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Your next party could be out of this world

Having an event at the W.A. Gayle Planetarium is a way to ensure that your event will be remembered for a while. No one expects a meeting to be held in a planetarium, what a way to get the meeting off to great start.

You can rent the planetarium and host your own party in the lobby, and then be treated to a show of your choosing in the auditorium. We can also accommodate meetings in the auditorium. With over 200 seats, the planetarium offers an excellent venue to host your next office meeting. Custom presentations can be shown on the dome ensuring everybody has the best seat in the house.

Call us at (334) 241-4799 for details.

 

The Planets

 














What exactly is a Planet?

A planet is defined as any of the nine (still being debated) large celestial bodies in the solar system that revolve around the sun and shine by reflected light

According to the International Astronomical Union, there are eight planets and five dwarf planets in the Solar System. In increasing distance from the Sun, these planets are:

  1. Mercury
  2. Venus
  3. Earth
  4. Mars
  5. Jupiter
  6. Saturn
  7. Uranus
  8. Neptune

Jupiter is the largest, at 318 Earth masses, while Mercury is smallest, at 0.055 Earth masses. As you have probably already correctly guessed, Earth has an Earth mass of 1.0… kinda pointless to explain but the facts are here for you anyway.



Mercury

Mercury is the innermost and smallest planet in the Solar System, orbiting the Sun once every 87.969 days. The orbit of Mercury has the highest eccentricity of all the Solar System planets, and it has the smallest axial tilt. It completes three rotations about the axis for every two orbits. The perihelion of Mercury's orbit precesses around the Sun at an excess of 43 arcseconds per century; a phenomenon that was explained in the 20th century by Albert Einstein's General Theory of Relativity. Mercury is bright when viewed from Earth, ranging from -2.0 to 5.5 in apparent magnitude, but is not easily seen as its greatest angular separation from the Sun is only 28.3°. Since Mercury is normally lost in the glare of the Sun, unless there is a solar eclipse, Mercury can only be viewed in morning or evening twilight.

Comparatively little is known about Mercury; ground-based telescopes reveal only an illuminated crescent with limited detail. The first of two spacecraft to visit the planet was Mariner 10, which mapped only about 45% of the planet’s surface from 1974 to 1975. The second is the messenger spacecraft, which mapped another 30% during its flyby of January 14, 2008. messenger will make one more pass by Mercury in 2009, followed by orbital insertion in 2011, and will then survey and map the entire planet.

Mercury is similar in appearance to the Moon: it is heavily cratered with regions of smooth plains, has no natural satellites and no substantial atmosphere. However, unlike the moon, it has a large iron core, which generates a magnetic field about 1% as strong as that of the Earth. It is an exceptionally dense planet due to the large relative size of its core. Surface temperatures range from about 90 to 700 K (-183 °C to 427 °C, -297 °F to 801 °F), with the subsolar point being the hottest and the bottoms of craters near the poles being the coldest.

Recorded observations of Mercury date back to at least the first millennium BC. Before the 4th century BC, Greek astronomers believed the planet to be two separate objects: one visible only at sunrise, which they called Apollo; the other visible only at sunset, which they called Hermes. The English name for the planet comes from the Romans, who named it after the Roman god Mercury, which they equated with the Greek Hermes. The astronomical symbol for Mercury is a stylized version of Hermes' caduceus.


 

 

Venus

 

Venus is the second-closest planet to the Sun, orbiting it every 224.7 Earth days. The planet is named after Venus, the Roman goddess of love. After the Moon, it is the brightest natural object in the night sky, reaching an apparent magnitude of -4.6. Because Venus is an inferior planet from Earth, it never appears to venture far from the Sun: its elongation reaches a maximum of 47.8°. Venus reaches its maximum brightness shortly before sunrise or shortly after sunset, for which reason it is often called the Morning Star or the Evening Star.

Classified as a terrestrial planet, it is sometimes called Earth's sister planet because they are similar in size, gravity, and bulk composition. Venus is covered with an opaque layer of highly reflective clouds of sulfuric acid, preventing its surface from being seen from space in visible light. Venus has the densest atmosphere of all the terrestrial planets, consisting mostly of carbon dioxide, as it has no carbon cycle to lock carbon back into rocks and surface features, nor organic life to absorb it in biomass. A younger Venus is believed to have possessed Earth-like oceans, but these totally evaporated as the temperature rose, leaving a dusty dry desertscape with many slab-like rocks. The water has most likely dissociated, and, because of the lack of a planetary magnetic field, the hydrogen has been swept into interplanetary space by the solar wind. The atmospheric pressure at the planet's surface is 92 times that of the Earth.

Venus's surface was a subject of speculation, until some of its secrets were revealed by planetary science in the twentieth century. It was finally mapped in detail by Project Magellan in 1990–91. The ground shows evidence of extensive volcanism, and the sulfur in the atmosphere may indicate that there have been some recent eruptions. However, it is an enigma why no evidence of lava flow accompanies any of the visible caldera. There are a low number of impact craters, demonstrating that the surface is relatively young, approximately half a billion years old. There is no evidence for plate tectonics, possibly because its crust is too strong to subduct without water to make it less viscous. Instead, Venus may lose its internal heat in periodic massive resurfacing events.


 

Earth

 

Earth is the third planet from the Sun. It is the fifth largest of the eight planets in the solar system, and the largest of the terrestrial planets (non-gas planets) in the Solar System in terms of diameter, mass and density. It is also referred to as the World, the Blue Planet, and Terra.

Home to millions of species, including humans, Earth is the only place in the universe where life is known to exist. The planet formed 4.54 billion years ago, and life appeared on its surface within a billion years. Since then, Earth's biosphere has significantly altered the atmosphere and other abiotic conditions on the planet, enabling the proliferation of aerobic organisms as well as the formation of the ozone layer which, together with Earth's magnetic field, blocks harmful radiation, permitting life on land. The physical properties of the Earth, as well as its geological history and orbit, allowed life to persist during this period. The world is expected to continue supporting life for another 1.5 billion years, after which the rising luminosity of the Sun will eliminate the biosphere.

Earth's outer surface is divided into several rigid segments, or tectonic plates, that gradually migrate across the surface over periods of many millions of years. About 71% of the surface is covered with salt-water oceans, the remainder consisting of continents and islands; liquid water, necessary for all known life, is not known to exist on any other planet's surface.[note 5][note 6] Earth's interior remains active, with a thick layer of relatively solid mantle, a liquid outer core that generates a magnetic field, and a solid iron inner core.

Earth interacts with other objects in outer space, including the Sun and the Moon. At present, Earth orbits the Sun once for every roughly 366.26 times it rotates about its axis. This length of time is a sidereal year, which is equal to 365.26 solar days. The Earth's axis of rotation is tilted 23.4° away from the perpendicular to its orbital plane, producing seasonal variations on the planet's surface with a period of one tropical year (365.24 solar days). Earth's only known natural satellite, the Moon, which began orbiting it about 4.53 billion years ago, provides ocean tides, stabilizes the axial tilt and gradually slows the planet's rotation. Between approximately 4.1 and 3.8 billion years ago, asteroid impacts during the Late Heavy Bombardment caused significant changes to the surface environment.

Both the mineral resources of the planet, as well as the products of the biosphere, contribute resources that are used to support a global human population. The inhabitants are grouped into about 200 independent sovereign states, which interact through diplomacy, travel, trade and military action. Human cultures have developed many views of the planet, including personification as a deity, a belief in a flat Earth or in Earth being the center of the universe, and a modern perspective of the world as an integrated environment that requires stewardship.


 

Mars

 

Mars is the fourth planet from the Sun in the Solar System. The planet is named after Mars, the Roman god of war. It is also referred to as the Red Planet because of its reddish appearance, due to iron oxide prevalent on its surface.

Mars is a terrestrial planet with a thin atmosphere, having surface features reminiscent both of the impact craters of the Moon and the volcanoes, valleys, deserts and polar ice caps of Earth. It is the site of Olympus Mons, the highest known mountain in the Solar System, and of Valles Marineris, the largest canyon. Furthermore, in June 2008 three articles published in Nature, presented evidence of an enormous impact crater in Mars's northern hemisphere, 10,600 km long by 8,500 km wide, or roughly four times larger than the largest impact crater yet discovered, the South Pole-Aitken basin. In addition to its geographical features, Mars' rotational period and seasonal cycles are likewise similar to those of Earth.

Until the first flyby of Mars by Mariner 4 in 1965, many speculated that there might be liquid water on the planet's surface. This was based on observations of periodic variations in light and dark patches, particularly in the polar latitudes, which looked like seas and continents, while long, dark striations were interpreted by some observers as irrigation channels for liquid water. These straight line features were later proven not to exist and were instead explained as optical illusions. Still, of all the planets in the Solar System other than Earth, Mars is the most likely to harbor liquid water, and perhaps life. Radar data from Mars Express and the Mars Reconnaissance Orbiter, have revealed the presence of large quantities of water ice both at the poles and at mid-latitudes. The Phoenix Mars Lander directly sampled water ice in shallow martian soil on July 31, 2008.

Mars is currently host to three functional orbiting spacecraft: Mars Odyssey, Mars Express, and the Mars Reconnaissance Orbiter. With the exception of Earth, this is more than any planet in the Solar System. The surface is also home to the two Mars Exploration Rovers, Spirit and Opportunity and several inert landers and rovers, both successful and unsuccessful. The Phoenix lander recently completed its mission on the surface. Geological evidence gathered by these and preceding missions suggests that Mars previously had large-scale water coverage, while observations also indicate that small geyser-like water flows have occurred during the past decade.[12] Observations by NASA's Mars Global Surveyor show evidence that parts of the southern polar ice cap have been receding.

Mars has two moons, Phobos and Deimos, which are small and irregularly shaped. These may be captured asteroids, similar to 5261 Eureka, a Martian Trojan asteroid. Mars can be seen from Earth with the naked eye. Its apparent magnitude reaches -2.9, a brightness surpassed only by Venus, the Moon, and the Sun, although most of the time Jupiter will appear brighter to the naked eye than Mars. Mars has an average opposition distance of 78 million km, but can come as close as 55.7 million km during a close approach, such as occurred in 2003.


 

Jupiter

 

Jupiter is the fifth planet from the Sun and the largest planet within the Solar System. It is a gas giant with a mass slightly less than one-thousandth that of the Sun but is two and a half times the mass of all of the other planets in our Solar System combined. Jupiter is classified as a gas giant along with Saturn, Uranus and Neptune. Together, these four planets are sometimes referred to as the Jovian planets.

The planet was known by astronomers of ancient times and was associated with the mythology and religious beliefs of many cultures. The Romans named the planet after the Roman god Jupiter. When viewed from Earth, Jupiter can reach an apparent magnitude of -2.8, making it on average the third-brightest object in the night sky after the Moon and Venus. Mars can briefly exceed Jupiter's brightness at certain points in its orbit.

Jupiter is primarily composed of hydrogen with a quarter of its mass being helium; it may also have a rocky core of heavier elements. Because of its rapid rotation, Jupiter's shape is that of an oblate spheroid, it possesses a slight but noticeable bulge around the equator. The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries. A prominent result is the Great Red Spot, a giant storm that is known to have existed since at least the 17th century when it was first seen by telescope. Surrounding the planet is a faint planetary ring system and a powerful magnetosphere. There are also at least 63 moons, including the four large moons called the Galilean moons that were first discovered by Galileo Galilei in 1610. Ganymede, the largest of these moons, has a diameter greater than that of the planet Mercury.

Jupiter has been explored on several occasions by robotic spacecraft, most notably during the early Pioneer and Voyager flyby missions and later by the Galileo orbiter. The most recent probe to visit Jupiter was the Pluto-bound New Horizons spacecraft in late February 2007. The probe used the gravity from Jupiter to increase its speed. Future targets for exploration in the Jovian system include the possible ice-covered liquid ocean on the moon Europa.


 

Saturn

 

Saturn is the sixth planet from the Sun and the second largest planet in the Solar System, after Jupiter. Saturn, along with Jupiter, Uranus and Neptune, is classified as a gas giant. Together, these four planets are sometimes referred to as the Jovian, meaning Jupiter-like, planets.

Saturn is named after the Roman god Saturn (that became the namesake of Saturday), equated to the Greek Kronos (the Titan father of Zeus) the Babylonian Ninurta and to the Hindu Shani. Saturn's symbol represents the god's sickle.

The planet Saturn is composed of hydrogen, with small proportions of helium and trace elements. The interior consists of a small core of rock and ice, surrounded by a thick layer of metallic hydrogen and a gaseous outer layer. The outer atmosphere is generally bland in appearance, although long-lived features can appear. Wind speeds on Saturn can reach 1,800 kph, significantly faster than those on Jupiter. Saturn has a planetary magnetic field intermediate in strength between that of Earth and the more powerful field around Jupiter.

Saturn has a prominent system of rings, consisting mostly of ice particles with a smaller amount of rocky debris and dust. Sixty-one known moons orbit the planet, not counting hundreds of moonlets within the rings. Titan, Saturn's largest and the Solar System's second largest moon (after Jupiter's Ganymede), is larger than the planet Mercury and is the only moon in the Solar System to possess a significant atmosphere.


 

Uranus

 

Uranus is the seventh planet from the Sun, and the third-largest and fourth most massive planet in the Solar System. It is named after the ancient Greek deity of the sky Uranus the father of Kronos (Saturn) and grandfather of Zeus (Jupiter). Though it is visible to the naked eye like the five classical planets, it was never recognized as a planet by ancient observers because of its dimness and slow orbit. Sir William Herschel announced its discovery on March 13, 1781, expanding the known boundaries of the Solar System for the first time in modern history. Uranus was also the first planet discovered with a telescope.

Uranus is similar in composition to Neptune, and both have different compositions from those of the larger gas giants Jupiter and Saturn. As such, astronomers sometimes place them in a separate category, the ice giants. Uranus's atmosphere, while similar to Jupiter's and Saturn's in being composed primarily of hydrogen and helium, contains a higher proportion of ices such as water, ammonia and methane, along with traces of hydrocarbons. It is the coldest planetary atmosphere in the Solar System, with a minimum temperature of 49 K (-224 °C). It has a complex, layered cloud structure, with water thought to make up the lowest clouds, and methane thought to make up the uppermost layer of clouds. In contrast the interior of Uranus is mainly composed of ices and rock.

Like the other giant planets, Uranus has a ring system, a magnetosphere, and numerous moons. The Uranian system has a unique configuration among the planets because its axis of rotation is tilted sideways, nearly into the plane of its revolution about the Sun. As such, its north and south poles lie where most other planets have their equators. Seen from Earth, Uranus's rings can sometimes appear to circle the planet like an archery target and its moons revolve around it like the hands of a clock, though in 2007 and 2008 the rings appeared edge-on. In 1986, images from Voyager 2 showed Uranus as a virtually featureless planet in visible light without the cloud bands or storms associated with the other giants. However, terrestrial observers have seen signs of seasonal change and increased weather activity in recent years as Uranus approached its equinox. The wind speeds on Uranus can reach 250 meters per second, thats equal to 560 mph.


 

Neptune

 

Neptune is the eighth planet from the Sun in our Solar System. Named for the Roman god of the sea, it is the fourth-largest planet by diameter and the third-largest by mass. Neptune is 17 times the mass of Earth and is slightly more massive than its near-twin Uranus, which is 15 Earth masses and not as dense. On average, Neptune orbits the Sun at a distance of 30.1 AU, approximately 30 times the Earth-Sun distance. Its astronomical symbol is a stylized version of the god Neptune's trident.

Discovered on September 23, 1846, Neptune was the first planet found by mathematical prediction rather than by empirical observation. Unexpected changes in the orbit of Uranus led astronomers to deduce that its orbit was subject to gravitational perturbation by an unknown planet. Neptune was subsequently found within a degree of its predicted position, and its largest moon, Triton, was discovered shortly thereafter, though none of the planet's remaining 12 moons were located telescopically until the 20th century. Neptune has been visited by only one spacecraft, Voyager 2, which flew by the planet on August 25, 1989.

Neptune is similar in composition to Uranus, and both have compositions which differ from those of the larger gas giants Jupiter and Saturn. Neptune's atmosphere, while similar to Jupiter's and Saturn's in that it is composed primarily of hydrogen and helium, along with traces of hydrocarbons and possibly nitrogen, contains a higher proportion of ices such as water, ammonia and methane. Astronomers sometimes categorize Uranus and Neptune as ice giants in order to emphasize these distinctions. The interior of Neptune, like that of Uranus, is primarily composed of ices and rock. Traces of methane in the outermost regions in part account for the planet's blue appearance.

In contrast to the relatively featureless atmosphere of Uranus, Neptune's atmosphere is notable for its active and visible weather patterns. At the time of the 1989 Voyager 2 flyby, for example, the planet's southern hemisphere possessed a Great Dark Spot comparable to the Great Red Spot on Jupiter. These weather patterns are driven by the strongest sustained winds of any planet in the Solar System, with recorded wind speeds as high as 2100 km/h. Because of its great distance from the Sun, Neptune's outer atmosphere is one of the coldest places in the Solar System, with temperatures at its cloud tops approaching -218 °C (55 K). Temperatures at the planet's centre, however, are approximately 5,400 K (5,000 °C). Neptune has a faint and fragmented ring system, which may have been detected during the 1960s but was only indisputably confirmed in 1989 by Voyager 2.



The Moon

The Moon is Earth's only natural satellite and the fifth largest satellite in the Solar System. The average centre-to-centre distance from the Earth to the Moon is 384,403 kilometres (238,857 mi), about thirty times the diameter of the Earth. The common centre of mass of the system (the barycentre) is located at about 1,700 kilometres (1,100 mi)—a quarter the Earth's radius—beneath the surface of the Earth. The Moon makes a complete orbit around the Earth every 27.3 days[nb 3] (the orbital period), and the periodic variations in the geometry of the Earth –Moon–Sun system are responsible for the phases of the Moon, which repeat every 29.5 days[nb 4] (the synodic period).

The Moon's diameter is 3,474 kilometres (2,159 mi),[4] a little more than a quarter of that of the Earth. Thus, the Moon's surface area is less than a tenth that of the Earth (about a quarter the Earth's land area, approximately as large as Russia, Canada, and the United States combined), and its volume is about 2 percent that of Earth. The pull of gravity at its surface is about 17 percent of that at the Earth's surface.

The Moon is the only celestial body on which human beings have made a manned landing. While the Soviet Union's Luna programme was the first to reach the Moon with unmanned spacecraft, the NASA Apollo program achieved the only manned missions to date, beginning with the first manned lunar mission by Apollo 8 in 1968, and six manned lunar landings between 1969 and 1972 – the first being Apollo 11 in 1969. Human exploration of the Moon temporarily ceased with the conclusion of the Apollo program, although a few robotic landers and orbiters have been sent to the Moon since that time. The U.S. has committed to return to the Moon by 2018.



The Sun

 

The Sun is the star at the center of the Solar System. The Earth and other matter (including other planets, asteroids, meteoroids, comets, and dust) orbit the Sun, which by itself accounts for about 99.86% of the Solar System's mass. The mean distance of the Sun from the Earth is approximately 149.6 million kilometers (1 AU), and its light travels this distance in 8 minutes and 19 seconds. This distance varies throughout the year from a minimum of 147.1 million kilometers (0.9833 AU) on the perihelion (around 3 January), to a maximum of 152.1 million kilometers (1.017 AU) on the aphelion (around 4 July). Energy from the Sun, in the form of sunlight, supports almost all life on Earth via photosynthesis, and drives the Earth's climate and weather. The Sun consists of hydrogen (about 74% of its mass, or 92% of its volume), helium (about 24% of mass, 7% of volume), and trace quantities of other elements, including iron, nickel, oxygen, silicon, sulfur, magnesium, carbon, neon, calcium, and chromium. The Sun has a spectral class of G2V. G2 means that it has a surface temperature of approximately 5,780 K (5,510 °C) giving it a white color, which often appears as yellow when seen from the surface of the Earth because of atmospheric scattering. It is this scattering of light at the blue end of the spectrum that gives the surrounding sky its color. The Sun's spectrum contains lines of ionized and neutral metals as well as very weak hydrogen lines. The V (Roman five) in the spectral class indicates that the Sun, like most stars, is a main sequence star. This means that it generates its energy by nuclear fusion of hydrogen nuclei into helium. There are more than 100 million G2 class stars in our galaxy. Once regarded as a small and relatively insignificant star, the Sun is now presumed to be brighter than 85% of the stars in the galaxy, most of which are red dwarfs.

The Sun's hot corona continuously expands in space creating the solar wind, a hypersonic stream of charged particles that extends to the heliopause at roughly 100 AU. The bubble in the interstellar medium formed by the solar wind, the heliosphere, is the largest continuous structure in the Solar System.

The Sun is currently traveling through the Local Interstellar Cloud in the low-density Local Bubble zone of diffuse high-temperature gas, in the inner rim of the Orion Arm of the Milky Way Galaxy, between the larger Perseus and Sagittarius arms of the galaxy. Of the 50 nearest stellar systems within 17 light-years (1.6×1014 km) from the Earth, the Sun ranks 4th in mass. Slightly different values for the magnitude have been published, for example 4.85 and 4.81. The Sun orbits the center of the Milky Way galaxy at a distance of approximately 24,000–26,000 light years from the galactic center, moving generally in the direction of Cygnus and completing one revolution in about 225–250 million years (one Galactic year). Its orbital speed was thought to be 220 ± 20, km/s but a new estimate gives 251 km/s. Since our galaxy is moving with respect to the cosmic microwave background radiation (CMB) in the direction of Hydra with a speed of 550 km/s, the Sun's resultant velocity with respect to the CMB is about 370 km/s in the direction of Crater or Leo.

Welcome, the latest information available for special events is posted below. New information will be posted as available. Typically, events on this page are annual events which means if you missed one of them, they should be back again next year.

Tis the Season

December 2012

  • General Admission $ 6

This great show is about the coldest and darkest of seasons. yet a season which holds some of the warmest and brightest celebrations of the year. It traces the development of many of the world's endearing holiday customs, and how they involve lighting up the winter season, from the burning Yule log and sparkling Christmas tree lights, to the lighting of the Menorah and luminaries.

The show also recounts the historical religious and cultural rituals practiced during the time of winter solstice. not only Christian and Jewish, but also Celtic, Pagan, Nordic, Roman, Egyptian and Hopi. It also takes a look at some of our more light-hearted seasonal traditions: from gift-giving and kissing under the mistletoe to songs about lords a-leaping, and ladies dancing. And the custom of decking the halls with greenery and candles. St. Nicholas, Sinterklaas, Kris Kringle, Father Christmas, and Santa Claus all drop by as well.

Naturally, there is some astronomy too. We catch a few Northern winter constellations, and we illustrate why we even have seasons. Demonstrating the Sun's path across the sky throughout the year, and the Earth's tilt and orbit around the Sun. And of course, we explore the possible astronomical explanations for a Star over Bethlehem. Last but not least: comets, meteors, novae and supernovae, and planetary conjunctions.



Ring World

Narrated by John Billingsley | Star Trek - Dr. Phlox

The Cassini-Huygens mission is a joint effort of the National Aeronautics and Space Administration, European Space Agency, and the Italian Space Agency. The mission is managed for NASA by the Jet Propulsion Laboratory of the California Institute of Technology.

The size of a school bus with a total weight of over 12,000 pounds, and an array of 18 packages of scientific instruments, Cassini-Huygens represents the combined effort of scientists and engineers in 18 countries, and is one of the largest, heaviest, and most sophisticated interplanetary spacecraft ever launched. It's destination? One of the most intriguing objects in our solar system. A world of unparalleled beauty and the undisputed Lord of the Rings, Saturn!

This program explains the route the spacecrafts will take to reach Saturn in July of 2004. Although the Pioneer and Voyager probes have visited this ringed world, in terms of information gathered from those spacecraft, Cassini-Huygens promises to run rings around them.

Light Years From Andromeda

Narrated by Michael Dorn | Star Trek - Worf

A beam of light leaves the Andromeda Galaxy and travels across the void of intergalactic space. On a planet located in a nearby galaxy, intelligent life evolves. As the light speeds across the light years, over the course of centuries, the primitives on the planet form cultures and civilizations, and begin to wonder about the universe surrounding them. Their awareness of the night sky increases, as the beam of light draws nearer to their planet. When the light reaches the Earth, some of the descendants of the early hunters have just escaped the bonds of their world's gravity, and visited the Moon. In modern times, scientific study of space help the planet's current inhabitants to understand the properties of light, and the ways that understanding shapes our further knowledge of the universe.


Through the Eyes of Hubble

Narrated by Gates McFadden | Star Trek - Dr. Beverly Crusher

This program tells the dramatic story of the stunning repair mission of NASA's Hubble Space Telescope and the ensuing stream of dramatic images and science. Through the Eyes of Hubble combines computer graphics, multi-screened video projections, and dozens of special effect projectors to present a celestial array of spectacular Hubble discoveries. Included in the show are observations of the Comet Shoemaker-Levy 9 crash into Jupiter, atmospheric storms on Saturn, the birth and death of stars, colliding galaxies, evidence of the existence of black holes, and many other discoveries that may shed light on the fate of the cosmos itself.

Through the Eyes of Hubble is the product of a unique collaboration between the Henry Buhl, Jr. Planetarium at Pittsburgh Carnegie Science Center and the Space Telescope Science Institute, Baltimore MD.


Larry Cat In Space

This show is a playful, imaginative cartoon presentation about an inquisitive cat who takes a trip to the Moon. Through Larry's eyes, we observe his human family, a group of enthusiastic sky-watchers. Larry notes how human time differs from cat time. Diana takes a job on the Moon, and sadly leaves Larry behind. Larry figures out a way to hide in her clothes trunk. The trunk and Larry are loaded onto the Space Plane, which takes him to space station Freedom.

From there, he is transferred to the Lunar Shuttle. During weightlessness, the trunk opens. Larry floats out into the cabin, and looks out the window. When Diana discovers Larry, he leaps to greet her, but sails over her head, since he only weighs two pounds in lunar gravity. He meets the rest of Imbrium Village's inhabitants, including the evil Commander Stone, who orders Diana to return Larry to Earth. The Moon base crew petitions to keep Larry, and the Commander relents. He even makes Larry a cat space suit. When Larry ventures outside, he spots the Earth, looking a lot like the Moon did from the porch at home.

Larry Cat In Space is primarily targeted at grades 1-3, although everyone loves an entertaining, fun story! Parents and children alike will enjoy the show, and learn something about the Moon, too!


A Trip Into Space

Narrated by Jon Bell | Hallstrom Planetarium

In this program you will discover the answers to the most commonly asked questions about astronomy. Some of the questions this program will address are:

  • Why there are different phases of the moon as well as the basic features of the moon
  • Why we have solar and lunar eclipses
  • What are black holes
  • Why we have tides
  • Why we have day, night and the reasons for the seasons
  • The difference between the sun and the planets
  • Why do conditions vary on each planet
  • What is the Milky Way Galaxy
  • How many Galaxies are there

This wonderful family program is presented using a variety of multi-media effects, and is sure to captivate audiences of all ages.


Bear Tales and Other Grizzly Stories

Join us on a family camping trip under the stars, and listen in as the family is regaled by Grandpa Ben's lively tales about the night sky. Hear stories from ancient Greece and Egypt, up to modern tales about Blackbeard the pirate. Learn why the bears in the sky have long tails…or is that tales?

Grandpa takes us on a tour of the spring time constellations, explaining how and why they are there. He draws freely from all mythologies and his own imagination to explain the stars' position in the night sky. The result is a fun and educational show that can be enjoyed by audiences of all ages, all year long. Be the first in your neck of the woods to see this show. You'll 'bearly' contain yourself!


Dinosaurs

Ever since the discovery of ancient bones and the first use of the word dinosaur to describe the creatures they once were, people around the world have been fascinated by these prehistoric beasts. Share the excitement and wonder at the diversity and magnificence of these beings, who once dominated the earth as no other group of creatures has since. Presented in a smoothly-flowing narrative style, Dinosaurs takes you back for the feel of the time of the dinosaurs, and explains how geologic time works in a method that is effective and easy to understand.

 

Stars to Starfish

Stars to Starfish explores the mysteries and wonders of our oceans by comparing the exploration of the ocean, with that of deep space. Throughout most of our history, man has been preoccupied only with the surface of the sea, much like early astronomers were preoccupied with only the stars they could see. By learning the mysteries of the seas and oceans, scientist and astronomers are hoping to use this information in unraveling many of the mysteries of space. Can life possibly exist in some of the extreme environments we find on the other planets of our solar system? This program integrates the newest form of media presentation available in the planetarium, by displaying stunning underwater photography.

 

The Secret of the Cardboard Rocket

Two children build a rocket out of a packing crate and ponder the wonders of the universe, while discovering the power of their own imaginations. The Secret of the Cardboard Rocket gives an introduction to the solar system, with the aid of a talking astronomy book, and a lot of imagination. A great family show, and a wonderful and new exciting way to introduce astronomy to children.

planetarium-outside

 

The Planetarium was built in 1968 and opened in 1969. It is situated across from Jackson Hospita in beautiful Oak Park (1010 Forest Avenue, Montgomery AL 36106). The Planetarium has recently undergone its first major renovation which included adding twenty-two projectors, including video projection, a new sound system, and the introduction of Laser Light Shows.

The W.A. Gayle Planetarium features over 200 theater style seats and is one of the largest Planetariums between Atlanta and New Orleans. During the past five years, close to 100,000 K-12 students have attended a variety of daily educational shows offered at the Planetarium. See displays from NASA, and visit the Planetarium Gift Shop. It's…Out of this World!

PUBLIC SHOWS 

The Planetarium's Public shows are offered according to the schedule below. Reservations are not required for these presentations.

  • 3:00 on Monday
  • 3:00 on Tuesday
  • 3:00 on Wednesday
  • 3:00 on Thursday
  • 2:00 on Sunday

Doors open fifteen minutes before show time. Each presentation start promptly and unfortunately, no admission is allowed after the show has started.

Admission is just $5! Children under five are admitted free and young at heart over sixty-five are $4


SCHOOL FIELD TRIPS OR GROUP RESERVATIONS 

Educational programs are scheduled for schools and groups according to the schedule below

  • 9:30 • 10:30 • 11:30 • 1:00 • 2:00 - Monday:
  • 9:30 • 10:30 • 11:30 • 1:00 • 2:00 - Tuesday:
  • 9:30 • 10:30 • 11:30 • 1:00 • 2:00 - Wednesday:
  • 9:30 • 10:30 • 11:30 • 1:00 • 2:00 - Thursday:
  • 9:30 • 10:30 • 11:30 - Friday:

Each presentation lasts one hour and includes an Educational Astronomy Presentation and the Discovery Store gift shop. Reservations are required for these presentations.

Cancellation Policy: Advance cancellation notice is required. If you fail to cancel your appointment a deposit will be required for all future scheduled appointments by your school. The deposit will be non-refundable, but will be deducted from the total bill when your group checks in.

To make your reservation, simply call (334) 241-4799. A confirmation card will be mailed to you. We also offer the opportunity to pre-shop in our Discovery Store gift shop by using an order form.

HOURS OF OPERATION 

With the exception of most Holidays, the Planetarium Office is open…

  • 7:30 - 4:30 Monday
  • 7:30 - 4:30 Tuesday
  • 7:30 - 4:30 Wednesday
  • 7:30 - 4:30 Thursday
  • 7:30 - 12:00 Friday

The planetarium staff is flexible in meeting your needs. Special events, such as birthday parties, meetings, conferences can be scheduled and conducted at the planetarium:

W.A. Gayle Planetarium 
1010 Forest Avenue 
Montgomery, AL 36106 
(334) 241-4799