
Under the Russian GOST 4543 standard, 20KHM (20Ð¥Ð) and 30KHMA (30Ð¥ÐÐ) are prominent chromium-molybdenum (Chrome Moly) alloy structural steels. In bar form, they are specified for applications demanding a reliable blend of tensile strength, fatigue resistance, and thermal stability.
The naming convention gives away their composition: 20/30 denotes the carbon content in hundredths of a percent, KH (Ð¥) represents Chromium, M (Ð) stands for Molybdenum, and the A (Ð) at the end of 30KHMA signifies a high-quality grade with stricter control over impurities like phosphorus and sulfur.
While both steels rely on the synergy of Chromium and Molybdenum to achieve depth-of-hardening and resist thermal degradation, they target different carbon ranges:
| Element | GOST 20KHM (20Ð¥Ð) | GOST 30KHMA (30Ð¥ÐÐ) | Primary Role |
| Carbon (C) | $0.22\% - 0.29\%$ | $0.26\% - 0.33\%$ | Controls core hardness and strength. |
| Chromium (Cr) | $0.90\% - 1.20\%$ | $0.80\% - 1.10\%$ | Enhances hardenability and wear resistance. |
| Molybdenum (Mo) | $0.15\% - 0.30\%$ | $0.15\% - 0.25\%$ | Eliminates temper brittleness; raises creep strength. |
| Manganese (Mn) | $0.60\% - 0.90\%$ | $0.40\% - 0.70\%$ | Deoxidizes and aids deep through-hardening. |
| Silicon (Si) | $\le 0.40\%$ | $0.17\% - 0.37\%$ | Boosts overall elastic limits. |
| Phosphorus / Sulfur | $\le 0.025\% / \le 0.035\%$ | $\le 0.025\% / \le 0.025\%$ | (Stricter limits in "A" quality to minimize defects). |
The structural behavior of these two bar stocks differs primarily due to the carbon shift:
Because of its lower carbon content, 20KHM yields lower baseline hardness but offers excellent impact toughness and superior weldability compared to 30KHMA.
Key Use Case: It handles dynamic, high-impact, and vibrational loads beautifully. It is heavily favored in high-pressure piping components, flanges, and structural boiler parts operating at elevated temperatures (up to 450°Câ500°C).
With more carbon and an elite "A" refinement classification, 30KHMA can be heat-treated to significantly higher tensile strengths and yield points. It is officially classified as a relaxation-resistant steel.
Key Use Case: It excels under continuous high-stress loads without stretching or deforming over time. This makes it the standard choice for massive industrial fasteners, turbine rotors, heavy-duty studs, gears, and shafts working in extreme power transmission profiles.
When these bars are supplied or heat-treated via Oil Quenching ($\sim$880°C) and High-Temperature Tempering ($\sim$540°Câ650°C), they achieve highly robust structural properties:
Tensile Strength ($R_m$):
20KHM: $\sim$ 650 â 850 MPa (highly dependent on cross-section diameter)
30KHMA: $\ge$ 930 MPa (often reaching 1000+ MPa in smaller bar profiles)
Yield Strength ($R_e$):
20KHM: $\ge$ 450 â 500 MPa
30KHMA: $\ge$ 735 MPa
Brinell Hardness (HBW):
Annealed State (+A): Both grades sit comfortably $\le$ 212â229 HB, rendering them highly machinable for complex CNC cutting or drilling before final heat treatment.
Fully Hardened State: 30KHMA can achieve surface hardpoints well suited for friction interfaces.
If you are replacing GOST-specified bars with Western or Asian standards, these grades serve as the closest equivalents:
| GOST Grade | US (AISI/SAE) | European (EN / DIN) | Japan (JIS) | China (GB) |
| 20KHM | AISI 4120 / 4125 | 22CrMo4 / 25CrMo4 ($1.7218$) | SCM 420 / 425 | 20CrMo |
| 30KHMA | AISI 4130 / 4135 | 30CrMo4 / 34CrMo4 ($1.7220$) | SCM 430 / 432 | 30CrMo / 30CrMoA |
â ï¸ Fabrication Warning
Welding: 20KHM can be welded with proper preheating ($\sim$150°Câ200°C) and low-hydrogen electrodes. 30KHMA is much more difficult to weld due to its higher carbon equivalent. It has "limited weldability" and requires mandatory preheating up to 250°Câ300°C followed by immediate post-weld heat treatment (PWHT) to prevent brittle heat-affected zones (HAZ) and hydrogen cold-cracking.
Forging: Both steels should be forged within the $1230^\circ\text{C}$ to $950^\circ\text{C}$ window, with a controlled slow cool down to avoid internal thermal cracking.
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