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	<title>Comments on: Star found, older than Abe Vigoda</title>
	<atom:link href="http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/feed/" rel="self" type="application/rss+xml" />
	<link>http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/</link>
	<description>I am an astronomer, writer, and skeptic. I likes reality the way it is, and I aims to keep it that way. My real name is Phil Plait, and I run the Bad Astronomy blog.</description>
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		<title>By: Sweet Yummy Reality</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/comment-page-1/#comment-36099</link>
		<dc:creator>Sweet Yummy Reality</dc:creator>
		<pubDate>Mon, 21 Apr 2008 21:21:57 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/#comment-36099</guid>
		<description>[...] important about it. Since Phil Plait over at BadAstronomy has already boiled down the science, I&#8217;ll just link to his post.      No Comments so far      Leave a comment Line and paragraph breaks automatic, e-mail address [...]</description>
		<content:encoded><![CDATA[<p>[...] important about it. Since Phil Plait over at BadAstronomy has already boiled down the science, I&#8217;ll just link to his post.      No Comments so far      Leave a comment Line and paragraph breaks automatic, e-mail address [...]</p>
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		<title>By: Brian</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/comment-page-1/#comment-36098</link>
		<dc:creator>Brian</dc:creator>
		<pubDate>Sun, 13 May 2007 21:35:15 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/#comment-36098</guid>
		<description>Lab Lemming,

Thank you again.</description>
		<content:encoded><![CDATA[<p>Lab Lemming,</p>
<p>Thank you again.</p>
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		<title>By: Lab Lemming</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/comment-page-1/#comment-36097</link>
		<dc:creator>Lab Lemming</dc:creator>
		<pubDate>Sun, 13 May 2007 21:12:13 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/#comment-36097</guid>
		<description>Brian:
Evidently one of the biggest problems is that the best U peak overlaps the C-N peak.  So you need either very low C,N stars, or hot stars (to break the molecular bond).  But of course, hot stars have shorter life expectancy. As a result, I think the two stars that they looked at are giant branch stars- they are not main sequence red dwarves.</description>
		<content:encoded><![CDATA[<p>Brian:<br />
Evidently one of the biggest problems is that the best U peak overlaps the C-N peak.  So you need either very low C,N stars, or hot stars (to break the molecular bond).  But of course, hot stars have shorter life expectancy. As a result, I think the two stars that they looked at are giant branch stars- they are not main sequence red dwarves.</p>
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		<title>By: Brian</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/comment-page-1/#comment-36096</link>
		<dc:creator>Brian</dc:creator>
		<pubDate>Sun, 13 May 2007 18:20:27 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/#comment-36096</guid>
		<description>Lab Lemming,

Thanx.  A lot of that was in accord with my suppositions.  I had not considered the possibility of her using more than 1 model, although it now seems obviously proper technique to consider several.  I had wondered why no one mentioned the lead.

It must be quite difficult to find suitable candidates for this sort of analysis.</description>
		<content:encoded><![CDATA[<p>Lab Lemming,</p>
<p>Thanx.  A lot of that was in accord with my suppositions.  I had not considered the possibility of her using more than 1 model, although it now seems obviously proper technique to consider several.  I had wondered why no one mentioned the lead.</p>
<p>It must be quite difficult to find suitable candidates for this sort of analysis.</p>
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		<title>By: Lab Lemming</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/comment-page-1/#comment-36095</link>
		<dc:creator>Lab Lemming</dc:creator>
		<pubDate>Sun, 13 May 2007 04:40:40 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/#comment-36095</guid>
		<description>Found the paper at arxiv, I&#039;ll blog it once my conference talk is done.

Basically-
1. assume initial Eu, Ir, Os, Th, U ratios at production (she uses 4 or 5 different models)
2. Assume star forms immediatly after heavy elements are produced (this is what happened in our system- why not extrapolate to the universe)
3. Assume the difference between measured and expected U and Th is due to radioactive decay
4. use decay constants to determine age.

She does all this, and ends up with an answer of 13.2 +/- 2.5 Ga.

Most of the error seems to be from the initial composition assumptions adn disagreement between the stable Os, Ir, or Eu, and not the analysis.

The decay product of Th and U, Pb, cannot be measured, as there is a spectral interference.</description>
		<content:encoded><![CDATA[<p>Found the paper at arxiv, I&#8217;ll blog it once my conference talk is done.</p>
<p>Basically-<br />
1. assume initial Eu, Ir, Os, Th, U ratios at production (she uses 4 or 5 different models)<br />
2. Assume star forms immediatly after heavy elements are produced (this is what happened in our system- why not extrapolate to the universe)<br />
3. Assume the difference between measured and expected U and Th is due to radioactive decay<br />
4. use decay constants to determine age.</p>
<p>She does all this, and ends up with an answer of 13.2 +/- 2.5 Ga.</p>
<p>Most of the error seems to be from the initial composition assumptions adn disagreement between the stable Os, Ir, or Eu, and not the analysis.</p>
<p>The decay product of Th and U, Pb, cannot be measured, as there is a spectral interference.</p>
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		<title>By: Brian</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/comment-page-1/#comment-36094</link>
		<dc:creator>Brian</dc:creator>
		<pubDate>Sun, 13 May 2007 04:07:07 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/#comment-36094</guid>
		<description>OK, one more try.
http://www.nature.com/news/2007/070508/pf/070508-13_pf.html</description>
		<content:encoded><![CDATA[<p>OK, one more try.<br />
<a href="http://www.nature.com/news/2007/070508/pf/070508-13_pf.html" rel="nofollow">http://www.nature.com/news/2007/070508/pf/070508-13_pf.html</a></p>
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		<title>By: Brian</title>
		<link>http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/comment-page-1/#comment-36093</link>
		<dc:creator>Brian</dc:creator>
		<pubDate>Sun, 13 May 2007 03:59:22 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/badastronomy/2007/05/11/star-found-older-than-abe-vigoda/#comment-36093</guid>
		<description>I see the computer printed news@nature.com as an email address, but to access the article, go to www.nature.com/news/2007/070508.  There is more to the address, but that should get you somewhat close.</description>
		<content:encoded><![CDATA[<p>I see the computer printed <a href="mailto:news@nature.com">news@nature.com</a> as an email address, but to access the article, go to <a href="http://www.nature.com/news/2007/070508" rel="nofollow">http://www.nature.com/news/2007/070508</a>.  There is more to the address, but that should get you somewhat close.</p>
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