J/MNRAS/445/4395ivo://CDS.VizieR/J/MNRAS/445/4395doi:10.26093/cds/vizier.74454395CDSYildiz M.Celik Orhan Z.Kayhan C.Turkoglu G.E.2024-08-14T20:18:29Z2017-08-24T15:05:17ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frmultiple-starssolar-system-planetsstellar-masseseffective-temperatureIt is already stated in the previous studies that the radius of the giant planets is affected by stellar irradiation. The confirmed relation between radius and incident flux depends on planetary mass intervals. In this study, we show that there is a single relation between radius and irradiated energy per gram per second (l-), for all mass intervals. There is an extra increase in radius of planets if l- is higher than 1100 times energy received by the Earth (l_{earth}_). This is likely due to dissociation of molecules. The tidal interaction as a heating mechanism is also considered and found that its maximum effect on the inflation of planets is about 15 percent. We also compute age and heavy element abundances from the properties of host stars, given in the TEPCat catalogue (Southworth). The metallicity given in the literature is as [Fe/H]. However, the most abundant element is oxygen, and there is a reverse relation between the observed abundances [Fe/H] and [O/Fe]. Therefore, we first compute [O/H] from [Fe/H] by using observed abundances, and then find heavy element abundance from [O/H]. We also develop a new method for age determination. Using the ages we find, we analyse variation of both radius and mass of the planets with respect to time, and estimate the initial mass of the planets from the relation we derive for the first time. According to our results, the highly irradiated gas giants lose 5 percent of their mass in every 1Gyr.2014MNRAS.445.4395Yhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/445/4395CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-towww.astro.keele.ac.uk/jkt/tepcat : TEPCat data basehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/445/4395https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/445/4395http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/445/4395https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/445/4395https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/445/4395http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/445/4395GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/445/4395/tablea1 (Fundamental properties of the giant gas planets and their host stars (the data are taken from TEPCat))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/445/4395/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/445/4395/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/445/4395/tablea1?GETtext/xml+votable180.050000true102.0798833-3.10213330.0055555555555555566/790 876 1275 2335 2532 2551 2584 2711 3344 3876 4145 4241 4272 4990 5475 5730 6017 6181 6349 6381 6539 6638 7036 7208 7240 8197 8237 8825 9173 9355 9524 9811 10407 10730 10953 12342 12424 12644 12853 12862 12983 13143 13439 13680 13702 13941 14555 14567 14762 14764 14772 14779-14780 14816 14824-14826 14886 14914 14923 14936 14963 14973 15029 15040 15112 15129 15140 15143 15160 15162 15169 15218 15550 15950 16405 16432 16947 17172 17226 17300 17819 17851 18093 18510 18569 18943 20339 20382 20476 20780 21026 21876 21989 22001 22034 22040 22065 22078-22079 22120 22168-22169 22208 22505 22519 22816 22963 23620 24409 24428 24815 25132 25153 25194 25604 25950 26019 28433 28821-28822 29683 30240-30241 30293 30295 30344 30436 30450-30451 30456 30466 30485 31641 32564 32727 32749 33220 33719 33798 34708 34898 35210 35456 35993 36142 36165 36667 36794 37246-37247 37329 37923 38452 38682 39487 39673 40862 42936 43625 43775 43847 43960 44648 45051 45855 45922 46058 46316 46421 46437 47476 48358 48747 48803 48945https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/445/4395?format=asciidefaultJ/MNRAS/445/4395/tablea1Fundamental properties of the giant gas planets and their host stars (the data are taken from TEPCat)PlanetPlanet namemeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMassHost star masssolMassmeta.idfloatRadHost star radiussolRadmeta.idfloatTeffHost star effective temperatureKmeta.idintaSemi-major axisAUphys.size.smajAxisfloatPerPerioddtime.periodfloateEccentricitysrc.orbital.eccentricityfloatn_e[a] Note on e (1)meta.notecharMpPlanetary mass(1.898187x10+27kg)phys.massfloatRpPlanetary radius(7.1492x10+7m)phys.size.radiusfloatTeq? Equilibrium temperatureKphys.temperatureintnullableFIIncident flux (in Earth units)phot.flux.densityinte_FIrms uncertainty on FI (in Earth units)stat.errorintl-Energy received per unit mass per unit time (in l0 units)phys.energyinte_l-rms uncertainty on l- (in l0 units)stat.errorintlog(dE/dt)? Rate of energy dissipation due to tidal interactionlog(1e-07W)arith.rate;phys.energyfloatnullablee_log(dE/dt)? rms uncertainty on log(dE/dt)log(1e-07W)stat.errorfloatnullableAge? Age (2)Gyrtime.agefloatnullablee_Age? rms uncertainty on AgeGyrstat.error;time.agefloatnullableZ0Metallicity (2)phys.abund.Zfloate_Z0rms uncertainty on Z0stat.error;pos.cartesian.zfloatSimbadNameSimbad column added by the CDSmeta.idchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.main