Hallo!

Wegen Umzugs möchte ich ein paar Stücke, die ich noch abzugeben habe, "loswerden":

- Teilscheibe NWA 8210; LL3; 32,25g (TKW 0,41kg), Abmessungen ca. 50x42x6,2mm (Ahmed Pani Provenienz)
- Teilscheibe NWA 1774; R3,8-6; 1,70g (TKW 0,714kg) Abmessungen ca. 74x23x0,3mm (Lucy Cullen Provenienz)
- Kleines Individual Agoudal 5,6g
- Kleines Shrapnel-Individual Sikhote Alin ca. 12g

In den nachfolgenden Postings lade ich noch Detailfotos der Scheiben hoch.

Wer Interesse hat, gerne per PM ein Gebot abgeben (en bloc, inkl. Versand innerhalb Europas).
10% vom Erlös geht zudem an das Forum.

Danke & LG
Christian

Besten Dank für die Info, Andreas! 

Der Koblenz-Meteorit wurde von der Universität Münster untersucht. Es handelt sich um einen brekziierten Eukrit. Die folgenden Gefügebilder des Dünnschliffs wurden von Addi Bischoff (Universität Münster) angefertigt.

Viele Grüße, Andreas

ARTEMIS II

In 40 Minuten ist der Start geplant. Es geht wieder 'zweibeinig' Richtung Mond.

VIDEO-LIVESTREAM

NASA

Und noch eines:

In situ single-spot Rb/Sr cosmochronology of roedderite in the Ribbeck aubrite (asteroid 2024 BX1)

Christopher J. Barnes, Aleksander B?asiak, Helge Vinje Birgerheim, Matthias Konrad-Schmolke, Delia Rösel, Jaros?aw Majka, Thomas Zack

MAPS, Version of Record online: 01 April 2026

LINK (OPEN ACCESS)
PDF (OPEN ACCESS)

"The mineralogy and textures of several fragments from the Ribbeck aubrite were analyzed using a combination of scanning electron microscopy, electron microprobe analysis, ?Raman spectroscopy, and laser ablation inductively coupled reaction cell mass spectrometry (LA-ICP-MS/MS). The meteorite fragments are strongly brecciated and show evidence of shock melting. The silicate phases of the fragments predominantly consist of enstatite, albite, and roedderite, with subordinate forsterite, diopside, K-feldspar. Non-silicate phases include kamacite, troilite, oldhamite, and Fe-Ti, Fe-Mn, and Fe-Cr rich sulfides. Tridymite and cristobalite, the latter contained in Si-rich glass, are also present within one enstatite grain. Vesicular fusion crust is apparent in several fragments. The discovery of roedderite is the first reported for the Ribbeck aubrite. In situ Rb/Sr dating combined with chemical analysis of the roedderite was performed via laser ablation ICP-MS/MS using the single-spot dating approach. The average chemistry of 20 roedderite analyses is 68.7?wt% of SiO2, 23.1?wt% of MgO, 4.9?wt% of K2O, and 3.3?wt% of Na2O and is <0.1?wt% of FeO. The total concentrations of Rb and Sr are 282 and <1??g?g?1, respectively. Single-spot Rb/Sr dates from the same 20 analyses yielded a weighted average of 4570?±?27?Ma, interpreted as the formation age of the Ribbeck aubrite parent body. The result highlights advantages of single-spot Rb/Sr dating compared to short-lived isotopic systems (e.g., 26Al-26Mg, 53Mn-53Cr, and 129I-129Xe), long-lived systems with radiogenic noble gasses (e.g., 40K-40Ar and 238/235U-232Th-4He), and the conventional Rb/Sr isochron approach for meteorite cosmochronology."