EGU26-1902, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-1902
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 07 May, 10:45–12:30 (CEST), Display time Thursday, 07 May, 08:30–12:30
 
Hall X2, X2.63
Insights into Mogok Ruby–Sapphire Genesis from U–Pb Geochronology and Trace Elements
Khin Zaw and Arkar Moe Myint
Khin Zaw and Arkar Moe Myint

The Mogok Metamorphic Belt (MMB) consists of an interlayered suite of magmatic and metasedimentary rocks that record metamorphic conditions from low grade to upper amphibolite–granulite facies. Banded gneiss dominates the succession with subordinate quartzite and discontinuous marble layers. The Mogok area in the northern part of the MMB is a renowned gemstone tract notable for its world-class ruby, sapphire, and other gemstones. Marbles are major host rocks for best-quality pigeon blood ruby. The metamorphic rocks are associated with alkaline rocks (mostly sodic nepheline–syenite and syenite–pegmatite) which host exceptionally high-quality, royal blue sapphires. Searle et al. (2020) classified the alkaline host rocks as charnockite–syenite intrusions and identified multiple episodes of syenitic magmatism from the Jurassic to the Oligocene (170–168 Ma, ~68–63 Ma, and 44–21 Ma). U–Pb zircon dating of sapphire-bearing nepheline syenite from the Ondan district, approximately 40 km west of Mogok, yielded an age of 57.81 ± 0.5 Ma (Myo Min, 2016, per. com). U-Pb titanite ages from the ruby-bearing marbles and meta-skarns at Le Oo mine in the Mogok valley are 21 Ma, similar to titanite ages from an adjacent syenite (22 Ma) (Searle et al., 2020). Sutherland et al. (2019) considered that the Mogok rubies were formed at 32.4 Ma (U-Pb age of titanite inclusion in ruby) which is older than the 21 Ma U-Pb titanite age from the ruby-bearing marbles. Hence, the Mogok rubies were considered to have formed around 17-35 Ma. In comparison, the timing of the Mogok sapphires is debatable and not resolved yet (Akar Moe Myint et al., 2025 in press). The sapphires are associated with pegmatitic syenites of the Jurassic to Oligocene (Searle et al., 2020). Arkar Moe Myint et al. (2025, in press) dated zircon inclusions in Baw Mar (Mogok) sapphires using LA–ICP–MS U–Pb geochronology, yielding ages of 54.11 ± 1.6 Ma to 65.39 ± 1.77 Ma, which indicate the timing of sapphire formation in the Baw Mar area of Mogok. Precise LA-ICP-MS analysis of ruby and sapphire from Mook placer and in situ deposits reveal V can exceed 5000 ppm (Khin Zaw et al., 2015). Such values significantly exceed those elsewhere and are focused on a specific area, suggesting a geological control on V-rich ruby and sapphire distribution. These findings highlight vanadium as an important tracer for ruby, with vanadium and associated trace-element patterns, together with age dating, providing robust tools for geographic typing and fingerprinting.

References

Akar Moe Myint et al. 2025 (in press). Gem and Gemology.

Khin Zaw et al. 2015. Mineralium Deposita https://doi.org/10.1007/s00126-014-0545-0.

Searle et al. 2020. Tectonics https://doi.org/10.1029/2019TC005998.

Sutherland et al. 2019. Minerals https://doi.org/10.3390/min9010028.

 

How to cite: Zaw, K. and Moe Myint, A.: Insights into Mogok Ruby–Sapphire Genesis from U–Pb Geochronology and Trace Elements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1902, https://doi.org/10.5194/egusphere-egu26-1902, 2026.