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    <title language="eng">Analysis of Tidal Accelerations in the Solar System and in Extrasolar Planetary Systems</title>
    <abstract language="eng">Volcanism powered by tidal forces inside celestial bodies can provide enough energy to keep important solvents for living systems in the liquid phase. A prerequisite to calculate such tidal interactions and consequences is depending on simulations for tidal accelerations in a multi-body system. Unfortunately, from measurements in many extrasolar planetary systems, only few physical and orbital parameters are well-known enough for investigated celestial bodies. For calculating tidal acceleration vectors under missing most orbital parameter exactly, a simulation method is developed that is only based on a few basic parameters, easily measurable even in extrasolar planetary systems. Such a method as the one presented here allows finding a relation between the tidal acceleration vectors and potential heating inside celestial objects. Using the values and results of our model approach to our solar system as a “gold standard” for feasibility allowed us to classify this heating in relation to different forms of volcanism. This “gold standard” approach gave us a classification measure for the relevance of tidal heating in other extrasolar systems with a reduced availability of exact physical parameters. We help to estimate conditions for the identification of potential candidates for further sophisticated investigations by more complex established methods such as viscoelastic multi-body theories. As a first example, we applied the procedures developed here to the extrasolar planetary system TRAPPIST-1 as an example to check our working hypothesis.</abstract>
    <parentTitle language="eng">Applied Sciences</parentTitle>
    <identifier type="issn">2076-3417</identifier>
    <identifier type="doi">https://doi.org/10.3390/app11188624</identifier>
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Unfortunately, from measurements in many extrasolar planetary systems, only few physical and orbital parameters are well-known enough for investigated celestial bodies. For calculating tidal acceleration vectors under missing most orbital parameter exactly, a simulation method is developed that is only based on a few basic parameters, easily measurable even in extrasolar planetary systems. Such a method as the one presented here allows finding a relation between the tidal acceleration vectors and potential heating inside celestial objects. Using the values and results of our model approach to our solar system as a \u201cgold standard\u201d for feasibility allowed us to classify this heating in relation to different forms of volcanism. This \u201cgold standard\u201d approach gave us a classification measure for the relevance of tidal heating in other extrasolar systems with a reduced availability of exact physical parameters. We help to estimate conditions for the identification of potential candidates for further sophisticated investigations by more complex established methods such as viscoelastic multi-body theories. As a first example, we applied the procedures developed here to the extrasolar planetary system TRAPPIST-1 as an example to check our working hypothesis.&lt;\/jats:p&gt;","DOI":"10.3390\/app11188624","type":"journal-article","created":{"date-parts":[[2021,9,17]],"date-time":"2021-09-17T01:38:12Z","timestamp":1631842692000},"page":"8624","source":"Crossref","is-referenced-by-count":1,"title":["Analysis of Tidal Accelerations in the Solar System and in Extrasolar Planetary Systems"],"prefix":"10.3390","volume":"11","author":[{"ORCID":"http:\/\/orcid.org\/0000-0003-2603-4236","authenticated-orcid":false,"given":"Klaus","family":"Paschek","sequence":"first","affiliation":[{"name":"Department of Physics and Astronomy, Kirchhoff-Institute for Physics, Heidelberg University, Im Neuenheimer Feld 227, 69120 Heidelberg, Germany"}]},{"given":"Arthur","family":"Ro\u00dfmann","sequence":"additional","affiliation":[{"name":"Department of Physics and Astronomy, Kirchhoff-Institute for Physics, Heidelberg University, Im Neuenheimer Feld 227, 69120 Heidelberg, Germany"}]},{"ORCID":"http:\/\/orcid.org\/0000-0001-9430-1987","authenticated-orcid":false,"given":"Michael","family":"Hausmann","sequence":"additional","affiliation":[{"name":"Department of Physics and Astronomy, Kirchhoff-Institute for Physics, Heidelberg University, Im Neuenheimer Feld 227, 69120 Heidelberg, Germany"}]},{"ORCID":"http:\/\/orcid.org\/0000-0003-1992-6025","authenticated-orcid":false,"given":"Georg","family":"Hildenbrand","sequence":"additional","affiliation":[{"name":"Department of Physics and Astronomy, Kirchhoff-Institute for Physics, Heidelberg University, Im Neuenheimer Feld 227, 69120 Heidelberg, Germany"}]}],"member":"1968","published-online":{"date-parts":[[2021,9,16]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"892","DOI":"10.1126\/science.203.4383.892","article-title":"Melting of Io by tidal dissipation","volume":"203","author":"Peale","year":"1979","journal-title":"Science"},{"key":"ref_2","doi-asserted-by":"crossref","first-page":"535","DOI":"10.1016\/j.icarus.2007.03.001","article-title":"Tidal heating in Enceladus","volume":"188","author":"Meyer","year":"2007","journal-title":"Icarus"},{"key":"ref_3","doi-asserted-by":"crossref","first-page":"245","DOI":"10.1016\/j.icarus.2017.11.023","article-title":"Relevance of tidal heating on large TNOs","volume":"302","author":"Saxena","year":"2018","journal-title":"Icarus"},{"key":"ref_4","doi-asserted-by":"crossref","first-page":"95","DOI":"10.1088\/0004-637X\/767\/1\/95","article-title":"The occurrence rate of small planets around small stars","volume":"767","author":"Dressing","year":"2013","journal-title":"Astrophys. J."},{"key":"ref_5","doi-asserted-by":"crossref","first-page":"221","DOI":"10.1038\/nature17448","article-title":"Temperate Earth-sized planets transiting a nearby ultracool dwarf star","volume":"533","author":"Gillon","year":"2016","journal-title":"Nature"},{"key":"ref_6","doi-asserted-by":"crossref","first-page":"456","DOI":"10.1038\/nature21360","article-title":"Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1","volume":"542","author":"Gillon","year":"2017","journal-title":"Nature"},{"key":"ref_7","unstructured":"(2018, February 13). Solar System Bodies, Available online: https:\/\/ssd.jpl.nasa.gov\/?bodies."},{"key":"ref_8","unstructured":"(2018, February 13). JPL Small-Body Database Search Engine, Available online: https:\/\/ssd.jpl.nasa.gov\/sbdb_query.cgi."},{"key":"ref_9","unstructured":"Steadly, R.S., and Robinson, M.S. (2011). The Astronomical Almanac for the Year 2012: Data for Astronomy, Space Sciences, Geodesy, Surveying, Navigation and other Applications."},{"key":"ref_10","doi-asserted-by":"crossref","first-page":"30","DOI":"10.3847\/1538-4357\/aaa023","article-title":"Stellar parameters for Trappist-1","volume":"853","author":"Fernandes","year":"2018","journal-title":"Astrophys. J."},{"key":"ref_11","doi-asserted-by":"crossref","first-page":"A68","DOI":"10.1051\/0004-6361\/201732233","article-title":"The nature of the TRAPPIST-1 exoplanets","volume":"613","author":"Grimm","year":"2018","journal-title":"Astron. Astrophys."},{"key":"ref_12","doi-asserted-by":"crossref","first-page":"3577","DOI":"10.1093\/mnras\/sty051","article-title":"Early 2017 observations of TRAPPIST-1 with Spitzer","volume":"475","author":"Delrez","year":"2018","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"ref_13","unstructured":"Guennebaud, G., and Jacob, B. (2018, February 13). Eigen v3 [C++ library]. Available online: http:\/\/eigen.tuxfamily.org."},{"key":"ref_14","doi-asserted-by":"crossref","first-page":"58","DOI":"10.1126\/science.321.5885.58","article-title":"Mercury, up-close again. Introduction","volume":"321","author":"Hanson","year":"2008","journal-title":"Science"},{"key":"ref_15","doi-asserted-by":"crossref","first-page":"1853","DOI":"10.1126\/science.1211997","article-title":"Flood volcanism in the northern high latitudes of Mercury revealed by MESSENGER","volume":"333","author":"Head","year":"2011","journal-title":"Science"},{"key":"ref_16","doi-asserted-by":"crossref","first-page":"4762","DOI":"10.1002\/2015GL064088","article-title":"Active volcanism on Venus in the Ganiki Chasma rift zone","volume":"42","author":"Shalygin","year":"2015","journal-title":"Geophys. Res. Lett."},{"key":"ref_17","doi-asserted-by":"crossref","first-page":"E12003","DOI":"10.1029\/2012JE004231","article-title":"Simulating the thermochemical magmatic and tectonic evolution of Venus\u2019s mantle and lithosphere: Two-dimensional models","volume":"117","author":"Armann","year":"2012","journal-title":"J. Geophys. Res. Planets"},{"key":"ref_18","doi-asserted-by":"crossref","unstructured":"Ulmschneider, P. (2006). Intelligent Life in the Universe: Principles and Requirements Behind Its Emergence, Springer. [2nd ed.].","DOI":"10.1007\/3-540-32838-6"},{"key":"ref_19","doi-asserted-by":"crossref","unstructured":"Scholz, M. (2016). Astrobiologie, Springer Spektrum.","DOI":"10.1007\/978-3-662-47037-4"},{"key":"ref_20","doi-asserted-by":"crossref","first-page":"18","DOI":"10.1016\/j.pepi.2017.05.007","article-title":"Hot climate inhibits volcanism on Venus: Constraints from rock deformation experiments and argon isotope geochemistry","volume":"268","author":"Mikhail","year":"2017","journal-title":"Phys. Earth Planet. Inter."},{"key":"ref_21","first-page":"689","article-title":"Volcanism on the Moon","volume":"Volume 39","author":"Sigurdsson","year":"2015","journal-title":"The Encyclopedia of Volcanoes"},{"key":"ref_22","doi-asserted-by":"crossref","first-page":"309","DOI":"10.1126\/science.1199375","article-title":"Seismic detection of the lunar core","volume":"331","author":"Weber","year":"2011","journal-title":"Science"},{"key":"ref_23","doi-asserted-by":"crossref","first-page":"2019","DOI":"10.1126\/science.281.5385.2019","article-title":"Europa\u2019s differentiated internal structure: Inferences from four Galileo encounters","volume":"281","author":"Anderson","year":"1998","journal-title":"Science"},{"key":"ref_24","doi-asserted-by":"crossref","first-page":"62","DOI":"10.1016\/j.pss.2014.03.011","article-title":"Ganymede\u05f3s internal structure including thermodynamics of magnesium sulfate oceans in contact with ice","volume":"96","author":"Vance","year":"2014","journal-title":"Planet. Space Sci."},{"key":"ref_25","doi-asserted-by":"crossref","first-page":"77","DOI":"10.1126\/science.286.5437.77","article-title":"The Galilean satellites","volume":"286","author":"Showman","year":"1999","journal-title":"Science"},{"key":"ref_26","doi-asserted-by":"crossref","first-page":"1422","DOI":"10.1126\/science.1121254","article-title":"Enceladus\u2019 water vapor plume","volume":"311","author":"Hansen","year":"2006","journal-title":"Science"},{"key":"ref_27","doi-asserted-by":"crossref","first-page":"617","DOI":"10.1016\/S0032-0633(00)00039-8","article-title":"On the internal structure and dynamics of Titan","volume":"48","author":"Grasset","year":"2000","journal-title":"Planet. Space Sci."},{"key":"ref_28","doi-asserted-by":"crossref","first-page":"10088","DOI":"10.1002\/2016GL070650","article-title":"Enceladus\u2019s and Dione\u2019s floating ice shells supported by minimum stress isostasy","volume":"43","author":"Beuthe","year":"2016","journal-title":"Geophys. Res. Lett."},{"key":"ref_29","doi-asserted-by":"crossref","first-page":"258","DOI":"10.1016\/j.icarus.2006.06.005","article-title":"Subsurface oceans and deep interiors of medium-sized outer planet satellites and large trans-neptunian objects","volume":"185","author":"Hussmann","year":"2006","journal-title":"Icarus"},{"key":"ref_30","doi-asserted-by":"crossref","first-page":"394","DOI":"10.1016\/0019-1035(90)90125-S","article-title":"Tidal evolution of the Uranian satellites: III. Evolution through the Miranda-Umbriel 3:1, Miranda-Ariel 5:3, and Ariel-Umbriel 2:1 mean-motion commensurabilities","volume":"85","author":"Tittemore","year":"1990","journal-title":"Icarus"},{"key":"ref_31","doi-asserted-by":"crossref","unstructured":"Bergstralh, J.T., Miner, E.D., and Matthews, M.S. (1991). Uranus, The University of Arizona Press.","DOI":"10.2307\/j.ctv1v7zdtq"},{"key":"ref_32","doi-asserted-by":"crossref","first-page":"aaf4286","DOI":"10.1126\/science.aaf4286","article-title":"Cryovolcanism on Ceres","volume":"353","author":"Ruesch","year":"2016","journal-title":"Science"},{"key":"ref_33","doi-asserted-by":"crossref","first-page":"694","DOI":"10.1016\/j.icarus.2009.03.009","article-title":"Thermal evolution of Kuiper belt objects, with implications for cryovolcanism","volume":"202","author":"Desch","year":"2009","journal-title":"Icarus"},{"key":"ref_34","doi-asserted-by":"crossref","first-page":"A105","DOI":"10.1051\/0004-6361\/201015011","article-title":"High-contrast observations of (136108) Haumea","volume":"528","author":"Dumas","year":"2011","journal-title":"Astron. Astrophys."},{"key":"ref_35","doi-asserted-by":"crossref","first-page":"1234","DOI":"10.1086\/505706","article-title":"The solar neighborhood. XVI. Parallaxes from CTIOPI: Final results from the 1.5 m Telescope Program","volume":"132","author":"Costa","year":"2006","journal-title":"Astron. J."},{"key":"ref_36","doi-asserted-by":"crossref","first-page":"108","DOI":"10.1006\/icar.1993.1010","article-title":"Habitable zones around main sequence stars","volume":"101","author":"Kasting","year":"1993","journal-title":"Icarus"},{"key":"ref_37","doi-asserted-by":"crossref","first-page":"1373","DOI":"10.1051\/0004-6361:20078091","article-title":"Habitable planets around the star Gliese 581?","volume":"476","author":"Selsis","year":"2007","journal-title":"Astron. Astrophys."},{"key":"ref_38","doi-asserted-by":"crossref","first-page":"323","DOI":"10.1086\/665271","article-title":"The habitable zone gallery","volume":"124","author":"Kane","year":"2012","journal-title":"Publ. Astron. Soc. Pac."},{"key":"ref_39","doi-asserted-by":"crossref","first-page":"L8","DOI":"10.1088\/2041-8205\/767\/1\/L8","article-title":"A revised estimate of the occurrence rate of terrestrial planets in the habitable zones around Kepler M-dwarfs","volume":"767","author":"Kopparapu","year":"2013","journal-title":"Astrophys. J. Lett."},{"key":"ref_40","doi-asserted-by":"crossref","first-page":"3728","DOI":"10.1093\/mnras\/stw2578","article-title":"Water loss from terrestrial planets orbiting ultracool dwarfs: Implications for the planets of TRAPPIST-1","volume":"464","author":"Bolmont","year":"2017","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"ref_41","doi-asserted-by":"crossref","first-page":"121","DOI":"10.3847\/1538-3881\/aa859c","article-title":"Temporal evolution of the high-energy irradiation and water content of TRAPPIST-1 exoplanets","volume":"154","author":"Bourrier","year":"2017","journal-title":"Astron. J."},{"key":"ref_42","doi-asserted-by":"crossref","first-page":"76","DOI":"10.3847\/1538-4357\/aae36a","article-title":"Evolved climates and observational discriminants for the TRAPPIST-1 planetary system","volume":"867","author":"Lincowski","year":"2018","journal-title":"Astrophys. J."},{"key":"ref_43","doi-asserted-by":"crossref","first-page":"A37","DOI":"10.1051\/0004-6361\/201731992","article-title":"Interior structures and tidal heating in the TRAPPIST-1 planets","volume":"613","author":"Barr","year":"2018","journal-title":"Astron. Astrophys."},{"key":"ref_44","doi-asserted-by":"crossref","first-page":"878","DOI":"10.1038\/s41550-017-0284-0","article-title":"Magma oceans and enhanced volcanism on TRAPPIST-1 planets due to induction heating","volume":"1","author":"Kislyakova","year":"2017","journal-title":"Nat. Astron."},{"key":"ref_45","doi-asserted-by":"crossref","first-page":"390","DOI":"10.1016\/0019-1035(92)90155-Z","article-title":"A dynamical history of the inner Neptunian satellites","volume":"99","author":"Banfield","year":"1992","journal-title":"Icarus"},{"key":"ref_46","doi-asserted-by":"crossref","first-page":"447","DOI":"10.1016\/0019-1035(77)90101-4","article-title":"The supernova trigger for formation of the solar system","volume":"30","author":"Cameron","year":"1977","journal-title":"Icarus"},{"key":"ref_47","doi-asserted-by":"crossref","first-page":"79","DOI":"10.3847\/1538-4357\/ab9a38","article-title":"Aluminum-26 enrichment in the surface of protostellar disks due to protostellar cosmic rays","volume":"898","author":"Gaches","year":"2020","journal-title":"Astrophys. J."},{"key":"ref_48","doi-asserted-by":"crossref","first-page":"493","DOI":"10.1126\/science.aad0525","article-title":"Oxygen isotopic evidence for vigorous mixing during the Moon-forming giant impact","volume":"351","author":"Young","year":"2016","journal-title":"Science"},{"key":"ref_49","doi-asserted-by":"crossref","first-page":"110","DOI":"10.3847\/1538-4357\/aa7fea","article-title":"On the age of the TRAPPIST-1 system","volume":"845","author":"Burgasser","year":"2017","journal-title":"Astrophys. J."},{"key":"ref_50","doi-asserted-by":"crossref","first-page":"A2","DOI":"10.1051\/0004-6361\/201834254","article-title":"Tidal heating and the habitability of the TRAPPIST-1 exoplanets","volume":"624","author":"Dobos","year":"2019","journal-title":"Astron. Astrophys."},{"key":"ref_51","doi-asserted-by":"crossref","first-page":"22","DOI":"10.3847\/1538-4357\/ab0c21","article-title":"Tides between the TRAPPIST-1 planets","volume":"875","author":"Hay","year":"2019","journal-title":"Astrophys. J."},{"key":"ref_52","doi-asserted-by":"crossref","first-page":"170","DOI":"10.1088\/0004-637X\/799\/2\/170","article-title":"An ancient extrasolar system with five sub-Earth-size planets","volume":"799","author":"Campante","year":"2015","journal-title":"Astrophys. J."},{"key":"ref_53","doi-asserted-by":"crossref","first-page":"112","DOI":"10.1051\/0004-6361\/201015577","article-title":"The HARPS search for southern extra-solar planets: XXVIII. Up to seven planets orbiting HD 10180: Probing the architecture of low-mass planetary systems","volume":"528","author":"Lovis","year":"2011","journal-title":"Astron. Astrophys."},{"key":"ref_54","doi-asserted-by":"crossref","first-page":"A121","DOI":"10.1051\/0004-6361\/202038922","article-title":"Planetary system LHS 1140 revisited with ESPRESSO and TESS","volume":"642","author":"Figueira","year":"2020","journal-title":"Astron. Astrophys."},{"key":"ref_55","doi-asserted-by":"crossref","first-page":"53","DOI":"10.1038\/nature09760","article-title":"A closely packed system of low-mass, low-density planets transiting Kepler-11","volume":"470","author":"Lissauer","year":"2011","journal-title":"Nature"},{"key":"ref_56","doi-asserted-by":"crossref","first-page":"28","DOI":"10.1088\/0004-637X\/784\/1\/28","article-title":"The hunt for exomoons with Kepler (HEK). IV. A search for moons around eight M dwarfs","volume":"784","author":"Kipping","year":"2014","journal-title":"Astrophys. J."},{"key":"ref_57","doi-asserted-by":"crossref","first-page":"321","DOI":"10.1038\/nature14494","article-title":"The mass of the Mars-sized exoplanet Kepler-138 b from transit timing","volume":"522","author":"Rowe","year":"2015","journal-title":"Nature"},{"key":"ref_58","doi-asserted-by":"crossref","first-page":"A94","DOI":"10.1051\/0004-6361\/201118743","article-title":"\u201cTNOs are Cool\u201d: A survey of the trans-Neptunian region","volume":"541","author":"Vilenius","year":"2012","journal-title":"Astron. Astrophys."},{"key":"ref_59","doi-asserted-by":"crossref","first-page":"978","DOI":"10.1016\/j.icarus.2009.12.017","article-title":"(47171) 1999 TC36, A transneptunian triple","volume":"207","author":"Benecchi","year":"2010","journal-title":"Icarus"},{"key":"ref_60","doi-asserted-by":"crossref","first-page":"26","DOI":"10.1088\/0004-637X\/773\/1\/26","article-title":"The size, shape, albedo, density, and atmospheric limit of transneptunian object (50000) Quaoar from multi-chord stellar occultations","volume":"773","author":"Sicardy","year":"2013","journal-title":"Astrophys. J."},{"key":"ref_61","doi-asserted-by":"crossref","first-page":"357","DOI":"10.1016\/j.icarus.2012.11.004","article-title":"The mass, orbit, and tidal evolution of the Quaoar\u2013Weywot system","volume":"222","author":"Fraser","year":"2013","journal-title":"Icarus"},{"key":"ref_62","doi-asserted-by":"crossref","first-page":"184","DOI":"10.1016\/j.icarus.2005.01.007","article-title":"Diverse albedos of small trans-neptunian objects","volume":"176","author":"Grundy","year":"2005","journal-title":"Icarus"},{"key":"ref_63","doi-asserted-by":"crossref","first-page":"286","DOI":"10.1016\/j.icarus.2007.04.004","article-title":"The orbit, mass, size, albedo, and density of (65489) Ceto\/Phorcys: A tidally-evolved binary Centaur","volume":"191","author":"Grundy","year":"2007","journal-title":"Icarus"},{"key":"ref_64","doi-asserted-by":"crossref","first-page":"678","DOI":"10.1016\/j.icarus.2011.03.012","article-title":"Five new and three improved mutual orbits of transneptunian binaries","volume":"213","author":"Grundy","year":"2011","journal-title":"Icarus"},{"key":"ref_65","doi-asserted-by":"crossref","first-page":"A115","DOI":"10.1051\/0004-6361\/201117486","article-title":"Integral-field spectroscopy of (90482) Orcus-Vanth","volume":"534","author":"Carry","year":"2011","journal-title":"Astron. Astrophys."},{"key":"ref_66","doi-asserted-by":"crossref","first-page":"676","DOI":"10.1016\/j.icarus.2012.03.029","article-title":"Physical properties of trans-neptunian binaries (120347) Salacia\u2013Actaea and (42355) Typhon\u2013Echidna","volume":"219","author":"Stansberry","year":"2012","journal-title":"Icarus"},{"key":"ref_67","doi-asserted-by":"crossref","first-page":"4766","DOI":"10.1088\/0004-6256\/137\/6\/4766","article-title":"Orbits and masses of the satellites of the dwarft planet Humea (2003 EL61)","volume":"137","author":"Ragozzine","year":"2009","journal-title":"Astron. J."},{"key":"ref_68","doi-asserted-by":"crossref","first-page":"566","DOI":"10.1038\/nature11597","article-title":"Albedo and atmospheric constraints of dwarf planet Makemake from a stellar occultation","volume":"491","author":"Ortiz","year":"2012","journal-title":"Nature"},{"key":"ref_69","unstructured":"Sicardy, B., Ortiz, J.L., Assafin, M., Jehin, E., Maury, A., Lellouch, E., Gil-Hutton, R., Braga-Ribas, F., Colas, F., and Lecacheux, J. (2011, January 2\u20137). Size, density, albedo and atmosphere limit of dwarf planet Eris from a stellar occultation. Proceedings of the European Planetary Science Congress\u2014Division for Planetary Sciences (EPSC-DPS) Joint Meeting 2011, Nantes, France. Available online: http:\/\/meetingorganizer.copernicus.org\/EPSC-DPS2011\/EPSC-DPS2011-137-8.pdf."},{"key":"ref_70","doi-asserted-by":"crossref","first-page":"LP-1585","DOI":"10.1126\/science.1139415","article-title":"The mass of dwarf planet Eris","volume":"316","author":"Brown","year":"2007","journal-title":"Science"},{"key":"ref_71","doi-asserted-by":"crossref","first-page":"L7","DOI":"10.1088\/2041-8205\/767\/1\/L7","article-title":"On the size, shape, and density of dwarf planet Makemake","volume":"767","author":"Brown","year":"2013","journal-title":"Astrophys. J."},{"key":"ref_72","doi-asserted-by":"crossref","first-page":"130","DOI":"10.1016\/j.icarus.2015.04.036","article-title":"The mutual orbit, mass, and density of the large transneptunian binary system Varda and Ilmar\u00eb","volume":"257","author":"Grundy","year":"2015","journal-title":"Icarus"}],"container-title":["Applied Sciences"],"original-title":[],"language":"en","link":[{"URL":"https:\/\/www.mdpi.com\/2076-3417\/11\/18\/8624\/pdf","content-type":"unspecified","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2024,7,18]],"date-time":"2024-07-18T21:43:32Z","timestamp":1721339012000},"score":1,"resource":{"primary":{"URL":"https:\/\/www.mdpi.com\/2076-3417\/11\/18\/8624"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2021,9,16]]},"references-count":72,"journal-issue":{"issue":"18","published-online":{"date-parts":[[2021,9]]}},"alternative-id":["app11188624"],"URL":"http:\/\/dx.doi.org\/10.3390\/app11188624","relation":{},"ISSN":["2076-3417"],"issn-type":[{"value":"2076-3417","type":"electronic"}],"subject":[],"published":{"date-parts":[[2021,9,16]]}}}</enrichment>
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