NASA Study Predicted Outbreak of Deadly Virus

Scientists have long suspected that climatic variables like sea surface temperature and precipitation could foreshadow outbreaks of disease. Now, they have confirmation.

Responding to a deadly 1997 outbreak of the mosquito-borne disease Rift Valley fever, researchers had developed a “risk map,” pictured above, using NASA and National Oceanic and Atmospheric Administration measurements of sea surface temperatures, precipitation, and vegetation cover. As reported in a recent NASA-led study, the map gave public health officials in East Africa up to six weeks of warning for the 2006-2007 outbreak of the deadly Rift Valley fever in northeast Africa — enough time to lessen human impact.

On the map above, pink areas depict increased disease risk, while pale green areas reflect normal risk. Yellow dots represent reported Rift Valley fever cases in high-risk areas, while blue dots represent occurrences in non-risk areas. The researchers have detailed the map’s effectiveness in the Proceedings of the National Academy of Sciences.

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Scientists study a typical dambo habitat at Sukari Farm, a long-term Rift Valley Fever study site just outside Nairobi, Kenya. Dambos are natural breeding grounds for disease-carrying mosquitoes and can be observed from space with the aid of satellites. Credit: Assaf Anyamba

During an intense El Niño event in 1997, the largest known outbreak of Rift Valley fever spread across the Horn of Africa. About 90,000 people were infected with the virus, which is carried by mosquitoes and transmitted to humans by mosquito bites or through contact with infected livestock. That outbreak prompted the formation of a working group — funded by the U.S. Department of Defense Global Emerging Infections Surveillance and Response System — to try to predict future outbreaks.

The working group didn’t start from scratch. The link between the mosquito life cycle and vegetation growth was first described in a 1987 Science paper by co-authors Kenneth Linthicum of the U.S. Department of Agriculture and Compton Tucker of NASA’s Goddard Space Flight Center. Later, a 1999 Science paper described a link between Rift Valley fever and the El Niño-Southern Oscillation, a cyclical, global phenomenon of sea surface temperature changes that can contribute to extreme climate events around the world.

Building on that research, Assaf Anyamba of NASA Goddard and the University of Maryland, and his colleagues, set out to predict when conditions were ripe for excessive rainfall — and thus an outbreak. They started by examining satellite measurements of sea surface temperatures. One of the first indicators that El Niño will boost rainfall is a rise in the surface temperature of the eastern equatorial Pacific Ocean and the western equatorial Indian Ocean. Perhaps the most telling clue is a measure of the mosquito habitat itself. The researchers used a satellite-derived vegetation data set that measures the landscape’s “greenness.” Greener regions have more than the average amount of vegetation, which means more water and more potential habitat for infected mosquitoes. The resulting risk map for Rift Valley fever, showing areas of anomalous rainfall and vegetation growth over a three-month period, is updated and issued monthly as a means to guide ground-based mosquito and virus surveillance.

As early as September 2006, the monthly advisory from Anyamba and colleagues indicated an elevated risk of Rift Valley fever activity in East Africa. By November, Kenya’s government had begun collaborating with non-governmental organizations to implement disease mitigation measures—restricting animal movement, distributing mosquito bed nets, informing the public, and enacting programs to control mosquitoes and vaccinate animals. Between two and six weeks later—depending on the location—the disease was detected in humans.

After the 2006-2007 outbreak, Anyamba and colleagues assessed the effectiveness of the warning maps. They compared locations that had been identified as “at risk” with the locations where Rift Valley fever was reported. Of the 1,088 cases reported in Kenya, Somalia, and Tanzania, 64 percent fell within areas delineated on the risk map. The other 36 percent of cases did not occur within “at risk” areas, but none were more than 30 miles away, leading the researchers believe that they had identified most of the initial infection sites.

The potential for mapping the risk of disease outbreaks is not limited to Africa. Previous research has shown that risk maps are possible whenever the abundance of a virus can be linked to extremes in climate conditions. Chikungunya in east Africa and Hantavirus and West Nile virus in the United States, for example, have been linked to conditions of rainfall extremes.

“We are coming up on almost 30 years of vegetation data from satellites, which provides us with a good basis for predicting,” said Linthicum, co-author on the 1987 paper, upon his return from a Rift Valley fever workshop in Cairo, Egypt last month. “At this meeting, it was clear that using this tool as a basis for predictions has become accepted as the norm.”

Sources: NASA and the Proceedings of the National Academy of Sciences

Has Liquid Water Been Detected On Mars?

Growing water droplets on Phoenix's legs? (NASA)

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Liquid water may have been discovered by the late Phoenix Mars Lander. This astonishing (and controversial) claim comes from some very intriguing images of the lander’s leg shortly after Phoenix landed on the Red Planet last year. The series of black and white images appear to show droplets of water hanging off the robot’s bodywork in the shade; it seems possible that the water droplets were splashed from the surface during Phoenix’s rocket-assisted landing. Far from being static blobs, they appear to grow, much like water droplets here on Earth as water vapour is absorbed from the atmosphere.

But wait a minute, isn’t the Martian atmosphere too thin and too cold to accommodate liquid water? That’s where the perchlorate comes in

If liquid water has been found to exist on the surface of Mars, there will be huge implications for our understanding of the planet. Most tantalizingly, liquid water, on or near the planet’s surface, could aid the survival of microbial life, reinvigorating the search for extraterrestrial life on out interplanetary neighbour. But on a planet where the atmospheric pressure is 100 times less than on Earth, and temperatures reached a maximum of -20° Celcius during the Phoenix mission, why isn’t this “liquid water” candidate frozen?

The perchlorate discovery in the Martian soil was announced by the Phoenix team in August 2008, after an explosion of intense Internet conjecture caused by the “potential for life” announcement by an Aviation Week article days earlier. It turned out that the Phoenix instrumentation had found quantities of a toxic chemical called perchlorate known to be a hindrance to life as we know it. Although follow-up reports were slightly more positive about the presence of the chemical (a possible energy source for microbial life), the mood was fairly sombre. On a planet as unforgiving as Mars, any bad news is a severe knock for the hope of finding life.

However, regardless of perchlorate’s toxic effects on life, it may be helping out another one of life’s resources to stay in liquid form. If perchlorate is dissolved in significant quantities, water could remain as a liquid down to temperatures as low as -70°C. So could it be that the dissolved perchlorate salt is acting as a very impressive anti-freeze?

Nilton Renno from the University of Michigan and Phoenix team member, thinks it could be. “According to my calculations, you can have liquid saline solutions just below the surface almost anywhere on Mars,” he said.

Renno’s team carried out a series of laboratory experiments and found that the lander’s thrusters would have melted the top millimetre of ice in the regolith. The resulting water droplets may have been splashed onto the landers leg. If the concentration of perchlorate was high enough, the water could have remained in a liquid state during the Mars daytime. As time progressed, atmospheric water vapour may have been absorbed, hence the growing and shifting blobs of liquid on the leg. There is also the possibility that the droplets were splashed from pools of perchlorate-rich water already in a liquid state on the surface.

However, not everyone is convinced. Fellow Phoenix team member Michael Hecht from NASA’s Jet Propulsion Laboratory in Pasadena, California, thinks that the photographs actually show water ice, not liquid water. The “frost” changed shape as vapour from the air coalesced and froze to the leg. Renno points out that this is unlikely as any ice on the leg would be more likely to sublime, rather than grow, but Hecht believes this could happen if the leg was colder than its surroundings.

Renno’s team will be continuing tests on samples of perchlorate-rich water under Mars-like conditions for the next few months to understand the dynamics of water under these extreme conditions. What makes this even more interesting is that some microbial life on Earth has the ability to survive in very salty fluids, perhaps microbial alien life on Mars evolved in a similar environment where there were pools of liquid water maintained at extremely low temperatures by high concentrations of perchlorate salt

Source: New Scientist

Repaired too Late? Tevatron May Beat LHC in Hunt for Higgs Boson

The CDF detector at Fermilab's Tevatron accelerator (Fermilab)

[/caption]The Large Hadron Collider (LHC) is billed as the next great particle accelerator that will give us our best chance yet at discovering the illusive exchange particle (or boson) of the Higgs field. The discovery (or not) of the Higgs boson will answer so many questions about our universe, and our understanding of the quantum world could be revolutionized.

But there’s a problem. The LHC isn’t scheduled for restart until September 2009 (a full year after the last attempt) and particle collisions aren’t expected until October. Even then, high energy collisions won’t be likely until 2010, leaving the field wide open for competing accelerator facilities to redouble their efforts at making this historic discovery before the LHC goes online.

The Tevatron, at Fermi National Accelerator Laboratory (Fermilab) in Illinois, is currently the most powerful accelerator in the world and has refined high energy particle collisions so much, that scientists are estimating there is a 50% chance of a Higgs boson discovery by the end of 2009

If this was a USA vs. Europe competition to discover the Higgs particle, the Tevatron would have a clear advantage. Although it’s old (the first configuration was completed in 1984), and set to be superseded by the LHC in 2010, the Tevatron is a proven particle accelerator with an impressive track record. Accelerator techniques and technology have been refined, making high energy hadron collisions routine. However, Fermilab scientists are keen to emphasise that they aren’t trying to beat the LHC in the search for the Higgs boson.

We’re not racing CERN,” said Fermilab Director, Pier Oddone. He points out that there is a lot of collaborative work between Fermilab and CERN, therefore all scientists, no matter which continent they are on, are all working toward a common goal. In reality, I doubt this is the case. When searching for one of the most coveted prizes in modern quantum physics, it’s more of a case of ‘every lab for itself.’ Scientists in Fermilab have confirmed this, saying they are “working their tails off” analysing data from the Tevatron.

Indirectly, we’re helping them,” says Dmitri Denisov, DZero (one of the Tevatron’s detectors) spokesman, of his European competition. “They’re definitely feeling the heat and working a little harder.”

For the Standard Model to be complete, the Higgs particle must be found. If it does exist, physicists have put upper and lower bounds on its possible mass. Standing at a value between 114 and 184 GeV, this is well within the sensitivity of the Tevatron detectors. It should be a matter of time until the Higgs particle is discovered and physicists have calculated that if the Higgs particle can be created during a Tevatron high-energy proton-antiproton collision. They even give the Tevatron a 50:50 chance of a Higgs particle discovery by the New Year.

Last summer, both key particle experiments (CDF and DZero) focused on detecting Higgs particles with a mass of 170 GeV (at this value a particle would be easier to detect from the background noise). However, no Higgs particles were detected. Now physicists will expand the search above and below this value. Therefore, if the Higgs boson exists, it would be useful if it has a mass as close as possible to 170 GeV. Estimates suggest a 150 GeV Higgs boson could be discovered as early as this summer, well before the LHC has even been repaired. If the mass of the Higgs boson is around the 120 GeV mark, it might take Tevatron scientists until 2010 to verify whether a Higgs boson has been detected.

Source: New Scientist

New Satellite for Mapping CO2 Ready for Launch

The Orbiting Carbon Observatory (NASA)

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NASA’s first spacecraft dedicated to studying atmospheric carbon dioxide is ready for launch. The Orbiting Carbon Observatory, or OCO, is scheduled for liftoff aboard a Taurus XL rocket on February 24 from the Vandenberg Air Force Base, California at 1:51:30 a.m. PST. The spacecraft’s final polar orbit will be 438 miles. Carbon dioxide is the leading greenhouse gas driving changes in Earth’s climate. OCO will provide the first complete picture of human and natural carbon dioxide sources as well as their “sinks,” the places where carbon dioxide is pulled out of the atmosphere and stored.

OCO will map the global geographic distribution of the CO2 sources and sinks in the atmosphere and study their changes over time. The new observatory will dramatically improve global carbon dioxide data, collecting about eight million precise measurements every 16 days for at least two years.

CO2 is a critical component of the Earth’s atmosphere. Since the beginning of the industrial age, the concentration of CO2 has increased by about 38%, from about 280 parts per million to over 380 parts per million. Scientific studies indicate that CO2 is one of several gases that trap heat near the surface of the Earth. These gases are known as greenhouse gases. Many scientists have concluded that substantial increases in the abundance of CO2 will generate an increase in the Earth’s surface temperature. Historical records provide evidence of this trend, which is often called global warming. Current research indicates that continuing increases in atmospheric CO2 may modify the environment in a variety of ways. These changes may impact ocean currents, the jet stream and rain patterns. Some parts of the Earth might actually cool while the average temperature increases, and so this phenomenon is also called climate change.

OCO should help determine how much human-produced CO2 is contributing to climate change.

Source: NASA

Could Living Organisms Be Hiding Inside Olympus Mons?

Color mosaic of Mars' greatest mountain, Olympus Mons, viewed from orbit. Credit NASA/JPL

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From orbit, Olympus Mons dominates the landscape of the Tharsis region on Mars. At 24 kilometers (15 miles) high, and 550 kilometers (340 miles) in diameter, the huge volcano is over three times larger than Mount Everest. But Olympus Mons has a structure that is somewhat lopsided: it is elongated to the northwest, shortened to the southeast. A new study reveals that the ‘lopsidedness’ may mean warm magma and possibly water could be close enough to Olympus Mons’ surface to support thermophilic (heat-loving) bacteria like those found near hydrothermal vents on Earth.

While no volcanic activity has ever been seen or detected in Olympus Mons by orbiting spacecraft, the surface of the northwestern scarp has been dated from 115 million years old down to a region that is only 2 million years old. This is very recent in geological terms, suggesting that the mountain may yet have some ongoing volcanic activity.

To try and understand why Olympus Mons in lopsided, researchers Patrick J. McGovern and Julia K. Morgan from the Lunar and Planetary Institute, Universities Space Research Association, constructed detailed computer simulations of the volcano. They found the only way it could have the shape it does is if, when it was actively erupting, lava piled on top of layers of weak, water-laden clay sediments.

These layers could be hiding a trapped reservoir of water, if indeed Mars was once warmer and wetter. Whether that reservoir could still be warm, and if it could possibly hold life life remains uncertain. As of now, no orbiting satellites have any instruments that can penetrate the surface to look for a heat source.

This research was published in February 2009 in the journal Geology.

Source: The Geological Society of America

Space Tourist Sub-Orbital Flights From Hawaii?

Hawaii wants to have space tourism companies on the islands for faster transportation (NASA/Ian O'Neill)

[/caption]Private spaceflight companies seem to be getting closer and closer to the dream of launching a new breed of tourist on sub-orbital sightseeing tours. Since the late ’90’s the company Space Adventures has been sending millionaires on “trips of a lifetime”, but their most popular destination, the International Space Station, will stop hosting spaceflight participants at the end of this year as the Russian Soyuz spaceship wont have any more spare seats (as the crew on the station increase from three to six).

However, there are other private spaceflight companies beginning to realise the profits that could be made in space, not by dropping people off on the space station, but by launching them on short sub-orbital joyrides. They are building their own spaceships and even before the first rocket has ignited, there is growing competition for a piece of the space tourism market. Ticket prices have tumbled from the tens of millions (for a few days in orbit) to $200,000 (for a couple of hours on board a Virgin Galactic flight) to $95,000 (on board XCOR’s Lynx spaceplane for 30 minutes).

So, where should these companies launch their space tourists from? Although the space above the Mojave and New Mexico deserts are likely to be thundering to life within the next few years, a slightly more exotic destination is currently vying for a position in this burgeoning industry. Hawaii could be perfectly located not only for suborbital tourism, but for a revolution in global travel…

Space tourism is the next generation of humankind reaching for the stars,” said Jim Crisafulli, of the Hawaii State Office Aerospace Development.

The official is obviously referring to the conventional take-off and landing spaceplane designs by the likes of Rocketplane Global’s XP Vehicle and XCOR Aerospace’s Lynx. The XP, for example, uses conventional aircraft jet engines to attain a certain height and then the onboard rocket engine takes over, quickly taking the passengers to an altitude of 100km, allowing a few minutes of weightlessness. Judging by the Hawaii news source, the Hawaii officials appear to be referring to Rocketplane Global, as the online video shows an animated movie of the XP taking off much like a conventional jet.

What these are, are basically converted jet aircraft that take off and land at airports like normal jet aircraft. But once they get up to about 30,000 feet fire a rocket at the back of the plane, and this will take it up 62 miles,” Crisafulli added.

However, before you get caught up in dreams of sipping your Mai Tai on the beach, watching the palm trees sway with deep blue Pacific water lapping the golden sands of Maui, only to see a spaceplane rip through the skies, the Hawaii authorities have to justify the cost of an expensive Federal Aviation Administration (FAA) licence to allow a Hawaii spaceport.

Although tickets to space are getting cheaper, the first flights will still be expensive. After all, who has nearly $100,000 to $200,000 to spend on a short suborbital flight? However, optimistic estimates place a price of $5,000 per ticket in 5-7 years when these spaceplanes are bigger, carrying up to 100 people into space.

I know that’s still a little pricey, but to be able to experience space in the process is just tremendous and we think there will be a fairly significant market for this,” said Crisafulli.

Apparently four US spaceflight companies have approached Hawaii with requests to do business in the centre of the Pacific Ocean, so it appears the space visionaries think there is money to be made in this exotic location.

There may also be another, more practical reason for pushing to gain FAA approval for suborbital flight; it could revolutionize transportation to and from the isolated US state. “Having a flight from Hawaii to California maybe take 1 hour or 90 minutes, and a flight from Hawaii to Japan could take less than an hour,” said Senator Will Espero.

Source: KHON2

Galaxy Zoo 2 Launches

Galaxy Zoo.

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Do you Zoo? Well, now you can Zoo 2. Galaxy Zoo, that is. Galaxy Zoo 2 is a new version of the highly successful project that enables members of the public to take part in astronomy research online. But the research is now getting more interesting, and shall we say, more provocative? The original site only asked members of the public to say whether a galaxy was spiral or elliptical, and which way it was rotating, Galaxy Zoo 2 asks users to delve deeper into 250,000 of the brightest and best galaxies to search for the strange and unusual. “We we were so surprised about how many people participated in Galaxy Zoo and how good they were at this,” said Dr. Chris Lintott of Oxford University, one of the founders of Galaxy Zoo. “But now the idea is to ask for more detailed classifications. So it’s a Faustian pact we’re making with our users. We want them to spend more time with each galaxy, so it’s not just this fly by night, quick one-night stand of galaxy classification. We want them to get to know each galaxy a little bit better, have dinner first and all of that. But as a compromise, we have only a quarter of a million of the most interesting galaxies, the brightest, and the nearest. So you’ll spend more time looking at galaxies, but they’re prettier.”

At latest count, Galaxy Zoo has 182,383 users, (which Lintott notes is more people than live in Guam or Sunderland) who have performed 74,503,984 classifications of galaxies.

Lintott told Universe Today that Galaxy Zoo is a classic pub idea that worked. “I was working with Kevin Schawinski of Yale University on galaxies,” he said, and to get accurate data, they needed to classify a large number of galaxies. “We’d heard about Stardust at Home, which is an amazing project. I was impressed they were able to do this, to get people search for dust grains. And we’ve got all these pretty pictures of galaxies to look at, so surely people would like to look at galaxies. We put the site together, and we’ve been overwhelmed with the response.”

Galaxies from Galaxy Zoo.
Galaxies from Galaxy Zoo.

The human eye and brain are better at doing pattern recognition tasks than a computer. Lintott noted that astronomers have spent 70 years classifying galaxies according the laws that Hubble put down, but only by classifying a really large number are astronomers going to have any sense of what the population of different types of galaxies are.

“Is there really any difference between and Sa and an Sb galaxy?” asked Lintott. “They’re defined by different tightnesses of spiral arms and different bulge shapes, but we want to know, do they live in the same place or do they have the same star formation histories or what is going on with the black holes? So we need to classify many galaxies into these categories. So that’s the idea for Zoo 2. Rather than getting people to remember the categories we have a series of questions that you go through so we get individual information about the galaxies.”

As with the original site people are free to look at and describe as many galaxies as they like – even five minutes’ work will provide a valuable contribution. Galaxy Zoo 2 is intended to be even more fun as galaxies are pitted against each other in “Galaxy Wars” (which one is more spirally?) and users can compete against their friends to describe more objects as well as record their best finds.

Zoo 2 has been in a test phase for a couple of months, and everything seems to be working well, as hundreds of thousands of classifications have already been done in the new version. “There was a worry that maybe we had exhausted people’s tolerance for galaxies, but apparently not,” said Lintott.

To join in on the fun, check out Galaxy Zoo.

The BBC talked with Chris Lintott, too, and they have a nice video overview of Galaxy Zoo and Zoo 2.

Source: Interview with Chris Lintott.

The Milky Way Spiral

Artist impression of the Milky Way.

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If you’ve seen an image of the Milky Way from above or below, you will certainly notice that it has a spiral structure. Not all galaxies are created equal, though, as there are many, known as elliptical galaxies, that are blob-like, while others have irregular shapes. Ours is of a class of galaxies called barred spirals, because it has a rectangular bar in the middle of the galactic disk.

The Milky Way has four main spiral arms: the Norma and Cygnus arm, Sagittarius, Scutum-Crux, and Perseus. The Sun is located in a minor arm, or spur, named the Orion Spur. The galactic disk itself is about 100,000 light years across, and the bar at the center is estimated to be about 27,000 light years long.

Why is the Milky Way a spiral? This is due to its rotation, or rather, the rotation of matter inside the galactic disk around the center. It’s not as if the stars themselves stay in the spiral arms, and rotate around the center of the galaxy, though: if they did this, the arms would wind in tighter and tighter over time (2 billion years or so), since the stars in the center revolve faster than those further out.

The spirals are actually what is called a density wave or standing wave. The best way to describe this is the analogy of a traffic jam: cars travel on a busy road in a city, bunching up in jams over the course of a day at certain sections. But the cars move through the jam eventually, and other cars pile up behind them in the jam. The wave is at a certain location, with bunches of matter piling up there for a while, then moving on to be replaced by other matter. As dust and gas is compressed in the spirals, it is heated up and results in the formation of new stars. This star formation makes the trailing edge of the spiral brighter, and places the density wave “ahead”, where dimmer, redder stars are starting to be compressed.

When you see an image of the Milky Way like the one above, it’s not actually a photo of our galaxy. Since we inhabit the disk and have no way (currently) of going above or below, images of the Milky Way are generated by computers or artists. Astronomers have determined that the Milky Way is a spiral galaxy by mapping the movements of stars and hydrogen clouds in the disk.

The Milky Way is far from being the only spiral galaxy in the Universe. To view images of other spiral galaxies, go to the aptly-named Spiral Galaxies website, or NASA’s Astronomy Picture of the Day Spiral Galaxy Index.

To learn more about the Milky Way, check out Episode 99 of Astronomy Cast, or visit the rest of the Milky Way section in the Guide to Space.

Source: University of Wisconsin-Madison News

The Milky Way Could have Billions of Earths

Exoplanets like the Earth might be more common than we think. Image Credit: ESO

With the upcoming launch in March of the Kepler mission to find extrasolar planets, there is quite a lot of buzz about the possibility of finding habitable planets outside of our Solar System. Kepler will be the first satellite telescope with the capability to find Earth-size and smaller planets. At the most recent meeting of the American Association for the Advancement of Science (AAAS) in Chicago, Dr. Alan Boss is quoted by numerous media outlets as saying that there could be billions of Earth-like planets in the Milky Way alone, and that we may find an Earth-like planet orbiting a large proportion of the stars in the Universe.

“There are something like a few dozen solar-type stars within something like 30 light years of the sun, and I would think that a good number of those — perhaps half of them would have Earth-like planets. So, I think there’s a very good chance that we’ll find some Earth-like planets within 10, 20, or 30 light years of the Sun,” Dr. Boss said in an AAAS podcast interview.

Dr. Boss is an astronomer at the Carnegie Institution of Washington Department of Terrestrial Magnetism, and is the author of The Crowded Universe, a book on the likelihood of finding life and habitable planets outside of our Solar System.

“Not only are they probably habitable but they probably are also going to be inhabited. But I think that most likely the nearby ‘Earths’ are going to be inhabited with things which are perhaps more common to what Earth was like three or four billion years ago,” Dr. Boss told the BBC. In other words, it’s more likely that bacteria-like lifeforms abound, rather than more advanced alien life.

This sort of postulation about the existence of extraterrestrial life (and intelligence) falls under the paradigm of the Drake Equation, named after the astronomer Frank Drake. The Drake Equation incorporates all of the variables one should take into account when trying to calculate the number of technologically advanced civilizations elsewhere in the Universe. Depending on what numbers you put into the equation, the answer ranges from zero to trillions. There is wide speculation about the existence of life elsewhere in the Universe.

To date, the closest thing to an Earth-sized planet discovered outside of our Solar System is CoRoT-Exo-7b, with a diameter of less than twice that of the Earth.

The speculation by Dr. Boss and others will be put to the test later this year when the Kepler satellite gets up and running. Set to launch on March 9th, 2009, the Kepler mission will utilize a 0.95 meter telescope to view one section of the sky containing over 100,000 stars for the entirety of the mission, which will last at least 3.5 years.

The prospect of life existing elsewhere is exciting, to be sure, and we’ll be keeping you posted here on Universe Today when any of the potentially billions of Earth-like planets are discovered!

Source: BBC, EurekAlert

Weekend Fireballs Not Satellite Debris

Bolide in Italy. Credit: Ferruccio Zanotti of Ferrara, Italy, via Spaceweather.com


A fireball seen over Texas during the daytime on Sunday, Feb. 15th, triggered widespread reports that debris from the recent satellite collision was falling to Earth. The FAA even issued a statement that airplanes should watch for falling debris. However, those reports and statements were premature. Researchers have studied video of the event and concluded that the object was more likely a natural meteoroid about one meter wide traveling more than 20 km/s–much faster than orbital debris. Meteoroids hit Earth every day, and the Texas fireball was apparently one of them. Additionally, a spokeswoman for U.S. Strategic Command said the fireball spotted in the Texas skies Sunday was unrelated to the satellite collision. And as always, the Bad Astronomer was on top of it from the beginning, so check out his first post here (which includes several updates as the news broke), and a follow-up here. There were other fireballs, too….

There was one bolide event in central Kentucky on Friday, February 13. People heard loud booms, felt their houses shake, and saw a fireball streaking through the sky. This occurred just hours after another fireball at least 10 times brighter than a full Moon lit up the sky over Italy. Although it is tempting to attribute these events to debris from the Feb. 10th collision of the Iridium 33 and Kosmos 2251 satellites, the Kentucky and Italy fireballs also seem to be meteoroids, not manmade objects. Italian scientists are studying the ground track of their fireball, which was recorded by multiple cameras, and they will soon begin to hunt for meteorites.
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Air Force Major Regina Winchester said that Joint Space Operations Center at California’s Vandenberg Air Force Base has been monitoring the debris from the collision, and that could not have caused the dramatic sight. She also said the fireball was not related to the estimated 18,000 man-made objects that the center also monitors.

“There was no predicted re-entry,” Winchester said about the objects in Earth’s orbit.

She said it was likely a natural phenomenon such as a meteorite.

Check out Spaceweather.com for more pictures, video and info.

Sources: Bad Astronomy, Spaceweather.com, Dallas News