Niobium-1% zirconium is used in rocketry and in the nuclear industry. It is regarded as a low-strength alloy. C-103, which is 89% Nb, 10% Hf and 1% Ti, is used for the rocket nozzle of the
Apollo service module and the
Merlin vacuum engines; it is regarded as a medium-strength alloy. It is typically produced using gas atomization or plasma atomization techniques. It is particularly used in additive manufacturing (3D printing) and
powder metallurgy processes. Due to its corrosion resistance and high thermal efficiency, C103 helps reduce material waste and environmental pollution. High-strength alloys include C-129Y (10% tungsten, 10% hafnium, 0.1%
yttrium, balance niobium), Cb-752 (10% tungsten, 2.5% zirconium), and the even higher strength C-3009 (61% niobium, 30% hafnium, 9% tungsten); these can be used at temperatures up to 1650 °C with acceptable strength, though are expensive and hard to form. Nb-Hf-Ti is an alloy powder consisting of
niobium (Nb),
hafnium (Hf), and a small amount of
titanium (Ti) provides high strength, ductility, high-temperature stability, and remarkable corrosion resistance. It is used in manufacturing biocompatible implants and devices such as
orthopedic implants and
dental prosthetics. Niobium alloys in general are inconvenient to weld: both sides of the weld must be protected with a stream of
inert gas, because hot niobium will react with oxygen and nitrogen in the air. It is also necessary to take care (e.g. hard chrome-plating of all copper tooling) to avoid copper contamination.
High Temperature Performance While Nb alloys exhibit high strength at high temperatures, Nb has high affinity to C, N, and O (known as interstitial impurities). Variation in interstitial impurity content can result in subsequent variation in strength and performance. To mitigate this effect,
thermal barrier coating are often required for Nb-alloys at high temperatures. Additionally, elements that have a higher interstitial affinity, such as Zr, can be added to mitigate negative effects and form
precipitates. High temperature deformation of Nb alloys is dominated by
creep deformation. Nb-based alloys are a class 1 solid solution material. Class 1 creep is denoted by a slow initial strain rate and reduced strain in the primary regime. This behavior is due to
solute drag creep being the dominate strengthening mechanism in most Nb alloys. The table below shows deformation properties of various high temperature Nb alloys in various temperature regimes. While data for deformation properties of Cb-752 and Nb-1Zr are limited, the creep properties of C103 are better studied. The creep properties of C103 are well studied. This alloy is primarily solid solution (SS) strengthened alloy
, with no intentional second phases. Strengthening is believed to primarily be contributed by the addition of 10 wt% Hf, due to the +18.58% atomic volume mismatch with Nb. Ti is also alloyed into C103 at 3 wt%, but the atomic volume mismatch is too small to contribute to solute drag creep, at only -3% volume difference between Nb. While Ti does not contribute to the high temperature strength of C103, it does act as a low temperature (< 500 °C) SS strengthener. The small addition of Zr (0.48 atm%), makes it unlikely to contribute to solute drag creep, despite having a high atomic volume mismatch with Nb at +27.11%. Based on this information, it can be assumed that the
activation energy of diffusion for creep is close to that for the activation energy for diffusion of Hf within Nb. While there is no explicit data for the activation energy, it is estimated to be within 2% of the activation energy for diffusion of Ti (~368 kJ/mol) and Zr (364 kJ/mol) within Nb. ==References==