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

<HSTProposal
   Phase1ID="313"
   Phase2ID="10666"
   Phase="Phase I"
   AptVersion="Version 14.0 ">
   <!--**********************************************************************************************************************-->
   <!--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 14.0 "
            SubmissionCounter="1"
            SubmissionSuccessCounter="0"
            HasErrors="false"
            Cycle="14"
            IncludeSysInfo="true"
            NotificationAddress="cimpey@as.arizona.edu">
            
            <SystemInformation
               os.arch="x86"
               os.name="Windows 2000"
               os.version="5.0"
               java.version="1.4.1_03"
               linux.distribution="not available"
               linux.version="not available" />
            
            <SubmissionComments />
            
            <SubmissionLog>  Assigned ID: 313
----- Submission 1 (Fri Jan 21 19:40:47 GMT 2005) -----
</SubmissionLog>
            
            <DiagnosticJustification />
         </SubmissionData>
      </ToolDataItem>
   </ToolData>
   
   <ProposalInformation
      Category="AR"
      PureParallelProposal="false"
      Cycle="14">
      
      <Title>The ACS Mosaic of M51 and the Intersection of Research and Education</Title>
      
      <Abstract>This archive proposal is based on the opportunity afforded by the new six-pointing mosaic of M 51, taken as part of the Hubble Heritage project. The goal is to produce a set of educational activities for non-science majors taking introductory astronomy courses. In the first phase, the subject of this archive proposal, surface photometry and aperture photometry will be carried out for selected regions that are typical of (a) the nucleus, (b) the bulge, (c) an inner spiral arm, (d) an inter-arm region, (e) an outer spiral arm, (f) the nucleus of the companion, (g) an off-nuclear region in the companion, (h) the edge of the disk, (i) the tidal tail connecting the two galaxies, and (j) a region displaced from both galaxies. A fully registered true-color image will also be created. In the second phase, the subject of a companion E/PO proposal to be submitted later this year, instructional modules will be created based on the ten sample regions, where each can be viewed and measured by students using Java web tools. The goals of the activities will be to use research-level astronomical data to teach about (a) the range of stellar colors, (b) stellar luminosity, (c) different stellar populations, (d) effects of dust, (e) active nuclei, (f) the significance of angular resolution, and (g) the concept of surface brightness. The potential audience for these new materials is the 250,000 students who take introductory astronomy courses each year at colleges across the country.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Chris"
         LastName="Impey"
         ESAMember="false"
         UniqueID="1000">
         
         <Address
            Institution="University of Arizona"
            USState="AZ"
            Country="USA" />
      </PrincipalInvestigator>
      
      <Questions>
         
         <Phase2Questions>
            
            <ObservingDescription />
            
            <RealtimeJustification />
            
            <CalibrationJustification />
            
            <AdditionalComments />
         </Phase2Questions>
      </Questions>
      
      <Orbits
         ThisCyclePrimary="1"
         ThisCycleParallel="0"
         NextCyclePrimary="0"
         NextCycleParallel="0"
         AfterNextPrimary="0"
         AfterNextParallel="0"
         ThisCycle2GyroPrimary="0"
         ThisCycle2GyroParallel="0"
         NextCycle2GyroPrimary="0"
         NextCycle2GyroParallel="0"
         AfterNext2GyroPrimary="0"
         AfterNext2GyroParallel="0" />
      
      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="C:\Documents and Settings\Administrator\All Documents\Cathy's Stuff\HST Cycle 14\m51.pdf">
         
         <ScientificCategory>GALAXIES</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="INTERACTING AND MERGING GALAXIES" />
         
         <ScientificKeyword2
            Keyword="SPIRAL GALAXIES" />
         
         <ScientificKeyword3
            Keyword="STAR FORMATION" />
         
         <ScientificKeyword4
            Keyword="STELLAR POPULATIONS IN EXTERNAL GALAXIES" />
         
         <ScientificKeyword5
            Keyword="YOUNG STAR CLUSTERS IN EXTERNAL GALAXIES" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <Budget>45000</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>


