Just when you thought it was safe to check your email...

For the sixth year in a row, a message about the Red Planet is popping up in email boxes around the world. It instructs readers to go outside after dark on August 27th and behold the sky. "Mars will look as large as the full moon," it says. "No one alive today will ever see this again."

Don't believe it.

Here's what will really happen if you go outside after dark on August 27th. Nothing. Mars won't be there. On that date, the red planet will be nearly 250 million km away from Earth and completely absent from the evening sky.

Right: Only in Photoshop does Mars appear as large as a full Moon.

The Mars Hoax got its start in 2003 when Earth and Mars really did have a close encounter. On Aug. 27th of that year, Mars was only 56 million km away, a 60,000-year record for martian close approaches to Earth. Someone sent an email alerting friends to the event. The message contained some misunderstandings and omissions—but what email doesn't? A piece of advanced technology called the "forward button" did the rest.

Tolerant readers may say that the Mars Hoax is not really a hoax, because it is not an intentional trick. The composer probably believed everything he or she wrote in the message. If that's true, a better name might be the "Mars Misunderstanding" or maybe the "Confusing-Email-About-Mars-You-Should-Delete-and-Not-Forward-to-Anyone-Except-Your-In-Laws."

Another aspect of the Mars Hoax: It says Mars will look as large as the full Moon if you magnify it 75x using a backyard telescope. The italicized text is usually omitted from verbal and written summaries of the Hoax. (For example, see the beginning of this story.) Does this fine print make the Mars Hoax true? After all, if you magnify the tiny disk of Mars 75x, it does subtend an angle about the same as the Moon.

No. Even with magnification, Mars does not look the same as a full Moon.

This has more to do with the mysterious inner workings of the human brain than cold, hard physics. Looking at Mars magnified 75x through a slender black tube (the eyepiece of a telescope) and looking at the full Moon shining unfettered in the open sky are two very different experiences.

Above: Mars in August 2003 during a 60,000-year record close approach. Even then, the planet resembled a bright star, not a full Moon. Photo credit: John Nemy & Carol Legate of Whistler, B.C.

A good reference is the Moon Illusion. Moons on the horizon look huge; Moons directly overhead look smaller. In both cases, it is the same Moon, but the human mind perceives the size of the Moon differently depending on its surroundings.

Likewise, your perception of Mars is affected by the planet's surroundings. Locate the planet at the end of a little dark tunnel, and it is going to look tiny regardless of magnification.

Bummer!

To see Mars as big as a full Moon, you'll need a rocketship, and that may take some time. Meanwhile, beware the Mars Hoax.

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(CNN) -- On July 23, 1969, as Apollo 11 hurtled back towards Earth, there was a problem -- a problem only a kid could solve.

At age 10, Greg Force reaches his arm into a tiny hole to fix an antenna crucial to Apollo 11.

It sounds like something out of a movie, but that's what it came down to as Apollo 11 sped back towards Earth after landing on the moon in 1969.

It was around 10:00 at night on July 23, and 10-year-old Greg Force was at home with his mom and three brothers. His father, Charles Force, was at work. Charles Force was the director of the NASA tracking station in Guam, where the family was living.

The Guam tracking station was to play a critical role in the return of Apollo 11 to Earth. A powerful antenna there connected NASA communications with Apollo 11, and the antenna was the only way for NASA to make its last communications with the astronauts before splashdown. But at the last minute on that night, a bearing in the antenna failed, rendering it nearly useless.

To properly replace the bearing would have required dismantling the entire antenna, and there was simply no time. So Charles Force thought of a creative solution: If he could get more grease around the failed bearing, it would probably be fine. The only problem was, nobody at the station had an arm small enough to actually reach in through the two-and-a-half inch opening and pack grease around the bearing.

And that's when Greg was called in to save the day. Charles Force sent someone out to his home to pick up Greg. Once at the tracking station, Greg reached into the tiny hole and packed grease around the failed bearing. It worked, and the station was able to successfully complete its communications role in the mission. Apollo 11 splashed down safely the next day.

At the time, Greg didn't think what he was doing was a big deal, and 40 years later, he's still modest about his role in the mission.

"That's all I did, was put my hand in and put grease on it," he says. If he hadn't been there, NASA would not have been able to make its last communications with the mission before splashdown, but Greg says "it wasn't life or death, [from] my understanding."

"My dad explained to me why it was important," he says, "but it kind of caught me by surprise afterwards, all the attention."

That attention came from the media and even the astronauts themselves. Greg's small but important part in Apollo 11 was a story told by news outlets around the world. He even got a nice thank-you note from Neil Armstrong, whom he met when Armstrong went on a tour of NASA stations with the other astronauts to thank the staff after the mission. "To Greg," reads the note, which Armstrong wrote on a newspaper clipping of Greg's story, "with thanks for your help on Apollo 11. Neil Armstrong."

Perhaps not surprisingly, like many other kids who grew up during the Apollo era, Greg dreamed of becoming an astronaut. He says he remembers visiting his dad's office to listen to astronauts communicating with NASA officials on the ground.

"We could sit and listen to the actual communication with the astronauts as it was happening, and it was hard to understand, but I loved to do that," he says. "On Guam we didn't have good television coverage, so I think I listened to the [moon] landing on the radio. To me it was a huge thing."

Greg pursued his dreams of space exploration all the way through college, where he majored in physics. Unfortunately, he was unable to pass the vision test for the space program because of his colorblindness, but even that couldn't squelch his interest. Greg went on to get his pilot's license, and even though his career now as a gymnastics school owner isn't exactly space-related, he says that "ever since then, I've followed the space program."

And as a lover of space exploration, Greg hopes to see more missions to the moon.

"I think it would be an important step as far as going further, like to Mars," he says. "I would love to see us go back to the moon."

But for now, on the 40th anniversary of the moon landing, he can remember the small but crucial role he played in bringing Apollo 11 home safely.

"It kind of caught me by surprise," he says, "but I'm real proud to have been even a little tiny part of it."
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A survey of space shuttle Atlantis' outer body has revealed that four tiles on the right side have "some dings" in them, the flight director said Tuesday.

Space shuttle Atlantis launched from Florida Monday on its way to the Hubble telescope.

"As we were going through the surveys we did see probably about 21 inches in all ... four tiles with some dings in them," Tony Ceccacci told reporters.

"To me, I'm not the tile expert, but they looked very minor."

He said tile experts will examine the dings, which are on the wing.

Ceccacci said an "event" occurred around 103 seconds into Monday's launch.

He said NASA is looking into what may have caused the nicks. Debris that fell off the external fuel tank during liftoff has been the culprit on previous flights.

Atlantis launched Monday afternoon for NASA's fifth and final repair visit to the Hubble Space Telescope, with which it is scheduled to rendezvous on Wednesday.

It has been seven years since NASA's last mission to service the Hubble, which was designed to go only about three years between fixes.

NASA canceled an Atlantis mission to extend Hubble's operational life in January 2004 because the trip was considered too risky in the wake of the 2003 Columbia tragedy, which killed seven astronauts.

That disaster was blamed on a hole punched in the front of the wing by debris during liftoff.

But public pressure and steps taken to increase shuttle safety led the U.S. space agency to reconsider.

Space shuttle Endeavour is on standby at the Kennedy Space Center in Florida in the unlikely event that NASA will need to rescue the Atlantis crew members during their 11-day mission. Read more!

Last October 16th was a big day for the Chinese astronomical community. Nearly 200 kilometers northeast of Beijing, at the Xinglong Observing Station of the National Astronomical Observatories of China (NAOC), leaders of the Chinese Academy of Sciences held a ceremony to celebrate the founding of something new and unique: LAMOST, the Large Sky Area Multi-Object Fiber Spectroscopic Telescope.

The LAMOST observatory buildings, aligned on the meridian.

Renjiang Xie

LAMOST is a survey instrument like no other. It was designed for maximum efficiency for one vital purpose: taking spectra of many millions of individually selected, very faint objects. Its designers had to find the best balance for this purpose between aperture, field of view, and many other factors.

The surface shape of LAMOST's 4-meter segmented primary mirror will be actively controlled, allowing the segments to be thin and light.

Renjiang Xie

The instrument's segmented thin mirror, seen above, has an aperture of 4 meters (160 inches), with the segments controlled by active-optics techniques. This aperture will enable LAMOST to obtain spectra of objects as faint as magnitude 20.5 magnitude in a 1.5-hour exposure.

LAMOST's fiber-optic image detector, seen from behind.

Renjiang Xie

That's not remarkable by today's standards — LAMOST's real power comes from its extraordinary field of view. The working focal plane is an immense 1.75 meters in diameter, corresponding to a 5° field on the sky.

As many as 4,000 optical fibers can be automatically positioned onto selected objects in the field, with each fiber feeding light to a spectral analyzer. As a result, the telescope has the highest spectrum-acquiring rate of any in the world.

Being a survey telescope, LAMOST needs to look only near the sky's north-south meridian to catch, in time, a large fraction of the celestial sphere passing across. As a result the telescope occupies special domes that look less like a traditional observatory than like some spaceport from a sci-fi movie.

“LAMOST’s equipment was completely installed by the end of August after four years’ of building," says Yongheng Zhao, the general manager of the project. "We are now in the stage of doing test observations and refining performance, which may take two years.”

With a diameter of some 500 meters (1,600 feet), FAST will be the world's largest radio dish. Click image for cross-section diagram.

NAOC / Chinese Academy of Sciences

FAST Radio Dish

Meanwhile, the ambitious Five hundred-meter Aperture Spherical radio Telescope (FAST) has been allocated government funds of nearly 700 million RMB yuan (nearly US$100 million). FAST will be built in a limestone karst valley in a sparsely populated mountanous area of Guizhou province about 1,800 kilometers southwest of Beijing.

FAST's dish will be composed of about 2,000 active panels, each 15 meters square, that can reshape into a paraboloidal surface for pointing in any direction as much as 40° from the zenith. Construction has begun and should be finished in 2014. FAST is expected to be 10 times as sensitive as the 300-meter dish radio telescope near Arecibo, Puerto Rico, currently the world's largest.
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In the game of astronomy, size matters. To get crisp, clear images of things billions of light years away, a telescope needs to be big.

"The bigger the better," says astronomer Harley Thronson, who leads advanced concept studies in astronomy at the Goddard Space Flight Center. And he thinks "NASA's new Ares V rocket is going to completely change the rules of the game."

Ares V is the rocket that will deliver NASA's next manned lunar lander to the moon as well as all the cargo needed for a lunar base. Its roomy shroud could hold about eight school buses, and the rocket will pack enough power to boost almost 180,000 kg (396,000 lbs -- about 16 or 17 school buses) into low Earth orbit. Ares V can haul six times more mass and three times the volume the space shuttle can.

"Imagine the kind of telescope a rocket like that could launch," says Thronson. "It could revolutionize astronomy."

Right: The roomy shroud of the Ares V could hold about eight school buses. Credit: NASA

Optical engineer Phil Stahl of the Marshall Space Flight Center offers this example: "Ares V could carry an 8-meter diameter monolithic telescope, something that we already have the technology to build. The risk would be relatively low, and there are some big cost advantages in not having to cram a large telescope into a smaller launcher."

For comparison, he points out that Hubble is only 2.4 meters wide.

An 8-meter monolithic telescope would see things more than three times as sharply as Hubble can. More importantly, in the same amount of observing time, the larger mirror would see objects that are about 11 times fainter than Hubble sees because the 8-meter telescope has 11 times the light collecting area.

But Ares V can go yet bigger. It could transport a huge segmented telescope – one with several separate mirror panels that are folded up for transport like the James Webb Space Telescope--but three times the size!

The Space Telescope Science Institute's Marc Postman has been planning a 16-meter segmented optical/ultraviolet telescope called ATLAST, short for Advanced Technology Large-Aperture Space Telescope. The science from an aperture its size would be spectacular.

"ATLAST would be nearly 2000 times more sensitive than the Hubble Telescope and would provide images about seven times sharper than either Hubble or James Webb," says Postman. "It could help us find the long sought answer to a very compelling question -- 'Is there life elsewhere in the galaxy?'"

ATLAST's superior sensitivity would allow astronomers to hugely increase their sample size of stars for observation. Then, discovery of planets hospitable to life could be just around the corner!

"With our space-based telescope, we could obtain the spectrum of Earth-mass planets orbiting a huge number of nearby [60 - 70 light years from Earth] stars," says Postman. "We could detect any oxygen and water in the planets' spectral signatures. ATLAST could also precisely determine the birth dates of stars in nearby galaxies, giving us an accurate description of how galaxies assemble their stars."

This telescope could also probe the link between galaxies and black holes. Scientists know that almost all modern galaxies have supermassive black holes in their centers. "There must be a fundamental relationship between the formation of supermassive black holes and the formation of galaxies," explains Postman, "but we don't understand the nature of that relationship. Do black holes form first and act as seeds for the growth of galaxies around them? Or do galaxies form first and serve as incubators for supermassive black holes? A large UV/optical telescope could answer this question: If our telescope finds ancient galaxies that do not have supermassive black holes in their centers, it will mean galaxies can exist without them."

Dan Lester of the University of Texas at Austin envisions another 16-meter telescope, this one for detecting far-infrared wavelengths.

"The far-infrared telescope is quite different from, and quite complementary to, the optical telescopes of Stahl and Postman," says Lester. "In the far-infrared part of the spectrum, we generally aren't looking at starlight itself, but at the glow of warm dust and gas that surrounds the stars. In the very early stages of star formation, the proto-star is surrounded by layers of dust that visible light can't penetrate. Our telescope will allow us to see down into the innards of these giant dense clouds that are forming stars deep inside."

Observations in the far-infrared are especially challenging. These long wavelengths are hundreds of times larger than visible light, so it's hard to get a clear picture. "A very big telescope is necessary for good clarity at IR wavelengths," notes Lester.


Like the telescopes of Stahl and Postman, Lester's Single Aperture Far-Infrared Telescope ('SAFIR' for short), comes in two flavors for the Ares V: an 8-meter monolithic version and a 16-meter segmented version. Lester realized that, with an Ares V, he could launch an 8-meter telescope that didn't need complicated folding and unfolding. "But on the other hand, if we don't mind adding the complexity and cost of folding and still use an Ares V, we could launch a really mammoth telescope," says Lester.

In addition to all the above telescopes, Ares V could boost an 8-meter-class X-ray telescope into space. NASA's highly-successful Chandra X-ray Observatory has a 1 meter diameter mirror, so just imagine what an 8-meter Chandra might reveal!

Roger Brissenden of the Chandra X-ray Center is excited about the possibility of a future 8-meter-class X-ray telescope called Gen-X.

"Gen-X would be an extraordinarily powerful X-ray observatory that could open up new frontiers in astrophysics," he says. "This telescope will observe the very first black holes, stars and galaxies, born just a few hundred million years after the Big Bang, and help us determine how these evolve with time. Right now, the study of the young universe is almost purely in the realm of theory, but with Gen-X's extreme sensitivity (more than 1000 times that of Chandra) these early objects would be revealed."

Indeed, Ares V flings shutters open wide on our view of the cosmos. It shakes off the shackles of mass and volume constraints from science missions and sweeps us into deep space to view "...a hundred things/ You have not dreamed of."

"We could get incredible astronomy from this big rocket," says Thronson, a professional dreamer. "I can't wait." Read more!

International Year of Astronomy 2009

by the Editors of Sky & Telescope

---

IAU

New Year's Day marks the beginning of what will undoubtedly be more than 12 months of celebrating astronomy. The International Astronomical Union (IAU) has designated 2009 as the International Year of Astronomy (IYA2009) to commemorate the 400th anniversary of Galileo's first celestial observations using a telescope. IYA2009 has been endorsed by the United Nations Educational, Scientific, and Cultural Organization (UNESCO) and the U.N. General Assembly.

Much of IYA2009's activities revolve around 11 Cornerstone Projects. While some initiatives are already underway, others still remain under development. The links to their individual sites are listed below. You'll find even more information at U.S. National Node. If you don't live in the U.S., see IYA2009's main site for a link to your country's node.

100 Hours of Astronomy: 400 Years in the Making
The Galileoscope: Millions of People Looking at the Sky
Cosmic Diary: The Life of an Astronomer
Portal to the Universe: A One-stop Universe of News
She Is an Astronomer: Breaking Down Misconceptions
Dark Skies Awareness: Seeing in the Dark
Astronomy and World Heritage: Universal Treasures
Galileo Teacher Training Program: Teaching the Teachers
Universe Awareness: One Place in the Cosmos
From Earth to the Universe: The Beauty of Science
Developing Astronomy Globally: Astronomy for All

And while it's not an official Cornerstone Project, the amateur-led The Earth at Night project is another important element for IYA2009.

Make room on your iPod for the 365 Days of Astronomy Podcast. There's a fact-filled, fun episode every day.

We're happy to provide the article "The Year to Celebrate Astronomy" by organizers Catherine Cesarsky, Pedro Russo, and Lars Lindberg Christensen from the January 2009 issue of Sky & Telescope as a free download in PDF format. (To display PDF files, download and install the free Adobe Reader.)

Be sure to check out the official movie of IYA2009: Eyes on the Skies produced by the European Space Agency and European Southern Observatory.

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HOUSTON -- Nations around the world will join together to mark a milestone in space exploration this week, celebrating the 10th birthday of a unique research laboratory, the International Space Station.

Now the largest spacecraft ever built, the orbital assembly of the space station began with the launch from Kazakhstan of its first bus-sized component, Zarya, on Nov. 20, 1998. The launch began an international construction project of unprecedented complexity and sophistication.

The station is a venture of international cooperation among NASA, the Russian Federal Space Agency, Canadian Space Agency, Japan Aerospace Exploration Agency, or JAXA, and 11 members of the European Space Agency, or ESA: Belgium, Denmark, France, Germany, Italy, the Netherlands, Norway, Spain, Sweden, Switzerland and the United Kingdom. More than 100,000 people in space agencies and contractor facilities in 37 U.S. states and throughout the world are involved in this endeavor.
"The station's capability and sheer size today are truly amazing," said International Space Station Program Manager Mike Suffredini. "The tremendous technological achievement in orbit is matched only by the cooperation and perseverance of its partners on the ground. We have overcome differences in language, geography and engineering philosophies to succeed."

Only a few weeks after the U.S.-funded, Russian-built, Zarya module was launched from Kazakhstan, the space shuttle carried aloft the Unity connector module in December 1998. Constructed on opposite sides of Earth, Unity and Zarya met for the first time in space and were joined to begin the orbital station's assembly and a decade of peaceful cooperation.

Ten years later, the station's mass has expanded to more than 627,000 pounds, and its interior volume is more than 25,000 cubic feet, comparable to the size of a five-bedroom house. Since Zarya's launch as the early command, control and power module, there have been 29 additional construction flights to the station: 27 aboard the space shuttle and two additional Russian launches.

One hundred sixty seven individual representing 14 countries have visited the complex. Crews have eaten some 19,000 meals aboard the station since the first crew took up residence in 2000. Through the course of 114 spacewalks and unmatched robotic construction in space, the station's truss structure has grown to 291 feet long so far. Its solar arrays now span to 28,800 square feet, large enough to cover six basketball courts.

The International Space Station hosts 19 research facilities, including nine sponsored by NASA, eight by ESA and two by JAXA. Cooperation among international teams of humans and robots is expected to become a mainstay of space exploration throughout our solar system. The 2005 NASA Authorization Act recognized the U.S. orbital segment as the first national laboratory beyond Earth, opening it for additional research by other government agencies, academia and the private sector.

"With the International Space Station, we have learned so many things -- and we're going to take that knowledge and apply it to flying to the moon and Mars," said Expedition 18 Commander Mike Fincke, now aboard the station. "Everything we're learning so close to home, only 240 miles away from the planet, we can apply to the moon 240,000 miles away."

To take a virtual tour of the International Space Station and learn more about the current mission, visit:

http://www.nasa.gov/station


To find out how to see the station from your own backyard, visit:

http://www.spaceflight.nasa.gov/realdata/sightings
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