Description
Eibach Pro-Spacer Wheel Spacers – 1992-1997 BMW 318is & Additional Applications lets 1992-1997 BMW 318is & Additional Applications owners change effective wheel offset using Eibach's matched spacer hardware, with the available thicknesses organized as selectable variants.
A spacer can solve one clearance problem while creating another, so the ideal size depends on the entire wheel, tire, suspension, and body combination rather than the vehicle model alone.
Application focus: This page is tied to chassis E36, E34, E32; engine/application 3.2L, 3.0L, V8; drivetrain RWD, RWD | xDrive; trim/submodel Coupe, M Coupe, 3.0i; factory-option notes including Excludes Self Leveling; w/Rear Air Suspension. Those details matter because Eibach may assign different components within the same model generation.
What makes this application specific: This page is tied to Eibach part S90-2-15-001 for 1992-1997 BMW 318is & Additional Applications, not a generic version of the same suspension product.
Why This Eibach Setup Makes Sense
- Widen Your Stance - For Better Handling.
- Made from High-Strength Aircraft-Aluminum Alloy.
- Precision Engineered Hub-Centric - for Perfect Fit and Wheel Balance.
- Reduced Weight Compared to Steel Wheel Spacers.
Product Details
- Eibach package: 15mm Pair
- Product family: PRO-SPACER
- Eibach part number: S90-2-15-001
What This Listing Represents
15mm Pair. The selected Eibach part number determines the exact component or kit supplied.
Fitment Notes
- Wheel Bolts and Wheel Studs sold separately. Recommend purchasing wheel bolts or studs with extended length equivalent to the thickness of the wheel spacer. Example, 15mm thick spacer would require a 15mm (0.6") longer wheel stud or wheel bolt.
Installation Planning
Measure twice before selecting thickness, then verify hub engagement, wheel seating, fastener length, and tire-to-body clearance after installation.
Fitment data is application-specific. Confirm the selected Eibach part number against the exact vehicle configuration before ordering.