Stability design of slopes in carbonatite complexes characterised by brecciation

The Southern African Institute of Mining and Metallurgy
D. Moses J. A. Onyango
Organization:
The Southern African Institute of Mining and Metallurgy
Pages:
11
File Size:
5581 KB
Publication Date:
Sep 1, 2025

Abstract

Carbonatites are generally competent rock masses with rock mass rating class II rating 60–74. In spite of their competency, they tend to be affected by weak features like manganese-iron veins and/or in situ rock damage due to brecciation associated with carbonatite complexes. Rock slope failure in such hard rocks is complex since such structures within the rock mass form weak links that could potentially control slope instability. In this contribution, a numerical simulation using phase2 v 7.0 was carried out to investigate the influence of in situ rock damage on the stability of mine pit walls. The outcome reveals that, the existence of breccia in the competent rock mass has the capability to reduce the slope stability performance particularly at gentle dipping angles of emplacement in close range to the slope toe. However, as the emplacement position of breccia moves away from the pit wall, the stability performance increases at gentle dipping angle <50º. On the contrary, at the dipping angle of 50° the performance of slope reduced, and at steeper angles >50° the impact becomes negligible. Thus, from a series of analyses, mine design in brecciated rock masses, the ratio of 1:5 between the breccia distance from slope toe and pit depth should be implemented to counter its impact, and if the breccia is within or close to the pit limit, a deliberate effort must be made to mine it out.
Citation

APA: D. Moses J. A. Onyango  (2025)  Stability design of slopes in carbonatite complexes characterised by brecciation

MLA: D. Moses J. A. Onyango Stability design of slopes in carbonatite complexes characterised by brecciation. The Southern African Institute of Mining and Metallurgy, 2025.

Export
Purchase this Article for $25.00

Create a Guest account to purchase this file
- or -
Log in to your existing Guest account