<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>0185-1101</journal-id>
<journal-title><![CDATA[Revista mexicana de astronomía y astrofísica]]></journal-title>
<abbrev-journal-title><![CDATA[Rev. mex. astron. astrofis]]></abbrev-journal-title>
<issn>0185-1101</issn>
<publisher>
<publisher-name><![CDATA[Universidad Nacional Autónoma de México, Instituto de Astronomía]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0185-11012015000200011</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Do comets C/1861 G1 (Thatcher) and C/1861 J1 (Great Comet) have a common origin?]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Branham]]></surname>
<given-names><![CDATA[Richard L.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Instituto Argentino de Nivología, Glaciología y Ciencias Ambientales  ]]></institution>
<addr-line><![CDATA[Mendoza ]]></addr-line>
<country>Argentina</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>00</month>
<year>2015</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>00</month>
<year>2015</year>
</pub-date>
<volume>51</volume>
<numero>2</numero>
<fpage>245</fpage>
<lpage>251</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0185-11012015000200011&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0185-11012015000200011&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0185-11012015000200011&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="es"><p><![CDATA[Con el objeto de mejorar la órbita de Oppolzer de 1864, se calcula una nueva órbita para el Cometa C/1861 G1 (Thatcher), el cual está asociado a la lluvia de estrellas de las Líridas. La nueva órbita se basa en 649 observaciones hechas entre el 11 de abril y el 7 de septiembre de 1861, 326 en ascensión recta y 323 en declinación. La órbita final utiliza los residuos calculados con la función de ponderación de Welsch. El período del cometa, 416 ± 0.56 años, concuerda con el de Oppolzer, 415 años, pero otros elementos orbitales, como la inclinación, discrepan. Si bien los residuos post-perihelio se presentan relativamente al azar, con una probabilidad del 52.1% de serlo, los residuos pre-perihelio no son azarosos, lo cual indica posibles desviaciones del movimiento kepleriano debidas a la expulsión de material meteorítico. El Cometa Thatcher no está relacionado con el Gran Cometa de 1861.]]></p></abstract>
<abstract abstract-type="short" xml:lang="en"><p><![CDATA[A new orbit is calculated for Comet C/1861 G1 (Thatcher), associated with the Lyrid meteor shower, to replace Oppolzer's orbit of 1864. The new orbit is based upon 649 observations, 326 in right ascension and 323 in declination, made between 11 April 1861 and 7 Sept. 1861. The final orbit uses residuals calculated with the Welsch weighting function. The comet's period of 416.87 ± 0.56 yr agrees with Oppolzer's period of 415 yr athough other elements such as the inclination differ. Although the post-perihelion residuals are relatively random, 52.1% probability of randomness, pre-perihelion residuals lack randomness indicating possible deviations from Keplerian motion caused by ejection of meteoritic material. Comet Thatcher is unrelated to the Great comet of 1861.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[celestial mechanics]]></kwd>
<kwd lng="en"><![CDATA[comets]]></kwd>
<kwd lng="en"><![CDATA[methods]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[  	    <p align="center"><font face="verdana" size="4"><b>Do comets C/1861 G1 (Thatcher) and C/1861 J1 (Great Comet) have a common origin?</b></font></p>  	    <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="center"><font face="verdana" size="2"><b>Richard L. Branham, Jr.</b></font></p>  	    <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="justify"><font face="verdana" size="2"><i>IANIGLA, C.C. 330, 5500 Mendoza, Argentina.</i> (<a href="mailto:rbranham@lab.cricyt.edu.ar">rbranham@lab.cricyt.edu.ar</a>).</font></p>  	    <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="justify"><font face="verdana" size="2">Received 2015 June 16.    <br> 	Accepted 2015 August 7.</font></p>  	    <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2"><b>RESUMEN</b></font></p>  	    <p align="justify"><font face="verdana" size="2">Con el objeto de mejorar la &oacute;rbita de Oppolzer de 1864, se calcula una nueva &oacute;rbita para el Cometa C/1861 G1 (Thatcher), el cual est&aacute; asociado a la lluvia de estrellas de las L&iacute;ridas. La nueva &oacute;rbita se basa en 649 observaciones hechas entre el 11 de abril y el 7 de septiembre de 1861, 326 en ascensi&oacute;n recta y 323 en declinaci&oacute;n. La &oacute;rbita final utiliza los residuos calculados con la funci&oacute;n de ponderaci&oacute;n de Welsch. El per&iacute;odo del cometa, 416 &plusmn; 0.56 a&ntilde;os, concuerda con el de Oppolzer, 415 a&ntilde;os, pero otros elementos orbitales, como la inclinaci&oacute;n, discrepan. Si bien los residuos post&#45;perihelio se presentan relativamente al azar, con una probabilidad del 52.1% de serlo, los residuos pre&#45;perihelio no son azarosos, lo cual indica posibles desviaciones del movimiento kepleriano debidas a la expulsi&oacute;n de material meteor&iacute;tico. El Cometa Thatcher no est&aacute; relacionado con el Gran Cometa de 1861.</font></p>  	    <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="justify"><font face="verdana" size="2"><b>ABSTRACT</b></font></p>  	    <p align="justify"><font face="verdana" size="2">A new orbit is calculated for Comet C/1861 G1 (Thatcher), associated with the Lyrid meteor shower, to replace Oppolzer's orbit of 1864. The new orbit is based upon 649 observations, 326 in right ascension and 323 in declination, made between 11 April 1861 and 7 Sept. 1861. The final orbit uses residuals calculated with the Welsch weighting function. The comet's period of 416.87 &plusmn; 0.56 yr agrees with Oppolzer's period of 415 yr athough other elements such as the inclination differ. Although the post&#45;perihelion residuals are relatively random, 52.1% probability of randomness, pre&#45;perihelion residuals lack randomness indicating possible deviations from Keplerian motion caused by ejection of meteoritic material. Comet Thatcher is unrelated to the Great comet of 1861.</font></p>  	    <p align="justify"><font face="verdana" size="2"><b>Key Words:</b> celestial mechanics &#151; comets: individual &#151; methods: data analysis.</font></p>  	    <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="justify"><font face="verdana" size="2"><a href="/pdf/rmaa/v51n2/v51n2a11.pdf" target="_blank">DESCARGAR ART&Iacute;CULO EN FORMATO PDF</a></font></p>  	    <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="justify"><font face="verdana" size="2"><b>REFERENCES</b></font></p>  	    ]]></body>
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