Ceramics & Hard Materials

Ultra-High-Temperature Ceramics

Borides and carbides of Hf, Zr, and Ta with melting points beyond 3000 °C — candidate leading edges and propulsion liners for hypersonic flight where superalloys vaporize.

At a glance

Class Statistics

Compounds Tracked
1,173
Multi-Source DFT
170
With Synthesis Routes
1
Avg. Agreement
0.83 / 1.00
Overview

What are Ultra-High-Temperature Ceramics?

Ultra-high-temperature ceramics (UHTCs) represent a specialized class of refractory materials defined by their exceptional thermal stability, typically maintaining structural integrity at temperatures exceeding three thousand degrees Celsius. Chemically, these materials are primarily composed of transition metal borides, carbides, and nitrides, with hafnium, zirconium, and tantalum serving as the foundational metallic elements. Unlike conventional superalloys that suffer from rapid oxidation and mechanical degradation at extreme temperatures, UHTCs possess strong covalent bonding and high lattice energy, which contribute to their remarkable resistance to thermal shock and chemical erosion. These materials are critical for the advancement of aerospace and defense technologies, particularly in the development of hypersonic flight vehicles. In such environments, airframes encounter intense aerodynamic heating that would cause traditional metallic components to vaporize or lose load-bearing capacity. By utilizing UHTCs for leading edges, nose cones, and propulsion system liners, engineers can design vehicles capable of sustained high-speed travel through the atmosphere. Notable members of this class include hafnium diboride and zirconium diboride, often modified with silicon carbide to enhance oxidation resistance through the formation of a protective surface glass layer. As global interest in hypersonic travel and space exploration grows, UHTCs remain at the forefront of materials research, bridging the gap between current aerospace limitations and the extreme conditions of high-Mach flight.

Members

Top Ultra-High-Temperature Ceramics

Ranked by data richness — literature synthesis coverage, multi-source DFT corroboration, and patent activity.

FormulaBand GapBest EAH (eV/atom)StabilityDFT SourcesRecipes
Hf3N40.92–1.26 eV0.0000On hull (stable)30
C4Zr40.48 eV0.0000On hull (stable)30
HfC0.30 eV0.0000On hull (stable)20
TaN0.04 eV0.0000On hull (stable)20
ZrC0.48 eV0.0000On hull (stable)20
C2Zr20.48 eV0.0000On hull (stable)20
C6Zr60.48 eV0.0000On hull (stable)30
CZr0.48 eV0.0000On hull (stable)20
HfN20.58–1.19 eV0.4150Above hull20
Ti3N40.10–1.76 eV0.1046Above hull20
Zr3N40.56–0.98 eV0.0000On hull (stable)20
HfNMetallic / not reported0.0000On hull (stable)30
TiCMetallic / not reported0.0000On hull (stable)22
N2Ta20.04 eV0.0000On hull (stable)20
N4Ta40.04 eV0.0000On hull (stable)20
C1Hf10.30 eV0.0000On hull (stable)10
C1Zr10.48 eV0.0000On hull (stable)10
NTa0.04 eV0.0000On hull (stable)10
Ta3N51.21 eV0.0000On hull (stable)20
C4Hf40.30 eV0.0000On hull (stable)20
Hf3N2Metallic / not reported0.0000On hull (stable)40
Nb3N50.70 eV0.0146Near hull (likely stable)20
C8Hf80.30 eV0.0000On hull (stable)20
C8Zr80.48 eV0.0000On hull (stable)20
N1Ta10.04 eV0.0000On hull (stable)10
C2Hf20.30 eV0.0000On hull (stable)10
C6Hf60.30 eV0.0000On hull (stable)20
N3Ta30.04 eV0.0000On hull (stable)10
Hf4N80.58–1.19 eV0.4150Above hull20
B2Ta2Metallic / not reported0.0000On hull (stable)30
Hf6N80.92–1.26 eV0.0000On hull (stable)20
N4Ti30.10–1.76 eV0.1046Above hull20
N8Ta80.04 eV0.0000On hull (stable)10
Hf4N3Metallic / not reported0.0435Metastable30
C3Hf30.30 eV0.0000On hull (stable)10
C3Zr30.48 eV0.0000On hull (stable)10
N36Ta360.04 eV0.0000On hull (stable)10
Hf2N40.58–1.19 eV0.4150Above hull10
C12Hf120.30 eV0.0000On hull (stable)10
C12Zr120.48 eV0.0000On hull (stable)10
C4Ta4Metallic / not reported0.0000On hull (stable)30
B2Hf2Metallic / not reported0.3499Above hull20
HfBMetallic / not reported0.3499Above hull20
Nb2CMetallic / not reported0.0000On hull (stable)20
Nb2NMetallic / not reported0.0000On hull (stable)20
NbBMetallic / not reported0.0000On hull (stable)20
NbCMetallic / not reported0.0298Metastable20
NbNMetallic / not reported0.0000On hull (stable)20
Ta2NMetallic / not reported0.0000On hull (stable)20
TaBMetallic / not reported0.0000On hull (stable)20
Reference

Frequently Asked Questions

How many ultra-high-temperature ceramics are in the database?

1,173 ultra-high-temperature ceramics are tracked, of which 170 have multi-source DFT validation and 1 have documented synthesis routes.

More questions
What is the most data-rich ultra-high-temperature ceramic?
Hf3N4 is the most thoroughly characterized, with 65 reported structures.
Which ultra-high-temperature ceramic has the widest band gap?
Among the top compounds, Ti3N4 has the widest reported DFT band gap (1.76 eV).
What differentiates UHTCs from standard ceramics?
UHTCs are distinguished by their ability to withstand extreme thermal environments that would cause standard ceramics or metals to melt, soften, or undergo catastrophic oxidation.
Why is silicon carbide often added to UHTCs?
Silicon carbide is frequently incorporated as an additive to improve oxidation resistance; at high temperatures, it reacts to form a stable, protective oxide layer that shields the underlying material from further degradation.
Are UHTCs suitable for all high-temperature applications?
While highly effective for extreme heat, UHTCs can be brittle and difficult to manufacture into complex shapes, which limits their use to specific components where thermal resistance is the primary requirement.
How do UHTCs perform under hypersonic flight conditions?
They are ideal for hypersonic flight because they maintain their shape and mechanical strength under the intense heat generated by atmospheric friction, preventing the structural failure that would occur with conventional materials.
Explore

Related Material Classes

Screen ultra-high-temperature ceramics computationally

Evaluate stability, supply-chain risk, and patent whitespace before committing lab resources.

Explore the Platform →