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<td>Physics Colloquium Friday, February 14, 2014</td>
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<th nowrap="nowrap" valign="BASELINE" align="RIGHT">Date: </th>
<td>Mon, 10 Feb 2014 16:23:43 +0000</td>
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<th nowrap="nowrap" valign="BASELINE" align="RIGHT">From: </th>
<td>Wilkinson, Eleonor V <a class="moz-txt-link-rfc2396E" href="mailto:evwilk@wm.edu"><evwilk@wm.edu></a></td>
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<th nowrap="nowrap" valign="BASELINE" align="RIGHT">To: </th>
<td>'<a class="moz-txt-link-abbreviated" href="mailto:physics0607@physics.wm.edu">physics0607@physics.wm.edu</a>'
<a class="moz-txt-link-rfc2396E" href="mailto:physics0607@physics.wm.edu"><physics0607@physics.wm.edu></a></td>
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<p class="MsoNormal"><b><u><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black">PHYSICS
COLLOQUIUM</span></u></b><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black">Friday, February
14, 2014</span><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black">4:00 PM
</span><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black">Small Hall, Room
111</span><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black"> </span><o:p></o:p></p>
<p class="MsoNormal"><b><span
style="font-size:14.0pt;font-family:"Times New
Roman","serif";color:black">Dr. D. Chris
Benner
</span></b><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:14.0pt;font-family:"Times New
Roman","serif";color:black">College of
William & Mary<o:p></o:p></span></p>
<p class="MsoNormal"><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black"> </span><o:p></o:p></p>
<p class="MsoNormal"><b><span
style="font-size:14.0pt;font-family:"Times New
Roman","serif";color:black">Title of Talk:</span></b><o:p></o:p></p>
<p class="MsoNormal"><i><span
style="font-size:14.0pt;font-family:"Times New
Roman","serif";color:black">“Methane in the
Outer Solar System: A Century and a Half Later”</span></i><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black"> </span><o:p></o:p></p>
<p class="MsoNormal"><b><span
style="font-size:14.0pt;font-family:"Times New
Roman","serif";color:black">Abstract:</span></b><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black">In 1802 Wollaston
first saw the solar spectral lines that Fraunhofer
rediscovered in 1814. By the 1860s strong spectral
features, later found to be due to methane, were found to
dominate the spectra of all of the atmospheres of the outer
solar system. There has followed a century and a half of
efforts to first identify, then quantify these spectral
bands which are essential to the study of the energy
transfer, structure and chemical composition of the
atmospheres. The bands in the visible and near infrared
regions are so complex and the outer solar system physical
conditions so extreme that it was thought that proper
laboratory study was still at least decades away. However,
a combination of the intracavity laser spectrometer of the
University of Missouri at St. Louis and the College of
William and Mary multispectrum nonlinear least squares
spectrum fitting technique have determined the basic
measurements for the 890 nm band. It is now possible to
properly model an outer solar system atmosphere in this
band.
<a moz-do-not-send="true"
href="https://events.wm.edu/event/view/physics/35290">https://events.wm.edu/event/view/physics/35290</a>
<o:p></o:p></span></p>
<p class="MsoNormal"><b><i><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black"><o:p> </o:p></span></i></b></p>
<p class="MsoNormal"><b><i><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black"><o:p> </o:p></span></i></b></p>
<p class="MsoNormal"><b><i><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black">*Refreshments
will be served in Room 122 at 3:30 PM</span></i></b><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black"> </span><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black"> </span><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black"> </span><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black"> </span><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black">Thanks,</span><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:12.0pt;font-family:"Times New
Roman","serif";color:black">Elle</span><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:10.0pt;font-family:"Times New
Roman","serif";color:black"> </span><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:10.0pt;font-family:"Times New
Roman","serif";color:black">******</span><o:p></o:p></p>
<p class="MsoNormal"><b><span
style="font-size:12.0pt;font-family:"Monotype
Corsiva";color:#1F497D">Eleonor V. Wilkinson</span></b><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:9.0pt;font-family:"Georgia","serif"">Administrative
& Office Specialist
</span><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:9.0pt;font-family:"Georgia","serif"">The
College of William & Mary-Physics<br>
Small Hall, Room 123<br>
300 Ukrop Way<br>
Williamsburg, VA 23185</span><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:9.0pt;font-family:"Times New
Roman","serif";color:black">Telephone:
757-221-3503</span><o:p></o:p></p>
<p class="MsoNormal"><span
style="font-size:9.0pt;font-family:"Times New
Roman","serif";color:black">Fax: 757-221-3540</span><o:p></o:p></p>
<p class="MsoPlainText"> <o:p></o:p></p>
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