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<ri:Resource created="2022-05-11T08:24:48Z" 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>Photometry and radial velocity of LTT 1445A</title><shortName>J/AJ/163/168</shortName><identifier>ivo://CDS.VizieR/J/AJ/163/168</identifier><altIdentifier>doi:10.26093/cds/vizier.51630168</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Winters J.G.</name></creator><creator><name>Cloutier R.</name></creator><creator><name>Medina A.A.</name></creator><creator><name>Irwin J.M.</name></creator><creator><name>Charbonneau D.,Astudillo-Defru N.</name></creator><creator><name>Bonfils X.</name></creator><creator><name>Howard A.W.</name></creator><creator><name>Isaacson H.</name></creator><creator><name>Bean J.L.,Seifahrt A.</name></creator><creator><name>Teske J.K.</name></creator><creator><name>Eastman J.D.</name></creator><creator><name>Twicken J.D.</name></creator><creator><name>Collins K.A.,Jensen E.L.N.</name></creator><creator><name>Quinn S.N.</name></creator><creator><name>Payne M.J.</name></creator><creator><name>Kristiansen M.H.</name></creator><creator><name>Spencer A.,Vanderburg A.</name></creator><creator><name>Zechmeister M.</name></creator><creator><name>Weiss L.M.</name></creator><creator><name>Wang S.X.</name></creator><creator><name>Wang G.</name></creator><creator><name>Udry S.,Terentev I.A.</name></creator><creator><name>Sturmer J.</name></creator><creator><name>Stefansson G.</name></creator><creator><name>Shporer A.</name></creator><creator><name>Shectman S.,Sefako R.</name></creator><creator><name>Schwengeler H.M.</name></creator><creator><name>Schwarz R.P.</name></creator><creator><name>Scarsdale N.</name></creator><creator><name>Rubenzahl R.A.,Roy A.</name></creator><creator><name>Rosenthal L.J.</name></creator><creator><name>Robertson P.</name></creator><creator><name>Petigura E.A.</name></creator><creator><name>Pepe F.</name></creator><creator><name>Omohundro M.,Murphy J.M.A.</name></creator><creator><name>Murgas F.</name></creator><creator><name>Mocnik T.</name></creator><creator><name>Montet B.T.</name></creator><creator><name>Mennickent R.</name></creator><creator><name>Mayo A.W.,Massey B.</name></creator><creator><name>Lubin J.</name></creator><creator><name>Lovis C.</name></creator><creator><name>Lewin P.</name></creator><creator><name>Kasper D.</name></creator><creator><name>Kane S.R.</name></creator><creator><name>Jenkins J.M.,Huber D.</name></creator><creator><name>Horne K.</name></creator><creator><name>Hill M.L.</name></creator><creator><name>Gorrini P.</name></creator><creator><name>Giacalone S.</name></creator><creator><name>Fulton B.,Forveille T.</name></creator><creator><name>Figueira P.</name></creator><creator><name>Fetherolf T.</name></creator><creator><name>Dressing C.</name></creator><creator><name>Diaz R.F.,Delfosse X.</name></creator><creator><name>Dalba P.A.</name></creator><creator><name>Dai F.</name></creator><creator><name>Cortes C.C.</name></creator><creator><name>Crossfield I.J.M.</name></creator><creator><name>Crane J.D.,Conti D.M.</name></creator><creator><name>Collins K.I.</name></creator><creator><name>Chontos A.</name></creator><creator><name>Butler R.P.</name></creator><creator><name>Brown P.</name></creator><creator><name>Brady M.,Behmard A.</name></creator><creator><name>Beard C.</name></creator><creator><name>Batalha N.M.</name></creator><creator><name>Almenara J.-M.</name></creator><date role="Updated">2025-02-24T08:59:58Z</date><date role="Created">2022-05-11T08:24:48Z</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>m-stars</subject><subject>exoplanets</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>photometry</subject><subject>radial-velocity</subject><description>LTT1445 is a hierarchical triple M-dwarf star system located at a distance of 6.86pc. The primary star LTT1445A (0.257M{sun}) is known to host the transiting planet LTT1445Ab with an orbital period of 5.36days, making it the second-closest known transiting exoplanet system, and the closest one for which the host is an M dwarf. Using Transiting Exoplanet Survey Satellite data, we present the discovery of a second planet in the LTT1445 system, with an orbital period of 3.12days. We combine radial-velocity measurements obtained from the five spectrographs, Echelle Spectrograph for Rocky Exoplanets and Stable Spectroscopic Observations, High Accuracy Radial Velocity Planet Searcher, High-Resolution Echelle Spectrometer, MAROON-X, and Planet Finder Spectrograph to establish that the new world also orbits LTT1445A. We determine the mass and radius of LTT1445Ab to be 2.87{+/-}0.25M{Earth} and 1.304_-0.060_^+0.067^R{Earth}, consistent with an Earth-like composition. For the newly discovered LTT 1445Ac, we measure a mass of 1.54_-0.19_^+0.20^M{Earth} and a minimum radius of 1.15R{Earth}, but we cannot determine the radius directly as the signal-to-noise ratio of our light curve permits both grazing and nongrazing configurations. Using MEarth photometry and ground-based spectroscopy, we establish that star C (0.161M{sun}) is likely the source of the 1.4day rotation period, and star B (0.215M{sun}) has a likely rotation period of 6.7days. We estimate a probable rotation period of 85days for LTT1445A. Thus, this triple M-dwarf system appears to be in a special evolutionary stage where the most massive M dwarf has spun down, the intermediate mass M dwarf is in the process of spinning down, while the least massive stellar component has not yet begun to spin down.</description><source format="bibcode">2022AJ....163..168W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/163/168</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/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/112">J/ApJ/757/112 : Stellar diameters. 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