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Hey folks-- just a note; I have started writing a regular column for Astronomy Magazine's website. The first one is online:
Everything's Under the Sun. The column is monthly, and the second one is already done (for November) and the third is being checked by my crack team of editors (actually, my wife). |
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Oh, so now you're a Contributing Editor? [img]/phpBB/images/smiles/icon_wink.gif[/img] Congradulations on the new column. BTW, I don't remember off the top of my head, but what happened with your deal with the German Magazine?
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"You can't convince a believer of anything; for their belief is not based on evidence, it's based on a deep seated need to believe." [Carl Sagan] |
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------ [img]/phpBB/images/smiles/icon_biggrin.gif[/img] THE FOLLOWING POST IS A JOKE [img]/phpBB/images/smiles/icon_razz.gif[/img] -------
Well well well, if it isn't mister big shot astronomer getting YET ANOTHER source of income! [img]/phpBB/images/smiles/icon_razz.gif[/img] [img]/phpBB/images/smiles/icon_biggrin.gif[/img] Just like movie stars, pro-athletes and rock stars, scientists can never get enough of anything! [img]/phpBB/images/smiles/icon_smile.gif[/img] [img]/phpBB/images/smiles/icon_razz.gif[/img] [img]/phpBB/images/smiles/icon_razz.gif[/img] [img]/phpBB/images/smiles/icon_biggrin.gif[/img] Congratulations! And may your new found source of revenues bring you many a new possessions which in turn will bring you joy! [img]/phpBB/images/smiles/icon_smile.gif[/img] [img]/phpBB/images/smiles/icon_razz.gif[/img] [img]/phpBB/images/smiles/icon_razz.gif[/img] [img]/phpBB/images/smiles/icon_biggrin.gif[/img] Joking! Come on! Where's your sense of humor! |
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Bad Astronomer:
That is a great article! I have saved the site. I subscribe to a number of science journals and magazines and have always liked Astronomy magazine (to which I subscribe), because it handles such a variety of topics in astrophysics and cosmology, as well as the expected astronomy topics. I am well acquainted with many of the writers from other sources, to which I also subscribe, such as SCIENCE. ljbrs [img]/phpBB/images/smiles/icon_biggrin.gif[/img] [img]/phpBB/images/smiles/icon_biggrin.gif[/img] [img]/phpBB/images/smiles/icon_biggrin.gif[/img] |
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I suppose it all comes down to definition. Most non-astronomers would compare our Sun against the stars that are visible with the naked eye. Given that as a criteria our Sun looses it "A" grade (unless of course we assume the unique perspective of planet Earth).
Jeff |
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Heh. Actually, I didn't even think to mention that the Sun is solitary and not part of a multiple system, nor did I think about the high metallicity. Figures. Well, I can't think of everything. [img]/phpBB/images/smiles/icon_wink.gif[/img]
Thanks for the comments, folks. |
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...And that, my liege, is how we know the Earth to be banana-shaped. --Sir Bedevere |
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Or was this just another pad-post? [img]/phpBB/images/smiles/icon_smile.gif[/img] |
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Good article. I've always appreciated Astronomy Magazine. Some years ago I joined a literary "festival" promoted by them, about the tension "Science vs Religion", sending a 1000 word article. It was a nice gesture from them. Harboring the reader's points of view is something that indicates a high level of concern and professionalism. From that moment on Astronomy became my most cherished "light" astronomy magazine. I Wish you success!
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BA,
I was under the impression that brown dwarfs were massive enough to fuse deuterium but not massive enough to fuse hydrogen and that red dwarfs were the smallest stars that "burn" hydrogen.
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Any day you wake up on "the right side of the dirt" is a good day. T. Anderson |
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All *Main Sequence* stars are *dwarf* stars, including our Sun (Sol). Now a *White Dwarf* star is different from an ordinary *Main Sequence* dwarf star and is, instead, a compact star at the end of its evolutionary cycle and definitely not on the Main Sequence. White Dwart stars are extremely compact and must be under 1.44 Solar Masses (the *Chandrasekhar Limit* for White Dwarf stars). The Sun will eventually become a White Dwarf star. Before that time, it will leave the Main Sequence and go through the Red Giant stage, shedding its outer layers in a complicated process before it eventually collapses into a compact White Dwarf star. This evolutionary period will not occur for approximately 5 billion years, so do not hold your breath in anticipation...
ljbrs [img]/phpBB/images/smiles/icon_biggrin.gif[/img] <font size=-1>[ This Message was edited by: ljbrs on 2001-10-27 19:50 ]</font> |
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20011028 12:46 A.M. PST (yep) HUb' "LEFT:"
On 2001-10-26 11:35, wrote: Everythings Under the Sun (p1 __________________________________________________ _______________ WARNING: The page you have accessed is dependent on JAVASCRIPT which is not supported by your browser. Due to this limitation, you may experience unexpected results within this site. __________________________________________________ _______________ [INLINE] [1][LINK] [2][USEMAP] [INLINE] [INLINE] [3][LINK] |
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Rich as opposed to how much is in the Earth? Yes, probably. The spectral lines tell us that much. But rich in comparison to the overall sun? Not at all. H and He outmoles heavier elements by many orders of magnitude. The heavier elements you're thinking of were created in supergiants, so all the non-H and non-He in our solar system came from some long deceased star. (Our sun has no where near the mass needed to fuse Helium into Carbon when its Hydrogen fuel runs out in 5 billion years or so.) |