A piece of igneous rock found in the surroundings of Puerto Angelo in Mexico (PAGZ-1) has been analyzed. Before it has been sawed it showed some textures similar to those characteristic of a meteorite. Also its location of discovery is close to the places historically tied to meteorites. In the field of igneous rocks and meteorites the methods used to determine in which group the specific specimen belongs are petrological, mineralogical, geochemical and radiometric. Data are acquired macroscopically, with optical microscope, using EDS-SEM (Scanning Electron Microscopy - Energy-dispersive X-ray spectroscopy), XRD (X-ray Diffraction), Raman spectrometry, geochemical analysis and dating using Rb-Sr method. Radiometric dating is a procedure used for more than half of a century, but have not yet been used in Slovenia untill now. Used procedure includes crushing and hand picking the specimen, melting and dissolving it in acid, separation of Rb from Sr, sample dissolution, and measurments of isotope rations on MC-ICP-MS (Multicollector-Inductively Coupled Plasma Mass Spectrometry). This procedure has many potential points where mistakes could happen. These are potential selective disolving and separation, lowering of detectoion trashold and a small amount of measured samples. Test samples showed an uncertanty of 22 Ma, which is also used for PAGZ-1. On basies of these methods we find out, that the analyzed rock is gabbro-norite, composed of pyroxene, plagioclase, biotite, hornblende and some other sulfides, sulfates and oxides, which were most likely consequence of hydro-thermal processes. Neither fusion crust nor regmaglipts were observed, although there are some pits 2 cm in diameter present. The derermined age is 201 ± 22 Ma and the initial 87Sr/86Sr ratio is 0.7042. It has a positive Eu anomaly. The comparison between the rocks in the surroundings of Puerto Angelo and the meteorite groups show that there are certain petrologic similarities with Lunar maria, that mineralogically PAGZ-1 is different to every known meteorite group, that the Eu anomaly is different to those in regional Mexican rock, and the age is not comparable to the local Mexican rocks but it overlaps with some Martian meteorite groups. On the basis of these findings the origin of PAGZ-1 cannot be definitely determined; however it does not belong to any known meteoritg group.
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