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    <Identification_Area>
        <logical_identifier>urn:nasa:pds:context:target:astrophysical.general_relativity</logical_identifier>
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        <title>Tests of General Relativity</title>
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    <Reference_List>
        <External_Reference>
            <reference_text>
                Bertotti, B., Iess, L., and Tortora, P. (2003),
                A Test of General Relativity using Radio Links with the Cassini Spacecraft,
                Nature, 425, 374–376.
            </reference_text>
            <description>
                Measurement of the effects of solar mass on propagation of X- and Ka-band
                Cassini radio signals along paths close to the Sun.  The results are
                consistent with predictions of standard general relativity to a precision
                nearly two orders of magnitude better than previous measurements.
            </description>
        </External_Reference>
        <External_Reference>
            <reference_text>
                Merkowitz, S.M. 
                Tests of Gravity Using Lunar Laser Ranging. 
                Living Reviews in Relativity 13, 7 (2010). 
                https://doi.org/10.12942/lrr-2010-7
            </reference_text>
            <description>
                A review of the gravitational science and technology of lunar laser 
                ranging and discussion of prospects for the future.  The three retroreflector
                arrays put on the Moon by the Apollo astronauts and the French built arrays 
                on the Soviet Lunokhod rovers have provided the most stringent tests of the 
                Strong Equivalence Principle and the time variation of Newton’s gravitational 
                constant.
            </description>
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        <name>Tests of General Relativity</name>
        <type>Astrophysical</type>
        <description>
              Tests of general relativity, which may include deflection and phase retardation 
              of electromagnetic waves passing massive objects (such as the Sun) and tests
              of the Strong Equivalence Principle and time variation of Newton's
              gravitational constant from lunar laser ranging.
        </description>
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