Exhibits

 

Orlando Science Center's exhibit halls feature a vast array of exciting interactive experiences! Learning has never been so fun with these hands on educational exhibits. From down to earth explorations in natural science to the high-tech world of simulation technology, everywhere you look, you'll find educational and entertaining opportunities to explore, experiment, and discover.

 

Traveling Exhibits

The Orlando Science Center is home to some of the most exciting traveling exhibits in the country. When these exhibits are in town they are only here for a limited time, so don’t miss the opportunity to see them!

 

Exhibit Halls

As great as our traveling exhibits are, there are some exhibits that are the staple of the Orlando Science Center. NatureWorks will have you up close and personal with some of nature’s most fascinating reptiles. At DinoDigs, you’ll step back into the prehistoric age. Discover the dynamic forces and systems that shape our Earth, as well as other planets in Our Planet, Our Universe. Explore such concepts as electricity and magnetism, lasers, soundwaves, and nature’s forces in Science Park. No visit to the Science Center is complete without a trip to KidsTown, an interactive world dedicated to our smaller explorers.

 

Science Live! Programs

What’s the difference between a great visit to a Science Center and a memorable visit? Live programs. Our exhibits are designed to inspire curiosity and exploration, our Science Live! programs are designed to bring the exhibits to life. Whether it’s a show in the Digital Adventure Theater or a one-to-one interaction with a volunteer at the Crosby Observatory, our live programs create the kind of impact that can last a lifetime.

 

Science Stations

Looking for little more “hard science” in your next Science Center visit? Look no further than the Science Stations located throughout the facility. Science Stations are a cross between exhibits and live programs in that they’re exhibits that typically include a live program to truly bring the experience to life. Science Stations provide an in-depth look at their respective subject matter in an entertaining way. Be sure to check your program schedule to see which Science Stations are conducting demonstrations on the day of your next visit.

 

Crosby Observatory

The aluminum-domed Crosby Observatory atop Orlando Science Center houses Florida's largest publicly accessible refractor telescope. This one-of-a-kind custom-built telescope, along with several smaller scopes, are available at selected times for solar and night sky viewing.

 

Before the invention of telescopes, viewing stars was a difficult task because they blurred together in a white streak formation across the sky. An ancient Greek myth states that this white streak was coined ‘Via Galactica’ or “road made of milk” and is how our galaxy came to be known as the Milky Way.

Milky_Way

Our solar system, along with hundreds of billions of stars, clouds of dust and gases lie throughout our Milky Way Galaxy. Imagine the galaxy like a pancake being stretched, with a huge bulge forming in the center. From there, huge groups of stars and dust particles fan out from the center, generating a spiral of curving, coiled and patterned arms.

Sometimes parts of the Milky Way can be viewed with the naked eye. On very clear, dark nights it appears as a band of milky starlight stretching across the sky. So the next time you look up at the night sky, you will know that the Milky Way is so much more than a candy bar!


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Measuring and evaluating the brightness of stars can be traced back to the Greek astronomer and mathematician Hipparchus during 190 - 120 BC. He is responsible for producing a catalogue of comparative brightness and positioning of over 850 stars. Hipparchus formed the apparent magnitude scale to determine the brightness of a star as seen by an observer from earth.

How does this scale work? The brighter the celestial object appears, the lower the value of its magnitude. For instance, the faintest objects you can see using the naked eye are indicated with a magnitude of 6, while the Sun on the apparent magnitude scale is –26.74. However, most of the stars we gaze at in an urban neighborhood with our eyes are usually somewhere around 3 to 4 and if using binoculars, the limit is 10. More recently, through the use of the powerful Hubble Space Telescope, astronomers have located stars with magnitudes of 30+. It is this basic classification from over 2,000 years ago that led to the magnitude scale that we still use today!


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The sky’s sheer size and beauty takes our breath away, but what exactly makes the sky so blue? Due to a phenomenon coined Rayleigh Scattering, the spectrum of colors ranging from violet to red, either pass through or deflect off of the earth’s atmosphere, which is made up of mostly nitrogen and oxygen. Longer wavelengths of red, yellow and orange colors of the spectrum have little affect on these tiny particles that make up our atmosphere.  However, shorter wavelengths of blue are deflected and are scattered all around us, causing the sky to appear blue no matter where we look.

Our Planet, Our Universe: Earth and Space, opening as a permanent exhibit on September 25, 2010, will provide guests the opportunity to discover and explore black holes, Martian terrain and of course, why our sky is blue. Allow us to beam you up to enjoy the vastness of the cosmos, as well as the complexity of our fascinating planet.

 

Blue_Sky


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Discovered in 1986 by Australian astronomer Malcolm Hartley, comet 103P or Hartley 2 is set for the closest encounter with earth in 24 years. This “dirty snowball” that is comprised of rock, dust, ice and frozen gases was visible in the constellation of Auriga as a fuzzy, green blur to Northern Hemisphere observers during Mid-October.

Through November, Southern Hemisphere stargazers can catch a glimpse of the comet as it travels away from earth, using the naked eye, binoculars and of course, a telescope. This year, Hartley 2 made its closest pass at a mere 11 million miles on October 20th and is calculated to orbit the Sun every 6 ½ years. EPOXI, or Extrasolar Planet Observation and Deep Impact Extended Investigation is a spacecraft that is due to make a flyby of Hartley 2 from only 600 miles away on November 4th. The mission plans to gather information on the comet’s surface and craters, as well as close-up images of dust and gas plumes.

Check back on our web site for "post fly by" information and updates!


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Most folks rarely give much of a thought to Torosaurus, except for the trivia answers to “Which animal has the longest skull of any land creature, ever?” But some people seem to feel inexplicably attached to this name, often and incorrectly translated as "bull lizard" (it's got big horns, and was ornery like a raging bull!). In reality it means "perforated lizard", in reference to the holes in its frill. These innocuously incomplete frill holes are at the center of the newest paleocontroversy, which has some scientists ready to erase the name Torosaurus from the dictionary altogether!

Torosaurus

See also: Obsolete.

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777 E. Princeton Street • Orlando, Florida 32803 • Phone: 407.514.2000 • TTY: 407.514.2005 • Toll Free: 888.OSC.4FUN • Email: gservices@osc.org
  Orlando Science Center is supported by United Arts of Central Florida, host of power2give.org/centralflorida and the collaborative Campaign for the Arts.
This project is funded in part by Orange County Government through the Arts & Cultural Affairs Program. Privacy Policy • Accessibility

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