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Hello! My name is Ian O'Neill and I've been writing for the Universe Today since December 2007. I am a solar physics doctor, but my space interests are wide-ranging. Since becoming a science writer I have been drawn to the more extreme astrophysics concepts (like black hole dynamics), high energy physics (getting excited about the LHC!) and general space colonization efforts. I am also heavily involved with the Mars Homestead project (run by the Mars Foundation), an international organization to advance our settlement concepts on Mars. I also run my own space physics blog: Astroengine.com, be sure to check it out!
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Europe’s most advanced robotic spaceship, the Automated Transfer Vehicle (ATV), has effectively ended its 6-month mission to the International Space Station (ISS). It successfully undocked today (Friday) at 21:29 GMT to begin its slow 3 week journey toward the Earth’s atmosphere where it is set for re-entry on September 29th. This was the first ever ATV to be launched and was named after the 19th Century novelist, Jules Verne; another four ATVs are scheduled for construction. Jules Verne’s re-entry is set for night time over an uninhabited region of the Pacific Ocean and NASA will use this opportunity to monitor the fireball so the characteristics of re-entering spacecraft can be studied…
It might seem like a waste – after all, the ATV cost 1.3 billion euros or 1.9 billion dollars to build – but Jules Verne was designed to be a single-use, disposable resupply ship for the space station. However, its duties as a supply ship weren’t restricted to grocery deliveries. After it was launched in March, the ATV underwent a series of tests in space to prepare it for arrival at the station on April 3rd. When attached to the station, the ATV surpassed all expectations and performed many tasks that hadn’t been considered by mission control. Although the ATV provided a valuable re-boost option for the station (four times in total), it also provided the thrust to slow the ISS down to avoid a chunk of satellite debris in August. The ship was also a welcome retreat for the crew of the station, giving them a roomy volume for recreation and cleaning chores. I think Jules Verne will be sorely missed.
So, like the Russian Progress 29 resupply ship that was dropped from the station on Wednesday, Jules Verne was packed up with several tonnes of trash and unwanted equipment from the ISS and jettisoned into space.
The ATV will now use its remaining fuel to park its 13.5 tonne mass in a new orbit for the following three weeks before it is commanded to drop from orbit and begin re-entry. Jules Verne’s fiery suicide will happen at night so scientists can gain an insight into how large objects behave when they burn up in the Earth’s atmosphere. To monitor the event, NASA will deploy two aircraft with radar, UV and other sensors to track the incoming ATV.
“Even though our schedule has been very busy at the ATV Control Centre, I couldn’t have wished for a better mission,” – Herve Come, ESA’s ATV lead mission director.
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A strange Kuiper Belt Object (KBO) has been discovered orbiting the Sun in the wrong direction. The object, designated as 2008 KV42 but nicknamed Drac (after Dracula, as vampires are fabled to have the ability to walk on walls), has a highly inclined orbit of 103.5°. Drac is a rarity as very few objects in the Solar System have retrograde orbits; in fact this kind of orbit is usually exclusive to Halley-type comets that have orbits that take them very close to the Sun. Drac on the other hand travels through the Kuiper Belt in a stable orbit at a distance of between 20-70 AU from the Sun. This finding has puzzled astronomers, but Drac may provide clues as to where Halley-type objects originate…
When an object has an inclination of more than 90° from the ecliptic, its direction of motion becomes retrograde when compared with the majority of the Sun’s satellites that share a common, or “prograde” orbital direction. This type of orbit is usually reserved for long-period comets thought to originate from the mysterious Oort Cloud. However, Drac stands out from the crowd as it orbits the Sun from the distance of Uranus to more than twice that of Neptune. Halley-type comets come much closer to the Sun.
Researchers led by Brett Gladman of the University of British Columbia observed the 50 km (30 mile) diameter object in May. Drac (or 2008 KV42) appears to have an extremely stable orbit, and its possibly been that way for hundreds of millions of years. Although Drac orbits through the Kuiper Belt, astronomers do not believe it originates there. “It’s certainly intriguing to ask where it comes from,” says Brian Marsden of the Minor Planet Center in Cambridge, Massachusetts.
Gladman believes the object originated far beyond the Kuiper Belt, possibly from the same volume of space believed to breed Halley-type comets with highly tilted (often retrograde) orbital periods of between 20-200 years. Gladman and his colleagues believe Drac came from a region beyond the Kuiper Belt, but it didn’t come from the Oort Cloud (some 20,000 to 200,000 AU from the Sun). The researchers believe 2008 KV42 was born in a region 2000-5000 AU from the Sun, a theorized volume of the Solar System called the inner Oort Cloud.
It seems likely that Drac was gravitationally disturbed from its home in the inner Oort Cloud by a passing star, or some other disturbance in its local space. It then fell toward the inner Solar System where it found its new home near the Kuiper Belt. Gladman believes that 2008 KV42 may be a “transition object” on its way to becoming a Halley-type comet. However, it will need to be disturbed again before it breaks free of its current stable orbit to fall closer to the Sun.
The British Columbia team have found a collection of 20 KBOs with steeply inclined orbits, but Drac, the vampire of the Solar System, is the only one orbiting in the wrong direction…
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OK, I’ve just wasted an hour in simulated space, checking out some of the active and junked satellites orbiting our planet. Google Earth can be an addictive thing at the best of times, but when 13,000 of the satellites in Earth orbit can be viewed by a new plug-in for the program, you may find yourself hooked for longer than usual. The United States Strategic Command keeps very close tabs on what is orbiting our planet and where they are at any given time, and now with the help of Google Earth, you can explore the satellites, plot their orbital trajectories and see just how crowded space can be. Never before have geostationary communication satellites been so interesting!
Tracking space junk is paramount to all our activities in space. Every time we put a “useful” satellite into orbit – to service our communication needs, monitor the weather or spy on other countries – we are amplifying the growing space junk problem surrounding Earth. In February, I wrote a Universe Today article reporting on Google Earth’s ability to plot all known bits of space junk orbiting the Earth. I think it shocked many to see the problem in dazzling 3D. Now a new plug-in has been released detailing the positions of 13,000 alive and dead satellites being tracked by the US military.
At the end of last month, the danger of discarded satellite parts became all too real for the crew of the International Space Station. Nancy wrote about the heroic efforts of the (soon to be dumped) ATV that boosted the station clear of passing debris from a disintegrated Russian satellite. According to officials, the ATV carried out a 5 minute burn, slowing the station and lowering its orbit by 1.5 km (1 mile). The chunk of Russian spy satellite was allowed to pass without incident.
Now you can see the space debris being carefully watched by the US and do some satellite tracking yourself. This new Google Earth plug-in (.kmz file for Google Earth) allows you not only to get information on the 13,000 objects tracked by the US Strategic Command, it also lets you plot their orbits. All the way from low Earth to geostationary orbits, you can access information about who launched the satellite, whether it is active or not, its launch date, mass and orbital information (apogee/perigee). By clicking “Display Trajectory in Fixed Frame” in the information panel that appears when you select the satellite, the orbital path is displayed. It is worth noting that this is the orbital trajectory in relation to the Earth’s rotation (or the “fixed frame”), so geostationary satellites will appear to have no orbital motion, as you’d expect.
I spent a long time clicking on the various satellites, constantly surprised by the huge number of inactive satellites there were. I also checked out some information on satellites I’d never heard of (like the active InSat-3A/4B geostationary communication satellites I found oscillating around each other, pictured).
Although it is shocking to see the sheer number of satellites out there (reminding me that Kessler Syndrome could be a very real threat in the future), learning about the stuff orbiting Earth was great fun.
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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.
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.
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Last year, students from Rhode Island School of Design (RISD) were set one of the best coursework projects I’ve ever heard of. The project title was called “Design for extreme environments” and it was sponsored by NASA. By extreme environments, we are talking about the Moon, and by design, we are talking about arriving at new concepts as to how to prevent lunar dust contamination inside future lunar habitats. Since the task was first set, the enthusiastic RSID team have arrived at a concept that NASA will be using in the planning of the 2020 return to the lunar surface…
The Moon is a dirty place. During the Apollo missions, dust from the lunar surface got everywhere. The biggest problem for astronauts came when the tiny, sharp shards of regolith (pulverized bits of rock from billions of years of meteorite impacts) was disturbed by the moon buggy as the lunar explorers travelled across the dusty surface. One event in particular stands out as the problems lunar dust can cause. In 1972, Apollo 17 astronauts Gene Cernan and Jack Schmitt had accidentally damaged the wheel arch of their moon buggy. The result was a dreaded “rooster tail” was they drove, kicking up dust into the vacuum, causing it to cover everything, including spacesuit visors. This would lead to vision impairment, scratches of the protective visor coating and ultimately respiratory problems when transported inside the lunar module (“LEM”). Fortunately Cernan and Schmitt managed to repair their moon buggy with a roll of duct tape, possibly saving the lunar surface mission.
Moon dust contamination was inevitable however, even inside the sealed LEM. So, with the possibility of extended manned exploration of the Moon and Mars from the year 2020, NASA is re-evaluating the challenges astronauts will face when combating this potentially dangerous foe. Many scientists are especially worried about the health of manned settlements should lunar dust be allowed into habitats. Breathing the stuff in could be as dangerous as breathing in asbestos. When working with the dusty cancer-causing material down here on Earth, specialist breathing apparatus must be worn at all times. If this were to be the case on the Moon, to fight the health risks associated with breathing in moon dust, short-term and long-term damage could be inflicted on the young colony.
This is where the RISD project comes in. In preparation for a possible manned return to the Moon in just over a decade, NASA decided to tap into the ingenuity of students from the design school to arrive at some novel ideas as to how eliminate the risk of letting lunar dust into a future moon buggy. Several design and engineering students and graduates from RISD’s Industrial Design Department took part in a RISD/NASA research internship focusing on elements of a future lunar module – the descent stage, habitat and ascent stage. The 2007 summer internship focused on the dust problem.
The students investigated a “suitlock” design, an airlock that uses the astronauts’ space suits as part of the operation to remove any contaminants. To make access to the lunar surface quick and routine, the research focused on using an existing rear-entry space suit that would be stored inside an air- and dust-tight seal, but the astronauts would be able to slide into the suit whilst keeping the suit itself separate from the habitat interior. To see how the RISD concept works, view the full-scale mock-up video of the demonstration session.
The RISD concept was taken from paper and consolidated into a full-scale rigid mock up. The design can now be evaluated by NASA for possible inclusion in the future exploration of the Moon. This project for the RISD interns is obviously a valuable experience for the students taking their vision and turning it into a “real-world” application, but NASA has the chance to learn from the fertile imaginations of design and engineering graduates, possibly taking the exploration of space in an unexpected but advantageous direction…
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In a dress rehearsal for the disposal of the European Automated Transfer Vehicle (ATV) in two days time, the Russian Progress 29 resupply ship was undocked from the International Space Station (ISS) on Monday from its Earth-facing berth on the station’s Russian Zarya control module. The vessel, having performed its resupply duties back in May, has now been filled with waste from the crew and sent on its week-long journey toward a fiery re-entry. But the tough automated resupply ship still has some work to do, it will carry out some experimental rocket tests before it makes its final plunge over the Pacific Ocean…
The Russian automated resupply vessel has been overlooked recently. This unmanned craft has a long history of space supply tasks, ferrying food, water, equipment and other supplies to the orbital crews and then being filled with rubbish to be disposed of during re-entry. The current expendable Progress vehicle, the Progress M (interestingly based on the manned Soyuz design), was first launched in 1989 to service the Mir Space Station. 43 flights later, it was chosen as the principal resupply vehicle for the ISS. The current Progress mission, Progress 29, marks the 29th Progress flight to the orbital outpost, but unfortunately, like all the Progress flights before it the ship has undocked and it will begin deorbit manoeuvres to burn up in the atmosphere.
According to NASA, the undocking procedure was completed as expected at 3:46 pm EDT, Monday afternoon. “It went very well, exactly as planned,” stated NASA spokesperson Kelly Humphries at the Johnson Space Center in Houston. Russian Federal Space Agency officials added that Progress 29 will remain in orbit until September 9th to carry out experiments on the plasma environment surrounding its engines. Once complete, the craft will be instructed to begin its final kamikaze task and plunge into the atmosphere over the South Pacific. Should any charred remains be left over after the burn, the debris will fall safely into a pre-designated area of the ocean.
Progress 29 was launched on May 14th and docked with the ISS two days later. This mission replaced Progress 28, which in April had also been unceremoniously dropped from space. Progress 29 delivered 2.3 tonnes of supplies to the ISS crew which currently include cosmonauts Sergei Volkov and Oleg Kononenko with astronaut Greg Chamitoff.
But this is only the first part of ISS dumping duties this week. On Friday, ESA Jules Verne will end its work (the first ever ATV mission), be filled with station trash and also dropped from orbit. I’m sure the ATV looked down nervously on Progress 29 as it disappeared from view knowing it’s only two days from the long drop back to Earth…
For my fourth appearance on Captain Jack’s Paranormal Radio show, I’ve been invited back to discuss a recent Universe Today article I wrote detailing some of my favourite Solar System mysteries. These mysteries include the coronal heating problem, the “Mars Curse” and Uranus’ tilt. I don’t have many answers, but there should be some surprises thrown in. Most likely Jack and I will meander into different topics, so it should be fun to listen in!
For more information on the show, see tonight’s profile. Remember, the show will be airing live over several US cities, satellite radio and the Internet. For more information on where it will be airing, check out the Paranormal Radio homepage. To listen to the live podcast, starting at 6pm (PST), 9pm (EST) or 2am (GMT), download the .pls file to activate your podcast-listening software, or use the popup Media Player (plugin needed).
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According to an internal email, NASA staff have been instructed to initiate a study into extending the operational lifetime of the Shuttle to bridge the 5-year gap between planned Shuttle retirement and Constellation commencement. In an apparent U-turn in the US space agency’s policy, NASA Administrator Michael Griffin has ordered a feasibility study to assess whether the ageing space vehicle fleet, first launched in 1981, can operate until 2015. This news comes at a time when concern is mounting for the US dependence on the Soyuz system after 2010, especially since the recent political chill between the US and Russia…
This news may come as a surprise to many, especially since Michael Griffin’s remarks that to extend the life of the Shuttle fleet could put astronauts in danger and cripple the agency’s fledgling Constellation program. However, there has been mounting political pressure on NASA to find an alternative to depending on the Russian space agency’s Soyuz spacecraft to access the International Space Station in the five years before the brand new Constellation Program is scheduled to launch by 2015. The recent military action in the South Ossetia region of Georgia has helped to increase political tensions; this is possibly one of the main contributing factors to the initiation of this feasibility study. Both US Presidential candidates, Barack Obama (Dem) and John McCain (Rep), are also pushing for a solution to the problematic “5-year gap.”
NASA officials have confirmed the internal email’s authenticity received by the Orlando Sentinel, a Florida-based news agency, but were keen to point out that it was too soon to say what the study’s reach would be.
In the email sent out on Wednesday by John Coggeshall, manager of manifest and schedules at Johnson Space Center in Houston, he said, “We want to focus on helping bridge the gap of U.S. vehicles traveling to the ISS (International Space Station) as efficiently as possible.” However, NASA spokesman John Yembrick was keen to point out to an Associated Press journalist that although the email was sent out, it was premature and “…the parameters of the study have not yet been defined.”
Griffin has, until now, been opposed to extending the Shuttle program primarily due to financial reasons; the effort and funds required could hurt the Constellation Program. But it would seem that world events and politics could be forcing him to reconsider…
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The Automated Transfer Vehicle (A T V) Jules Verne will undock from the International Space Station (ISS) on September 5th to begin three weeks of autonomous flight, setting it up for a suicidal re-entry on September 29th. The ATV has been loaded with refuse and unwanted equipment from the ISS set to burn up in the Earth’s upper atmosphere marking the end of the life of Europe’s most advanced space vehicle. To record the event, both NASA and the European Space Agency will be photographing and videoing the descent…
The Russian Federal Space Agency Roscosmos announced the date for the end of the Jules Verne mission to the ISS on Thursday. This news comes after a highly successful period for the European ATV, proving the ATV can be used for extensive re-supply tasks and provide the station with a valuable re-boost and space debris avoidance options.
This first ATV, also known as “Jules Verne” (as it delivered two original manuscripts written by the 19th Century author to the station), was launched from French Guiana in South America on board an Ariane-5 heavy-lift rocket on March 5th. During this busy time for the Space Station, the ATV had to remain in a “parking orbit” for nearly a month before delivering supplies to the ISS crew on April 3th. Only when Space Shuttle Endeavour (STS-123) had undocked and landed on March 26th could the ATV approach and dock.
Since then, the ATV has proven to be a valuable addition to the station, surpassing all expectations. The ISS crew will miss Jules Verne as the roomy temporary supply vessel has provided a great area for the crew to sleep and wash, plus one of its empty tanks has been used to store 110 litres of condensation water. These extra (unexpected) uses prompted mission control to extend the life of the mission for an extra month.
But all good things come to an end and the ATV will undock on September 5th to begin its journey back to Earth as a fireball at the end of September. The ATV will be dropping up to six tonnes of unwanted equipment and waste from the station into a pre-designated area of the Pacific Ocean. But ESA and NASA will be watching, photographing and videoing Jules Verne’s final service to the ISS crew…
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Of all the things that could possibly go wrong for the US space agency, you wouldn’t expect the security ID badge holder of NASA employees to rank very high on the list of “risks.” Unfortunately, the new high-tech security badge holders recently issued to NASA employees have been identified as having a fairly problematic health and safety design flaw. Should the badges’ metal clasps be installed incorrectly, they could pose a projectile risk, possibly causing serious eye injuries…
Admittedly, this isn’t big news in the realms of the space exploration, but it is news nonetheless, proving that even NASA cannot escape from clerical design flaws. In an effort to fall in line with President Bush’s Homeland Security Presidential Directive-12, NASA employees have to carry a new type of badge which is protected against being read from a distance and also provides the wearer with some freedom as to when they want to show it. Unfortunately, there is a design flaw with the badge and on August 15th, NASA had to issue a warning to Kennedy Space Center employees stating that the new Identity Stronghold badge holder has the “potential to introduce dangerous Foreign Object Damage (FOD) to flight hardware areas and can cause personnel injury if the metal clips are installed improperly.”
According to new guidelines, when removing the badge, the employee must not aim the metal clips at a colleague as it could create a potential eye injury hazard, technically known as Foreign (or Flying) Object Damage (FOD). I’d imaging this being an acute problem during security checks, guards flinching as employees show their badges, fearful of a metal clasp flying at their faces. Not only that, employees are advised not to play with their badges around sensitive electronics:
“The badge holder may separate with little effort, allowing the clips, the front half of the holder and badge ID to separate creating a significant FOD hazard in controlled areas […] Personnel should ensure the badge holder is not worn, or is properly secured, in the vicinity of sensitive flight hardware, such as electronics, where FOD may be an issue […] When removing your badge, do not point [the] end with metal clips towards your face or another person.” – Randy Aden, Office of Protective Services, Jet Propulsion Lab.
Use of the badge holder, made by the Florida-based company Identity Stronghold, has now been suspended and a temporary clear plastic holder is being used in its place. The Stronghold design was chosen as it has an “electromagnetically opaque sleeve to prevent the card from being read at a distance and to give the user some control over when and where the card is exposed for reading,” according to the source Information Week article.
Interestingly, the Identity Stronghold website proudly states that its Secure Badgeholder “has been awarded the 2008 GOOD DESIGN award for product design.” I don’t think the “GOOD DESIGN” award was good enough.
Fortunately there have been no reports of serious card holder-related FOD injuries so far. Who would have thought an ID badge could be so dangerous?