Fast Food Delivery: Progress Docks With ISS

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A new Progress cargo carrier docked to the International Space Station’s Pirs docking compartment early Wednesday, bringing almost 2.5 tons of fuel, air, water and other supplies to the station and its three-member crew. One of the first items unpacked were fresh tomatoes and lettuce, to be used for an anticipated culinary treat of “space hamburgers” for the crew.

This is the ISS’s 27th unpiloted Progress spacecraft to bring supplies to the station. The Progress launched from the Baikonur Cosmodrome in Kazakhstan on Dec. 23 at 2:21 am EST, and docked with the ISS on Dec. 26 at 3:14 am EST. About three hours later, the crew began unloading the supplies, which includes more than 1,900 pounds of propellant, over 100 pounds of oxygen and 2,921 pounds of dry cargo. Part of the dry cargo are Christmas presents for Expedition 16 commander Peggy Whitson and flight engineer Dan Tani, as well as birthday gifts for Russian flight engineer Yuri Malenchenko, who turned 46 on Saturday.

In an earlier press conference Whitson mentioned she was especially looking forward to receiving the “fixingsâ€? for hamburgers, especially since the crew wouldn’t be able to enjoy the Christmas meal that space shuttle Atlantis was supposed to bring on its flight, originally scheduled for early December. The shuttle will now launch no earlier than January 10 due to problems with engine cutoff sensors in the shuttle’s external fuel tank. Whitson said she had created space hamburgers during her previous stay on the station, Expedition 5, and wanted to reproduce the meal for her current crew.

The previous Progress ship was undocked from the station last Friday, after it was filled with trash and unneeded equipment from the station. It will be deorbited for destruction on re-entry in mid-January after conducting Earth observation experiments.

Original News Source: NASA Press Release

It’s a Bird! It’s Tinker Bell! It’sThree Galaxies!

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There once was a galaxy known as ESO 593-IG 008. It was thought to be a relatively mild-mannered galaxy, even though scientists believed it was a collision of two different galaxies; one a barred spiral and the other an irregular galaxy. But now, an international team of astronomers has discovered that it actually is a stunning rare case of three interacting galaxies, with the third galaxy forming stars at a frantic rate.

Using adaptive optics on the European Southern Observatory’s (ESO) Very Large Telescope (VLT), astronomers were able to see through the all-pervasive dust clouds of the object that has been dubbed as “The Bird” because of its resemblance to a winged creature. With the adaptive optics of what’s called the NACO instrument, very fine details were able to be resolved.

“Examples of mergers of three galaxies of roughly similar sizes are rare,” says Petri Vaisanen, lead author of the paper which will appear in the journal of the Royal Astronomical Society. “Only the near-infrared VLT observations made it possible to identify the triple merger nature of the system in this case.”

NACO is the combination of NAOS – Nasmyth Adaptive Optics System that is equipped with both visible and infrared sensors, and CONICA, a Near-Infrared Imager and Spectrograph.

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Looking like a bird or a cosmic Tinker Bell, the NACO images show two unmistakable galaxies that form the body and wings of “The Bird.” Astronomers were surprised with the new images that identify a third, clearly separate component that forms the head. This irregular, yet fairly massive galaxy is forming stars violently, at a rate of nearly 200 solar masses per year. It appears to be the major source of infrared luminosity in the system, even though it is the smallest of the three galaxies. The other two galaxies appear to be at a quieter stage of their interaction-induced star formation history. The object is 650 million light years distant but it is quite large with the “wings” alone extending more than 100,000 light-years, or the size of our own Milky Way.

Subsequent optical spectroscopy with the new Southern African Large Telescope, and archive mid-infrared data from the NASA Spitzer space observatory, confirmed the separate nature of the ‘head’, but also added further surprises. The ‘head’ and major parts of the ‘Bird’ are moving apart at more than 400 km/s (1.4 million km/h). Observing such high velocities is very rare in merging galaxies.

“The Bird” belongs to the prestigious family of luminous infrared galaxies, with an infrared luminosity nearly one thousand billion times that of the Sun. This family of galaxies has long been thought to signpost important events in galaxy evolution, such as mergers of galaxies, which in turn trigger bursts of star formation, and may eventually lead to the formation of a single elliptical galaxy.

The galaxy is also designated as IRAS 19115-2124. The ESO is more formally known as the European Organization for Astronomical Research in the Southern Hemisphere.

Original News Source: ESO Press Release:

What’s Up this Week: December 24 – December 31, 2007

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Please note that this is going to be the last edition of the What’s Up series of articles on Universe Today. From here on out, Tammy’s daily skywatching guide will be published in a book called the Night Sky Companion. Tammy is still writing for Universe Today, and will be posting articles about skywatching and events on a regular basis.

Monday, December 24 – Twas the night before Christmas in a sky filled with stars… And low on the horizon are the Yule Moon and Mars! That’s right. It’s the Full Yule Moon, and arriving at the same time Mars reaches opposition. For many viewers, the spectacular pair will rise with Mars less than a degree south of Luna… But a pairing this close means a few lucky observers could be in for an occultation event! Be sure to check IOTA for possible times and locations.

Today in 1968, Apollo 8 became the first manned spacecraft to orbit the Moon. Let’s celebrate that by having a look at the lunar surface. On the eastern limb we see the bright splash ray patterns surrounding ancient Furnerius – yet the rays themselves emanate from much younger crater Furnerius A. All over the surface, we see small points light up and the testament to the Moon’s violent past written in its scarred lines. Take a look now at the western limb… For the sunrise is about to advance around it.

Until this date, no man had seen with his own eyes what lay beyond. Frank Borman, James Lovell and William Anders were to become the first to directly view the “dark side” and the first to witness earthrise over the Moon. As the days ahead bring the terminator around to the eastern limb, let your mind take flight to the distant orb and enjoy its landscape as the shadows take on new angles and old features become new again.

“And from the crew of Apollo 8, we close, with good night, good luck, a Merry Christmas, and God bless all of you, all of you on the good Earth.” (Astronaut Frank Borman)

Tuesday, December 25 – Wishing you all the very best for the Christmas season! Like a present, Sir Isaac Newton was born on this day 1642 – Newton was the British “inventor” of calculus and a huge amount of what we now consider modern classical physics. Even young children are aware of his simple laws of motion and gravity. It wasn’t until the time of Einstein until things changed!

In keeping with the season, tonight’s astronomical object is a celebration of both starlight and asterism. Located 10 degrees east of Betelgeuse (RA 06 41 00.00 Dec +09 53 -0.0), NGC 2264 will be a challenging object thanks to the Moon. Also known as the “Christmas Tree Cluster,” this bright asterism of approximately 20 bright stars and over 100 fainter ones is embroiled in a faint nebula that will be lost to bright skies, leaving only the delightful Christmas tree shape adorned with stars.

The very brightest of these stars, S Monocerotis, is 5th magnitude and will show clearly in the finderscope, and will be seen as a double at magnification. Steady skies will reveal that the “star” at the top of our “tree” is also a visual double. Many of the stars will also appear to have companions, as well as tints of silver as gold. The visual effect of this splendid open cluster is well worth the challenge it presents. Happy Holidays!

Wednesday, December 26 – Is it gone yet? Nope. The Moon will rise a little later this evening, but we’re going to run ahead of it tonight and enjoy some studies in Auriga! Looking roughly like a pentagon in shape, start by identifying the brightest of these stars – Capella. Due south of it is the second brightest star, El Nath. By aiming binoculars at El Nath, go north about one-third the distance between the two and enjoy all the stars!

You will note two very conspicuous clusters of stars in this area, and so did Le Gentil in 1749. Binoculars will reveal the pair in the same field, as will telescopes using lowest power. The dimmest of these is M38, and it will appear vaguely cruciform in shape. At roughly 4200 light-years away, larger aperture will be needed to resolve the 100 or so fainter members. About two and a half degrees to the southeast you will see the much brighter M36. More easily resolved in binoculars and small scopes, this “jewel box” galactic cluster is quite young – and about 100 light-years closer!

Thursday, December 27 – Born today in 1571 was Johannes Kepler – Danish astronomer and assistant to Tycho Brahe. Kepler used Brahe’s copious notes of Mars’ positions to help formulate his three laws of planetary motion. These laws are still in use today.

Is it gone yet? No. The Moon will be along shortly, but we still have time to set our sights about halfway between Theta Aurigae and El Nath. Our study object will be the open cluster M37. Apparently discovered by Messier himself in 1764, this galactic cluster will appear almost nebula-like to binoculars and very small telescopes – but comes to perfect resolution with larger instruments.

At around 4700 light-years away, and spanning a massive 25 light-years, M37 is often billed as the finest of the three Aurigan opens for bigger scopes. Offering beautiful resolvability, this one contains around 150 members down to magnitude 12, and has a total population in excess of 500.

What makes it unique? As you view, you will note the presence of several red giants. For the most part, open clusters are comprised of stars that are all about the same age, but the brightest star in M37 appears orange in color and not blue! So what exactly is going on in here? Apparently some of these big, bright stars have evolved much faster – consuming their fuel at an incredible rate. Other stars in this cluster are still quite young on a cosmic scale, yet they all left the “nursery” at the same time! In theory, this allows us to judge the relative age of open clusters. For example, M36 is around 30 million years old and M38 about 40, but the presence of the red giants in M37 puts its estimated age at 150 million years! Just awesome…

Friday, December 28 – Today we celebrate the birth of Arthur S. Eddington. Born in 1882, Eddington was a British theoretical astrophysicist whose work was fundamental to interpreting and explaining stellar nature. He also coined the phrase “expanding universe” to refer to the mutual recession of the galaxies.

Is it gone yet? Not yet… But before the Moon rises tonight, let’s enjoy the early dark skies and go to our maps west of M36 and M38 to identify AE Aurigae. As an unusual variable, AE is normally around 6th magnitude and resides approximately 1600 light-years distant. The beauty in this region is not particularly the star itself but the faint nebula in which it resides. Known as IC 405, this is an area of mostly dust and very little gas. What makes this view so entertaining is that we are looking at a “runaway” star.

It is believed that AE originated in the M42 region in Orion. Cruising along at a very respectable speed of 130 kilometers per second, AE flew the “stellar nest” some 2.7 million years ago! Although IC 405 is not directly related to AE, there is evidence within the nebula that areas have been cleared of their dust by the rapid northward motion of the star. AE’s hot, blue illumination and high energy photons fuel what little gas is contained within the region, and its light reflects off the surrounding dust as well. Although we cannot “see” with our eyes like a photograph, together this pair makes an outstanding view for the small backyard telescope, and it is known as “The Flaming Star.”

And when the Moon rises? Look for Regulus less than one half degree to its north and Saturn another two degrees further. This could be an occultation of Regulus, so be sure to check IOTA!

Saturday, December 29 – If you’re up before dawn this morning, take the time to step outside and view the simple beauty of the ecliptic plane. To the west, Mars hangs just above the horizon with Saturn not far above it. The Moon dances high overhead and Venus shines just before the rising Sun. In a matter of weeks, Jupiter will return again to the morning skies!

Is it gone yet? Not yet. Since the Moon won’t begin to interfere for quite a while after the skies turn dark, this would be a great opportunity to locate an easy Messier object – M34. If you remember our previous study stars Almach and Algol, you’re halfway there. Draw an imaginary line between them and look with your binoculars or finder scope just a shade north of center.

In binoculars, M34 will show around a dozen fainter stars clustered together, and perhaps a dozen more scattered around the field. Small telescopes at low power will appreciate M34 for its resolvability and the distinctive orange star in the center. Larger aperture scopes will need to stay at lowest power to appreciate the 18 light-year span of this 100 million year old cluster, but take the time to power up and study. You will find many challenging doubles inside!

Sunday, December 30 – Is it gone yet? Not quite! The Moon will be along much later, but not before we’ve had an opportunity to head for another northern gem, M76.

Located in western Perseus just slightly less than one degree north-northwest of Phi, M76 is often referred to as “The Little Dumbbell.” Originally discovered by Messier’s assistant MÈchain in September of 1780, Charles didn’t get around to cataloging it for another six weeks. What a shame it took him so long to view this fine planetary nebula! Its central star is one of the hottest known, but its resemblance to M27 is what makes it so fascinating.

Looking very much like a miniaturization of the much larger M27, M76 is rather faint at magnitude 11, but is quite achievable in scopes of 114mm in aperture or larger. It is small, but its irregular shape makes this planetary nebula a real “class act!”

For our Southern Hemisphere friends, get thee out there and view Eta Carinae! First recorded by Halley in 1677, this nebular variable star left even the great Sir John Herschel at a loss to describe its true beauty and complexities. This “slow nova” is filled with all the wonders that we “northerners” can only dream about…

Monday, December 31 – Today is the birthday of Robert G. Aitken. Born in 1864, Aitken was a prolific American observer who discovered and catalogued more than 3100 double and binary stars. Just look at what a prolific observer YOU have become in just a year!

Is it gone yet? No. The Moon will be around much later tonight, but the year 2007 is just about ended. Try celebrating in a unique and inspiring way! Go observing…

In the hours before midnight, you could take a cosmic journey that spans millions of light-years. In the northern hemisphere, visit with the Andromeda Galaxy again – or the Small and Large Magellanic Clouds if you live in the South. Feast your eyes on vast and wondrous displays of stars like the “Double Cluster” in Perseus, or the “Jewel Box” – the Kappa Crucis star cluster. Rejoice in the birth of new stars by voyaging to M42 – the Orion Nebula… And remember the old by returning to M1 – the Crab Nebula. Take delight in the movements of our own solar system by watching Mars rise, or peeking in on Saturn’s rings as it follows behind. Perhaps the ISS will make a pass over your area tonight, or maybe only a single star will shine through your cloudy sky. It may be something as spectacular as watching a meteor go down in a blaze of glory, or as quiet and contemplative as watching the Moon rise as the year ends.

Now take a moment to look up at the stars and think about all the billions of years that they have been in the making and all the time that it has taken for the light to reach us. Salute! Our observing year has been wonderful together… And I’ll look for you under the stars! I hope you’ll join me again when 2008 begins as “The Night Sky Companion.”

May all your journeys be at light speed!

Magnetic “Ropes” Connect the Northern Lights to the Solar Wind

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This discovery comes just in time to light up Christmas: new observations of the Northern Lights – a spectacular phenomenon that lights up the night sky – show them to be more intricate than previously thought.

The Northern Lights were observed by NASA’s Time History of Events and Macroscale Interactions during Substorms (THEMIS), a system of ground cameras and five orbiting micro-satellites that work in combination to observe the phenomenon better than with a single satellite. This allowed scientists to map and understand the mechanisms of the Northern Lights better than before by giving them a 3D picture of the events.

The Northern Lights or “Aurora Borealis” occur when charged particles coming from the Sun interact with the Earth’s magnetic field. THEMIS found evidence that there are magnetic “ropes” — long, wound magnetic field lines that resemble the braids of a rope – connecting the Earth’s magnetic field with the solar wind. Particles are channeled through these ropes, which last a short time, and are focused in certain regions, boosting the energy of the Aurora Borealis.

“THEMIS encountered its first magnetic rope on May 20,” said David Sibeck, project scientist for the mission at NASA’s Goddard Space Flight Center in Greenbelt, MD. “It was very large, about as wide as Earth, and located approximately 40,000 miles (70,000 km) above Earth’s surface in a region called the magnetopause.”

The magnetopause is where the Earth’s magnetic field meets the solar wind.

Electromagnetic explosions were also observed by THEMIS at the bow shock of the Earth’s magnetic field. The bow shock is where the magnetosphere bunches up as the Earth travels through space, kind of like how the waves in the front of a boat moving through the water are closer together than those behind the boat.

Sibeck said of the explosions,”It is where the solar wind first feels the effects of Earth’s magnetic field. Sometimes a burst of electrical current within the solar wind will hit the bow shock and – Bang! We get an explosion.”

The results were presented at the meeting of the American Geophysical Union in San Francisco this month. THEMIS will continue to observe the Aurora Borealis over the next two years, taking measurements of ions, electrons and electromagnetic radiation in space. Scientists from the US, Canada, Western Europe, Russia and Japan are contributing to the study of Earth’s own Christmas lights.

Original Source: NASA Press Release

How Long is a Day on Saturn?

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If you were on the surface of Saturn, how long would a day last? This has remained a mystery for scientists, because the thick clouds of gas obscure the surface of the planet from direct observation by telescopes or orbiters. Below all those clouds there is a surface that rotates at a constant speed. Since scientists can’t directly see the surface, they’ve taken another approach: listening.

You can also check out these cool telescopes that will help you see the beauty of planet Saturn.

With the help of radio emissions that come from the interior of Saturn, scientists have been able to close in on its rotation period. Charged particles trapped in the interior emit radio waves when they interact with Saturn’s magnetic field, at about 100 Kilohertz. It’s as if Saturn had its own radio station broadcasting at a certain frequency, and as the magnetic field deep inside the planet rotates it changes the frequency of the station.

Voyager measured these emissions for nine months when it passed by in the 1980s, and the rotation was calculated to be 10 hours 39 minutes 24 seconds, with an uncertainty of 7 seconds. The Ulysses spacecraft also monitored the emissions 15 years later, and came up with a result of 10 hours 45 minutes 45 seconds, with a 36 second margin of error.

Wait, that’s 6 minutes of difference! Either Saturn slowed down a lot over the years, or something else is going on. Cassini has been measuring these same radio emissions with its Radio and Plasma Wave Science instrument, and has observed that in addition to this long-period variation, the rotation differs by as much as one percent in a week.

Scientists think that this could be due to two different things: the solar wind coming from the Sun is interfering with the measurements, or particles from Enceladus’ geysers are affecting the magnetic field. Both of these would cause the radio emissions to vary, and they could be causing the different results simultaneously.

Cassini’s new data strongly suggests that the solar wind is a likely culprit: there is a variation in the measurements of the short-period rotation every 25 days, which corresponds with the rotation of the Sun as seen from Saturn. The speed of the solar wind, too, varies the measurements, so must be accounted for. Enceladus could be the cause of the long-term difference, but more measurements are needed to see if this is definitely the case, or if there is yet another factor.

Nailing down the rotation of Saturn will be helpful in calculating the true wind speeds of the clouds, and give important clues about the composition and distribution of the interior. Once the interference from the solar wind and Enceladus are taken into account, the true rotation of Saturn can be determined precisely.

Then only one question remains: do they have commercials on Saturn FM?

Source: ESA News Release

Hinode Discovers the Sun’s Hidden Sparkle

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Blinking spots of intense light are being observed all over the lower atmosphere of the Sun. Not just in the active regions, but in polar regions, quiet regions, sunspots, coronal holes and loops. These small explosions fire elegant jets of hot solar matter into space, generating X-rays as they go. Although X-ray jets are known to have existed for many years, the Japanese Hinode observatory is seeing these small flares with unprecedented clarity, showing us that X-ray jets may yet hold the answers to some of the most puzzling questions about the Sun and its hot corona.

Although a comparatively small mission (weighing 875 kg and operating just three instruments), Hinode is showing the world some stunning high resolution pictures of our nearest star. In Earth orbit and kitted out with an optical telescope (the Solar Optical Telescope, SOT), Extreme ultraviolet Imaging Spectrometer (EIS) and an X-Ray Telescope (XRT), the light emitted from the Sun can be split into its component optical, ultraviolet and X-ray wavelengths. This in itself is not new, but never before has mankind been able to view the Sun in such detail.

It is widely believed that the violent, churning solar surface may be the root cause of accelerating the solar wind (blasting hot solar particles into space at a mind-blowing 1.6 million kilometers per hour) and heating the million plus degree solar atmosphere. But the small-scale processes close to the Sun driving the whole system are only just beginning to come into focus.

Up until now, small-scale turbulent processes have been impossible to observe. Generally, any feature below 1000 km in size has remained undetected. Much like trying to follow a golf ball in flight from 200 meters away, it is very difficult (try it!). Compare this with Hinode, the same golf ball can be resolved by the SOT instrument from nearly 2000 km away. That’s one powerful telescope!

The limit of observable solar features has now been lifted. The SOT can resolve the fine structure of the solar surface to 180 km, this is an obvious improvement. Also, the EIS and XRT can capture images very quickly, one per second. The SOT can produce hi-res pictures every 5 minutes. Therefore, fast, explosive events such as flares can be tracked easier.

Putting this new technology to the test, a team led by Jonathan Cirtain, a solar physicist at NASA’s Marshall Space Flight Center, Huntsville, Alabama, has unveiled new results from research with the XRT instrument. X-ray jets in the highly dynamic chromosphere and lower corona appear to occur with greater regularity than previously thought.

X-ray jets are very important to solar physicists. As magnetic field lines are forced together, snap, and form new configurations, vast quantities of heat and light are generated in the form of a “microflare”. Although these are small events on a solar scale, they still generate huge amounts of energy, heating solar plasma to over 2 million Kelvin, create spurts of X-ray emitting plasma jets and generate waves. This is all very interesting, but why are jets so important?

The solar atmosphere (or corona) is hot. In fact, very hot. Actually, it is too hot. What I’m trying to say is that measurements of coronal particles tell us the atmosphere of the Sun is actually hotter than the Suns surface. Traditional thinking would suggest that this is wrong; all sorts of physical laws would be violated. The air around a light bulb isn’t hotter than the bulb itself, the heat from an object will decrease the further away you measure the temperature (obvious really). If you’re cold, you don’t move away from the fire, you get closer to it!

The Sun is different. Through interactions near the surface of the Sun between plasma and magnetic flux (a field known as “magnetohydrodynamics” – magneto = magnetic, hydro = fluid, dynamics = motion: “magnetic-fluid-motion” in plain English, or “MHD” for short), MHD waves are able to propagate and heat up the plasma. The MHD waves under scrutiny are known as “Alfvén wavesâ€? (named after Hannes Alfvén, 1908-1995, the plasma physics supremo) which, theoretically, carry enough energy from the Sun to heat the solar corona hotter than the solar surface. The one thing that has dogged the solar community for the last half a century is: how are Alfvén waves produced? Solar flares have always been a candidate as a source, but observation suggested that there wasn’t enough flares to generate enough waves. But now, with advanced optics used by Hinode, many small-scale events appear to be common… bringing us back to our X-ray jets…

Previously, only the largest X-ray jets have been observed, putting this phenomenon at the bottom of the priority list. NASA’s Marshall Space Flight Center group has now turned this idea on its head by observing hundreds of jet events each and every day:

“We now see that jets happen all the time, as often as 240 times a day. They appear at all latitudes, within coronal holes, inside sunspot groups, out in the middle of nowhere–in short, wherever we look on the sun we find these jets. They are a major form of solar activity” – Jonathan Cirtain, Marshall Space Flight Center.

So, this little solar probe has very quickly changed our views on solar physics. Launched on September 23, 2006, by a consortium of countries including Japan, USA and Europe, Hinode has already revolutionized our thinking about how the Sun works. Not only looking deep into the chaotic processes in the solar chromosphere, it is also finding new sources where Alfvén waves may be generated. Jets are now confirmed as common events that occur all over the Sun. Could they provide the corona with enough Alfvén waves to heat the Sun’s corona more than the Sun itself? I don’t know. But what I do know is, the sight of solar jets flashing to life in these movies is awesome, especially as you see the jet launch into space from the original flash. This is also a very good time to be seeing this amazing phenomenon, as Jonathan Cirtain points out the site of solar jets reminds him of “the twinkle of Christmas lights, randomly oriented. It’s very pretty”. Even the Sun is getting festive.

MIT Shoots For the Moon

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The Moon is a pretty popular destination these days: Google’s X-Prize is already getting applicants, Kaguya and Chang’e-1 are currently snapping pictures and taking measurements, and both India and the U.S. have missions lined up to launch in the next 10 years or so. MIT announced last week that it would join in on the fun, designing a spacecraft to study the Moon, schedule for launch in 2011.

In cooperation with NASA, MIT head a up a mission to send two satellites to simultaneously study the gravity field of the Moon in detail. Named GRAIL (Gravity Recovery and Interior Laboratory), the mission will study the gravity of the Moon to shed light on its thermal history and composition. By using two satellites to do so, GRAIL will create a map of the Moon’s gravity field that is 1,000 times more accurate than previous maps.

“After the three-month mission is completed, we will know the lunar gravitational field better than we know Earth’s,” said Maria Zuber, head of MIT’s Department of Earth, Atmospheric and Planetary Sciences, who will lead the mission.

GRAIL will use a similar method employed by GRACE (Gravity Recovery and Climate Experiment), a mission that has been mapping Earth’s gravitational field since 2002: two satellites constantly measure the distance between each other with great accuracy, thus creating a map as they orbit the Earth and travel through its gravity field.

GRACE uses GPS technology for the positioning of the satellites, something impossible to do on the Moon. Instead, the GRAIL satellites will precisely monitor radio signals coming from the Earth. This technology could also be used in future missions to other planets such as Mars and Venus.

Knowing the interior composition and history of the Moon will allow scientists to have a better understanding of the history of other planets in our Solar System. The evolution of the Moon, and the history of its many impact craters will help to create models for its formation, which serves as a record of planetary formation in the inner planets. Any future missions to land on the Moon could also benefit from extended mapping of the gravity field, as landers could use this data to prevent crashes and help navigate to the surface.

The mission will cost an estimated $375 million. The satellites will be constructed by Lockheed Martin Space Systems in Denver, Colo. and NASA’s Jet Propulsion Laboratory will develop the communication and navigation systems.

Original Source: MIT Press Release

2009 Will Be the International Year of Astronomy

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Finally, astronomy is going to get the respect it deserves. The United Nations announced today that 2009 will be the International Year of Astronomy. There’ll be a concerted effort around the world to increase awareness about astronomy, and give people access to tools, techniques and knowledge.

The year coincides with 400 years since Galileo Galilei first pointed his telescope towards the heavens. He then went on to discover mountains and craters on the Moon, and the four major moons of Jupiter.

There are going to be many many events during the International Year of Astronomy. In fact, my Astronomy Cast co-host, Dr. Pamela Gay, is going to be the New Media Chair, and help administrate the IYA 2009 website. Apparently I’ve also been volunteered for several projects – I’ll keep you posted as the details are revealed to me.

You can access the International Year of Astronomy 2009 website here.

Original Source; IAU Press Release

Maybe Sulfur Dioxide, Not Carbon Dioxide, Kept Mars Warm

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Try to walk on Mars today, and the planet will simultaneously freeze and suffocate you. Not to mention the minimal air pressure and relentless radiation from space. But billions of years ago, the Red Planet was much warmer and liquid water flowed on its surface. Warm temperatures on Earth are maintained by the carbon cycle, but maybe another greenhouse gas – sulfur dioxide (SO2) – maintained the temperatures on Mars.

This is the hypothesis put forward by Harvard and MIT researchers, published in the December 21st edition of the journal Science.

Over millions of years on Earth, our climate has been controlled by the carbon cycle. Carbon dioxide is released from volcanoes, and then chemical reactions with silicate rocks on the Earth’s surface remove it back out of the atmosphere and turn it into limestone.

There are vast deposits of limestone on Earth; evidence that the carbon cycle has been going on for eons. But planetary geologists haven’t found any limestone on Mars. If the planet was kept warm, the limestone should be there.

Perhaps another greenhouse gas, sulfur dioxide – also released in vast quantities from volcanoes – kept the atmosphere warm. On Earth, sulfur dioxide is removed quickly from the atmosphere, since it’s even more reactive with silicate rocks than carbon dioxide.

“The sulfur dioxide would essentially preempt the role of carbon dioxide in surface weathering reactions,” says Itay Halevy, the first author of the report. “The presence of even a small amount of sulfur dioxide in the atmosphere would contribute to the warmer climate, and also prevent limestone deposits from forming.”

So if this is true, sulfur minerals, and not limestone, should have formed in bodies of water. This may help to explain the surprising discovery the rovers have made that sulfur minerals are an abundant component of Martian soils.

With sulfur dioxide, the Martian oceans would have been much more acidic than Earth’s oceans. There might have been periods on Earth when our atmosphere was similar, and there could be similar periods when sulfur kept us warm too.

The similarities and differences of the two planets still have much to teach scientists.

Original Source: Harvard News Release

Carnival of Space #34

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The 34th Carnival of Space has been posted to Rainer Gerhards’ Spaceflight blog. There are not one, but two lists of the top space photos in 2007. Enjoy galactic death rays, gravity suits for children, and scramjet research.

And if you’re interested in looking back, here’s an archive to all the past carnivals of space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, let me know if you can be a host, and I’ll schedule you into the calendar.