<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-06-01T02:01:52Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/87219" metadataPrefix="marc">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/87219</identifier><datestamp>2023-08-06T01:24:55Z</datestamp><setSpec>com_20.500.14352_14</setSpec><setSpec>col_20.500.14352_15</setSpec></header><metadata><record xmlns="http://www.loc.gov/MARC21/slim" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.loc.gov/MARC21/slim http://www.loc.gov/standards/marcxml/schema/MARC21slim.xsd">
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      <subfield code="a">Popescu, Marcel M.</subfield>
      <subfield code="e">author</subfield>
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   <datafield ind2=" " ind1=" " tag="720">
      <subfield code="a">Fuente Marcos, de la</subfield>
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   <datafield ind2=" " ind1=" " tag="720">
      <subfield code="a">De La Fuente Marcos, Raúl</subfield>
      <subfield code="e">author</subfield>
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   <datafield ind2=" " ind1=" " tag="260">
      <subfield code="c">2023-06-21</subfield>
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      <subfield code="a">Context. Near-Earth asteroids (NEAs) that may evolve into impactors deserve detailed threat assessment studies. Early physical characterization of a would-be impactor may help in optimizing impact mitigation plans. We first detected NEA 2023 DZ2 on 27–February–2023. After that, it was found to have a Minimum Orbit Intersection Distance (MOID) with Earth of 0.00005 au as well as an unusually high initial probability of becoming a near-term (in 2026) impactor.
Aims. We aim to perform a rapid but consistent dynamical and physical characterization of 2023 DZ2 as an example of a key response to mitigate the consequences of a potential impact.
Methods. We use a multi-pronged approach, drawing from various methods (observational/computational) and techniques (spectroscopy/photometry from multiple instruments), and bringing the data together to perform a rapid and robust threat assessment.
Results. The visible reflectance spectrum of 2023 DZ2 is consistent with that of an X-type asteroid. Light curves of this object obtained on two different nights give a rotation period P=6.2743±0.0005 min with an amplitude A=0.57±0.14 mag. We confirm that although its MOID is among the smallest known, 2023 DZ2 will not impact Earth in the foreseeable future as a result of secular near-resonant behaviour.
Conclusions. Our investigation shows that coordinated observation and interpretation of disparate data provides a robust approach from discovery to threat assessment when a virtual impactor is identified. We prove that critical information can be obtained within a few days after the announcement of the potential impactor.</subfield>
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      <subfield code="a">https://hdl.handle.net/20.500.14352/87219</subfield>
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   <datafield ind2="0" ind1="0" tag="245">
      <subfield code="a">Discovery and physical characterization as the first response to a potential asteroid collision: the case of 2023 DZ2</subfield>
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