With the CloudeChamber professional cloud chamber, you can observe the trails of alpha particles, beta particles, and cosmic rays with the naked eye. We deliver scientific experiences for schools, research institutes, and science centers.
Every second, hundreds of cosmic rays pass through your body — invisibly. The cloud chamber is the only device that lets you observe the imprints of the subatomic world with the naked eye.
The cloud chamber (Wilson chamber) is a particle physics detector invented by Scottish physicist Charles Thomson Rees Wilson in 1911, for which he received the Nobel Prize in 1927.
The device is a chamber filled with supersaturated alcohol vapor, in which ionizing radiation leaves visible condensation trails. You can observe with the naked eye the thick, straight tracks of alpha particles, the thin, winding paths of beta particles, and the long, traversing lines of cosmic rays.
Not a simulation. Not an animation. Real particles, in real time.
Cosmic ray trails — left by muons arriving from space
The characteristic thick, straight tracks of alpha particles
The winding trail of beta radiation — electron scattering
The bottom of the chamber is cooled to –30°C using a Peltier element cooler. This creates the supersaturated vapor inside the chamber. No dry ice needed — just a power source.
Isopropyl alcohol vapor fills the chamber. A supersaturated zone forms above the cold layer — this is the medium in which particles leave their trails.
When a charged particle passes through the vapor, it leaves ions in its wake. These ions act as condensation nuclei — this is where the alcohol vapor condenses.
The alcohol vapor condenses onto the ions — tiny droplets trace the particle's path. Visible to the naked eye, in real time! Alpha, beta, and cosmic rays each leave distinct tracks.
— Charles Thomson Rees Wilson, Nobel Prize-winning physicist
Thick, short, straight tracks. Two protons and two neutrons — helium-4 nuclei. They ionize strongly but have a short range.
α | He-4 nucleusThin, winding tracks. High-speed electrons or positrons. They are easily deflected by atoms — hence the erratic path.
β | e− electronLong, traversing tracks. High-speed muons arriving from outer space. They cross the entire chamber — multiple times per second.
μ | muonFor primary and secondary schools
For science centers and institutional use
For universities and research institutes
Peltier element cooling — turn it on, 15 minutes and it works. No need to deal with dry ice logistics.
The entire class can see the particle tracks magnified, on a projector or monitor simultaneously.
Experiment guide booklet, lesson plans, and worksheets aligned with the national core curriculum.
Complete on-site installation, training, and if any issues arise — we are there within 48 hours.
The ResearchChamber software automatically identifies particle types and measures their energy.
The Am-241 source activity is below the exemption threshold. Safe to use in a school environment.
"The students couldn't believe they were seeing real particles at first. When they understood that cosmic rays pass through them every second — that aha moment was unforgettable. Physics class has never been this alive."
"The cloud chamber has become our most popular exhibit. Visitors are expected to spend an average of 15 minutes at the cloud chamber — in practice they stay for 40 minutes. The top camera + projection solution is brilliant, everyone can see the particle tracks."
"The ResearchChamber's AI-based track analysis is revolutionary. Students don't need to perform manual measurements — the software automatically identifies the particle type, measures the energy, and exports the data. Perfect for both research and education."
It is not dangerous. The EduChamber package's Am-241 source (derived from smoke detectors) has extremely low activity, well below the exemption thresholds. The chamber also displays background radiation and cosmic rays — no additional source is needed for this. It can be safely used in a school environment.
The EduChamber and ScienceChamber packages use Peltier element cooling — no dry ice needed. It only requires a power source (230V). After turning on, it reaches operating temperature in 10-15 minutes and remains continuously operational.
Very well. The chamber's LED side illumination provides optimal contrast. In a dark room (with curtains drawn), the tracks are excellently visible. With the ScienceChamber package, the top camera + projector solution allows 30+ people to watch magnified simultaneously.
Yes. The EduChamber includes 12, the ScienceChamber 12, and the ResearchChamber 24 months of warranty. For the Pro and Research packages, on-site service within 48 hours is available. Remote support is unlimited for all packages.
Standard level: atomic physics, radioactivity, types of radiation (national curriculum). Advanced level: particle physics, cosmic rays, motion in magnetic fields. University: nuclear physics lab, particle physics practicum, detector technology. We include the experiment guide booklet and lesson plans aligned with the national curriculum.
Due to its size and ease of use, the EduChamber package is suitable for home scientific experimentation as well. However, it was primarily developed for educational institutions where teacher guidance and professional support are ensured.
Contact us and we will prepare a personalized quote within 24 hours. On-site demonstrations are also available.