11Analogues have been developed and characterised for both interplanetary dust and 12 meteoric smoke particles. These include amorphous materials with elemental compositions 13 similar to the olivine mineral solid solution series, a variety of iron oxides, undifferentiated 14 meteorites (chondrites) and minerals which can be considered good terrestrial proxies to 15 some phases present in meteorites. The products have been subjected to a suite of 16 analytical techniques to demonstrate their suitability as analogues for the target materials. 17