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<ri:Resource created="2010-04-19T13:44:26Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Lightcurves of 12 NEAs</title><shortName>J/A+A/511/A49</shortName><identifier>ivo://CDS.VizieR/J/A+A/511/A49</identifier><altIdentifier>doi:10.26093/cds/vizier.35110049</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kwiatkowski T.</name></creator><creator><name>Polinska M.</name></creator><creator><name>Loaring N.</name></creator><creator><name>Buckley D.A.H.</name></creator><creator><name>O'Donoghue D.,Kniazev A.</name></creator><creator><name>Romero Colmenero E.</name></creator><date role="Updated">2018-02-02T10:34:12Z</date><date role="Created">2010-04-19T13:44:26Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>surveys</subject><subject>solar-system</subject><subject>asteroids</subject><subject>ccd-photometry</subject><description>Very small asteroids (VSAs) are thought to be the building blocks of larger asteroids and, as such, are interesting to study. Many of these monolithic or deeply fractured objects display rapid rotations with periods as short as several minutes. Observations of such asteroids can reveal their spin limits, which can be related to the tensile strength of their interiors. The evolution of the spins of these objects is primarily shaped by the YORP effect, the theory of which needs comparison with observations. With the 10m SALT telescope, we observed VSAs belonging to near-Earth asteroids. The obtained lightcurves were used to derive synodical periods of rotation, amplitudes, and elongations of these bodies. Results for 14 rapidly rotating asteroids were reported in the first paper in this series. Here we show lightcurves of 2 fast rotators, 9 objects with periods &gt;=1h, and a possible non-principal axis rotator. We also list negative detections that most probably indicate asteroids with long periods and/or low amplitudes. Combining our results with the data from the literature, we obtain a set of 79 near-Earth VSAs with a median period of 0.25h (15min). By adjusting the spin limits predicted by theory to those observations, we find tentative evidence that the tensile strengths of VSAs, after scaling them to the same size, are of the same order as the minimum tensile strengths of stony meteoroids that undergo fragmentation under the atmospheric load.</description><source format="bibcode">2010A&amp;A...511A..49K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/511/A49</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/509/A94">J/A+A/509/A94 : Lightcurves of 14 NEAs (Kwiatkowski+, 2010)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/511/A49</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/511/A49</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/511/A49</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/511/A49</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/511/A49</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/511/A49</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/A+A/511/A49/table2</name><description>Summary of the results</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ast</name><description>Asteroid designation</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType><flag>primary</flag></column><column><name>Per</name><description>Rotation period</description><unit>h</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Per</name><description>Period uncertainty (max error/sigma)</description><unit>h</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Amp</name><description>Peak-to-peak lightcurve amplitude</description><unit>mag</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a/b</name><description>Maximum elongation (1)</description><ucd>phys.size.axisRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Diam</name><description>Effective diameter</description><unit>km</unit><ucd>phys.size.diameter</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Orb</name><description>Details of the orbit of this asteroid, from the astorb database</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/A+A/511/A49/table1</name><description>Aspect data and observing log</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ast</name><description>Designation of the asteroid</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Hmag</name><description>Absolute magnitude</description><unit>mag</unit><ucd>phys.magAbs;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Obs1.Date</name><description>Date of observation</description><ucd>time.epoch;obs</ucd><flag>nullable</flag></column><column><name>Obs1.Time</name><description>Observing time (beginning) (1)</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>Obs2.Time</name><description>Observing time (end) (1)</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>r</name><description>Asteroid-Sun distance (2)</description><unit>AU</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Delta</name><description>Asteroid-Earth distance (2)</description><unit>AU</unit><ucd>pos.distance;pos.geocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>alpha</name><description>Solar phase angle (2)</description><unit>deg</unit><ucd>pos.phaseAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ELON</name><description>Geocentric, ecliptic longitude (2)</description><unit>deg</unit><ucd>pos.ecliptic.lon</ucd></column><column><name>ELAT</name><description>Geocentric, ecliptic latitude (2)</description><unit>deg</unit><ucd>pos.ecliptic.lat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmag</name><description>Apparent magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SkyMov</name><description>Asteroid movement on the sky</description><unit>arcsec/min</unit><ucd>pos.pm</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Exp</name><description>Exposure time</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N1</name><description>Number of exposures taken</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N2</name><description>Number of exposures used</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/A+A/511/A49/list</name><description>List of all light curves</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ast</name><description>Asteroid name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>FileName</name><description>Name of the file containing the light curve</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>Title</name><description>Title of the file</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="32*">char</dataType></column></table></schema></tableset></ri:Resource>