Saturday, December 31, 2011

Space / Astronomy: What's Hot Now: Astronomy - Space Exploration Activity Book for Kids

Space / Astronomy: What's Hot Now
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Astronomy - Space Exploration Activity Book for Kids
Dec 31st 2011, 11:16

Here's a fun activity book for young astronauts and astronomers from your About Astronomy and Space Guide. Open each page of the activity book and print it. You may print as many copies as you would like for personal use, but please leave the copyright notice in place.

Cover
Page 1
Page 2
Page 3
Page 4
Page 5
Page 6
Page 7
Page 8
Page 9
Page 10
Page 11
Page 12
Page 13
Page 14
Page 15
Page 16
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Page 27

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Space / Astronomy: What's Hot Now: Meteorite Hunters

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Meteorite Hunters
Dec 31st 2011, 11:16

When a meteorite is found, the ANSMET (Antarctic Search for Meteorites) team records its location, size, color, amount of fusion crust, probable type, and anything else that might be important.

Some of their tools are similar to those used by the Apollo astronauts to collect samples, and some are the latest high-tech (like Global Positioning Satellite navigation). The team takes great care not to contaminate the meteorites. Meteorites are handled only with stainless steel instruments, and are immediately sealed in sterile plastic or aluminum foil packages. Meteorites collected by the ANSMET team in Antarctica are packed in dry ice to mimic conditions in the field and shipped to the Antarctic Meteorite Laboratory at NASA's Johnson Space Center in Houston, Texas.

Meteorite Hunters Full Size Image
Image Credit: NASA Johnson Space Center

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Space / Astronomy: What's Hot Now: Moon Landing Sites

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Moon Landing Sites
Dec 31st 2011, 11:16

Pictures of the Moon - Moon Landing Sites

Pictures of the Moon - Moon Landing Sites

National Space Science Data Center, NASA Goddard Space Flight Center

This image shows the locations of many spacecraft that have landed on the Moon. Green triangles are Apollo missions, yellow are NASA Surveyor missions and red are Russian Luna spacecraft.

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Friday, December 30, 2011

Space / Astronomy: What's Hot Now: Visiting Johnson Space Center

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Visiting Johnson Space Center
Dec 30th 2011, 11:07

Hours of Operation:


Space Center Houston is open every day of the year, with the exception of December 25.

Summer: June 10am - 7pm, July 9am - 7pm, August 10am-5pm, 10am - 7pm Weekends

Winter: Mon - Fri 10am - 5pm, Sat - Sun 10am - 6pm

Admission Cost:

  • Adults $18.95
  • Children (4-11) $14.95
  • Seniors $17.95
  • Parking $5.00
  • Group Rates (15 or more) are available. Please call 281â€"244â€"2105 for more information
Location:
Space Center Houston is located at: 1601 NASA Parkway
Houston, TX 77058
approximately 25 miles South of downtown Houston in the NASA/Clear Lake area.
Phone 281-244-2100
Website

What to Do

Space Center theater - Sponsored By: Northrop Grumman:


People of all ages are fascinated with what it takes to be an astronaut. This attraction shows the excitement, the commitment and the risks taken by the people who fly in space. Here we can see the evolution of the equipment and the training of the men and women who dreamed to be astronauts. We want guests to experience first hand what it takes to be an astronaut. The film, shown on a 5-story tall screen, takes the viewer by the heart to bring them into the life of an astronaut from the time they receive notification of their acceptance into the training program to their first mission.

Blast Off Theater:


The only place in the world where you can personally experience the thrill of launching into space like a real astronaut. Not just a movie; it's the thrill of personally feeling the launch into space - from the rocket boosters to the billowing exhaust.

Visitors said about their trips:

"It's like IMAX in 10D!"
"There's nothing like it in the whole world!"

After docking at the International Space Station, guests enter the Blastoff Theater for an update on current shuttle missions, as well as details on the exploration of Mars.

NASA Tram Tour:


With this behind-the-scenes journey through NASA's Johnson Space Center, you may visit the Historic Mission Control Center, the Space Vehicle Mockup Facility or the current Mission Control Center. Before returning to Space Center Houston, you can visit the "all new" Saturn V Complex at Rocket Park. Occasionally, the tour may visit other facilities, such as the Sonny Carter Training Facility or Neutral Buoyancy Laboratory. You may even get to see astronauts training for upcoming missions.

*The buildings visited on the tram tour are real working areas of Johnson Space Center and are subject to close without notice.

Astronaut Gallery:


The Astronaut Gallery is an unparalleled exhibit outside Northrop Grumman Theater featuring the world's best collection of spacesuits. Astronaut John Young's ejection suit and Judy Resnik's T-38 flightsuit are two of the many spacesuits on display.

The walls of the Astronaut Gallery also contain portraits and crew photos of every U.S. astronaut who has flown in space.

The Feel Of Space:
The Living in Space module simulates what life could be like for astronauts aboard the space station. A Mission Briefing Officer gives a live presentation on how astronauts live in a space environment.

It uses humor to show how the smallest tasks like showering and eating are complicated by a microgravity environment. A volunteer from the audience helps to prove the point.

Beyond the Living in Space Module are 24 part task trainers that use sophisticated computer technology to provide visitors with the experience of landing the orbiter, retrieving a satellite or exploring the shuttle systems.

Starship Gallery:

The journey into space begins with the film "On Human Destiny" at the Destiny Theater. Artifacts and hardware on display in the Starship Gallery trace the progression of America's Manned Space Flight.

This incredible collection includes: an original model of the Goddard Rocket; the actual Mercury Atlas 9 "Faith 7" capsule flown by Gordon Cooper; the Gemini V Spacecraft piloted by Pete Conrad and Gordon Cooper; a Lunar Roving Vehicle Trainer, the Apollo 17 Command Module, the giant Skylab Trainer, and the Apollo-Soyuz Trainer.

Kids Space Place:

Kids Space Place was created for children of all ages who have always dreamed of experiencing the same things astronauts do in space.

Interactive exhibits and themed area make exploring the different aspects of space and the manned space flight program loads of fun.

Inside Kids Space Place, guests can explore and experiment commanding the space shuttle or living on the space station.

*Age and/or height restrictions may apply on some activites.

Level 9 Tour:

Go Behind the Scenes. See where the Astronauts "Hang Out"!

The Level Nine Tour takes you behind the scenes to see the real world of NASA up close and personal. On this four-hour tour you will see things that only the astronauts see and eat what and where they eat.

All your questions will be answered by a very knowledgeable Tour Guide as you discover the secrets that have been kept behind closed doors for years.

The Level Nine Tour is Monday-Friday and includes a FREE HOT LUNCH in the astronauts' cafeteria which makes it a "Big Bang" for your buck! The only security clearance is that you must be 14 years of age or older.

HURRY! Only 12 Level Nine admissions are available each day. RESERVE YOUR SPECIALLY PRICED ADMISSION NOW ONLINE or by calling Group Sales 281-244-2115. Advanced reservations must be made at least one day prior to visit. Purchase admission until all spots filled on the day of your visit at the Space Center Houston Information Desk. Tour begins promptly at 11:45 am.

The Level Nine Tour sites include:

  • Building 3 - Astronaut Cafeteria (Enjoy a free lunch where the astronauts eat everyday.)
  • Building 2 - Teague Auditorium (Artifacts)
  • Building 7 - Space Suit Displays
  • Building 9NE - Space Vehicle Mock-up Facility (Observation Catwalk)
  • Building 30S - New Mission Control Center (Viewing Areas)
  • Building 30N - Historic Mission Control Center
  • Building 32 - Space Environment Simulation Lab (Vacuum Chamber)
  • Sonny Carter Training Facility - Neutral Buoyancy Lab (Observation Catwalk) Building availability subject to change based on safety regulation and astronaut training schedules.
Become A Member.
2 Great Ways to Save!
  • Individual Membership: $20.95 Only $2.00 more than a full price adult admission!
  • Family Of Four Membership: $79.95 Less than $1.05 more per person than a full price adult admission!
    *Add-ons only $19.75
Plus receive...
  • 10% discount on food
  • 10% discount on souvenirs
  • Free parking for an entire year
  • Free admission for an entire year
Space Center Houston Memberships available now at the Ticket Window and Membership Desk.

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Space / Astronomy: What's Hot Now: Constellations Pictures - Canis Major - Picture of the Constellation Canis Major

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Constellations Pictures - Canis Major - Picture of the Constellation Canis Major
Dec 30th 2011, 11:07

From , former Guide

The Greater Dog - Genitive: Can Majoris Abbreviations: CMa, C Maj Right Ascension, (h): 7 Declination, (deg): 20S

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Space / Astronomy: What's Hot Now: Moon Color Composite

Space / Astronomy: What's Hot Now
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Moon Color Composite
Dec 30th 2011, 11:07

This color image of the Moon was taken by the Galileo spacecraft at 9:35 a.m. PST Dec. 9, 1990, at a range of about 350,000 miles. The color composite uses monochrome images taken through violet, red, and near-infrared filters.

The concentric, circular Orientale basin, 600 miles across, is near the center; the nearside is to the right, the far side to the left. At the upper right is the large, dark Oceanus Procellarum; below it is the smaller Mare Humorum. These, like the small dark Mare Orientale in the center of the basin, formed over 3 billion years ago as basaltic lava flows.

At the lower left, among the southern cratered highlands of the far side, is the South-Pole-Aitken basin, similar to Orientale but twice as great in diameter and much older and more degraded by cratering and weathering. The cratered highlands of the near and far sides and the Maria are covered with scattered bright, young ray craters.

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Space / Astronomy: What's Hot Now: First Image of the Far Side of the Moon

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First Image of the Far Side of the Moon
Dec 30th 2011, 11:07

The Luna 3 spacecraft returned the first views ever of the far side of the Moon. The first image was taken at 03:30 UT on 7 October at a distance of 63,500 km after Luna 3 had passed the Moon and looked back at the sunlit far side. The last image was taken 40 minutes later from 66,700 km. A total of 29 photographs were taken, covering 70% of the far side. The photographs were very noisy and of low resolution, but many features could be recognized.

This is the first image returned by Luna 3. Taken by the wide-angle lens, it showed the far side of the Moon was very different from the near side, most noticeably in its lack of lunar maria (the dark areas).

The right three-quarters of the disk are the far side. The dark spot at upper right is Mare Moscoviense, the dark area at lower left is Mare Smythii. The small dark circle at lower right with the white dot in the center is the crater Tsiolkovskiy and its central peak.

The Moon is 3475 km in diameter and north is up in this image. (Luna 3-1)

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Thursday, December 29, 2011

Space / Astronomy: What's Hot Now: Pictures of the Star Sirius - The Dog Star, Sirius, and its Tiny Companion

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Pictures of the Star Sirius - The Dog Star, Sirius, and its Tiny Companion
Dec 29th 2011, 11:08

This Hubble Space Telescope image shows Sirius A, the brightest star in our nighttime sky, along with its faint, tiny stellar companion, Sirius B. Astronomers overexposed the image of Sirius A [at center] so that the dim Sirius B [tiny dot at lower left] could be seen. The cross-shaped diffraction spikes and concentric rings around Sirius A, and the small ring around Sirius B, are artifacts produced within the telescope's imaging system. The two stars revolve around each other every 50 years. Sirius A, only 8.6 light-years from Earth, is the fifth closest star system known.

Sirius B, a white dwarf, is very faint because of its tiny size, only 7,500 miles in diameter. White dwarfs are the leftover remnants of stars similar to the sun. They have exhausted their nuclear fuel sources and have collapsed down to a very small size. Sirius B is about 10,000 times fainter than Sirius A. The white dwarf's feeble light makes it a challenge to study, because its light is swamped in the glare of its brighter companion as seen from telescopes on Earth. However, using the keen eye of Hubble's Space Telescope Imaging Spectrograph (STIS), astronomers have now been able to isolate the light from Sirius B and disperse it into a spectrum. STIS measured light from Sirius B being stretched to longer, redder wavelengths due to the white dwarf's powerful gravitational pull. Based on those measurements, astronomers have calculated Sirius B's mass at 98 percent that of the sun. Analysis of the white dwarf's spectrum also has allowed astronomers to refine the estimate for its surface temperature to about 44,900 degrees Fahrenheit (25,200 degrees Kelvin).

Accurately determining the masses of white dwarfs is fundamentally important to understanding stellar evolution. The sun will eventually become a white dwarf. White dwarfs are also the source of Type Ia supernova explosions, which are used because of their brightness to measure the distance to distant galaxies and the expansion rate of the universe. Measurements based on Type Ia supernovae are fundamental to understanding "dark energy," a dominant repulsive force stretching the universe apart. Also, the method used to determine the white dwarf's mass relies on one of the key predictions of Einstein's theory of General Relativity: that light loses energy when it attempts to escape the gravity of a compact star. This effect is known as the gravitational redshift of the light.

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Space / Astronomy: What's Hot Now: Valentina Tereshkova Biography

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Valentina Tereshkova Biography
Dec 29th 2011, 11:08

Valentina Tereshkova was born to a peasant family in the Yaroslavl' region of the former USSR on March 6, 1937. Yaroslavl is now a part of Russia.

Soon after starting work in a textile mill at the age of 18, Valentina joined an amateur parachuting club. She was a hard worker. Later, at the age of 24, she applied to become a cosmonaut. Just earlier that year, 1961, the Soviet space program began to consider sending women into space. The Soviets were looking for another "first" at which to beat the United States.

Overseen by the first person in space, Yuri Gagarin, the selection process began mid-1961. Since there weren't many female pilots, women parachutists made an excellent field to choose from. Valentina Tereshkova, three other women parachutists, and a female pilot were selected to train as cosmonauts in 1962.

As per the paranoia of the time, the entire program was shrouded in secrecy. When she left for training, Tereshkova reportedly told her mother she was going to a training camp for an elite skydiving team. It wasn't until the flight was announced on the radio that her mother learned the truth. The identities of the other women in the cosmonaut program were not revealed until the late 1980s. Valentina Tereshkova was the only one of the group to go into space.

The historic first flight of a female cosmonaut was slated to concur with the second dual flight (a mission on which two craft would be in orbit at the same time, and ground control would maneuver them to within 5 km (3 mi) of each other). Scheduled for June of the following year, the flight left only about 15 months for training. Basic training for the women was very similar to that of the male cosmonauts. It included classroom study, parachute jumps, and time in an aerobatic jet. They were all commissioned as second lieutenants in the Soviet Air Force. At that time, the air force had control over the cosmonaut program.

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Space / Astronomy: What's Hot Now: Pluto Picture - Sedna Size Comparisons

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Pluto Picture - Sedna Size Comparisons
Dec 29th 2011, 11:08

From , former Guide

Sedna Size Comparisons

Sedna Size Comparisons

NASA Jet Propulsion Laboratory (NASA-JPL)

The artist's rendition shows the newly discovered planet-like object, dubbed "Sedna," in relation to other bodies in the solar system, including Earth and its Moon; Pluto; and Quaoar, a planetoid beyond Pluto that was until now the largest known object beyond Pluto. The diameter of Sedna is slightly smaller than Pluto's but likely somewhat larger than Quaoar.

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Wednesday, December 28, 2011

Space / Astronomy: What's Hot Now: Earth Pictures - Earth - Departing Image by Galileo

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Earth Pictures - Earth - Departing Image by Galileo
Dec 28th 2011, 11:08

This color image of the Earth was taken by the Galileo spacecraft on December 11 as it departed on its 3-year flight to Jupiter, about 2 1/2 days after the second Earth flyby. The distance to Earth is about 1.9 million kilometers (1.2 million miles). Antarctica is visible at the bottom of the image, and dawn is rising over the Pacific Ocean. The Galileo project, whose primary mission is the exploration of the Jupiter system in 1995-97, is managed for NASA's Office of Space Science and Applications by the Jet Propulsion Laboratory.

Discover Earth's companion. Check out these images in our Moon Pictures Gallery.

Our Geology Guide also has some great links to Earth Images from Space. Check them out.

Discover the rest of the galactic neighborhood with our Solar System Tour.

Learn your way around the night sky with a Sky Map. They're free.

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Space / Astronomy: What's Hot Now: Visual Tour of Solar System

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Visual Tour of Solar System
Dec 28th 2011, 11:08

Mercury Pictures Gallery
Mercury Information

The closest planet to the Sun, Mercury was named after the Roman god of commerce, travel and thievery. The existence of this 8th largest planet has been known of since before the third century BC. The Greeks gave it two names, Apollo for when it appeared as a morning star and Hermes when it came as an evening star.

Mercury is a planet of extremes. It speeds around the Sun in a wildly elliptical (non-circular) orbit that takes it as close as 47 million km and as far as 70 million km from the Sun. The planet completes a trip around the Sun every 88 days, speeding through space at nearly 50 km per second, faster than any other planet. Because it is so close to the Sun, temperatures on its surface can reach a scorching 467 degrees Celsius. But because the planet has hardly any atmosphere to keep it warm, nighttime temperatures can drop to a frigid -183 degrees Celsius.

Mercury has no known moons or satellites.

This Image of "Mercury" was produced from USGS I-1149, 1979.

After Mercury, we head further away from the sun to reach Venus.

Also, check out our Full Detail Solar System Tour

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Space / Astronomy: What's Hot Now: Deadly Christmas Tsunami 2004

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Deadly Christmas Tsunami 2004
Dec 28th 2011, 11:08

On December 26, 2004, a tsunami swept across the Indian ocean, spawned by a magnitude 9.0 earthquake off the coast of Sumatra. Aside from Indonesia, the island nation of Sri Lanka likely suffered the most tsunami casualties, with the death toll over 155,000.

DigitalGlobe’s Quickbird satellite captured an image of the tsunami devestation around Kalutara, Sri Lanka, on December 26, 2004, at 10:20 a.m. local timeâ€"about an hour after the first in the series of waves hit. A Quickbird image taken on January 1, 2004, shows the normal ocean conditions. Water is flowing out of the inundated area and back into the sea, creating turbulence offshore. Some near-shore streets and yards are covered with muddy water. It is possible that the image was acquired in a “trough” between wave crests. Imagery of nearby beaches shows that the edge of the ocean had receded about 150 meters from the shoreline just prior to the tsunami.

High-resolution Tsunami images:

Other Great Resources from About Astronomy and Space

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Tuesday, December 27, 2011

Space / Astronomy: What's Hot Now: Constellations Pictures - Cassiopeia - Picture of the Constellation Cassiopeia

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Constellations Pictures - Cassiopeia - Picture of the Constellation Cassiopeia
Dec 27th 2011, 11:07

From , former Guide

Cassiopeia, wife of Cepheus, the Ethiopian king of Joppa, and mother of Andromeda. - Genitive: Cassiopeiae Abbreviations: Cas, Cass Right Ascension, (h): 1 Declination, (deg): 60N

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Space / Astronomy: What's Hot Now: Santa Claus in Space

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Santa Claus in Space
Dec 27th 2011, 11:07

Just a few years ago, the folks at Science@NASA had a chance to interview the big guy, himself, Santa Clause. Here's that interview, which was conducted Christmas Eve, 1998.

In just a few hours the Jolly Old Elf will brush the fireplace ash out of his beard, don his famous red suit, and begin the serious work of delivering presents all over the world. It's a job he's done in the same way for a long, long time, but times may be changing. As humans and space probes travel to other worlds, the possibility of Christmas on other planets can no longer be ignored, and the prospect of delivering presents throughout the solar system is, well, turning Santa's hair white.

In an exclusive interview, Science@NASA visited Santa Claus at his secret North Pole workshop. He took a break from final preparations to talk about how he'll maintain his legendary delivery system as humankind inhabits other worlds.

"The Moon won't be too much of a challenge," Santa told us. "I figure the lunar colonies will keep Earth time, so I'll just add them to my route. The reindeer will gripe about having to put on spacesuits, but we'll get used to it."

"Mars is going to start to stretch us a bit. See, it takes 687 days to go around the Sun. That's about two of our Earth years. So every other year I'll have two Christmas runs to make, the Earth-Moon run and the Mars run. We'll really have to 'haul Rudolph,' as the reindeer are fond of saying. Fortunately, a Martian day is 37 minutes longer than an Earth day, so we can still do our usual overnight delivery. Some of the planets have much shorter days than Earth! ... Excuse me a moment."

One of the senior elves was asking about overtime to complete a special batch of toys.

"I worry about the elves," Santa continued. "They count on a slack period to fix the factory and retool for the next year. I'll have to hire more helpers if we're going to service the Moon and Mars, too."

What about the other planets?

"Well, I've given them some thought", explained Santa. "Take Venus, for example. It's a tough environment - high temperatures, and a thick, choking carbon dioxide atmosphere. Plus, the clouds are made of sulfuric acid. Talk about air pollution. Venus circles the sun every 224 days, so Christmas will come about every eight Earth months. That's a little more often than we're used to here on Earth, but it'll be easy to deliver all the presents in one night. Venus's day is 243 times longer than ours. I'll have all the time in the world - their world - to deliver. Everyone gets their presents on the same day, no matter when I deliver. Ho, ho, ho!"

"Now, the closest planet to the Sun is Mercury," he went on, wagging his finger in a professorial fashion. Santa really knew a lot about the solar system.

"You'd think that Mercury would be the hottest planet, but Venus is actually a little warmer, on average, because of the greenhouse effect in its carbon dioxide atmosphere. That's not to say Mercury isn't hot -- it's scorching! Daytime temperatures reach 5000 degrees C. The appealing thing about Mercury, at least for the kids, is that the planet's year is just 88 Earth days long. Imagine that! Christmas every 88 days. It's a bit too often if you ask me, but that's gravity for you."

Santa paused for a moment.

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Monday, December 26, 2011

Space / Astronomy: What's Hot Now: Apollo 8 Christmas Eve Message

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Apollo 8 Christmas Eve Message
Dec 26th 2011, 11:07

Much like the shepherds and wise men during the first Christmas, people around the world had their attention turned toward the heavens on Dec. 24, 1968, when the Apollo 8 crew delivered its famous Christmas Eve broadcast from lunar orbit. Commander Frank Borman, Command Module Pilot Jim Lovell and Lunar Module Pilot William Anders became the first humans to orbit the Moon on Christmas Eve 1968. They were also the first astronauts to spend Christmas in space.

Available Formats:

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Space / Astronomy: What's Hot Now: Taxing the Trekkie

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Taxing the Trekkie
Dec 26th 2011, 11:07

Date: 2002 The 2003 budget for NASA was just over $15 Billion. Yet, that is just a drop in the bucket to what is truly required to fund space exploration. Many of us would like to see the space exploration program expanded, but in this age of budget cuts and tax cuts, it is not likely to happen.

So, the question arises, how do we pay for all this new technology?

A congressional candidate in Alabama, Michael Williams, had a unique proposal: Create a Science Fiction tax, aimed ar Star Trek & Star Wars fans.

Williams, a Republican who was running for the 5th Congressional District seat, proposes a “NASA tax” of 1% on all science fiction books, comic books, space sciences books and any other space-related literature. In his platform, Williams also said the tax would apply to “space, space-related, and science fiction toys, puzzles and games.” So, anyone watching a new Star Trek or Star Wars movie, or reading any science fiction book would have to pay extra to this fund.

Not wanting to appear merely pro-tax, he also proposes to increase tax depreciation for research and development expenses to levels similar to those tax breaks provided by European governments.

Twenty-eight year old Williams holds a master’s degree in political science from the University of Alabama and currently works in a Publix Supermarket. The popularity of his ideas was be tested by the public in a June 4th, 2003 primary. He lost.

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Saturday, December 24, 2011

Space / Astronomy: What's Hot Now: Space Shuttle Orbiter Rear

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Space Shuttle Orbiter Rear
Dec 24th 2011, 11:10

Forward Section

Airlock

The airlock provides access for spacewalks, known as extravehicular activity, or EVA. It can be located in one of several places: inside the Orbiter crew module in the middeck area mounted to the aft bulkhead, outside the cabin also mounted to the bulkhead or on top of a tunnel adapter that can connect the pressurized Spacehab module with the Orbiter cabin. A docking module can also serve as an EVA airlock.

The airlock contains two spacesuits, expendables for two six-hour payload EVAs & one contingency or emergency EVA, & mobility aids such as handrails to enable the crew to perform a variety of tasks. The airlock allows two crewmen room for changing spacesuits.

Midfuselage

In addition to forming the payload bay of the Orbiter, the midfuselage supports the payload bay doors, hinges & tiedown fittings, the forward wing glove & various Orbiter system components.

Each payload bay door supports four radiator panels. When the doors are opened, the tilting radiators are unlatched & moved to the proper position. This allows heat radiation from both sides of the panels, whereas the four aft radiator panels radiate from the upper side only.

Some payloads may not be attached directly to the Orbiter but to payload carriers that are attached to the Orbiter. The inertial upper stage, pressurized modules or any specialized cradle for holding a payload are typical carriers.

The Remote Manipulator System, or RMS, is a 15.2-meter (50-foot) long articulating arm remotely controlled from the flight deck of the Orbiter. The elbow & wrist movements permit payloads to be grappled for deployment out of the payload bay or retrieved & secured for return to Earth.

A television camera & lights near the outer end of the arm permit the operator to see on television monitors what his hands are doing. In addition, three floodlights are located along each side of the payload bay.

Aft Fuselage

The aft fuselage consists of the left & right orbital maneuvering systems, Space Shuttle main engines, body flap, vertical tail & Orbiter/external tank rear attachments.

The forward bulkhead closes off the aft fuselage from the midfuselage. The upper portion of the bulkhead attaches to the vertical tail. The internal thrust structure supports the three Space Shuttle main engines, low pressure turbopumps & propellant lines.

Forward Section

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Friday, December 23, 2011

Space / Astronomy: 2011 Space Image of the Year

Space / Astronomy
Get the latest headlines from the Space / Astronomy GuideSite. // via fulltextrssfeed.com
2011 Space Image of the Year
Dec 23rd 2011, 20:51

I find it amusing that so many of the "Top [insert generic topic of interest here] of 2011" lists come out in October or November, more than a month before the actual end of the year. In fact, the 2012 (yes 2012!) North American Car of the Year has already been determined by Motor Trend, several weeks before the end of 2011! (Though they sort of get a pass since Car manufacturers seems to designate the model years of their cars about 6 months ahead of the actual calendar year.)

In any event, I found myself behind schedule decided to be clever and actually waited until the last week of 2011 to designate my 2011 space image of the year.

Good thing too.

The above image (a larger, printable version can be found here) was released by Hubblesite on December 15, 2011.

From Hubble: The bipolar star-forming region, called Sharpless 2-106, or S106 for short, looks like a soaring, celestial snow angel. The outstretched "wings" of the nebula record the contrasting imprint of heat and motion against the backdrop of a colder medium. Twin lobes of super-hot gas, glowing blue in this image, stretch outward from the central star. This hot gas creates the "wings" of our angel. A ring of dust and gas orbiting the star acts like a belt, cinching the expanding nebula into an "hourglass" shape.

You can find the full details here. Enjoy!

Credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA), and the Subaru Telescope (National Astronomical Observatory of Japan)

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Space / Astronomy: What's Hot Now: Astronomy 101 - Astronomy H...

Space / Astronomy: What's Hot Now
These articles that had the largest increase in popularity over the last week // via fulltextrssfeed.com
Astronomy 101 - Astronomy H...
Dec 23rd 2011, 11:08

The early theories of the Universe and astronomy, while very clever, all had the same problem. They were all based on incorrect information and beliefs. To create an accurate model, you must first begin with accurate data.

Thanks to the observations of Tycho Brahe, his assistant, Johannes Kepler was able to determine that the circle was not the correct geometric form to explain planetary motions. As a mathematician, he knew that a circle is just a specialized ellipse. Utilizing non-circular ellipses, he was able to calculate orbits, which correctly predicted planetary positions. He couldn’t directly measure a planet's exact orbital sizes, but he was able to measure the ratio by using his equation and Brahe's observations.

Kepler had explained how planets moved, but he still couldn’t explain why. Up till this time, scientists believed that objects tended to stay at rest. Observation had shown that all motion eventually ceases and unmoving objects did not begin to move on their own. So, why would planets?

In the early 17th century, Galileo Galilei used surfaces of varying smoothness to slide blocks across. He found that rough tables made objects slow down at a faster rate than smooth ones. Extrapolating from these observations, he theorized that if a surface were completely smooth, objects would continue moving forever.

If you’ve studied physics, you’ll recognize this as the basis for the theory of inertia. Objects in motion tend to stay in motion in a straight line, and objects at rest tend to stay at rest, unless acted upon by an external force.

Now they knew why the planets were moving, but why in a circle? Why not keep traveling in straight lines and fly off into deep space?

This was answered by Sir Isaac Newton when he published Philosophiae Naturalis Principia Mathematica. He theorized that the external force that kept the planets in orbit was the pull of gravity. According to Newton, the same force that causes an apple falls to the ground also explains why the moon continually "falls" around the Earth.

Meanwhile, our view of the Universe kept evolving. While Tycho Brahe’s attempt to compromise with the Copernican theory and the Ptolemaic model led to an awkward mess, his observations helped Johannes Kepler calculate his three laws of planetary motion, which gave a more accurate picture. Galileo’s discovery of the moons of Jupiter with the newly invented telescope lent credence to the sun-centered model of the solar system.

Starting with Brahe’s years of observation, the work of Kepler, Galileo, and Newton were part of a new era of science, where observation, not philosophy was king. Scientists no longer tried to match data to theory. This would lead to a real renaissance in astronomy and cosmology as well as science in general.

Assignment

Read more about Galileo Galilei, Tycho Brahe, Johannes Kepler and Sir Isaac Newton. Don't forget the discussion Forum.

Third Lesson > Modern Astronomy > Lesson 3, 4, 5, 6, 7, 8, 9, 10

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Space / Astronomy: What's Hot Now: Astronomy 101 - Modern Astr...

Space / Astronomy: What's Hot Now
These articles that had the largest increase in popularity over the last week // via fulltextrssfeed.com
Astronomy 101 - Modern Astr...
Dec 23rd 2011, 11:08

Some people have called Tycho Brahe the Father of Modern Astronomy, but I tend to believe that title belongs to Galileo Galilei. However, Brahe did advance the science more than anyone in the past, simply by using his senses, rather than philosophy to study the sky.

What Brahe began, his assistant, Johannes Kepler expanded upon. His Laws of Planetary Motion were a major building block in the foundation of modern astronomy.

Galileo began the modern age of science, but others continued it. Here, in brief, are some of the other bright lights that helped bring Astronomy to its current place.

  • Edmund Halley (1656-1742) was a British Astronomer who was also a big fan of Sir Isaac Newton. After encouraging Newton to write his Principia, Halley then published it at his own expense. Not stopping to rest on the fame of another, he went on to calculate the orbits of comets, including the one named after him.
  • Sir William Herschel (1738-1822), though born in Germany, was a British astronomer. He discovered Uranus in 1781 coined the word asteroids. He also catalogued about 2000 nebulae, discovered several satellites of Uranus and Saturn, studied the rotation of planets. Discovered and studied binary stars. He discovered two satellites each orbiting Uranus and Saturn. He studied the rotation period of many planets, the motion of double stars, and nebulae. He cataloged more than 800 double stars and contributed new information on the constitution of nebulae. Herschel was the first to propose that these nebulae were composed of stars. He is considered the founder of sidereal astronomy.
  • Albert Einstein (1879-1955) was a German-born American physicist and Nobel laureate. He may be the most well-known scientist of the 20th century. In 1915, he developed his general theory of relativity, which states that the speed of light is constant and that the curvature of space and the passage of time are linked to gravity. Thinking the universe was unchanging, he inserted his "cosmological constant" into his calculations to make them fit his belief.
  • Willem de Sitter: (1872 - 1934), a Dutch astronomer, removed Einstein's cosmological constant and used the theory of relativity to show that the universe may always be expanding.
  • Georges-Henri Lemaitre: (1894 - 1966) was not only a Belgian astronomer, he was also a Jesuit priest. Discovering the writings of Russian mathematician, Alexander Friedmann, Lemaitre took his solution for an expanding universe and theorized that if the universe is expanding, if we follow it back to the starting point, then our universe began as a great "cosmic egg" which exploded and expanded outward. Lemaitre is called by some, the father of the Big Bang Theory.
  • Edwin P. Hubble (1889-1953), American Astronomer. In the 1920s, Albert Einstein stated, "I have made my greatest blunder." This pronouncement came when Edwin Hubble demonstrated that the universe was not static and Einstein's cosmological constant was not necessary. Utilizing improved telescopic devices, he was also able to confirm that those "fuzzy" objects astronomers had seen for years were in fact other galaxies.
  • Thomas Gold (1920 - 2004) is an American astronomer. Though it is generally believed that Gold's "Steady State" theory of the universe is incorrect, he has made many major contributions to our knowledge of the universe, including the nature of pulsars as rotating neutron stars, and the origin of planetary hydrocarbons.
That brings us into the twentieth century. There have been and are many other great brains in the field of astronomy, but it's time to get away from history for now. We'll meet some of these other astronomers throughout the rest of our lessons. Next lesson, let's look at numbers.

Assignment

Read more about Edmond Halley, Albert Einstein, and The Hubble Telescope. Don't forget the discussion Forum.

Fourth Lesson > Big Numbers > Lesson 4, 5, 6, 7, 8, 9, 10

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