Return-Path: richmond@a188-l009.rit.edu Delivery-Date: Thu Apr 27 14:31:13 2000 Return-Path: Received: from filer2.isc.rit.edu (filer2.isc.rit.edu [129.21.2.226]) by a188-l009.rit.edu (8.8.7/8.8.7) with ESMTP id OAA21442 for ; Thu, 27 Apr 2000 14:31:13 -0400 Received: from osfmail.isc.rit.edu by osfmail.isc.rit.edu (PMDF V5.2-32 #41785) id <0FTO00701U3S5B@osfmail.isc.rit.edu> for richmond@a188-l009.rit.edu (ORCPT rfc822;mwrsps@rit.edu); Thu, 27 Apr 2000 14:31:04 -0400 (EDT) Received: from vms3.isc.rit.edu ("port 3383"@[129.21.3.10]) by osfmail.isc.rit.edu (PMDF V5.2-32 #41785) with ESMTP id <0FTO00A38U3OO1@osfmail.isc.rit.edu> for mwrsps@osfmail.isc.rit.edu (ORCPT rfc822;mwrsps@rit.edu); Thu, 27 Apr 2000 14:31:04 -0400 (EDT) Received: from ritvax.isc.rit.edu by ritvax.isc.rit.edu (PMDF V5.2-32 #41784) id <01JOQFEH3QG2HNJ6GE@ritvax.isc.rit.edu> for mwrsps@grace.rit.edu (ORCPT rfc822;mwrsps@rit.edu); Thu, 27 Apr 2000 14:31:05 -0400 (EDT) Received: from a188-l009.rit.edu ([129.21.188.9]) by ritvax.isc.rit.edu (PMDF V5.2-32 #41784) with ESMTP id <01JOQFEFJ8UYHG204U@ritvax.isc.rit.edu> for mwrsps@ritvax.isc.rit.edu (ORCPT rfc822;mwrsps@rit.edu); Thu, 27 Apr 2000 14:31:04 -0400 (EDT) Received: from a188-l009.rit.edu (richmond@localhost [127.0.0.1]) by a188-l009.rit.edu (8.8.7/8.8.7) with ESMTP id OAA21429; Thu, 27 Apr 2000 14:30:58 -0400 Date: Thu, 27 Apr 2000 14:30:58 -0400 From: Stupendous Man Subject: Re: questions about supernovae To: "Lauren C." Cc: mwrsps@ritvax.isc.rit.edu Message-id: <200004271830.OAA21429@a188-l009.rit.edu> X-VMS-To: IN%"muse@lightlink.com" "Lauren C." X-VMS-Cc: IN%"mwrsps@ritvax.isc.rit.edu" MIME-version: 1.0 X-Mailer: exmh version 2.0.2 Content-type: TEXT/PLAIN; CHARSET=US-ASCII Content-transfer-encoding: 7BIT Lauren, Some of the questions you ask can be answered by reading material at the following sites: Lots of pictures of recent supernovae: http://www.ggw.org/asras/supernova.html Effects of a supernova on life on nearby planets: http://a188-L009.rit.edu/richmond/answers/snrisks.txt > ok, 1) what is a supernova A star which explodes. There are two main mechanisms which can cause a star to explode: a. one type of star is called a "white dwarf" -- it is very small (only about the size of the Earth) and very dense. If a companion star dumps lots of material onto a white dwarf, so that the mass of the white dwarf grows bigger than a certain limit, then nuclear reactions occur inside the white dwarf and blow it apart (like a giant thermonuclear bomb) b. very massive stars -- more than 10 times the mass of our Sun -- build up big cores of iron at their centers. When such a star runs out of fuel, the core of iron collapses on itself, shrinking in a few seconds to a tiny ball, only ten miles or so across. This ball is made of neutrons. The ball rebounds a bit just after it forms, and sends a shock wave outwards through the star, which shoves all the outer layers into space. > 2) what are the effects while it is happening if there are any In brief, the star becomes very hot (over 100,000 degrees), and starts expanding at 3,000 to 10,000 kilometers per second. It emits lots of radiation: X-rays, UV, visible light, infrared, and radio waves. > 3) what are the effects after it happens There's a big shell of gas expanding at high speed away from where the star used to be. In the second type of supernova, there may be a neutron star left over at the center of the explosion; or there may be a black hole; or there may be nothing. > 4) are there any warning signs to a supernova Not really. In the second type of supernova, it takes a few hours after the collapse of the core for the shock wave to reach the surface of the star. It is possible to detect particles called neutrinos, produced at the moment of the collapse, during this period of a few hours, and so gain a VERY SHORT advance notice. But it wouldn't be enough to run away successfully. > 5)how is the space around the explosion effected It is filled with lots of radiation, and eventually gas from the outer layers of the star pass through it. > 6)why have there only been 3 supernovas in our galaxy? Um, there have been more than that observed in our galaxy. Read http://a188-L009.rit.edu/richmond/answers/historical.html or a book called "The Historical Supernovae", by Clark and Stephenson. > 7) why is it more common in others Huh? I don't undestand this question. > 8) what are supernova rements? "Remnants" are whatever is left over after a supernova occurs. In some cases, there may be a neutron star or black hole at the center of the explosion. In all cases, there is a big mass of hot gas expanding outwards at high speeds. We can detect the hot gas for several tens of thousands of years after the explosion. > 9) how long do the rements stay Well, we can detect remnants in our own galaxy which are many thousands of years old. But when we look at other galaxies, the remnants are so distant that they disappear from our view after a few decades or so. > 10) could you tell me about the diffrence between type1 and type2 > supernovas See the answer to question 1. The first class of explosions, due to white dwarfs which accrete too much extra material, are called "Type Ia" supernovae. The second class of explosions, in which a massive star runs out of fuel and its core collapses, are called "Type II" supernovae. You can find a fuller description of the types of supernovae at http://a188-l009.rit.edu/richmond/answers/sntypes.txt > thanks a bunch its a real help You are welcome. -- ----- Michael Richmond "This is the heart that broke my finger." mwrsps@rit.edu http://stupendous.rit.edu/richmond/