<?xml version="1.0" encoding="UTF-8"?>
<?xml-model href="https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1700.sch" schematypens="http://purl.oclc.org/dsdl/schematron"?>
<Product_Context xmlns="http://pds.nasa.gov/pds4/pds/v1"
 xmlns:pds="http://pds.nasa.gov/pds4/pds/v1"  xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
 xsi:schemaLocation="http://pds.nasa.gov/pds4/pds/v1 https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1700.xsd">
    
    <Identification_Area>
        <logical_identifier>urn:nasa:pds:context:target:calibration_field.ob_star</logical_identifier>
        <version_id>1.0</version_id>
        <title>OB_STAR</title>
        <information_model_version>1.7.0.0</information_model_version>
        <product_class>Product_Context</product_class>
        <Modification_History>
            <Modification_Detail>
                <modification_date>2016-10-01</modification_date>
                <version_id>1.0</version_id>
                <description>
                    extracted metadata from PDS3 catalog and
                    modified to comply with PDS4 Information Model
                </description>
            </Modification_Detail>
        </Modification_History>
    </Identification_Area>

    <Target>
        <name>OB_STAR</name>
        <type>Calibration Field</type> <!--RChen/EN was Calibration-->

        <description>
      An arbitrary chosen OB star. These are hot, massive stars of
      spectral types O or B which form in loosely organized groups
      called OB associations. They are short lived, and thus don&amp;apos;t
      move very far from where they were formed within their life.
      During their lifetime, they will emit copious amounts of
      ultraviolet radiation. This radiation rapidly ionizes the
      surrounding interstellar gas of the giant molecular cloud,
      forming an H II region.
        </description>
    </Target>
</Product_Context>
