<?xml version="1.0" encoding="UTF-8"?>
<?xml-model href="https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1F00.sch" schematypens="http://purl.oclc.org/dsdl/schematron"?>
<Product_Context xmlns="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_1F00.xsd">
    
    <Identification_Area>
        <logical_identifier>urn:nasa:pds:context:instrument_host:spacecraft.gp</logical_identifier>
        <version_id>1.1</version_id>
        <title>GALILEO PROBE</title>
        <information_model_version>1.15.0.0</information_model_version>
        <product_class>Product_Context</product_class>
        <Modification_History>
            <Modification_Detail>
                <modification_date>2021-02-24</modification_date>
                <version_id>1.1</version_id>
                <description>
                    Changed inst LIDs from
                      u:n:p:c:i:instID.scID to
                      u:n:p:c:i:scID.instID
                    And per "Guide toPDS4 Context Products" v1.7,
                    changed all lidvid_reference to lid_reference
                </description>
            </Modification_Detail>
            <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>

    <Reference_List>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:investigation:mission.galileo</lid_reference>
            <reference_type>instrument_host_to_investigation</reference_type>
        </Internal_Reference>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:instrument:gp.asi</lid_reference>
            <reference_type>instrument_host_to_instrument</reference_type>
        </Internal_Reference>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:instrument:gp.dwe</lid_reference>
            <reference_type>instrument_host_to_instrument</reference_type>
        </Internal_Reference>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:instrument:gp.epi</lid_reference>
            <reference_type>instrument_host_to_instrument</reference_type>
        </Internal_Reference>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:instrument:gp.gpms</lid_reference>
            <reference_type>instrument_host_to_instrument</reference_type>
        </Internal_Reference>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:instrument:gp.had</lid_reference>
            <reference_type>instrument_host_to_instrument</reference_type>
        </Internal_Reference>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:instrument:gp.lrd</lid_reference>
            <reference_type>instrument_host_to_instrument</reference_type>
        </Internal_Reference>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:instrument:gp.nep</lid_reference>
            <reference_type>instrument_host_to_instrument</reference_type>
        </Internal_Reference>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:instrument:gp.nfr</lid_reference>
            <reference_type>instrument_host_to_instrument</reference_type>
        </Internal_Reference>
        <Internal_Reference>
            <lid_reference>urn:nasa:pds:context:target:planet.jupiter</lid_reference>
            <reference_type>instrument_host_to_target</reference_type>
        </Internal_Reference>
        <External_Reference>
            <reference_text>
                   Yeates, C.M., T.V. Johnson, L. Colin, F.P. Fanale, L. Frank, and D.M. Hunten,
                   Galileo: Exploration of Jupiter&apos;s System, NASA SP-479 (REPLACED BY
                   YEATESETAL1985), 1985.
            </reference_text>
            <description>reference.GLL1985</description>
        </External_Reference>
        <External_Reference>
            <reference_text>
                   D&apos;Amario, L.A., L.E. Bright, and A.A. Wolf, Space Science Reviews, Volume 60
                   Numbers 1-4, 1992, The Galileo Mission, Kluwer Academic Publishers, 1992.
            </reference_text>
            <description>reference.SSR1992</description>
        </External_Reference>
    </Reference_List>
    
    <Instrument_Host>
        <name>GALILEO PROBE</name>
        <type>Spacecraft</type>
        <naif_host_id>GP</naif_host_id>

        <description>
 
 
         Instrument Host Overview
         ========================
 
         The Galileo spacecraft consists of two parts, an orbiter
         (SPACECRAFT_ID = &apos;GO&apos;) and a probe (SPACECRAFT_ID = &apos;GP&apos;).
         Spacecraft power is provided by two radioisotope
         thermoelectric generators. Propulsion is accomplished via a
         bipropellant system of twelve 10- newton thrusters and one
         400 newton engine. The command and data subsystem consists
         of multiple microprocesors and a high-speed data bus.
 
         The Galileo atmospheric probe will be deployed from the
         orbiter 150 days prior to Jupiter encounter. The probe
         consists of a deceleration module and a descent module. It
         weighs about 331 kilograms, half of which is the heat
         shield. After entering the Jovian atmosphere and slowing its
         descent, the descent module deploys a 2.5 meter parachute
         and begins transmitting data from its instruments at a rate
         of 128 bits per second. (Refer to Yeates, et al, 1985;
         Johnson, et al, 1992.)
 
       Platform Description
       --------------------
 
         Platform PROBE DESCENT MODULE
 
           The atmospheric descent module contains seven scientific
           instruments: the atmospheric structure instrument (ASI), the
           neutral mass spectrometer (NMS), the helium abundance
           detector (HAD), the nephelometer (NEP), the net-flux
           radiometer (NFR), the lightning and radio emissions detector
           (LRD), and the energetic particles instrument (EPI). The
           instruments are contained in hermetically sealed housings
           designed to withstand a pressure of 20 bars. The instrument
           data are transmitted to the orbiter over two simultaneously
           operating channels in the L band. (Refer to Yeates, et al,
           1985; Johnson, et al, 1992.)

        </description>
    </Instrument_Host>
</Product_Context>
