Germanium
Germanium is a brittle, silvery metalloid best known for its role in the birth of solid-state electronics. It sits between silicon and tin on the periodic table and shares their knack for semiconductor behavior, but its most valuable modern trick is being nearly transparent to infrared light.
- Group · Period
- 14 · 4
- At room temp
- solid
- Melts at
- 1211.4 K
- Density
- 5.323 g/cm³
- Discovered
- 1886
Uses
Germanium’s ability to bend and transmit infrared light without absorbing it makes it the material of choice for lenses in thermal imaging cameras, night-vision equipment, and infrared sensors used in industrial and military systems. In the fiber-optic industry, germanium oxide is added to the glass core of optical fibers to fine-tune how light bends inside them, which is essential for long-distance data transmission. Germanium is also alloyed into high-efficiency, multi-junction solar cells used on satellites and space probes, where reliability matters more than cost.
Beyond optics, germanium compounds serve as catalysts in the production of PET plastic, the polymer used in beverage bottles and synthetic fibers. It was also one of the first semiconductor materials used commercially in electronics, forming the basis of early transistors and diodes before silicon became the industry standard.
History
Germanium’s story begins on paper rather than in a laboratory. In 1871, Dmitri Mendeleev noticed a gap in his periodic table between silicon and tin and predicted a missing element he called eka-silicon, going so far as to estimate its density and how its compounds would behave. Fifteen years later, in 1886, German chemist Clemens Winkler isolated the element from a rare mineral called argyrodite and found its properties matched Mendeleev’s forecast remarkably closely. Winkler named the new element germanium in honor of his home country, and its discovery became one of the strongest early confirmations that the periodic table captured a genuine pattern in nature rather than just a convenient way of organizing known elements.
Fun facts
- Germanium's existence and properties were predicted with striking accuracy by Dmitri Mendeleev in 1871, years before it was ever found — he called it eka-silicon.
- It's transparent to infrared light even though it looks like an ordinary opaque metal to the naked eye, which is why it's used in thermal camera lenses.
- Germanium was one of the first materials used to build a working transistor in 1947, before silicon took over the semiconductor industry.
Frequently asked questions
Why is germanium considered such an important element in chemistry history?
It's the textbook example of a successful scientific prediction. Mendeleev left a gap in his periodic table for an undiscovered element and forecast its density, color and compounds in detail. When Clemens Winkler isolated germanium in 1886, the match was close enough to convince many remaining skeptics that the periodic table reflected something real about atomic structure.
Is germanium a metal or a nonmetal?
Neither, exactly — it's a metalloid. Germanium has a metallic luster and crystal structure similar to silicon, but it conducts electricity only moderately well and only under the right conditions, which is precisely the behavior that makes semiconductors useful.
If germanium was used in early transistors, why do we use silicon now?
Silicon is far more abundant and cheaper to refine, and it forms a more stable, higher-quality oxide layer during chip manufacturing, which matters enormously for miniaturized circuits. Germanium never disappeared, though — it just moved into niches like infrared optics and high-efficiency solar cells.
Compounds
3 notable compounds containing Ge
- GeH4gas
Germane
A colorless, flammable gas with a tetrahedral molecule much like methane, but far less stable and prone to decomposing into germanium metal and hydrogen. It's produced synthetically rather than found in nature.
Used for: Source gas for doping semiconductors by chemical vapor deposition
- GeO2oxide
Germanium dioxide
A white crystalline solid also called germania, structurally similar to silica with germanium bonded to oxygen in a tetrahedral network. It's the main industrial source of purified germanium metal.
Used for: Doping agent for optical fiber cores
- GeCl4industrial
Germanium tetrachloride
A colorless, fuming liquid that hydrolyzes readily in moist air to form germanium dioxide and hydrochloric acid. It serves as the key industrial precursor for high-purity germanium compounds.
Used for: Precursor for germanium-doped optical fiber cores
Isotopes
32 known isotopes
Swipe to see all columns →
| Isotope | Natural abundance | Half-life | Decay mode | Mass excess | Binding energy / nucleon | Decay width |
|---|---|---|---|---|---|---|
| Ge-70 stable | 20.52% | Stable | — | -70,562.04 keV | 8,721.7 keV | — |
| Ge-72 stable | 27.45% | Stable | — | -72,585.91 keV | 8,731.75 keV | — |
| Ge-73 stable | 7.76% | Stable | — | -71,297.53 keV | 8,705.05 keV | — |
| Ge-74 stable | 36.52% | Stable | — | -73,422.45 keV | 8,725.2 keV | — |
| Ge-76 stable | 7.75% | Stable | — | -73,212.9 keV | 8,705.24 keV | — |
Show all 32 isotopes
| Ge-59 | — | 13.3 ms | Two-proton emission (0.2%), Electron capture / beta-plus decay | -16,370 keV | 7,924 keV | 3.43 × 10-14 eV |
| Ge-60 | — | 110 ns | Electron capture / beta-plus decay, ECP | -27,530 keV | 8,113 keV | 4.15 × 10-9 eV |
| Ge-61 | — | 44 ms | Electron capture / beta-plus decay (100%), ECP (62%) | -33,790 keV | 8,215 keV | 1.04 × 10-14 eV |
| Ge-62 | — | 129 ms | Electron capture / beta-plus decay (100%), ECP | -42,140 keV | 8,347 keV | 3.54 × 10-15 eV |
| Ge-63 | — | 150 ms | Electron capture / beta-plus decay (100%) | -46,921.22 keV | 8,418.72 keV | 3.04 × 10-15 eV |
| Ge-64 | — | 63.7 s | Electron capture / beta-plus decay (100%), ECP | -54,315.5 keV | 8,528.82 keV | 7.16 × 10-18 eV |
| Ge-65 | — | 30.9 s | Electron capture / beta-plus decay (100%), ECP (0.011%) | -56,478.22 keV | 8,555.06 keV | 1.48 × 10-17 eV |
| Ge-66 | — | 2.26 h | Electron capture / beta-plus decay (100%) | -61,607.04 keV | 8,625.44 keV | 5.61 × 10-20 eV |
| Ge-67 | — | 18.9 m | Electron capture / beta-plus decay (100%) | -62,673.72 keV | 8,633.09 keV | 4.02 × 10-19 eV |
| Ge-68 | — | 270.93 d | Electron capture (100%) | -66,978.8 keV | 8,688.14 keV | 1.95 × 10-23 eV |
| Ge-69 | — | 39.05 h | Electron capture / beta-plus decay (100%) | -67,100.67 keV | 8,680.96 keV | 3.25 × 10-21 eV |
| Ge-71 | — | 11.43 d | Electron capture (100%) | -69,906.66 keV | 8,703.31 keV | 4.62 × 10-22 eV |
| Ge-75 | — | 82.78 m | Beta-minus decay (100%) | -71,856.97 keV | 8,695.61 keV | 9.19 × 10-20 eV |
| Ge-77 | — | 11.211 h | Beta-minus decay (100%) | -71,212.87 keV | 8,671.03 keV | 1.13 × 10-20 eV |
| Ge-78 | — | 88.0 m | Beta-minus decay (100%) | -71,862.06 keV | 8,671.66 keV | 8.64 × 10-20 eV |
| Ge-79 | — | 18.98 s | Beta-minus decay (100%) | -69,527.18 keV | 8,634.51 keV | 2.40 × 10-17 eV |
| Ge-80 | — | 29.5 s | Beta-minus decay (100%) | -69,535.31 keV | 8,627.57 keV | 1.55 × 10-17 eV |
| Ge-81 | — | 7.6 s | Beta-minus decay (100%) | -66,291.7 keV | 8,580.66 keV | 6.00 × 10-17 eV |
| Ge-82 | — | 4.0 s | Beta-minus decay (100%) | -65,415.08 keV | 8,563.76 keV | 1.14 × 10-16 eV |
| Ge-83 | — | 1.85 s | Beta-minus decay (100%), Beta-minus, neutron emission | -60,976.44 keV | 8,504.35 keV | 2.47 × 10-16 eV |
| Ge-84 | — | 0.954 s | Beta-minus decay (100%), Beta-minus, neutron emission (10.2%) | -58,148.44 keV | 8,465.52 keV | 4.78 × 10-16 eV |
| Ge-85 | — | 503 ms | Beta-minus decay (100%), Beta-minus, neutron emission (16.5%), B-2N | -53,123.43 keV | 8,401.77 keV | 9.07 × 10-16 eV |
| Ge-86 | — | 226 ms | Beta-minus decay (100%), Beta-minus, neutron emission (45%) | -49,399.93 keV | 8,354.63 keV | 2.02 × 10-15 eV |
| Ge-87 | — | 0.14 s | Beta-minus decay (100%), Beta-minus, neutron emission | -43,590 keV | 8,285 keV | 3.26 × 10-15 eV |
| Ge-88 | — | 300 ns | Beta-minus decay, Beta-minus, neutron emission | -39,520 keV | 8,236 keV | 1.52 × 10-9 eV |
| Ge-89 | — | — | Beta-minus decay (100%), Beta-minus, neutron emission, B-2N | -33,040 keV | 8,161 keV | — |
| Ge-90 | — | — | Beta-minus decay (100%), B-2N, Beta-minus, neutron emission | -28,470 keV | 8,109 keV | — |