Vestaite is a rare titanium-rich oxide mineral identified primarily in HED (howardite-eucrite-diogenite) meteorites originating from the asteroid Vesta. It typically occurs as small grains associated with pyroxene and plagioclase in basaltic or igneous meteoritic compositions.
Is this vestaite?
2-step field checkRun through these checks against the specimen in your hand. The more boxes tick, the more confident the ID.
- 1Test the hardnessTry to scratch vestaite with a known reference. Vestaite sits at Mohs 5-6, softer than the next harder reference, harder than the previous one.
- 2Look at form & habitCrystal system: monoclinic. Typical habit: anhedral to subhedral grains.
Often confused with
Vestaite vs. its common look-alikes, and how to tell them apart in the field.
Often found alongside vestaite
Minerals reported to co-occur with vestaite. Spotting these in float or country rock is a strong cue you are in the right ground.
All properties
- Chemical formula
- (TiFe)Ti₃O₉
- Mohs hardness
- 5-6
- Density
- 4.86 g/cm³
- Transparency
- Transparent
- Crystal system
- Monoclinic
- Crystal habit
- Anhedral to subhedral grains
- Rarity
- Rare
- Uses
- Scientific research
- Host rock
- In two titanium-rich, shock melt pockets (20-30 mm in size), which are enclosed by former plagioclase (now maskelynite, plagioclase, and tissintite), augite and ilmenite in a basaltic eucrite meteorite
Where rockhounds find vestaite
Classic worldwide localities
- Vesta asteroid
- Meteorites
Field-hunting tip
Where it forms: In two titanium-rich, shock melt pockets (20-30 mm in size), which are enclosed by former plagioclase (now maskelynite, plagioclase, and tissintite), augite and ilmenite in a basaltic eucrite meteorite. If you start seeing corundum, ilmenite, al-ti-rich pyroxene in float, you are in the right ground. Typical habit: anhedral to subhedral grains. Train your eye for that shape before scanning the outcrop.



