyde!burl!ulysses!mhuxl!ihnp4!zehntel!hplabs!hao!seismo!ut-sally!utastro!dipper From: dipper@utastro.UUCP (Debbie Byrd) Newsgroups: ut.stardate,net.astro Subject: Stardate jul 18 Message-ID: <238@utastro.UUCP> Date: Wed, 25-Jul-84 02:00:23 EDT Article-I.D.: utastro.238 Posted: Wed Jul 25 02:00:23 1984 Date-Received: Sat, 21-Jul-84 04:22:58 EDT Organization: UTexas Astronomy Dept., Austin, Texas Lines: 43 Early morning risers can look for a star whose name means Wonderful. More on Mira -- in a moment. July 18 Mira's Maximum A few hours before dawn the constellation Cetus the Whale rises above the eastern horizon -- to be visible in the southeast. Cetus is not an especially prominent constellation -- but it contains a star known as Mira -- which is Latin for Wonderful Star. Mira earned this name because it was the first variable star discovered. Variable stars are stars that change in brightness. Sometimes Mira is bright enough to be seen with the naked eye -- and at other times it dims into invisibility. In the year 1596, an astronomer plotted the location of Mira while making a map of the stars. He must have been surprised when Mira disappeared from view. But Mira returned to visibility again -- it always does. Many different types of variable stars are now known to exist. Some brighten and fade with great regularity -- others are a little irregular -- like Mira, which has a cycle of about eleven months. Mira sometimes reaches maximum brightness a little ahead of schedule -- and it's sometimes a little brighter than usual. That was the case last year -- Mira at maximum was a little on the bright side. This year it just so happens that Mira's maximum brightness occurred about mid-June -- when the star was on the other side of the sun from the Earth and hidden in the sun's glare. Mira has now come out of the sun and may be in the predawn sky. The star is now on the down side of its cycle -- getting dimmer -- but possibly still visible to the naked eye. The only way to know for sure is to take a look. (Sky chart??) Script by Diana Hadley and Deborah Byrd. (Conversation with Janet Mattei, AAVSO, 4-5-84) (c) Copyright 1983, 1984 McDonald Observatory, University of Texas at Austin