Lab Equipment
Spectroscope reference, inverse band-matching, and UV fluorescence interpretation: the three lab-instrument tools used alongside RI and SG to confirm a gemmological identification.
Chelsea Filter
Expected colour reactions for gem identification
The Chelsea filter transmits deep red and yellow-green light, filtering out other wavelengths. Chromium-bearing gems fluoresce red.
Emerald (Natural Colombian)
Chrome-coloured emeralds fluoresce
Emerald (Natural Zambian)
Iron-rich, less chromium
Emerald (Synthetic)
Often brighter than natural
Ruby (Natural)
Chromium fluorescence
Sapphire (Blue)
No chromium, no reaction
Synthetic Blue Spinel
Cobalt-coloured shows red
Synthetic Green Glass
Chromium in glass
Alexandrite
Strong chromium content
Jadeite (Natural)
Dyed jadeite may show pink
Peridot
Iron-coloured, no reaction
Diamond
No reaction expected
Important Limitations
- • Not definitive: Chelsea filter alone cannot prove natural vs synthetic
- • Origin matters: Different emerald sources react differently
- • Lighting critical: Use strong light source for best results
- • Combine tests: Always use with other identification methods
How It Works
The Chelsea filter is a didymium glass filter that transmits deep red (around 690nm) and yellow-green (around 570nm) light. Gems containing chromium fluoresce under the filter, appearing red or pink. This is especially useful for screening emeralds and detecting some synthetic stones.
Spectroscope Calculator
Wavelength ↔ colour converter and absorption line reference
Enter a wavelength (380-780nm) to see its colour, or browse common absorption lines by gem.
Common Absorption Lines (15)
Ruby
StrongChromium doublet at 694.2 and 692.9nm
Ruby
MediumBroad band
Ruby
MediumFine line
Emerald
WeakChromium line
Emerald
WeakChromium doublet
Alexandrite
StrongChromium doublet
Jadeite (Green)
MediumChromium (dyed may show)
Demantoid Garnet
StrongCharacteristic horsetail band
Zircon
StrongUranium lines
Diamond (Yellow)
MediumCape series
Peridot
StrongIron triplet
Peridot
StrongCentral line of triplet
Peridot
StrongIron triplet
Sapphire (Blue)
MediumIron-titanium
Aquamarine
WeakIron absorption
Spectroscope Usage
- • Use a strong white light source for best results
- • Absorption lines appear as dark bands against bright spectrum
- • Some gems show many lines, others show few or none
- • Position matters - some lines only visible in certain orientations
Spectroscope Band Matcher
Tick observed absorption bands to rank candidate species
Tick every absorption line you can see in the spectroscope. The reasoner ranks species whose stored band patterns match. Selective (diagnostic) bands are weighted more heavily.
Observed bands
UV Fluorescence Lookup
Match observed long-wave / short-wave UV reactions to gem species
Observe the stone under both long-wave (365 nm) and short-wave (254 nm) UV in a darkened cabinet and report what you see. The reasoner ranks species whose stored fluorescence text matches your observation.
Long-wave (365 nm)
Short-wave (254 nm)
Heavy Liquid Reference
SG separation guide by liquid density
Heavy liquids separate gems by specific gravity. Select a liquid to see which gems float or sink.
Heavy Liquids
Gem SG Reference
⚠️ Safety Warning
- • Heavy liquids are highly toxic - avoid skin contact and fumes
- • Always use gloves, safety glasses, and work in a fume hood
- • Store in sealed containers away from light (causes decomposition)
- • Never use with porous or fractured stones - liquid can be absorbed
- • Dispose of according to hazardous waste regulations
Alternative: Hydrostatic Weighing
For most gem identification, hydrostatic weighing (measuring weight in air vs water) is safer and more accurate than heavy liquids. Heavy liquids are mainly used for quick separation of parcels or when hydrostatic equipment isn't available.
About these lab tools & methodology
The spectroscope records which wavelengths of visible light a gem absorbs. Strong selective absorption bands are diagnostic: the 693 nm doublet in ruby, the 450 nm band in synthetic blue spinel, the 415 nm line in cape diamonds. Each species produces a characteristic pattern determined by the transition-metal impurities or rare-earth elements present in its crystal structure. The spectroscope calculator on this page displays the expected absorption pattern for 16 commonly encountered gem species, drawing from a curated reference table that lists band positions, relative strengths, and the diagnostic significance of each line. Viewing known patterns before working at the bench helps calibrate the eye and sets a reliable expectation for what a positive identification looks like.
The band-matcher inverts this workflow. Rather than looking up a known species and reading off its bands, you enter the wavelengths you actually observe and the tool returns the species whose reference pattern best matches your input. Matching is tolerance-windowed; a band recorded at 692 nm will still match the 693 nm ruby reference, and selective diagnostic bands are weighted more heavily than broad general-absorption regions. This makes the band-matcher especially useful when a stone shows one strong diagnostic line alongside several weaker features that might be confused for another species. The output lists confidence-ranked candidates, not a single forced answer, which mirrors the conditional reasoning a trained gemmologist applies at the bench.
UV fluorescence adds a complementary data point without any contact with the stone. A strong blue long-wave (LWUV) reaction in diamond, absent under short-wave (SWUV), points away from moissanite or cubic zirconia. Conversely, a strong SWUV reaction with weak or absent LWUV is characteristic of certain synthetic ruby flux products. The UV fluorescence lookup parses the freeform fluorescence descriptions stored in the mineral database (for example, "inert to strong blue LWUV, weak yellow SWUV") into structured fields: LWUV colour and intensity, SWUV colour and intensity, and a phosphorescence flag for materials such as natural hyalite opal that continue to glow after the UV source is removed. Intensity is scored on a four-step scale (inert, weak, moderate, strong) to allow ranked comparison across species.
Together the spectroscope and UV fluorescence instruments cover complementary parts of the electromagnetic spectrum and together with RI and SG they form the core analytical toolkit of the FGA Diploma practical examination. These tools are designed to function as both learning aids and bench references: they explain the underlying physics, display the reference data, and support the step-by-step reasoning process that moves an observation toward a confident, defensible identification.