<?xml version="1.0" encoding="ISO-8859-1"?>

<HSTProposal
   Phase1ID="703"
   Phase2ID="10940"
   Phase="Phase I"
   AptVersion="Version 15.0 ">
   <!--**********************************************************************************************************************-->
   <!--This file is automatically generated and should not be edited by hand. Editing this file directly is at your own risk.-->
   <!--**********************************************************************************************************************-->
   
   <ToolData>
      
      <ToolDataItem
         Key="SubmissionData">
         
         <SubmissionData
            AptVersion="Version 15.0 "
            SubmissionCounter="1"
            SubmissionSuccessCounter="0"
            HasErrors="false"
            Cycle="15"
            IncludeSysInfo="true"
            NotificationAddress="buie@lowell.edu"
            AssignedID="703">
            
            <SystemInformation
               os.arch="i386"
               os.name="Linux"
               os.version="2.4.24-emp_2424sw"
               java.version="1.4.2_06"
               linux.distribution="SuSE"
               linux.version="9.0 " />
            
            <SubmissionComments />
            
            <SubmissionLog>  Assigned ID: 703
----- Submission 1 (Sat Jan 28 00:57:35 GMT 2006) -----
</SubmissionLog>
            
            <DiagnosticJustification />
         </SubmissionData>
      </ToolDataItem>
   </ToolData>
   
   <ProposalInformation
      Category="AR"
      PureParallelProposal="false"
      Cycle="15">
      
      <Title>Constraints on the Formation and Evolution of the Pluto System</Title>
      
      <Abstract>We propose a detailed program of analysis based on archival HST data
and mutual event photometry to address several goals related to the
Pluto system.  A new analysis of HST images of Pluto from 1992 and
1993 should reveal the two new satellites recently discovered, with
the longer temporal baseline greatly improving their orbital periods.
Application of the new Pluto surface maps derived from HST data obtained
in 2002 and 2003 to the astrometry extracted from the HST images from
1992 and 1993 will remove the center-of-light to center-of-body offset,
thereby improving the orbit of Charon, especially after being combined
with the more recent astrometry.  With these new constraints on the orbit
of Charon and the new stellar occultation constraint on the radius
of Charon, we intend to derive a new radius for Pluto by imposing these
values on the mutual event photometry.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Marc"
         MiddleInitial="W."
         LastName="Buie"
         ESAMember="false"
         UniqueID="286"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="Lowell Observatory"
            USState="AZ"
            Country="USA" />
      </PrincipalInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="William"
         MiddleInitial="M."
         LastName="Grundy"
         ESAMember="false"
         UniqueID="4452"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="Lowell Observatory"
            USState="AZ"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="David"
         LastName="Tholen"
         ESAMember="false"
         UniqueID="2565"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="University of Hawaii"
            USState="HI"
            Country="USA" />
      </CoInvestigator>
      
      <Questions>
         
         <Phase2Questions>
            
            <ObservingDescription />
            
            <RealtimeJustification />
            
            <CalibrationJustification />
            
            <AdditionalComments />
         </Phase2Questions>
      </Questions>
      
      <Orbits
         ThisCycle2GyroPrimary="1"
         ThisCycle2GyroParallel="0"
         NextCycle2GyroPrimary="0"
         NextCycle2GyroParallel="0"
         AfterNext2GyroPrimary="0"
         AfterNext2GyroParallel="0" />
      
      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="/home/buie/cycle15/ar.pdf">
         
         <ScientificCategory>SOLAR SYSTEM</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="ASTROMETRY" />
         
         <ScientificKeyword2
            Keyword="KUIPER BELT OBJECTS" />
         
         <ScientificKeyword3
            Keyword="PLANETARY SATELLITES" />
         
         <ScientificKeyword4
            Keyword="SURFACES OF PLANETS/MOONS/OTHER" />
         
         <ScientificKeyword5
            Keyword="SUPPORT OF NASA PLANETARY MISSIONS" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <Budget>110000</Budget>
         
         <CalibProp>false</CalibProp>
         
         <SpitzerHours>0.0</SpitzerHours>
         
         <SpitzerLarge>false</SpitzerLarge>
         
         <Treasury>false</Treasury>
         
         <Legacy>false</Legacy>
         
         <Theory>false</Theory>
         
         <LargeProgram>false</LargeProgram>
      </Phase1ProposalInformation>
      
      <Phase2ProposalInformation
         PCFlag="false">
         
         <Availability>SUPPORTED</Availability>
      </Phase2ProposalInformation>
   </ProposalInformation>
   
   <Targets />
   
   <Observations />
   
   <Patterns />
   
   <Visits />
</HSTProposal>


