Titanium(II) oxide

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Titanium(II) oxide
Titanium(II) oxide
Titanium(II) oxide
Names
IUPAC name
Titanium(II) oxide
Other names
Titanium monoxide
Identifiers
3D model (JSmol)
ChEBI
ChemSpider
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EC Number
  • 235-236-5
E number Lua error in Module:Wikidata at line 880: attempt to index field 'wikibase' (a nil value).
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  • InChI=1S/O.Ti/q-2;+2
    Key: VKRWBTVMYISSEF-UHFFFAOYSA-N
  • InChI=1S/O.Ti
    Key: OGIDPMRJRNCKJF-UHFFFAOYSA-N
  • [O-2].[Ti+2]
Properties
TiO
Molar mass 63.866 g/mol
Appearance bronze crystals
Density 4.95 g/cm3
Melting point 1,750 °C (3,180 °F; 2,020 K)
Structure
cubic
Hazards
Flash point Non-flammable
Related compounds
Titanium(III) oxide
Titanium(III,IV) oxide
Titanium(IV) oxide
Except where otherwise noted, data are given for materials in their standard state (at 25 °C [77 °F], 100 kPa).
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Titanium(II) oxide (TiO) is an inorganic chemical compound of titanium and oxygen. It can be prepared from titanium dioxide and titanium metal at 1500 °C.[1] It is non-stoichiometric in a range TiO0.7 to TiO1.3 and this is caused by vacancies of either Ti or O in the defect rock salt structure.[1] In pure TiO 15% of both Ti and O sites are vacant,[1] as the vacancies allow metal-metal bonding between adjacent Ti centres. Careful annealing can cause ordering of the vacancies producing a monoclinic form which has 5 TiO units in the primitive cell that exhibits lower resistivity.[2] A high temperature form with titanium atoms with trigonal prismatic coordination is also known.[3] Acid solutions of TiO are stable for a short time then decompose to give hydrogen:[1]

2 Ti2+(aq) + 2 H+(aq) → 2 Ti3+(aq) + H2(g)

Gas-phase TiO shows strong bands in the optical spectra of cool (M-type) stars.[4][5] In 2017, TiO was claimed to be detected in an exoplanet atmosphere for the first time; a result which is still debated in the literature.[6][7] Additionally, evidence has been obtained for the presence of the diatomic molecule TiO in the interstellar medium.[8]

References

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