With the latest projection technology, using real science data,
we bring the real universe to you. Get closer to the wonders of the universe while travelling with us through time and space.
An educative, inspiring, fun and exhilarating trip
that will stick in your mind forever!
"Yet, for most of us, the most memorable sight was not of the moon but of our beautiful blue and white home, moving majestically around the sun, all alone in the infinite black space."
Alan Bean
Fourth person to walk on the moon
Our Space Dome is designed to explore science, astronomy, geology and geography in an interactive way bringing the power of digital planetariums and LIPS methodology (Live, Interactive Planetarium Shows) to children and communities all around the UK. We provide immersive educational experiences that make learning stick! Either if you are looking for the 'wow factor' of a large immersive display environment to entertain large numbers of viewers or want to educate a group in science topics, we are here to help.
Why us? We base our presentations in real scientific data to bring the real universe to our domes. Our projectors can capture real Earth data as well as space data. For example, in our show about Mars we can present the different layers of the planet in a 360 degree view using real scientific data, providing this way a deep study of the planet. We can explore its volcanoes, polar ice caps, canyons and thin clouds obtaining a better understanding of the planet in its three-dimensional structure.
We use the latest projection technology and go beyond simulators to offer an experience that feels real. We focus on quality and learning impact along with showing the wonders of our universe and bringing an exciting experience that the audience will never forget.
Check out our exciting Space Dome Programme below and if you require a specific topic that’s not on the list, just get in touch as we will very likely be able to help.
We'll dive into:
- The planets
- Small bodies: asteroids, comets, meteoroids and dwarf planets.
We will dive into a space exploration with our focus on Jupiter, Saturn, the moon and Apollo Moon missions.
Some of the questions we'll dive into:
-How the eye works and shows us different
colours.
-The rainbow.
-Why do we have daytime and night-time?
-How do we know so much about the stars?
-Why do the stars have different colours and
brightness?
How your ear drums work to hear sound? What sound looks like, how your eyes work to capture the light and how images are created?
Deep into light and sound with us in this interactive and immersive session.
Explore and learn how sound and light travel. Get to ‘see’ sound in many different ways. Learn about rainbow and colours; refraction and reflection and much more. We’ll use examples from solar system with the moon and sun in 3D.
We travel the constellations of the autumn sky and the ancient Greek myths after which they were named. A mixture of mythological stories together with real science in the sky and space. The constellations are used in science as a map to the sky allowing the location of black holes, alien solar systems and star clusters and galaxies to be explored.
Covering climate, ocean currents, ocean life and the changing world.
An immersive fulldome program that explores the inner workings of Earth’s climate engine. With visualizations based on satellite monitoring data and advanced supercomputer simulations, this cutting-edge production follows a trail of energy that flows from the Sun into the interlocking systems that shape our climate: the atmosphere, oceans, and the biosphere.
Audiences will ride along on swirling ocean and wind currents, dive into the heart of a monster hurricane, come face-to-face with sharks and gigantic whales, and fly into roiling volcanoes. Year 3 to adult age range.
'Introduction to Stargazing' uses all the projectors below to give a star field and tour of the night's sky.
The Science Dome has three star projectors which project a star field on the inner surface of the dome. The purpose is to demonstrate how the sky appears in the night sky and also how to observe various planets and shooting stars.
One star projector is produced using a computer with state of the art Stellarium software. This can also be downloaded and used on a PC desktop. Visit the link below.
The other two projectors use actual film of the real night sky and project a star field accurately with 10,000 stars. The star field moves across the dome also showing shooting stars and the moon.
‘Oasis in Space’ transports the audience on a startling and beautiful voyage through our universe, galaxy and solar system in search of liquid water, a key ingredient for life on Earth. Suitable for Year 5 to adult age range.
The formation of the early universe, star birth and death, collision of giant galaxies and black holes.
Suitable for year 5 to adult.
We will learn about how different habitats (including micro-habitats) provide for the basic needs of different kinds of animals and plants, and how they depend on each other.
We will also look into describing and understanding key aspects of:
Physical geography, including: climate zones, biomes and vegetation belts, rivers, mountains, volcanoes and earthquakes, and the water cycle.
Human geography, including: types of settlement and land use, economic activity including trade links, and the distribution of natural resources including energy, food, minerals and water.
Including elements such as underwater volcanoes, bioluminescence and tides.
Under the Sea:
We learn that many years ago sailing boats used to follow the stars for navigation. We take a journey on a boat and then go under the sea. We'll listen many stories by sailors about life in the sea, and much more!
Start journey to the bottom of the sea by a submarine and back again. The planetarium shows the Australian landscape and the Australian stars and refers to the southern cross and compass using the constellations. The Great Barrier reef and other under the sea locations are shown.
Pirates and the Sea:
'Pirates show with many ship wrecks. Pictures of sailing ships, pirates ships and flags from a 360 degree view. Australian stars and the southern cross and compass will be also covered.
We have pictures of caves and rocks which can be used for smuggling.
Minibeast:
We will learn and explore the world of minibeast. Minibeasts are small invertebrates and include arthropods such as spiders, insects, woodlice, centipedes and millipedes, as well as slugs and snails and worms.
Tropical Reefs:
Learn the secrets of the "rainforests of the sea" as you and your visitors embark on an oceanic safari to the world’s most vibrant — and endangered — marine ecosystems.
Learn about the biology of corals, and how reefs support some of the planet's most complex food webs.
Endangered animals:
The natural environment.
What are endangered animals?
Why are some species in danger?
• Habitat Loss (Destruction and Fragmentation)
• Invasive Species
• Pollution
• Poaching
• Overuse
Science: Recognise that the population of some animals/species are in danger of becoming extinct through loss of habitat, decline in food source or persecution for example.
The interdependence of living organisms and food chains.
How humans affect the local environment.
Geography: Causes and consequences of how places and environments change - Living in my world: caring for places and environments and the importance of being a global citizen.
How can we help prevent the extinction of endangered animals?
We will explore the topic of endangered animals in our 360 degrees mobile planetarium and invite children to reflect on the importance of keeping a balanced ecosystem. From tiny species to the biggest creatures, they all contribute to the equilibrium of nature.
Ecosystems are groups of plants and animals that are found in the same area and interact with each other bringing a healthy state to the ecosystems when they act in harmony. Each species that is lost triggers the loss of other species within its ecosystem. Plants, animals and all type of micro-organism bring balance to the ecosystem (forests, grasslands, rivers, oceans…) maintaining it healthy. Preserving wildlife helps not only to the ecosystem but also provides cures to deadly diseases, purifies environment (clean air, water and land). Allowing our environment to become contaminated, we risk our own health.
Healthy forests, grasslands, rivers, oceans… are the result of a balanced ecosystem.
Adaptation and evolution. In “Natural Selection” we will join Darwin on his voyage with the HMS Beagle to the Galapagos Islands where he was inspired to develop his later theory of transmutation by natural selection. Join us in the thrill of a scientific discovery, the adventure of science and the beauty of nature.
Start of life on Earth and possible life in the solar system.
We will learn about Earth's ancient history by looking at the planet from space and then showing the pictures of the surface changing through time.
Pupils will learn the following;
The award-winning Supervolcanoes looks back at rare classes of eruptions that have marshaled the energy that lurks, like a sleeping dragon, beneath the surface of planet Earth. The program moves beyond Earth to explore the impact of giant volcanic eruptions around our solar system.
Audiences will fly down to Neptune’s frigid moon Triton, and onto the ultimate volcanic world: Jupiter’s moon Io. On a visit to a legendary North American hot spot, Yellowstone National Park, the film asks: can a supervolcano erupt in our time?
Narrated by Benedict Cumberbatch.
Bournemouth, Wimborne (Dorset), Brighton, Trowbridge, London, Leeds, and Newark in Nottinghamshire covering the whole of the UK and EIRE.
Contact us for further information and bookings on 01202304734, send us an email to sciencedome@ntlworld.com,
or alternatively click the bottom down below and fill in the form. We will get in touch with you soon after we receive your request.
Got a question? We’re here to help.
We cover all the UK and EIRE on request. In some ocassions a travel and/or hotel supplement might be applied if we are required to travel a distance from a base.
Get in touch and we will give you a free quote.
The Science Dome operates eleven mobile digital domes . The dimensions of these domes go from 5-8 meters diameter and 3-5 meters height. Being able to provide different sizes and designs to fit all school and village halls.
For the “wow” factor of a large immersive display environment to entertain large numbers of viewers at a show (or other such venue) our immersive 8m diameter domes would be the ideal match. Being 5.2 metres high, this dome offers a large feature in any show.
Our domes provide different sizes and designs to cater to your needs. Their capacity rank from 25-50 adults till 35-60 primary children in a session.
Get in touch, we will give you a precise feedback according to the type of audience or students' age to help with the organisation.
Of course you can.
Get in touch and we will help you organise the sessions.
Check out our other domes: Dinosaur Dome, Fractals Dome and Bio Dome to explore deeper all the different topics we can cover.
For Schools Service:
Full day visit cost ranges £530 (excluding VAT) with a typical day including up to five class shows.
Half day costs for three shows is £430.
We may charge extra for a sixth show during the day. If your school is located near one of our dome bases (see below), then we may be able to come for a half day. Please apply for half day rates if the case.
Please be aware that we charge a travel and hotel supplement if we are required to travel a distance from a base.
For Youth Clubs, Scout Groups and Adults Groups:
Prices start from £175 per session (an hour). Please contact us and will give you a totally free quote according to the type of service you require.
For Outdoor Events:
The cost for a smaller 25 person size dome (30 with children) is £750 per day, plus VAT and travel costs.
The cost for the giant dome version 40 person dome (45 with children) is £950 per day, plus VAT and travel costs.
Please be aware that the cost reflects a two-man operation.
Both domes come with limited soft benches (seating 10 to 15), with cushions for the remaining space.
If cost is a problem and you are a school fair organiser, for schools fairs we may be able to earn an income for the school by a modest audience charge, with our spilt fees facility. No charge (as above) for booking but we charge the public on entrance and spilt the fees. Only available for schools to support in south of England, Hants and Dorset, travel and hire cost apply to rest of UK.
Because sound is just vibrating air and space has no air, sound has no medium or way to travel to be heard. If you were sitting in a space ship and another space ship exploded, you wouldn’t hear a thing!
Outer space is not completely empty. Even if it is nearly a perfect vacuum, it still contains something: low density of particles (predominantly hydrogen and helium), electromagnetic radiation, magnetic fields, neutrinos, dust, and cosmic rays.
The molecules present on Earth’s atmosphere scatter light from the sun off in all directions, including towards our eyes, resulting in the blue sky we see on the daytime. However, at night, when that part of Earth faces away from the Sun, space looks black because there is no nearby bright source of light, like the Sun, to be scattered. Now, in the absence of matter like in the outer space, with very few particles, there’s nothing between stars and planets to scatter light to our eyes. That’s why, from the moon, which has no atmosphere, the sky looks black day and night.
Learn more about this at https://starchild.gsfc.nasa.gov/docs/StarChild/questions/
A new experiment has revealed that oxygen atoms cling tightly to stardust, preventing them from joining together to form oxygen molecules. Read more about it on https://www.science.org
In the early universe, there were no galaxies. Today, there are many billions. Astronomers use the fundamental laws of physics to deduce the basic story of galaxy formation. Galaxies form out of immense clouds of gas that collapse and rotate. As they evolve, stars form within them. Entire galaxies can collide, changing their appearance. Looking deep into space, we see galaxies at earlier stages in their lives, and learn more about their evolution.
Our Sun is four and a half billion years old and about halfway through its life. In 5 billion years time , the Sun will become a red giant. That means the Sun will get bigger and cooler at the same time. When that happens, it will be different than the Sun we know today. As a red giant, our Sun will become about 2,000 times brighter than it is now!
Read more about it on https://spaceplace.nasa.gov/sun-age
According to NASA, one would have to explode 100 billion tons of dynamite every second to match the energy produced by the sun!
Read more about it on https://www.nasa.gov
Eventually, the fuel of the sun, hydrogen, will run out. When this happens, the sun will begin to die. After the hydrogen runs out, there will be a period of 2-3 billion years whereby the sun will go through the phases of star death. Once the hydrogen runs out, our yellow dwarf star will begin to swell. It will swell to a size that will cause it to swallow Mercury, Venus, and Earth. It may even grow to overtake more of the planets. When the sun increases in size it will become a “red giant.” After this, it will lose many of its outer layers and eventually shrink to become a “white dwarf.” White dwarf stars are still very hot, but not nearly as hot as the sun is now. Finally, our star will fade out and become a “black dwarf,” where very little is left of its original form. Black dwarf stars are not hot and don’t put off any energy.
Read more about it on https://askanearthspacescientist.asu.edu/top-question/sun-dying
Venus rotates very slowly on its axis – one day on Venus lasts 243 Earth days. The planet orbits the Sun faster than Earth, however, so one year on Venus takes only about 225 Earth days, making a Venusian day longer than its year!
Read more about it on
Venus is hotter than Mercury because it has a much thicker atmosphere. Mercury is closer to the Sun but it has a very thin atmosphere and all the heat trapped goes out in space, while Venus with its much thicker atmosphere holds all the heat it gets.
Read more about it on https://www.vedantu.com/question-answer/which-is-the-hottest-planet-of-the-solar-system
And our planet Earth 4.543 billion years old.
Fossil discoveries point out that the earliest life forms were microorganisms (microbes).
And of course, what they do for our planet is amazing. They are the Earth's lungs!
Venus is permanently shrouded in thick, toxic clouds of sulfuric acid that start at an altitude of 28 to 43 miles (45-70 km).
The clouds smell like rotten eggs!
Mercury is one of the rocky planets along with Venus, Earth, and Mars. It has a solid surface that is covered with craters. In fact the surface looks very much like the moon.
Being so close to the sun, you might find it strange that Mercury could harbor any surface ice at all. But some parts of Mercury receives very little direct sunlight, and some craters remain constantly in the dark.
Many people get confused about comets, asteroids, meteoroids and meteors. We are going to explain them all here so that we can avoid getting lost in space!
Comets are leftovers from the dawn of our solar system around 4.6 billion years ago, and consist mostly of ice coated with dark organic material. That's why they are called cosmic snowballs. They are made of frozen gases, rock, and dust and they orbit the Sun. They have been referred to as "dirty snowballs." When frozen, they are the size of a small town. When a comet's orbit brings it close to the Sun, it heats up and spews dust and gases into a giant glowing head larger than most planets. The dust and gases form a tail that stretches away from the Sun for millions of miles. There are likely billions of comets orbiting our Sun in the Kuiper Belt and even more distant Oort Cloud.
The current number of known comets is: 3,856
Comets may yield important clues about the formation of our solar system. Comets may have brought water and organic compounds, the building blocks of life, to the early Earth and other parts of the solar system.
Asteroids, sometimes called minor planets, are rocky, airless remnants left over from the early formation of our solar system about 4.6 billion years ago. Their sizes range from 1 meter to hundreds of kilometers.
The majority of known asteroids orbit within the asteroid belt between Mars and Jupiter (the main asteroid belt), others share a planet's orbit around the Sun. It is currently believed that at least 5,000 asteroids cross the Earth's orbit, some coming very close (Near-Earth Asteroids). Large asteroids and comets hit the Earth only once every 100 million years or so, not something that happens very often!
Asteroids usually revolve around the Sun in elliptical orbits, but sometimes they can rotate quite erratically, tumbling as they go. More than 150 asteroids are known to have a small companion moon (some have two moons). There are also binary (double) asteroids, in which two rocky bodies of roughly equal size orbit each other, as well as triple asteroid systems.
The current known asteroid count is: 1,266,738.
Meteoroids are very small asteroids, with sizes between microns to 1 meter.
When meteoroids enter Earth’s atmosphere (or that of another planet, like Mars) at high speed and burn up, the fireballs or “shooting stars” are called meteors.
When a meteoroid survives a trip through the atmosphere and hits the ground, it’s called a meteorite.
Scientists estimate that about 48.5 tons of meteoric material falls on the Earth each day. Almost all the material is vaporized in Earth's atmosphere, leaving a bright trail fondly called "shooting stars."Several meteors per hour can usually be seen on any given night. When there are lots more meteors, you’re watching a meteor shower.
Learn more at
https://solarsystem.nasa.gov/asteroids-comets-and-meteors/comets/overview
All eight planets of the Solar System follow an anti-clockwise path around the Sun. Our solar system formed about 4.5 billion years ago from the collapse of a huge cloud of gas and dust. As it collapsed, it formed a solar nebula – a spinning, swirling disk of material. Collisions between dust and friction within the gas would drag material into the same motions as the majority of the gas and dust. At the center, gravity pulled more and more material in. Eventually, the pressure in the core was so great that hydrogen atoms began to combine and form helium, releasing a tremendous amount of energy. With that, our Sun was born, and it eventually amassed more than 99% of the available matter.
Matter farther out in the disk was also clumping together. These clumps smashed into one another, forming larger and larger objects. Some of them grew big enough for their gravity to shape them into spheres, becoming planets, dwarf planets, and large moons. In other cases, planets did not form: the asteroid belt is made of bits and pieces of the early solar system that could never quite come together into a planet. Other smaller leftover pieces became asteroids, comets, meteoroids, and small, irregular moons.
The general revolution of the disc would transfer to the rotating planets and to the Sun itself.
Most of the angular momentum of the Solar System is in the outer planets, both in rotation and orbital motion.
The Sun itself rotates very slowly, about once a month, while Jupiter and Saturn rotate once every ten hours.
More about this at
https://solarsystem.nasa.gov/solar-system/our-solar-system
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