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Ann: West Arunta Project - Luni Assay Results, page-354

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    Reply to @PutSauce

    Excellent coverage. I haven't looked at the other elements at Luni other than to register REEs are present as is some phosphate.

    The carbonatite that hosts the mineralisation is a relatively soft host rock. This makes open pit mining feasible and efficient. Added to the fact that we are seeing mineralisation begin on average beginning 30-40m due to the transported cover (fig 2 pg 3 of latest announcement - plus similar figure in previous announcements), this is the first big tick. Bearing in mind that Araxa utilises open pit mining very effectively in their operations.


    What did catch my attention was this paragraph. I suspect you will be aware of much of what is below.

    Not certain if FRESH carbonatite is necessarily going to be a soft host rock.

    https://hotcopper.com.au/data/attachments/5997/5997561-4d7f7580f87345eb5beeea123e5969e1.jpg
    The high grade lens from this May 23 image straddles the boundary so any future mining will have to deal with a combination of fresh and weathered. I would suspect there is some gradation in 'hardness' going to depth through a transitional zone. That will be part of ongoing geotech and mett work at the very least. The truly high grade sits above the base of complete oxidation in this EARLY section which may, or not, be representative.

    ============================

    In the post below you compare the current desert environment of the West Arunta with Araxa. Further west [30 odd years ago our company employed a geomorphologist to study the surface and weathering profile. Fascinating report mentioning evidence of multiple phases of dry and wet conditions that went over my head a lot. Sound vaguely familiar to today and climate change ideas?], and I suspect across much of Australia, the climate used to be more like Araxa - Miocene (20+- Mya) era with a climate that generated the widespread laterite profile (Breakaways, white clays, saprolite profile) that is currently in the slow process of being eroded. The profile varies from 0 to some 200m in depth. Luni has a relic of this measuring in the 10s of meters though not data that is commonly announced in any detail. I always had a lot of trouble getting my head around the terminology and preferred white and green clays which isn't very helpful.
    Current rainfall and climate bring their own challenges and benefits.


    ====================
    A partial case study

    Mt Weld is a zoned carbonatite. Mining (and exploration) there may give some hint of how Luni may be tackled for a different commodity. Mt W is best known for REEs but also hosts a wide range of other elements including Nb, phosphates and others. I remembered there was a significant amount of Nb. Some details courtesy of:.
    From Portergeo Database - Mount Weld
    Deposits not being mined at present, I think.

    Crown Deposit niobium, tantalum resources at January 2010 (Lynas Corp.)
    indicated + inferred resource - 37.7 Mt @ 1.07% Nb
    2O5, 1.16% TLnO, 0.09% Y2O3, 0.3% ZrO, 0.024% Ta2O5, 7.99% P2O5;
    Swan Deposit phosphate, as at March, 2011 (Lynas Corp.)
    indicated + inferred resource - 77 Mt @ 13.5% P
    2O5.


    An early Global resource (1990)
    The regolith over the carbonatite was estimated (1989) to contain an indicated resource of (Duncan and Willett, 1990):
    250 Mt @ 18% P
    2O5,
    270 Mt @ 0.9% Nb
    2O5,
    145 Mt @ 0.034% Ta
    2O5
    ,
    15.2 Mt @ 11.2% lanthanide + yttrium oxides.


    Lynas have generally focused on the high grade REEs but over the last couple of years have expanded exploration laterally and to depth.
    The high grade oxide zone appears to sit on top of a core of higher grade primary mineralisation that extends to some 700+m below surface. (Luni?)

    This LYC announcement of an exploration update contains a variant of what Luni may be. Worth a look for the near surface and deeper potential of a carbonatite.

    https://hotcopper.com.au/data/attachments/5997/5997807-2437c1359e0f66eb574ca46649444d70.jpg

    Histogram of results for MWEX10270.

    https://hotcopper.com.au/data/attachments/5997/5997819-ea261708fd8737402f6628facad8525d.jpghttps://hotcopper.com.au/data/attachments/5997/5997830-02e5ac922df3c784091b841d126819c1.jpg


    https://hotcopper.com.au/data/attachments/5997/5997848-a54f84afac1ce0608380231ee380a75a.jpg
    What does the footprint of surface drilling tell us about this model? Since I last played with this the yellow boundary has extended to the SW and probably swings up in the direction of, and beyond, hole L1.
    If the early inversion model is correct there is a zoned core of higher density material with lighter material (current near surface high Nb zones) which may extend to depth.
    Perhaps a revised model is needed?
    ====================
    Enough musing for today.
    So many different parts to the elephant that is Luni and hopefully the West Arunta. Needs much more work but well begun.





    Last edited by salpetie: 29/02/24
 
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