Nancy Atkinson, Author at Universe Today

October 14, 2008December 24, 2015 by Nancy Atkinson

Procedure to Repair Hubble Begins Wednesday

The Hubble Space Telescope. Credit: NASA

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The procedure to begin “brain surgery” on the Hubble Space Telescope will begin at 6:00 am EDT (10:00 GMT) on October 15. The venerable space telescope will be put into electronic hibernation; then engineering teams will work from the ground around the clock for two days to reconfigure a data handler system which failed two weeks ago. If the procedure is successful, science operations could resume as early as Friday, October 17. The Control Unit/Science Data Formatter, which relays science data to Earth, is a redundant system, with two sides. Side A has been used exclusively since the telescope’s launch over 18 years ago in 1990. Side B hasn’t been powered on since well before launch. “It is obviously a possibility that things will not come up,” said Art Whipple, manager of the Hubble Space Telescope Systems Management office at the Goddard Spaceflight Center in Greenbelt, Md. “We have very good confidence this will work. In addition, we have contingency plans built in at each step of the transition where if something does not go the way we expect it to, we’ll be able to back out and go down an alternate path.”

Whipple said there is very little aging that goes on with an unpowered component in space. “It’s actually a very benign storage environment,” he said.

In addition six associated components have to be switched over to a redundant side as well. “Five of the six redundant components in this data management system that will be brought on line have also not been powered since 1990,” said Whipple. “The command procedures to accomplish this transition have been thoroughly tested.”

Engineers and mission managers have been working the past two weeks, devising a plan and testing procedures. NASA headquarters gave approval for the activation on Tuesday.

The planned Hubble Servicing Mission 4, shuttle mission STS-125, would have launched today (Oct. 14) if the data handler had not gone off line. NASA has re-set a tentative launch date for mid-February. The seven member crew, commanded by veteran Scott Altman, will perform five back-to-back spacewalks to add new cameras, (the Wide Field Camera 3 (WFC3) and the Cosmic Origins Spectrograph), replace old batteries and gyroscopes, add docking equipment and upgrade the telescope’s guidance system. The astronauts will also attempt to fix the Space Telescope Imaging Spectrograph (STIS) and the Advanced Camera for Surveys (ACS). Those two were never designed to be repaired in orbit. In addition, a spare data handler system will brought up, after engineers test and certify the unit. That unit has not been turned on since 1992.

It has yet to be determined if the spare data handler will be ready by mid-February, and if the astronauts can be trained ready for the additional work required for the unit switch-out.

“We think in the first week or two in November we will have a much better handle on the actual state of the hardware,” Whipple said. “The paperwork says February should be supportable, but we should have much higher confidence (in November).”

Sources: NASA press release, NASA news conference

October 14, 2008December 24, 2015 by Nancy Atkinson

Single Species Ecosystem Gives Hope For Life on Other Planets

A species of life on Earth could possibly survive on Enceladus. Credit: JPL

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The discovery of solitary little critters deep beneath Earth’s surface has set the world of microbiology on its head while exciting astrobiologists about the possibility of life on other planets. A community of bacteria was found 2.8 kilometers below ground in a goldmine and it lives completely alone and completely independent of any other life forms. It also subsists without sunlight or oxygen. Planetary scientist Chris McKay, of NASA’s Ames Research Center says that the species Candidatus Desulforudis audaxviator is an amazing discovery, and represents the kind or organism that could survive below the surface of Mars or Saturn’s sixth largest moon Enceladus.

Nicknamed “the bold traveler,” the species was found in fluid-filled cracks of the Mponeng goldmine in South Africa. The discovery of the species contradicts the principle that all life on earth is part of one great, interdependent system.

Scientists extracted all of the DNA present within 5,600 liters of fluid from a fracture deep within the mine. Expecting to find a mix of species within the fluid, the researchers were surprised to find that 99.9% of the DNA belonged to one bacterium, a new species. The remaining DNA was contamination from the mine and the laboratory.

A community of a single species is almost unheard of in the microbial world. But this little bacteria has been happily living on its own and seems to have all of the genetic machinery to enable it to survive independently. Since it is the only species in the ecosystem, it must extract everything it needs from an otherwise dead environment.

Analysis by Dylan Chivian of the Lawrence Berkeley National Laboratory showed that D. audaxviator gets its energy from the radioactive decay of uranium in the surrounding rocks. It has genes to extract carbon from dissolved carbon dioxide and other genes to fix nitrogen, which comes from the surrounding rocks. Both carbon and nitrogen are essential building blocks for life as we know it.

D. audaxviator can also protect itself from environmental hazards by forming endospores – tough shells that protect its DNA and RNA from drying out, toxic chemicals and from starvation. It has a flagellum to help it navigate.

Every other species that we know of on Earth planet relies on other species for some benefit. For example, humans rely on plants to photosynthesize so that we can eat them. Also, other known ecosystems on Earth that don’t use sunlight directly, such as lifeforms found in deep sea vents, do use some form of photosynthesis. But this newly found species actually can’t handle oxygen

The water in which D. audaxviator lives has not seen the light of day in over 3 million years, and this could be an indication of how old the species is.

When we start to look for life on other planets, the discovery of this species will help broaden the horizons of our search.

Abstract detailing the discovery.

Sources: New Scientist

October 13, 2008December 24, 2015 by Nancy Atkinson

An Inside Look at Comet Holmes

The astronomy world buzzed in the Fall of 2007 when Comet Holmes – a normally humdrum, run-of-the-mill comet — unexpectedly flared and erupted. Its coma of gas and dust expanded away from the comet, extending to a volume larger than the Sun. Professional and amateur astronomers around the world turned their telescopes toward the spectacular event. Everyone wanted to know why the comet had suddenly exploded. The Hubble Space Telescope observed the comet, but provided few clues. And now, observations taken of the comet after the explosion by NASA’s Spitzer Space Telescope deepen the mystery, showing oddly behaving streamers in the shell of dust surrounding the nucleus of the comet. The data also offer a rare look at the material liberated from within the nucleus. “The data we got from Spitzer do not look like anything we typically see when looking at comets,” said Bill Reach of NASA’s Spitzer Science Center at Caltech.

Every six years, comet 17P/Holmes speeds away from Jupiter and heads inward toward the sun, traveling the same route typically without incident. However, twice in the last 116 years, in November 1892 and October 2007, comet Holmes exploded as it approached the asteroid belt, and brightened a millionfold overnight.

In an attempt to understand these odd occurrences, astronomers pointed NASA’s Spitzer Space Telescope at the comet in November 2007 and March 2008. By using Spitzer’s infrared spectrograph instrument, Reach and his colleagues were able to gain valuable insights into the composition of Holmes’ solid interior. Like a prism spreading visible-light into a rainbow, the spectrograph breaks up infrared light from the comet into its component parts, revealing the fingerprints of various chemicals.

The Spitzer Space Telescope. Credit: NASA

In November of 2007, Reach noticed a lot of fine silicate dust, or crystallized grains smaller than sand, like crushed gems. He noted that this particular observation revealed materials similar to those seen around other comets where grains have been treated violently, including NASA’s Deep Impact mission, which smashed a projectile into comet Tempel 1; NASA’s Stardust mission, which swept particles from comet Wild 2 into a collector at 13,000 miles per hour (21,000 kilometers per hour), and the outburst of comet Hale-Bopp in 1995.

“Comet dust is very sensitive, meaning that the grains are very easily destroyed, said Reach. “We think the fine silicates are produced in these violent events by the destruction of larger particles originating inside the comet nucleus.”

When Spitzer observed the same portion of the comet again in March 2008, the fine-grained silicate dust was gone and only larger particles were present. “The March observation tells us that there is a very small window for studying composition of comet dust after a violent event like comet Holmes’ outburst,” said Reach.

Comet Holmes not only has unusual dusty components, it also does not look like a typical comet. According to Jeremie Vaubaillon, a colleague of Reach’s at Caltech, pictures snapped from the ground shortly after the outburst revealed streamers in the shell of dust surrounding the comet. Scientists suspect they were produced after the explosion by fragments escaping the comet’s nucleus.

In November 2007, the streamers pointed away from the sun, which seemed natural because scientists believed that radiation from the sun was pushing these fragments straight back. However, when Spitzer imaged the same streamers in March 2008, they were surprised to find them still pointing in the same direction as five months before, even though the comet had moved and sunlight was arriving from a different location. “We have never seen anything like this in a comet before. The extended shape still needs to be fully understood,” said Vaubaillon.

He notes that the shell surrounding the comet also acts peculiarly. The shape of the shell did not change as expected from November 2007 to March 2008. Vaubaillon said this is because the dust grains seen in March 2008 are relatively large, approximately one millimeter in size, and thus harder to move.

“If the shell was comprised of smaller dust grains, it would have changed as the orientation of the sun changes with time,” said Vaubaillon. “This Spitzer image is very unique. No other telescope has seen comet Holmes in this much detail, five months after the explosion.”

“Like people, all comets are a little different. We’ve been studying comets for hundreds of years — 116 years in the case of comet Holmes — but still do not really understand them,” said Reach. “However, with the Spitzer observations and data from other telescopes, we are getting closer.”

Source: Spitzer Press Release

October 13, 2008April 26, 2016 by Nancy Atkinson

Mars Satellite’s First Weather Report

The Mars Reconnaissance Orbiter using its Mars Climate Sounder instrument. Credit: JPL

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The Mars Reconnaissance Orbiter has been circling Mars for over two years now, and has provided unprecedented views of the Red Planet with its HiRISE Camera. But did you also know that MRO is a weather-monitoring satellite, too? The Mars Climate Sounder instrument is examining the Martian atmosphere and has issued its first Mars weather report. “It has taken 20 years and three missions but we finally have an instrument in orbit that gives us a detailed view of the entire atmosphere of Mars and it is already giving us fresh insights into the Martian climate,” said Professor Fred Taylor of Oxford University. Within a paper issued by the Mars ‘weather team’ comes surprising news: during the freezing Martian winter the atmosphere above the planet’s South Pole is considerably warmer than predicted.

The team discovered that even in the depths of the Martian winter, when the planet’s South Pole is frozen and in total darkness, at an altitude of 30-80km the atmosphere is being heated to 180 Kelvin – that’s 10-20 Kelvin warmer than expected.

“Winter at the Martian South Pole is severe even by the standards of our Antarctic,” said Professor Taylor. “The Pole is shrouded in total darkness for many months and the carbon dioxide in the atmosphere freezes, creating blizzards and causing a thick layer of carbon dioxide ice to form across the surface. Yet what we’ve found is that 30 kilometers above the surface conditions are very different.”

The team, which also included Oxford physicists Dr Pat Irwin and Dr Simon Calcutt, believe that a vigorous circulation of the atmosphere – from the Martian equator to the Pole – is compressing the gas and causing the heating effect.

“It’s the same effect that warms the cylinder of a bicycle pump, or the pistons of a car engine, when you compress the gas inside,” said Taylor. “What we think we are observing is that the ‘engine’ of the Martian climate – this atmospheric circulation – is running as much as 50 per cent faster than our models predicted, resulting in this warming of the South Pole.”

These are just the first results from what the scientists hope will be many more years of study. In the long-term they hope to shed light on climate change on Mars, what controls it and what lessons can be drawn for climate change on Earth.

Studying the Martian climate helps us understand how a planet that was originally similar to Earth turned out so very different.

The team’s paper, ‘Intense polar temperature inversion in the middle atmosphere on Mars’, was published in Nature Geoscience on Oct. 12, 2008.

Source: Oxford University

October 13, 2008April 26, 2016 by Nancy Atkinson

Where Are the Images from Asteroid 2008 TC3?

Asteroid-2008-tc3. From Kite Power El Gouna web cam.

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One of the big news items last week was the prediction that an asteroid was on a collision course with Earth. Although it was a small space rock – estimates ranged from 1-5 meters (3-15 feet), scientists were excited because this was the first time an asteroid was discovered with an imminent known impact. Granted, we’d all probably feel a little safer if we knew about this asteroid, named 2008 TC3, days or months ahead of time instead of only 19 hours, but it’s a step in the right direction. Astronomers even predicted correctly the asteroid would come through the atmosphere over Africa. So with this prediction, many were hoping someone with a camera would be watching the skies of Sudan. But the flight path of the object was over a remote area and so far the only ground-based image that has surfaced is the one shown here, taken by a webcam from a beach in Egypt. (The words on the image indicate the objects on the beach — which were illuminated by the fairly distant explosion low on the horizon. ~~try to find the tiny bright spot in the center of the image — that’s the asteroid~~.) But we do have satellites constantly monitoring Earth’s atmosphere and a few of them captured images and data about 2008 TC3. However, it’s not known if any parts of the meteoroid hit the ground.

The explosion was recorded directly by the cameras of a European weather satellite called METEOSAT-8. This was taken in infrared, and the temperature scale on the right is in Kelvin.

Asteroid 2008 TC3 seen from space in infrared. Credit: EUMETSAT

Data from this satellite helped determine the asteroid entered Earth’s atmosphere at a velocity of 12.8 kilometers per second. “As it entered the Earth’s atmosphere, it compressed the air in front of it. The compression heated the air, which in turn heated the object to create a spectacular fireball, releasing huge amounts of energy as it disintegrated and exploded in the atmosphere, dozens of kilometers above ground,” the Eumetsat website explains. Meteostat also took a visible image:

Also, according JPL’s Near Earth Object Program, an undisclosed U.S. system has monitored the airburst and yielded a precise time (02:45:45 UTC) and explosive energy equivalent (0.9 to 1.0 kT of TNT). The NEO office also said, “Tthe follow-up astrometric observations from professional and sophisticated amateur astronomers alike were rather extraordinary, with 570 observations from 26 observatories being reported between the time of discovery by the Catalina Sky Survey to just before the object entered Earth’s shadow (57 minutes prior to impact).” These observations revealed a tumbling, rotating object. The CAST astronomical observatory created a “movie” of their observations of the asteroid before it entered into Earth’s shadow.

CAST astronomical obervatory in Italy created this 2008tc3 animation.

Here’s links to a few other ground based observatories and their pre-impact sightings: from Eric Allen of Observatoire du Cegep de Trois-Rivieres, Champlain, Quabec; from Ernesto Guido et al. of Remanzacco Observatory, Italy; from S.Korotkiy and T.Kryachko of Kazan State University Astrotel observatory, Russia

Also, SpaceWeather.com reported the crew of an airplane saw a flash in the sky which may have been from this object. But beyond that, sadly, there’s not many images available related to this extraordinary event. If any surface, we’ll be sure to post them.

Sources: SpaceWeather.com, Cosmos4U, Planetary Society Blog, JPL NEO Program

October 13, 2008December 24, 2015 by Nancy Atkinson

‘Little’ Gamma Ray Bursts Really Do Exist

Artist impression of a GRB. Credits: ESA, illustration by ESA/ECF

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Gamma-ray bursts (GRBs) are powerful blasts of energy that flash across the Universe. For a brief time, they are the brightest objects in the gamma-ray sky. Astronomers estimate that about 1,400 GRBs per year occur but because no one knows when and where they are going to appear, only a part of them happen to be detected. ESA’s Integral gamma-ray observatory detects about 10 GRBs a year, and those are of the big burst variety. But the spacecraft has observed several low-luminosity gamma-ray bursts, confirming the existence of an entire population of weaker bursts that have hardly been noticed so far. These aren’t just bursts from far away, but just weak bursts that are relatively close by. And astronomers are beginning to think these weak or faint variety of GRBs might be the most common.

When studying Integral’s gamma-ray burst data, Prof. Lorraine Hanlon from the School of Physics, University College Dublin, Ireland, and her colleagues, realized that some of the faintest bursts have distinctive gamma-ray emissions, and also present faint afterglows in the lower-energy X-ray and visible wavelengths.

Since, in general, GRBs are colossal explosions of energy triggered by the collision of very massive and compact objects such as neutron stars or black holes, or by the explosion of incredibly powerful supernovae, or hypernovae, one may think that these bursts are perceived as faint just because they take place very far away from us, in the remote corners of the Universe.

However, Prof. Hanlon and colleagues noticed that these faint bursts, just at the sensitivity threshold of IBIS, seem to originate in our cosmic neighborhood, within the nearby clusters of galaxies.

Distribution of faint GRBs. Credits: S. Foley/UCD

“If the bursts we have studied are so ‘close’ in cosmological terms, it means that they are faint from the beginning,” says Hanlon. “From this we can deduce that the processes triggering them could be less energetic than those generating the more powerful bursts we are more used to observing.”

The study team suggests that the faint bursts may be generated by the collapse of a massive star that does not present the characteristics of a supernova, or by the merger of two white dwarfs (small and dense stars about the size of Earth), or by the merger of a white dwarf with a neutron star or a black hole.

“Past observations had already hinted the existence of faint GRBs, and thanks to Integral’s sensitivity we can now say that an entire population of them exist,” added Hanlon. “Actually, their rate may even be higher than that of the most luminous GRBs but, just because they are weaker, we may be only able to see those which are relatively close by.”

“More Integral observations in the coming years will definitively help us understand the phenomenon of faint GRBs, and to explore the nature of this newly observed population,” she concluded.

Source: ESA

October 11, 2008December 24, 2015 by Nancy Atkinson

The Universe Is Not Expanding Uniformly

Partial map of the Local Group of galaxies. Credit: Planet Quest

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A few weeks ago, researchers announced the discovery of a “dark flow” of invisible matter tugging at distant galaxy clusters at the edge of the universe. Now comes more evidence of unseen and unknown forces in the cosmos, but this time its closer to home. A group of researchers have discovered that our particular part of the Universe — out to a distance of 400 million light years — is not expanding uniformly in all directions as expected. To be exact, the expansion is faster in one half of the sky than in the other. “It’s as if, in addition to the expansion, our ‘neighbourhood’ in the Universe has an extra kick in a certain direction,” says Mike Hudson from the University of Waterloo in Ontario, Canada. “We expected the expansion to become more uniform on increasingly larger scales, but that’s not what we found.” If confirmed, their findings will result in a new understanding of the origin of structure in the universe and possible revisions to the standard cosmological model.

Hudson and two other scientists have been conducting research on large-scale cosmic flows and the general expansion of the universe. This expansion increases the distances between galaxies steadily with time, and is called the Hubble flow. Deviations of the velocity of galaxies from the overall Hubble flow is called the “peculiar velocity.” By examining the peculiar velocities of clusters and superclusters scientists can obtain estimates of local mass concentrations that may be responsible for causing any deviations from the Hubble flow.

In particular, these researchers were attempting to address a longstanding question about the origin of the approximately 600 km/s peculiar velocity of the Local Group of galaxies, with respect to the Cosmic Microwave Background.

Using several different surveys they discovered that about 50% of the Local Group’s motion is faster than anticipated. To produce this motion, they believe there must be large unseen and unknown structures in the universe. They write, “The large value of the residual motion implies that there are significant velocities generated by very-large scale structures,” and the structures lie beyond the Local Group.

Brian McNamara, a University Research Chair in UW’s department of physics and astronomy, says Hudson is finding that much of the matter in the nearby universe moves as an ensemble with a surprisingly high speed. “If the work he and others are doing is confirmed, it will require a major revision in the way we think the universe came into being and how it evolved.”

Hudson and his colleagues have submitted a paper to the Royal Astronomical Society, and a preprint version is available here.

Sources: arXiv, University of Waterloo

October 10, 2008December 24, 2015 by Nancy Atkinson

Dust Could Point Out Earth-like Exoplanets

Zodiacal light can be seen in the sky before sunrise or after sunset. Credit: Yuri Beletsky/ESO Paranal

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The current exoplanet count — the number of planets astronomers have found orbiting other stars –stands at 312. That’s a lot of planets. But not a single one of them can be classified as Earth-like. We just don’t have the ability to detect planets that small yet. But it might help if we knew exactly where to look. New research using supercomputer simulations of dusty disks around sun-like stars show that planets nearly as small as Mars can create patterns in the dust that future telescopes may be able to detect. The research points to a new avenue in the search for habitable planets. “It may be a while before we can directly image earth-like planets around other stars but, before then, we’ll be able to detect the ornate and beautiful rings they carve in interplanetary dust,” says Christopher Stark, the study’s lead researcher at the University of Maryland, College Park.

Working with Marc Kuchner at NASA’s Goddard Space Flight Center in Greenbelt, Md., Stark modeled how 25,000 dust particles responded to the presence of a single planet — ranging from the mass of Mars to five times Earth’s — orbiting a sun-like star. Using NASA’s Thunderhead supercomputer at Goddard, the scientists ran 120 different simulations that varied the size of the dust particles and the planet’s mass and orbital distance.

“Our models use ten times as many particles as previous simulations. This allows us to study the contrast and shapes of ring structures,” Kuchner adds. From this data, the researchers mapped the density, brightness, and heat signature resulting from each set of parameters.

“It isn’t widely appreciated that planetary systems — including our own — contain lots of dust,” Stark adds. “We’re going to put that dust to work for us.”

Much of the dust in our solar system forms inward of Jupiter’s orbit, as comets crumble near the sun and asteroids of all sizes collide. The dust reflects sunlight and sometimes can be seen as a wedge-shaped sky glow — called the zodiacal light — before sunrise or after sunset.

Dust rings. Credit: NASA/Christopher Stark, GSFC

The computer models account for the dust’s response to gravity and other forces, including the star’s light. Starlight exerts a slight drag on small particles that makes them lose orbital energy and drift closer to the star.

“The particles spiral inward and then become temporarily trapped in resonances with the planet,” Kuchner explains. A resonance occurs whenever a particle’s orbital period is a small-number ratio — such as two-thirds or five-sixths — of the planet’s.

For example, if a dust particle makes three orbits around its star every time the planet completes one, the particle repeatedly will feel an extra gravitational tug at the same point in its orbit. For a time, this extra nudge can offset the drag force from starlight and the dust can settle into subtle ring-like structures.

“The particles spiral in toward the star, get trapped in one resonance, fall out of it, spiral in some more, become trapped in another resonance, and so on,” Kuchner says. Accounting for the complex interplay of forces on tens of thousands of particles required the mathematical horsepower of a supercomputer.

Some scientists note that the presence of large amounts of dust could present an obstacle to directly imaging earthlike planets. Future space missions — such as NASA’s James Webb Space Telescope, now under construction and scheduled for launch in 2013, and the proposed Terrestrial Planet Finder — will study nearby stars with dusty disks. The models created by Stark and Kuchner give astronomers a preview of dust structures that signal the presence of otherwise hidden worlds.

“Our catalog will help others infer a planet’s mass and orbital distance, as well as the dominant particle sizes in the rings,” Stark says.

Stark and Kuchner published their results in the October 10 issue of The Astrophysical Journal. Stark has made his atlas of exo-zodiacal dust simulations available online.

Source: Goddard Space Flight Center

October 10, 2008December 24, 2015 by Nancy Atkinson

Mars Science Laboratory: Still Alive, For Now

The Mars Science Laboratory. Credit: JPL

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The Mars Science Laboratory, the next generation of Mars rovers slated to head to Mars in 2009, is still alive, for the time being. The car-sized rover designed to look for life on Mars is over budget and behind schedule due to technical problems, and NASA officials met today to discuss their options. Potentially, Congress could pull the plug on the mission if cost overruns go too high. NASA Administrator Mike Griffin and Science Associate Administrator Ed Weiler were briefed, and met with mission managers in attempt to work out a potential solution. In a press briefing today, Doug McCuistion, director of the Mars Exploration Program at NASA headquarters said the rover’s progress will be assessed again in January, but the mission will need more money. “This is a really important scientific mission,” McCuistion said. “This is truly the push into the next decade for the Mars program and for the discovery for the potential for life on other planets…I fully believe that Congress will support us as we go forward on this because they recognize the importance of the mission as well.”

The panel of NASA officials at the briefing wouldn’t say where the money will come from or exactly how much will be needed to keep the rover on schedule and provide the engineers the resources they need to overcome the technical problems. But NASA will seek additional money from Congress and/or realign funds from other missions.

“If we’re going to launch in 2009 or 2011 additional budget resources are going to be necessary. The sources of that we cannot release until we get approval from the Office of Management and Budget and Congress,” said McCuistion.

Costs for MSL have already gone from the initial $1.5 billion to $1.9 billion. Launch is scheduled sometime between Sept. 15 and Oct. 15, 2009, but could be delayed until 2011 if the problems take more time to be resolved. Earth and Mars come closest to each other approximately every 26 months, providing favorable launch windows.

Problems with parachutes, actuators and other materials have delayed construction of the rover, and currently the contractors are working multiple shifts to make up for lost time. Mission managers hope tests of the rover can begin in November or December.

MSL will be three times as heavy and twice the width of the Mars Exploration Rovers (MERs) that landed in 2004, and will be able to travel twice as far. It will carry ten advanced scientific instruments and cameras. It will make the first precise landing and a predetermined site, using a guided entry system and a soft-landing system called the Sky Crane.

Source: NASA News Audio

October 10, 2008December 24, 2015 by Nancy Atkinson

365 Days of Astronomy Podcast

Hopefully you’ve heard about the International Year of Astronomy — a year long celebration in 2009 of the 400th anniversary of Galileo’s first look through the telescope. One part of that celebration is the 365 Days of Astronomy Podcast. There will be one podcast per day, every day, for all 365 days of 2009. The podcasts will be 5 to 10 minutes in duration, and will be available through the 365 Days of Astronomy website and an RSS feed. The 365 Days team has just put out a trailer encouraging everyone to listen every day:

Want to be part of the project?

Not only will you have the chance to listen each day, but you can participate as well. The podcast episodes will be written, recorded and produced by people around the world. Each day will have a specific topic or theme based on The 365 Days of Astronomy Calendar, a daily calendar of astronomical events, themes and ideas created by the IYA.

People participating can choose their own topics, all of which will need to be approved ahead of time. For all the details head on over to the website. And if you’ve never recorded anything before, never fear. There’s even information on how to record a podcast, as well as much more.

You can also follow 365 Days of Astronomy on Twitter.

And, if you thought you’ve heard the voice on the video before, its none other than the golden voice of Mat Kaplan from Planetary Radio.