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Severe Geomagnetic Storm Intervals in History And Future Prospects
http://www.spacew.com/swim/bigstorm.html http://www.spacew.com/swim/ssn-kp8.jpg |
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DON'T tell Charles Cagle about this!!!!!!!!!!
Clear, Dark, Steady Skies! (And considerate neighbors!!!) |
#4
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Would you include "supernova" as an "extreme storm"?
---JRC--- "Vincent van der Laan" wrote in message = ... =20 Just wondering: is it possible (in theory) that an extreme storm might = be severe enough to blow away our atmosphere? =20 Scary thought... (might want to move to Mars ![]() |
#5
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On 28-10-2003 23:53, in article ,
"John R. Copeland" wrote: Would you include "supernova" as an "extreme storm"? ---JRC--- I would, but the sun is too smal to go nova. It will first become a red giant and then it will slowly contract and cool down. |
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But Sirius IS big enough, AND it's big enough, AND it will go off someday.
Then we may just be toast. "Vincent van der Laan" wrote in message ... On 28-10-2003 23:53, in article , "John R. Copeland" wrote: Would you include "supernova" as an "extreme storm"? ---JRC--- I would, but the sun is too smal to go nova. It will first become a red giant and then it will slowly contract and cool down. -----= Posted via Newsfeeds.Com, Uncensored Usenet News =----- http://www.newsfeeds.com - The #1 Newsgroup Service in the World! -----== Over 100,000 Newsgroups - 19 Different Servers! =----- |
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To reply, remove the "z" if one appears in my address "Bob Greschke" wrote in message ... But Sirius IS big enough, AND it's big enough, AND it will go off someday. Then we may just be toast. I don't think any of US have anything to worry about... "Vincent van der Laan" wrote in message ... On 28-10-2003 23:53, in article , "John R. Copeland" wrote: Would you include "supernova" as an "extreme storm"? ---JRC--- I would, but the sun is too smal to go nova. It will first become a red giant and then it will slowly contract and cool down. -----= Posted via Newsfeeds.Com, Uncensored Usenet News =----- http://www.newsfeeds.com - The #1 Newsgroup Service in the World! -----== Over 100,000 Newsgroups - 19 Different Servers! =----- |
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Bob Greschke wrote:
But Sirius IS big enough, AND it's big enough, AND it will go off someday. Then we may just be toast. Sirius A is only 2.3 solar masses and will not go supernova. Instead it will become a red giant, but does not orbit close enough to its companion, Sirius B, a white dwarf to for gas to fall onto the little bugger and create a Type Ia supernova. Sirius A will eventually become a white dwarf like its companion that preceded it. This is what will happen to our sun too. |
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![]() "Bob Greschke" wrote in message ... But Sirius IS big enough, AND it's big enough, AND it will go off someday. Then we may just be toast. Sirius "A" IS one of the closest of stars to our own Sun (Sirius is a bit over 8 light-years away), but it's not large enough to go supernova. If current theories of stellar evolution hold, when Sirius has exhausted its nuclear fuel, it will eventually expand to a red giant phase (like our own Sun will) and eventually cool down to a white dwarf star. The type of supernova that many giant hot stars may experience is the Type II, which is the result of the collapse of the great star's core. Our own Sun is neither hot enough nor large enough to experience such a core collapse, and while Sirius *is* hotter than our Sun, it's not large enough to go Type II supernova (core collapse supernovae are reserved for the largest, hottest and most unstable stars). However, there is another type of supernova, the type IIa. These take the scenario of a duo of stars in which both companions revolve close to one another and one is larger than the other-- the typical scenario here is a red giant star and a close white dwarf companion. The small white dwarf star has a huge amount of matter compressed within its small sphere; the red giant companion is also massive, but its huge outer atmosphere is relatively sparse and has become massive via its expansion. If the two stars are close enough to each other, the smaller and more massive of the two can pull some of the atmosphere off the larger star. At a certain point (the Chandrasekhar limit, or approx. 1.3-1.4 solar masses) the small star cannot hold any more mass, and the 'borrowed' mass of its companion beyond that critical point ignites a thermonuclear reaction. Insofar as I know, Sirius's white dwarf companion star, the "Pup", orbits too far away from Sirius to cause the type 11a supernova. Jackie |
#10
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On Tue, 28 Oct 2003 23:30:23 +0100, Vincent van der Laan
wrote: On 28-10-2003 22:16, in article , "Sam Wormley" wrote: Severe Geomagnetic Storm Intervals in History And Future Prospects http://www.spacew.com/swim/bigstorm.html http://www.spacew.com/swim/ssn-kp8.jpg Just wondering: is it possible (in theory) that an extreme storm might be severe enough to blow away our atmosphere? Scary thought... (might want to move to Mars ![]() It's called a nova, and Mars wouldn't be far enough. Happy trails, Gary (net.yogi.bear) ------------------------------------------------ at the 51st percentile of ursine intelligence Gary D. Schwartz, Needham, MA, USA Please reply to: garyDOTschwartzATpoboxDOTcom |
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