Citizen Science: Unmannedspaceflight.com

Mosaic created by UMSF's James Canvin from images taken by the Opportunity rover, sol 1707. Credit: NASA/JPL/Cornell/James Canvin

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Note: This is the first in a series of articles about Citizen Science projects, where science is not just for professional scientists anymore!

The desire to seek out others of a like mind must be coded into our DNA. Take any subject — music, literature, art, science, math, sports, animals — you name it, and there is a group you can join to share your interest with others. Or if you can’t find a group, then you can start one and see who joins in. Doug Ellison is a great example. His online forum Unmannedspaceflight.com (UMSF) has become a place where a combination of interest in space exploration and serious “Photoshopping” has taken on new proportions. But it is also a place where the line between amateur interest and professional science is starting to blur.

Plainly put, the images, mosaics and movies created by the participants at UMSF are stunning. Whether it be a panoramic view from the top of Husband Hill on Mars, recalibrated images from the Pioneer or Voyager spacecraft to create 3D renderings or maps of the planets, or a movie of Opportunity roving on Meridiani Planum, the work being done at UMSF is a feast for the eyes. And this is all being done by amateurs who don’t receive any compensation for their painstaking handiwork, except for the joy of sharing their images with each other and the public, and perhaps converting a few space exploration naysayers along the way. They do their work using cheap, free, or even personally-created imaging software, to generate their labors of love.

Listen to Doug Ellison on today’s 365 Days of Astonomy podcast talk about “Bootleg Postcards: Armchair Astronauts Exploring the Solar System.

How it all began

Ellison’s interest in space exploration started with the Mars Pathfinder mission in 1997, where information and images from the mission were being shared online, just as the internet was starting to boom. But when his own country, England, led the Beagle 2 Lander mission to Mars in 2003, Ellison’s interest got a little more serious. “Being a Brit, I was proud of Beagle, and wanted to talk about it with others,” said Ellison, a media producer, “but I couldn’t find any online forums discussing the mission. So I started a Yahoo group, and about 40 or 50 people descended on it, and we posted updates about the mission.” And the online updates and discussions were serious – no talk about little green men, Martians or UFOs was allowed.

The Mars Exploration Rovers were also on Ellison’s radar, as he knew they were set to land just after Beagle 2, but he admits not paying all that much attention to the rovers. However, when all contact was lost with Beagle 2 after it separated from the Mars Express orbiter, Ellison turned his attention to the rovers. The firehose of images from the rovers was almost immediate after they landed in January 2004: Principal Investigator Steve Squyres and Pancam lead Jim Bell had both decided to post all the images online, making them available for anyone with internet access virtually the instant the data were beamed back to Earth from Mars.

“I saw all these JPEG images online at the rover site, and I couldn’t help myself!” said Ellison, who had also developed an interest in image editing. “I started making mosaics and movies from the rover images. And in the same way I couldn’t find anywhere to talk about Beagle, I couldn’t find a ‘sensible’ place to talk about the rovers, and where I could discuss the images.”

UMSF image that was used on the cover of Aviation Week magazine.   Credit:  NASA/JPL/ Cornell and Marco Di Lorenzo, Doug Ellison, Bernhard Braun,  and Kenneth Kremer
UMSF image that was used on the cover of Aviation Week magazine. Credit: NASA/JPL/ Cornell and Marco Di Lorenzo, Doug Ellison, Bernhard Braun, and Kenneth Kremer


Ellison noted he hadn’t yet found the BAUT (Bad Astronomy Universe Today) forum, but he noticed that almost any website or forum where Mars was the topic, the discussion would “soon turn to anomalism, nut-jobbery, and crazy-talk, so I was determined if I couldn’t find anything I would start my own site to post my images, etc.,” he said. “And if someone came along and said something like, ‘Oh there’s a skull, and there’s cannon,’ I just wasn’t going to have it,” he said.

Ellison never advertised or “pimped” the site, and the first year things were pretty quiet, with just a few dozen people joining in who were doing their own mosaics or global maps. Then the Cassini mission came along, and those images also went straight to a publicly accessible website, so a Cassini/Saturn section was added to the forum; then a Mars orbiter section and a New Horizons section – any mission where the images were available.

“So it expanded from just being a site about the rovers to any spacecraft that was going around taking pictures,” said Ellison, “so about a year after I started the site, I re-named it unmannedspaceflight.com.”

While the site hasn’t exploded or gone completely viral, it has quietly expanded to about 1,800 active members and about 30,000 visitors a month. “It spikes when there’s something interesting happening, such as the Phoenix landing, but otherwise its fairly steady, with about 100 or so really active people contributing images, with an awful lot of people who just like to hang around and look.”

The ‘Old Days’ and Now

It used to be difficult to get images from space missions, with enthusiasts having to wait weeks or months for a print magazine or book to publish pictures taken by spacecraft. But the internet has changed all that, and in addition, attitudes among the previously exclusive science community seem to be changing as well.

“NASA really does try to make data as accessible to the public as it can,” said Emily Lakdawalla from the Planetary Society, who writes the Planetary Blog. She has been a member of UMSF since 2005, and as a planetary geologist, enjoys working with space mission images. “Anybody in the world with net access can get to all the data ever taken by nearly every NASA planetary mission,” she said. “It is sort of like discovering the back rooms of the Smithsonian collections — they display only a few percent of their artifacts. NASA captions and press-releases only a few percent of their missions’ data, but it’s all online, waiting for people to discover and use it. UMSF is a community of people who live to do just that — delve into the museum vaults, discover wonders that few people on Earth have ever seen, dust them off, restore them, and display them to public view.”

As amateurs, Lakdawalla said, they can take liberties with the data that scientists usually can’t allow themselves to. If a data dropout creates an ugly stripe across an otherwise pretty image, a scientist will usually not fudge the data to make it look better. An amateur needs to have no such constraints; they can “futz” with the images, and produce eye-catching, print-ready images out of something that would have otherwise not been very interesting to non-scientists.

“The wonderful thing about UMSF is that the community there generally takes exactly the right level of liberties with the data,” said Lakdawalla, “basically, enough fudging as is required to prevent the viewer from being distracted by artifacts of the imaging process, but little enough to let the original space data do all the talking.”

A fanciful image of Opportunity's reflection in its heat sheild -- an image that was never taken, but created by Stuart Atkinson.  Credit: NASA/JPL/Stuart Atkinson
A fanciful image of Opportunity's reflection in its heat sheild -- an image that was never taken, but created by Stuart Atkinson. Credit: NASA/JPL/Stuart Atkinson

While there are many space-topic forums on the internet, UMSF is different for two very important reasons, said Stuart Atkinson, care worker for the elderly in the United Kingdom by day, who has been involved with UMSF since the old days of the Beagle discussions. “Firstly, because it has a strict – and strictly enforced – policy of not tolerating ‘off topic’ posts about such things as politics, manned spaceflight, alien babies or Bigfoots on Mars and things like that,” said Atkinson. “UMSF is, as its name suggests, a forum for discussing unmanned spaceflight – spaceprobes, basically, and if anyone comes along trying to flame, or cause trouble, or claim they’ve found a piece of wood or an alien skull in a zoomed-in-to-within-an-inch-of-its-life section of a Mars rover image then they’re in the wrong place.”

The strict “policing” of the site, performed by about a dozen or so moderators has created an environment where even scientists feel comfortable joining in on the discussions. “Planetary Scientist Ralph Lorenz has come over and talked about Titan’s dunes, and Alan Stern has joined in discussions about New Horizons, for example,” said Ellison.

Which is the other thing that makes it so special, added Atkinson. “Become a member of UMSF and you’ll find yourselves rubbing virtual shoulders with many of the men and women who actually work ON the missions… Mars Rover drivers, Deep Space Network operators, Mars geologists and climatologists, they’re all members of UMSF, and clearly love being able to take part in discussions about their work.”

Doug Ellison's creation of Phoenix's landing site for the Through the Eyes of the Phoenix Competition, organized by spacEurope in association with the mission's Education & Public Outreach program.
Doug Ellison's creation of Phoenix's landing site for the Through the Eyes of the Phoenix Competition, organized by spacEurope in association with the mission's Education & Public Outreach program.

But not only have scientists joined in on discussions, they’ve come to UMSF to ask for help. Ellison said a highlight of his involvement with UMSF was when John Spencer from the New Horizons mission came to the forum asking if the members had any ideas for New Horizon’s flyby of Jupiter. “He came onto the forum and said, we’re planning the science sequence for the Jupiter flyby and do any of you have any ideas of when we should take pictures, just because they will be cool and interesting images. And he gave us the link for the tool that would show us the view from the New Horizons trajectory at a particular time, at any direction we wanted.”

Suggestions from UMSF members were put into an amalgamation of ideas from scientists and four ideas from UMSF were chosen for the flyby.

“I could not believe it, that my little forum had become an engine to come up with ideas, and these ideas got sent to a $800 million spacecraft a half a billion kilometers away,” said Ellison. “And New Horizons took this amazing picture of Europa rising up behind Jupiter. The fact that he came to us, asked us for ideas, and actually used them just was amazing.”

“New Horizons really exemplifies the best of amateurs and professionals working together,” said Lakdawalla. “All missions like to take advantage of “Kodak moments,” and the longer lived ones, particularly MER and Cassini, get the leisure to plan to take a few pictures just because they’re pretty, or significant. New Horizons wanted to do that but had a ridiculously short time between launch and Jupiter… It was a great use of amateur effort, for the right purpose — not to do science, but to do what the amateurs do best (and better than most scientists) — make pretty pictures.”

As an example of what UMSF does with images, Lakdawalla took image of Jupiter’s moons Io and Europa that was captured by New Horizons’ LORRI instrument (Long Range Reconnaissance Imager), combined it with another image taken by the MVIC (Multispectral Visible Imaging Camera) visible- and near-infrared spectrometer, to create a truly spectacular image of the pair of moons.

Io and Europa together.  Credit: NASA / JHUAPL / SwRI / Emily Lakdawalla
Io and Europa together. Credit: NASA / JHUAPL / SwRI / Emily Lakdawalla


“Emily took the best data, combined them and made something better from it,” said Ellison. “I didn’t make the actual suggestion or create the actual picture but I’m very, very proud of those pictures because the people from New Horizons thought we’d come up with some sensible ideas and we did. It was an example of the amateur doing something truly spectacular.”

Ellison said starting UMSF has truly been life-changing. He has had the opportunity to meet scientists involved with the space missions, and even gave a presentation to the MER science team at Cornell University, which he said was “the highlight of my life.”

Images from UMSF have appeared on the cover of Aviaton Week, and several times on Astronomy Picture of the Day, including an incredible flyover movie of the Columbia Hills, and a great image from Opportunity of clouds and sand on Mars.

The work of another active UMSF member, James Canvin, showed up at a very special place: on the wall in the operations building for the Phoenix Mars Lander. It was visible during a visit by Sky at Night television show on BBC. “Recognition of that type, by people within the team running the mission itself is a huge honour,” said Canvin, who is a scientist for the United Kingdom’s main weather forecasting center. Canvin said image processing has become his main hobby, and countless hours have been spent writing the software to do the processing as well as producing the images themselves.

James Canvin's version of Phoenix' Mission Success Panorama, which includes 150 separate camera pointings taken from sols 13 to 43. Canvin produces his mosaics using software he developed for Mars Exploration Rover panoramas. This is an interim data product, considerably reduced in resolution from the original data. Credit: NASA / JPL / UA / Texas A & M / color mosaic by James Canvin
James Canvin's version of Phoenix' Mission Success Panorama, which includes 150 separate camera pointings taken from sols 13 to 43. Canvin produces his mosaics using software he developed for Mars Exploration Rover panoramas. This is an interim data product, considerably reduced in resolution from the original data. Credit: NASA / JPL / UA / Texas A & M / color mosaic by James Canvin


But perhaps the biggest reward of creating these “bootleg” images is the effect the images have on the general public.

“A big highlight is having my images seen (and getting positive feedback from) people who don’t normally follow spaceflight activities,” Canvin said. “I only ever post images to UMSF but occasionally I’ll see referrals coming from non-spaceflight related sites where somebody has re-posted the link with a “hey this is cool, look at this” type message. It’s nice that I have been able to help get the word out to a few people who might not have known what was going on Mars otherwise. During my time at UMSF I’ve really come to appreciate the value of working to bring the amazing sights of the solar system to as wide an audience as possible.”

Ellison also spends a lot of his time doing talks about space exploration at schools, and is working on applying for grant to do more activities with schools and even science centers. He also has plans for ways to make the tools created by the UMSF participants more accessible to more people by creating a “Wiki.” “What I want to do is extract the material and the knowledge that’s there collectively into a specialized Wiki around the things that get discussed,” said Ellison. “That will turn our sometimes idle banter into a usable, citable reference tool.” This would certainly be a tremendous resource for photography and digital imaging aficionados.

I Heart Spacecraft

UMSF is a true love affair with the images produced by our robotic spacecraft. “I was talking with (British historian) Allan Chapman,” said Ellison, “and he said this is amateur in the true sense of the word because amateur means love. And that’s true because people love doing this. We do it because it’s an adventure and it’s exploration that we can do.”

UMSF participants have created special tools to enhance the experience, like the Midnight Mars Browser written by Mike Howard. What began as a simple tool to automatically grab images when they became available, has evolved into an interactive tool that will download and sort the images, produce color composites, stereo anaglyphs and even re-project the imagery into virtual 3D space so that Pancam and Navcam imagery can be seen in context, site by site, sol by sol.

Once you start, creating your own images can also become something close to an addiction. “There’s a genuine chance for you to look at a little piece of the Mars that no one has set eyes on before,” said Ellison. “And that’s an incredibly powerful thing. The process how the pictures go online is all automated, and you think, ‘I should go to bed now, but the images will hit the web in about an hour, so I’ll stay up and wait for the pictures.’ And you make a mosaic and put it on the forum and then a hundred people can see this little bit of Mars that no one else has seen before.”

While in some people’s minds, what’s being done at UMSF brings up questions about the fair use of raw images from mission websites, it seems to point to a possible future where amateurs and scientists work together for the common good.

Doug Ellison's creation of the Columbia Hills using a combination of Hation of HiRISE images, rover images and a tool called Dreamscape.
Doug Ellison's creation of the Columbia Hills using a combination of Hation of HiRISE images, rover images and a tool called Dreamscape.

“Scott Maxwell (MER rover driver – see our three part interview with Maxwell) and I share a vision for a Mars 3.0,” said Ellison. “Mars 1.0 is when you have to wait for the press to come out with a single picture from a mission. 2.0 is roughly where we are now, where all the pictures come out and anyone can look at them. Mars 3.0 is finding a way whereby the enthusiastic public can contribute back in. I thought the New Horizons ‘Kodak moment’ was an example that it can work. It’s not sensible to hand the rover driving gloves off to amateurs or anything like that, but there has to be some sort of middle ground where there’s a type of ‘audience participation’ that can be done. The sheer numbers in the amateur community and the massively wide range of abilities they posses, they can actually make a contribution back to the missions.”

Ellison said he doesn’t know how it will eventually turn out, or even if a true amateur/professional partnership is even possible because of things like ITAR (International Traffic in Arms Regulations) and other restrictive laws that NASA and JPL must abide by.

But in the meantime, there’s much to enjoy from UMSF, even for the digitally-challenged. “Anyone can come and enjoy the pictures and watch what we’re doing,” said Ellison. “I’ve always maintained that you don’t have to register just to look at the pictures. So, come and click on the latest about Opportunity and look at the next day, and you’ll see someone will update the map, someone will make a new mosaic, and someone will make a movie: it will all happen and you can watch it. Or if you think you can wield Photoshop, and if you think you have some ideas, give us a try. As long as you don’t go into the realm of crazy, we’ll share what we know with you.”

Aurora Australis at the South Pole

Aurora Australis over the elevated station at Amundsen-Scott South Pole Station, Antarctica. Credit: Calee Allen, National Science Foundation

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I just had to share this gorgeous image of the Aurora Australis over the Amundsen-Scott South Pole Station in Antarctica. “Northerners” like myself occasionally get to see the Aurora Borealis, or Northern Lights, but fewer people get to the the Aurora Australis because so few people live in Antarctica during the austral winter. In both hemispheres however, the cause of these eerie light shows is the same: the solar wind passing through the Earth’s upper atmosphere. This image was taken in May of 2008, but was just recently posted by the National Science Foundation.

Here’s a link to a larger, hi-res version of the image above.

The Amundsen-Scott Station has been open for just a year, and below are more pictures and information.

Amundson-Scott Station. Credit: Keith Vanderlinde, National Science Foundation
Amundson-Scott Station. Credit: Keith Vanderlinde, National Science Foundation

Stars are visible in this image, also taken in May of 2008, during the short daytime in the winter at the South Pole. Amundsen-Scott South Pole Station sits at the Earth’s axis, atop a constantly shifting continental ice sheet nearly two miles thick. This is perhaps the world’s most remote research facility,

In January 2008, the National Science Foundation (NSF) dedicated the new station at the Pole, the third since 1956. The new station is larger and much more sophisticated than any previous structure built at the Pole. Research in a range of areas, from astrophysics to seismology, takes place at the station. The new elevated station contains dorm rooms, laboratories, office space, cafeteria and recreational facilities.

If you’d like to keep an eye on what’s going at the Station, there is a live web-cam that updates every 20 seconds.

There’s a huge amount of information about Amundsen-Scott Station at the NSF website.

Source: NSF

The Universe Today Top 10 Scientific Endeavours of 2008

The nominations are in, the votes have been counted and the Universe Today writers have been consulted; the Top 10 Scientific Endeavours of 2008 are decided! After much consideration by the readers of the Universe Today, it became quickly apparent what the popular choice would be, and some of the Top 10 may not come as a surprise. However, there are some nominations we weren’t expecting, and certainly cannot be found on any other “Top 10” list. Therefore, I believe the Universe Today’s Top 10 Scientific Endeavours of 2008 is the most comprehensive list out there, combining the votes of our readers, nominating a huge variety of articles available through one of the biggest space news websites on the Web.

For more information about the motivation behind the Universe Today’s Top 10, be sure to check out the nominations page

Without further ado, here is the Universe Today’s definitive Top 10 Scientific Endeavours of 2008…

10. Chandra X-ray Observatory

Chandra X-ray image of M84 (NASA/CXC/MPE/A.Finoguenov et al.); Radio (NSF/NRAO/VLA/ESO/R.A.Laing et al); Optical (SDSS)
Chandra X-ray image of M84 (NASA/CXC/MPE/A.Finoguenov et al.); Radio (NSF/NRAO/VLA/ESO/R.A.Laing et al); Optical (SDSS)
Launched on July 23rd 1999, NASA’s Chandra X-Ray observatory has opened our eyes to the X-ray Universe. Chandra was named in honour of the late Indian-American Nobel laureate, Subrahmanyan Chandrasekhar. Subrahmanyan was known to the world as Chandra (which also means “moon” or “luminous” in Sanskrit) and he was regarded as one of the most influential astrophysicists of the 20th Century. It is fitting that one of the most influential X-ray observatories of the start of the 21st Century should bear his name.

Chandra has benefited our understanding of the cosmos in so many ways, it is hard to single out one endeavour. In 2008 alone, it has been used to “weigh” supermassive black holes, it has spotted the X-ray echo of stars being ripped apart in the centre of galaxies, it has also seen the echoes of supernovae, taken data supporting the existence of magnetars, found evidence supporting the theory of dark matter and linked the existence of dark energy with the growth of galactic clusters.

In short, Chandra is an astounding mission, continuing to shape our understanding of known X-ray phenomena, providing us with a glimpse at the answers to some of the most puzzling questions of our time. Certainly one of the “Great Observatories”.

For more, check out The Universe Today articles filed under the category “Chandra”.

9. Epsilon Eridani

This artist's conception shows the closest known planetary system to our own, called Epsilon Eridani. Credit: NASA/JPL/Caltech
This artist's conception shows the closest known planetary system to our own, called Epsilon Eridani. Credit: NASA/JPL/Caltech
The star system of Epsilon Eridani has provided astronomers with a tantalizing look into past of our very own Solar System since 2000. Being the ninth closest star to our Sun, it is also fairly easy to observe. At approximately 850 million years old, it is effectively what our system will have looked like when it was young; scattered disks of asteroids and dust, with exoplanets orbiting the star. Astronomers have even half-jokingly formed the link between Star Trek‘s fictional world of “Vulcan” with one of the large exoplanets known to be shaping one of the asteroid belts.

In 2008, further work has been done analysing the structure of the Epsilon Eridani system and there is even more evidence to suggest the star system is the Solar System’s “twin”. Although the star itself is slightly smaller and cooler than the Sun, it does possess several unseen planets, creating an asteroid belt much like ours, plus an outer belt (analogous to our Kuiper Belt, but 20-times bigger). Regardless of the similarities between the Solar System and Epsilon Eridani, it is a phenomenal achievement to probe an alien star system, over 10 light years away, with such precision.

For more, check out “Spock’s Solar System Looks Like Ours”.

8. Galaxy Zoo’s discovery of Hanny’s Voorwerp

A highly scientific illustration of the Voorwerp (Galaxy Zoo)
A highly scientific illustration of the Voorwerp (Galaxy Zoo)
In Dutch, “Voorwerp” means “object” and this “object” was discovered by Dutch schoolteacher Hanny van Arkel last year using the Galaxy Zoo project. Since then, this strange astronomical entity has captivated enthusiasts and professionals alike. In May, astronomers came a step closer to understanding what this object was, as Bill Keel explains:

Our working hypothesis is that Hanny’s Voorwerp consists of dust and gas (maybe from a tidally disrupted dwarf galaxy) which is illuminated by a quasar outburst within IC 2497, an outburst which has faded dramatically within the last 100,000 years.”

Galaxy Zoo is a superb example on how enthusiasts can use an Internet-based system to observe and identify objects in the cosmos. I am sure Hanny’s Voorwerp will continue to captivate professionals and amateurs, ensuring Galaxy Zoo’s popularity through 2009 and beyond…

For more, check out “Galaxy Zoo Gets a Makeover”.

7. MESSENGER

The MESSENGER spacecraft at Mercury (NASA)
The MESSENGER spacecraft at Mercury (NASA)
The MErcury Surface, Space ENvironment, GEochemistry and Ranging (MESSENGER) spacecraft was launched by NASA in 2004 to begin an epic journey deep into the Solar System. Its eventual target would take it on a speedy roller-coaster ride via a series of Earth, Venus and Mercury flybys to slow its descent into the Sun’s extreme gravitational well. It won’t achieve orbital insertion until March 2011.

In January 2008, MESSENGER performed its first Mercury flyby. This is the first time for 30 years that the smallest planet* in the Solar System has been visited by a space mission (since the 1975 Mariner 10 mission flyby). There will be one more Mercury flyby until MESSENGER’s delta-v (change in velocity) has been slowed significantly to allow the spacecraft to be captured by the planet’s gravitational pull. During the January flyby, MESSENGER managed to capture some stunning images of the planet from an altitude of 200km. Then, in October the spacecraft made its second pass over Mercury’s surface from the same distance, revealing even more detail of the cratered, rocky surface.

After 3 decades, the mysterious planet, famous for being the closest planet to the Sun, is gradually revealing its secrets.

For more, check out “More Mercury from MESSENGER”.

*Of course, when MESSENGER was launched, it was travelling to the second smallest planet in the Solar System. As Pluto was demoted in 2006, Mercury is now the smallest planet, whereas Pluto is a “dwarf planet” or a “Plutoid”.

6. First exploding supernova observed

First supernova caught in the act (Alicia Soderberg, Princeton University)
First supernova caught in the act (Alicia Soderberg, Princeton University)
In January, something very special happened to a group of astronomers using NASA’s Swift X-ray satellite to study data from a month-old supernova remnant in a distant galaxy. In a case of “extreme serendipity”, the same galaxy produced another supernova the astronomers were able study right as it happened. This was the first time ever that astronomers caught a supernova in the act, we usually have to make do with studying the debris (or “remnant”) after a supernova has occurred.

It’s a really lucky chain of events — a surprise,” said Alicia Soderberg, who is leading the group studying data from the explosion. “It was all over in a matter of minutes.”

This discovery is critical to understanding the science behind the final moments of a massive stars life, improving and advancing stellar models.

For more, check out “Caught in the Act: Astronomers See Supernova As it Explodes“.

5. The Large Hadron Collider

The complexity of the Large Hadron Collider (CERN/LHC/GridPP)
The complexity of the Large Hadron Collider (CERN/LHC/GridPP)

2008 has been the year for particle accelerator physics. The Large Hadron Collider (LHC) is the biggest physics experiment ever built, primarily to search for the elusive Higgs boson (the “force carrier” of the Higgs field that is theorized to permeate through the entire Universe, giving matter its mass), is as famous as it is infamous.

Early in the year, months before the 27km-long particle accelerator ring went online to circulate its first protons, the world’s media was abuzz with the possible science that could revolutionize physics as we knew it. However, there’s a flip-side to that coin. There was an increasing opposition to the LHC, culminating in attempted legal action (that ultimately failed), based on the flawed thinking that the LHC could generate dangerous micro black holes, strangelets and a host of other hypothetical particles. This only served to stir up international interest in what the LHC was actually going to do, and by October 10th, a mix of concern and excitement built up to the grand “switch on”.

The first circulation was a success, proving the LHC worked and CERN scientists readied the most powerful particle accelerator for its first particle collisions. Unfortunately, the LHC hit its first stumbling block only days after the first online tests, culminating in a damaged transformer. However, even worse news was to come. A “quench” triggered by an electrical short between two of the superconducting magnets caused severe damage to one of the sections, knocking it offline for months while engineers make repairs. It now looks as if the LHC will recommence operations mid-2009.

Although many would argue the LHC shouldn’t be included in a “Top Ten Scientific Discoveries” (like Time Magazine’s Top Ten), as it hasn’t actually discovered anything yet, the LHC is a huge science and engineering endeavour, where its construction is as ground-breaking as the potential science it will be producing later this year.

For more, check out all the LHC articles on the Universe Today.

4. Cassini explores Saturn’s moon Enceladus

Artist impression of the view of Saturn from its moon Enceladus (Michael Carroll)

Having recently completed its initial four-year tour of duty around the ringed planet, Cassini had its mission extended through September 2010. In August 2009, the Sun will shine directly on Saturn’s equator, illuminating the northern hemisphere. It is for this reason, the new phase of Cassini’s operations has been called the “Cassini Equinox Mission”.

The principal reason for extension is to find answers to some of the most perplexing questions raised during the spacecraft’s flybys of the Saturnian moons, principally Enceladus, the small 500km-diameter natural satellite. Enceladus may only be a tenth of the size of Titan (Saturn’s biggest moon) but it is one of the most intriguing.

This year, far from being “just another” frozen moon, Enceladus has shown itself to be surprisingly dynamic, revealing complex plate tectonics and ejecting plumes of water as powerful geysers (of which Cassini has flown through and analysed). This has of course led to some interesting ideas about the potential for life in tidally-heated liquid water subsurface lakes.

Of all the geologic provinces in the Saturn system that Cassini has explored, none has been more thrilling or carries greater implications than the region at the southernmost portion of Enceladus,” said Carolyn Porco, Cassini imaging team leader.

For more, check out the Universe Today’s articles all about Enceladus.

3. SpaceX makes commercial spaceflight history

The SpaceX Falcon 9 being assembled at Cape Canaveral on Dec. 30th (SpaceX)
The SpaceX Falcon 9 being assembled at Cape Canaveral on Dec. 30th (SpaceX)

In August, the world watched in anticipation as SpaceX made its third attempt at becoming the world’s first commercial space flight company to launch a payload into orbit. Unfortunately, Flight 3 of the SpaceX Falcon 1 rocket became the third Falcon to fail, exploding high in the atmosphere after a stage separation (transient thrust) anomaly. It was a sad day not only for Elon Musk’s dream of providing affordable launch capabilities, but also for the promise of commercial space flight.

But in the true entrepreneurial spirit Musk has become synonymous with, his company turned Flight 3’s loss into a motivation to get it right the fourth time around. Only one month later, the Falcon 1 was readied for Flight 4 from the Kwajalein Atoll launch pad. On September 28th, SpaceX was propelled into the history books as the first ever private space company to design, build and launch a payload (albeit a “dummy” payload) into orbit.

Now SpaceX has proven itself to the world, the future has become very bright for commercial spaceflight. SpaceX not only got into orbit, they did it cheaply and quickly, setting the bar very high for its competitors. They also have a bold vision for the future; building bigger and more powerful rockets (the Falcon 9 for example), launching not only from the South Pacific, but also from the home of rocket launches: Cape Canaveral.

To top it all off, NASA has signed contracts worth $2.5 billion for private launch capabilities over the next decade, with SpaceX receiving a $1.6 billion share. All in all, it has been an outstanding year for SpaceX, and it looks like they might even be ready to supply the International Space Station in 2009, so watch this space.

For more, check out the SpaceX articles on the Universe Today.

2. Imaging exoplanets

Hubbles view of the exoplanet Fomalhaut b (NASA/HST)
Hubbles view of the exoplanet Fomalhaut b (NASA/HST)

We’ve known for many years that exoplanets orbit other stars and have observed them indirectly by looking at star “wobble” (due to gravitational effects of a massive exoplanet as it orbits) and exoplanet transits (as the planetary body passes in front of the star, reducing the amount of light received on Earth). This year astronomers went one better, they observed exoplanets directly, imaging the little dots as they orbit their host stars.

However, this honour doesn’t go to just one observatory, it goes to several. On November 13th, the Hubble Space Telescope team announced they have taken the first direct visible light images of an exoplanet orbiting the star Fomalhaut, 25 light years away. On the same day, a press release from a joint Keck and Gemini telescope campaign announced the first direct infrared images of multiple planets orbiting a star called HR8799, 140 light years away.

As if that wasn’t enough, on November 21st, astronomers using the ESO Very Large Telescope detected an exoplanet in a very compact orbit around Beta Pictoris, 70 light years from Earth.

These stunning glimpses of exoplanets have been made possible by the huge technological advancement in both ground-based and space-based observatory optics. Astronomers are now confident that they can go one step further as telescopes and techniques improve… how about looking for exomoons orbiting these exoplanets? Wow…

For more, check out the Universe Today’s Extra-Solar Planets category.

1. Phoenix Mars Lander

Capturing the world's attention: Phoenix (NASA/UA)
Catching the world's attention: Phoenix (NASA/UA)

In May, the Phoenix Mars Lander captured the world’s attention as it entered the Martian upper atmosphere to begin its “7 minutes of terror“, including a fiery re-entry, fast decent and rocket-powered controlled landing. The robotic lander touched down in the frozen arctic region of the planet to begin its three month campaign with panache. The mission was extended to five months as Phoenix wrestled with the dwindling winter sunlight powering its solar panels and battled against troublesome dust storms.

During its stay on Mars, Phoenix confirmed the presence of water ice, discovered a life-hindering (or, possibly, life-supporting) chemical called perchlorate, observed Martian weather conditions and generally aided our understanding of this unforgiving region of the Red Planet using its advanced suite of automated ovens and mini laboratories.

This mission was also remarkable for the efforts carried out here on Earth by the Phoenix team at NASA and the University of Arizona communicating cutting-edge and up-to-the-minute science via a variety of social platforms. Scientists blogged and Twittered from the moment the mission was launched to the moment Phoenix finally succumbed to a frozen coma in early November (and MarsPhoenix continues to tweet regular data analysis updates).

However, this short mission joined the two rugged Mars Exploration Rovers Spirit and Opportunity soldiering through the elements for the last five years, after repeatedly having their missions extended over four years past their warranty. Add these incredible surface missions to the armada of satellites (NASA’s Mars Reconnaissance Orbiter, Mars Odyssey and the European Space Agency’s Mars Express), and it becomes obvious that international efforts to study Mars have turned the once mysterious, dusty red globe into one of the most studied planetary bodies of the last decade.

*****

So, Phoenix and the continuing Mars program overwhelmed the popular vote in the Top 10 Science Endeavours of 2008, winning the number one spot convincingly. This was a very tough “Top 10” to compile, but with the help of Universe Today readers, the list became more varied than we could have possibly hoped.

Naturally, many worthy science endeavours didn’t make the cut and here’s the runners up:

Supermassive black hole confirmation at centre of Milky Way

ESA Automated Transfer Vehicle (ATV) Jules Verne

Imaging solar transition region with sounding rocket

Spectral analysis confirms detection of ethane on Titan

Ulysses mission ends

The Universe Today’s Top 10 Scientific Endeavours of 2008 highlights some of the huge scientific advances we have made in the last 12 months. 2009 promises to be even bigger, and with the help of the organizers of the International Year of Astronomy, global efforts in space won’t only be recognised, they will be celebrated.

Studying Black Holes Using a PlayStation 3

Binary waves from black holes. Image Credit: K. Thorne (Caltech) , T. Carnahan (NASA GSFC)

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If you’re a PlayStation 3 fan, or if you just received one as a holiday gift, you may be able to do more with the system than just gaming. A group of gravity researchers have configured 16 PlayStation 3’s together to create a type of supercomputer that is helping them estimate properties of the gravitational waves produced by the merger of two black holes. The research team from the University of Alabama in Huntsville and the University of Massachusetts, Dartmouth, calls their configuration the Gravity Grid, and they say the Sony PlayStation 3 has a number of unique features that make it particularly suited for scientific computation. Equally important, the raw computing power per dollar provided by the PS3 is significantly higher than anything else on the market today.

PlayStation 3s have also been used by the Folding@Home project, to harness the PS3’s technology to help study how proteins are formed in the human body and how they sometimes form incorrectly. This helps in research in several diseases such as Parkinson’s, Alzheimer’s, cystic fibrosis, and even Mad-Cow disease.

Front view of the cluster of PS3's. Credit:  GravityGrid
Front view of the cluster of PS3's. Credit: GravityGrid

The PS3 uses a powerful new processor called the Cell Broadband Engine to run its highly realistic games, and can connect to the Internet so gamers can download new programs and take each other on.

The PlayStation 3 cluster used by the gravity research team can solve some astrophysical problems, such as ones involving many calculations but low memory usage, equaling the speed of a rented super-computer.
“If we had rented computing time from a supercomputer center it would have cost us about $5,000 to run our [black hole] simulation one time. For this project we ran our simulation several dozens of times to test different parameters and circumstances,” study author Lior Burko told Inside Science News Service.

One of the unique features of the PS3 is that it is an open platform, where different system software can be run on it. It’s special processor has a main CPU (called the PPU) and six special compute engines (called SPUs) available for raw computation. Moreover, each SPU performs vector operations, which implies that they can compute on multiple data, in a single step.

But the low cost is especially attractive to university researchers. The Gravity Grid team received a partial donation from Sony, and are using “stock” PS3s for the cluster, with no hardware modifications and are networked together using inexpensive equipment.

Gravitational waves are “ripples” in space-time that travel at the speed of light. These were theoretically predicted by Einstein’s general relativity, but have never been directly observed. Other research is being done in this area by the newly constructed NSF LIGO laboratory and various other such observatories in Europe and Asia. The ESA and NASA also have a mission planned in the near future – the LISA mission – that will also be attempting to detect these waves. To learn more about these waves and the recent attempts to observe them, please visit the LISA mission website.

More information on the PS3 Gravity Grid.

Sources: USA Today, Gravity Grid

Nominations: The Universe Today Top 10 Scientific Endeavours of 2008

2008 has been a landmark year for space science and physics endeavour. We’ve peered deep into the cosmos and fitted new pieces into some of the most intriguing universal puzzles. We’ve explored other planets with technology we wouldn’t have recognised a decade ago. We’ve assembled some of the most complex experiments to test theories of the very small and the very big. 2008 has built strong foundations for the future of the exploration of the Universe in so many ways…

This week, Time Magazine published the top 10 “Scientific Discoveries” of 2008. Technically, as many readers pointed out, a few of the entries are not “discoveries”, they are “achievements”. Although this might have been the case, space exploration and physics dominated, with the #1 slot going to the LHC and #2 slot going to the Phoenix Mars Lander (#4 and #6 went to the Chinese spacewalk and exoplanets respectively). After reading the superb suggestion put forward by Astrofiend (thanks!), it was the push I needed to want to create a Universe Today version of a “Top 10” for 2008 (I’d love to do a top 20, but I have to find some time for Christmas shopping).

This top ten will focus on the last 12 months of Universe Today articles, so take a journey through the year’s events in space science and physics to find your favourite scientific endeavour of 2008. If you can’t find the article, just leave the name of the specific endeavour and we’ll do the rest. Please leave all nominations in the comments box below…

You have one week to get your nominations in (so your deadline is December 19th), and I’ll compile the list of winners hopefully in time for Christmas. The nominations will be considered not only according to popularity, but also chosen by your unbiased Universe Today team…

So, get nominating! You have 7 days…

“Leap Second” to be Added to World Clocks

The US Naval Observatory operates 70 cesium atomic clocks. Credit: USNO

If you ever feel like you need more time, here’s some great news: you’re actually going to get it. On December 31, 2008 a “leap second” will be added to the world’s clocks at 23 hours, 59 minutes and 59 seconds Coordinated Universal Time (UTC). This corresponds to 6:59:59 pm Eastern Standard Time, when the extra second will be inserted at the U.S. Naval Observatory’s Master Clock Facility in Washington, DC. This is the 24th leap second added to UTC, a uniform time-scale kept by atomic clocks around the world, since 1972. Coincidentally, Fraser and Pamela’s most recent episode of Astronomy Cast is about time, so if you want to know more about time and the atomic clocks used to provide precise timekeeping, check it out.

Historically, time was based on the mean rotation of the earth relative to celestial bodies and the second was defined in this reference frame. However, the invention of atomic clocks defined a much more precise “atomic time” scale and a second that is independent of the earth’s rotation. In 1970, an international agreement established two timescales: one based on the rotation of the earth and one based on atomic time.

Atomic clocks do not use radioactivity, but they use the exact frequency of the microwave spectral line emitted by atoms of the element cesium, in particular its isotope of atomic weight 133 (“Cs-133”). The integral of frequency is time, so this frequency, 9,192,631,770 hertz (Hz = cycles/second), and this provides the fundamental unit of time, which are measured by cesium clocks.

The problem is that the earth’s rotation is very gradually slowing down, which necessitates the periodic insertion of a “leap second” into the atomic timescale to keep the two within 1 second of each other. The International Earth Rotation and Reference Systems Service (IERS) is the organization which monitors the difference in the two timescales and calls for leap seconds to be inserted or removed when necessary.

Since 1972, leap seconds have been added at intervals varying from six months to seven years, with the last being inserted on December 31, 2005. The U.S. Naval Observatory is charged with the responsibility for the precise determination and dissemination of time for the Department of Defense and maintains its Master Clock. The U.S. Naval Observatory, together with the National Institute of Standards and Technology (NIST), determines time for the United States.

Source: US Naval Observatory

Teddy Bears Go To Space

Two of the teddy bears imaged in Near Space. Credit: CU Spaceflight

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I don’t think this is what Iran has in mind about launching animals into space, but … you never know. Four teddy bears voyaged to the edge of space on Monday, December 1st via high altitude helium balloon. This was done as an experiment by a student organization at Cambridge University in England, along with a science club and community college. The bears were lifted to 30,085 meters above sea level, and the goal of the experiment was to determine which materials provided the best insulation against the -53 ° C temperatures experienced during the journey. Each of the bears wore a different space suit designed by 11-13 year-olds who were took part in the experiment. But the main goal of the endeavor was to give young students the opportunity to try their hand at a real mission in sending objects into space.

“We want to offer young people the opportunity to get involved in the space industry whilst still at school and show that real-life science is something that is open to everybody” says Iain Waugh, chief aeronautical engineer of student-run Cambridge University Spaceflight.

“High altitude balloon flights are a fantastic way of encouraging interest in science. They are easy to understand, and produce amazing results,” said Daniel Strange, treasurer of CU Spaceflight.

Prelaunch of the high altitude balloon.  Credit: CU Spaceflight
Prelaunch of the high altitude balloon. Credit: CU Spaceflight

The payload which carried the bears was designed by CU Spaceflight and contained several cameras, a flight computer, GPS and a radio. During the 2 hour and 9 minute flight, the radio broadcasted the location of the payload to a chase team on the ground. The team predicted the landing site using wind speed data and arrived in time to see the payload and teddy bears drift slowly back down to earth by parachute.

CU Spaceflight is a student-run society aiming to reduce the cost of sub-orbital spaceflight. They have launched several payloads to near space on high-altitude helium balloons and are currently designing a system to launch a rocket from a balloon platform to outer space for under £1000 per launch. They have run several outreach events and are currently holding the UK Space Challenge 2009, as part of the University of Cambridge’s 800th Anniversary. Twenty four teams of science students aged 14-18 are competing to design a scientific experiment that will be taken to near space on a high-altitude helium balloon.

More images of the flight.
More information about Cambridge University Spaceflight.

Source: CU Spaceflight

Studying the Life Cycle of Butterflies and Spiders in Space

Will butterflies in space grow different to butterflies on Earth? (NASA, editing by Ian O'Neill)

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Space biology experiments have just arrived in the classroom. With a focus on hundreds of K-12 students, a University of Colorado, Boulder payload will be launched on board Space Shuttle Endeavour on November 14th carrying spiders and butterfly larvae. The purpose? To provide an educational research tool for youngsters, helping to develop their interest in biology and space science. The butterfly larvae will be studied over their complete life cycle in space; from larvae to pupae to butterfly to egg. Web-building spiders will be studied to see how their behaviour alters when lacking gravity. Both sets of experiments will then be compared with control subjects on the ground… I wish I had the chance to do this kind of research when in school. I wish I had the chance to do this kind of research now!

This program is an excellent example of using a national asset like the International Space Station to inspire K-12 students in science, technology, engineering and math,” said BioServe Director Louis Stodieck, principal investigator on the project. BioServe has flown two previous K-12 payloads as part of their CSI program on other shuttle flights to the International Space Station (ISS).

This particular experiment will study the activities and feeding habits of web-building spiders when in space, compared to spiders in the classroom. The hundreds of students from several locations in the US are involved in the project and will learn valuable research techniques along with boosting their interest in the sciences. After all, it isn’t every day you get a chance to carry out cutting-edge research on the world’s most extreme science laboratory!

The second set of experiments will be another space/Earth comparison, but this time a study of the full lifespan of painted lady butterflies. Four-day old pupae will be launched into space and watched via downlink video, still images and data from the ISS. Partners in the project include the Denver Museum of Nature and Science, the Butterfly Pavilion in Westminster, CO and the Baylor College of Medicine’s Center for Education Outeach.

BioServe is a non-profit, NASA funded organization hoping to include payloads on each of the remaining shuttle flights until retirement. “Between now and then, we are seeking sponsors for our educational payloads to enhance the learning opportunities for the K-12 community in Colorado and around the world,” added BioServe Payload Mission Manager Stefanie Countryman.

The full details on the project can be found on the University of Colorado pages.

This is where the strength of the International Space Station really comes into play. Real science being carried out by schools in the US to boost interest not only in space travel, but biology too. It’s a relief, I was getting a little tired hearing about busted toilets, interesting yet pointless boomerang “experiments”, more tests on sprouting seeds and the general discontent about the ISS being an anticlimax.

Let’s hope BioServe’s projects turn out well and all the students involved are inspired by the opportunities of space travel. Although I can’t help but feel sorry for the confused spiders and butterfly larvae when they realise there’s no “up” any more (I hope they don’t get space sick).

Source: UC Boulder

The LHC Will Revolutionize Physics. Can it Revolutionize the Internet Too?

One gigabyte per second? No problem. The LHC computing grid could revolutionize how we handle data over Internet (CERN)

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We already know that the Large Hadron Collider (LHC) will be the biggest, most expensive physics experiment ever carried out by mankind. Colliding relativistic particles at energies previously unimaginable (up to the 14 TeV mark by the end of the decade) will generate millions of particles (known and as yet to be discovered), that need to be tracked and characterized by huge particle detectors. This historic experiment will require a massive data collection and storage effort, re-writing the rules of data handling. Every five seconds, LHC collisions will generate the equivalent of a DVD-worth of data, that’s a data production rate of one gigabyte per second. To put this into perspective, an average household computer with a very good connection may be able to download data at a rate of one or two megabytes per second (if you are very lucky! I get 500 kilobytes/second). So, LHC engineers have designed a new kind of data handling method that can store and distribute petabytes (million-gigabytes) of data to LHC collaborators worldwide (without getting old and grey whilst waiting for a download).

In 1990, the European Organization for Nuclear Research (CERN) revolutionized the way in which we live. The previous year, Tim Berners-Lee, a CERN physicist, wrote a proposal for electronic information management. He put forward the idea that information could be transferred easily over the Internet using something called “hypertext.” As time went on Berners-Lee and collaborator Robert Cailliau, a systems engineer also at CERN, pieced together a single information network to help CERN scientists collaborate and share information from their personal computers without having to save it on cumbersome storage devices. Hypertext enabled users to browse and share text via web pages using hyperlinks. Berners-Lee then went on to create a browser-editor and soon realised this new form of communication could be shared by vast numbers of people. By May 1990, the CERN scientists called this new collaborative network the World Wide Web. In fact, CERN was responsible for the world’s first website: http://info.cern.ch/ and an early example of what this site looked like can be found via the World Wide Web Consortium website.

So CERN is no stranger to managing data over the Internet, but the brand new LHC will require special treatment. As highlighted by David Bader, executive director of high performance computing at the Georgia Institute of Technology, the current bandwidth allowed by the Internet is a huge bottleneck, making other forms of data sharing more desirable. “If I look at the LHC and what it’s doing for the future, the one thing that the Web hasn’t been able to do is manage a phenomenal wealth of data,” he said, meaning that it is easier to save large datasets on terabyte hard drives and then send them in the post to collaborators. Although CERN had addressed the collaborative nature of data sharing on the World Wide Web, the data the LHC will generate will easily overload the small bandwidths currently available.

How the LHC Computing Grid works (CERN/Scientific American)
How the LHC Computing Grid works (CERN/Scientific American)

This is why the LHC Computing Grid was designed. The grid handles vast LHC dataset production in tiers, the first (Tier 0) is located on-site at CERN near Geneva, Switzerland. Tier 0 consists of a huge parallel computer network containing 100,000 advanced CPUs that have been set up to immediately store and manage the raw data (1s and 0s of binary code) pumped out by the LHC. It is worth noting at this point, that not all the particle collisions will be detected by the sensors, only a very small fraction can be captured. Although only a comparatively small number of particles may be detected, this still translates into huge output.

Tier 0 manages portions of the data outputted by blasting it through dedicated 10 gigabit-per-second fibre optic lines to 11 Tier 1 sites across North America, Asia and Europe. This allows collaborators such as the Relativistic Heavy Ion Collider (RHIC) at the Brookhaven National Laboratory in New York to analyse data from the ALICE experiment, comparing results from the LHC lead ion collisions with their own heavy ion collision results.

From the Tier 1 international computers, datasets are packaged and sent to 140 Tier 2 computer networks located at universities, laboratories and private companies around the world. It is at this point that scientists will have access to the datasets to perform the conversion from the raw binary code into usable information about particle energies and trajectories.

The tier system is all well and good, but it wouldn’t work without a highly efficient type of software called “middleware.” When trying to access data, the user may want information that is spread throughout the petabytes of data on different servers in different formats. An open-source middleware platform called Globus will have the huge responsibility to gather the required information seamlessly as if that information is already sitting inside the researcher’s computer.

It is this combination of the tier system, fast connection and ingenious software that could be expanded beyond the LHC project. In a world where everything is becoming “on demand,” this kind of technology could make the Internet transparent to the end user. There would be instant access to everything from data produced by experiments on the other side of the planet, to viewing high definition movies without waiting for the download progress bar. Much like Berners-Lee’s invention of HTML, the LHC Computing Grid may revolutionize how we use the Internet.

Sources: Scientific American, CERN

TV Alert: Mythbusters and the Moon Hoax Myth

Mythbusters. Credit: CollectSpace

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On Wednesday August 27th, at 9 p.m. ET/PT in the US, the famed “Mythbusters” on the Discovery Channel will take on one of the biggest myths ever: the belief the Apollo Moon landings were faked. Some folks who lived through the 1960’s never believed the moon landings actually happened, and some how this belief persisted. In 2001 the Fox Channel aired a show “Conspiracy Theory: Did We Land on the Moon?” and the belief grew. But now the Mythbusters take on the HB’s (hoax believers) who say they have scientific evidence the moon landings were faked. Adam and Jamie will fight bad science with their usual good science. The results? We’ll have to wait and see until tonight. But here’s a preview:

I can’t wait!

For more info:
Mythbusters website.
Article on CollectSpace about the show, includes quotes from Phil Plait
Phil Plait’s Review of the show and links to his previous articles about the show
Phil’s debunking of the Fox moon hoax show