The space shuttle program has now come to an end and most of us are feeling a bit nostalgic. Want to look back over the past 30 years? This video does just that, showing all the shuttle missions in chronological order in just over 8 minutes. It’s a moving look at the missions, the people, and the shuttles themselves.
Huge Reservoir of Water Discovered in Space 30 Billion Trillion Miles Away
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From a Caltech Press Release:
Water really is everywhere. Two teams of astronomers, each led by scientists at the California Institute of Technology (Caltech), have discovered the largest and farthest reservoir of water ever detected in the universe. Looking from a distance of 30 billion trillion miles away into a quasar—one of the brightest and most violent objects in the cosmos—the researchers have found a mass of water vapor that’s at least 140 trillion times that of all the water in the world’s oceans combined, and 100,000 times more massive than the sun.
Because the quasar is so far away, its light has taken 12 billion years to reach Earth. The observations therefore reveal a time when the universe was just 1.6 billion years old. “The environment around this quasar is unique in that it’s producing this huge mass of water,” says Matt Bradford, a scientist at NASA’s Jet Propulsion Laboratory (JPL), and a visiting associate at Caltech. “It’s another demonstration that water is pervasive throughout the universe, even at the very earliest times.” Bradford leads one of two international teams of astronomers that have described their quasar findings in separate papers that have been accepted for publication in the Astrophysical Journal Letters.
Read Bradford & team’s paper here.
A quasar is powered by an enormous black hole that is steadily consuming a surrounding disk of gas and dust; as it eats, the quasar spews out huge amounts of energy. Both groups of astronomers studied a particular quasar called APM 08279+5255, which harbors a black hole 20 billion times more massive than the sun and produces as much energy as a thousand trillion suns.
Since astronomers expected water vapor to be present even in the early universe, the discovery of water is not itself a surprise, Bradford says. There’s water vapor in the Milky Way, although the total amount is 4,000 times less massive than in the quasar, as most of the Milky Way’s water is frozen in the form of ice.
Nevertheless, water vapor is an important trace gas that reveals the nature of the quasar. In this particular quasar, the water vapor is distributed around the black hole in a gaseous region spanning hundreds of light-years (a light-year is about six trillion miles), and its presence indicates that the gas is unusually warm and dense by astronomical standards. Although the gas is a chilly –53 degrees Celsius (–63 degrees Fahrenheit) and is 300 trillion times less dense than Earth’s atmosphere, it’s still five times hotter and 10 to 100 times denser than what’s typical in galaxies like the Milky Way.
The water vapor is just one of many kinds of gas that surround the quasar, and its presence indicates that the quasar is bathing the gas in both X-rays and infrared radiation. The interaction between the radiation and water vapor reveals properties of the gas and how the quasar influences it. For example, analyzing the water vapor shows how the radiation heats the rest of the gas. Furthermore, measurements of the water vapor and of other molecules, such as carbon monoxide, suggest that there is enough gas to feed the black hole until it grows to about six times its size. Whether this will happen is not clear, the astronomers say, since some of the gas may end up condensing into stars or may be ejected from the quasar.
Bradford’s team made their observations starting in 2008, using an instrument called Z-Spec at the Caltech Submillimeter Observatory (CSO), a 10-meter telescope near the summit of Mauna Kea in Hawaii. Z-Spec is an extremely sensitive spectrograph, requiring temperatures cooled to within 0.06 degrees Celsius above absolute zero. The instrument measures light in a region of the electromagnetic spectrum called the millimeter band, which lies between infrared and microwave wavelengths. The researchers’ discovery of water was possible only because Z-Spec’s spectral coverage is 10 times larger than that of previous spectrometers operating at these wavelengths. The astronomers made follow-up observations with the Combined Array for Research in Millimeter-Wave Astronomy (CARMA), an array of radio dishes in the Inyo Mountains of Southern California.
This discovery highlights the benefits of observing in the millimeter and submillimeter wavelengths, the astronomers say. The field has developed rapidly over the last two to three decades, and to reach the full potential of this line of research, the astronomers—including the study authors—are now designing CCAT, a 25-meter telescope to be built in the Atacama Desert in Chile. CCAT will allow astronomers to discover some of the earliest galaxies in the universe. By measuring the presence of water and other important trace gases, astronomers can study the composition of these primordial galaxies.
The second group, led by Dariusz Lis, senior research associate in physics at Caltech and deputy director of the CSO, used the Plateau de Bure Interferometer in the French Alps to find water. In 2010, Lis’s team was looking for traces of hydrogen fluoride in the spectrum of APM 08279+5255, but serendipitously detected a signal in the quasar’s spectrum that indicated the presence of water. The signal was at a frequency corresponding to radiation that is emitted when water transitions from a higher energy state to a lower one. While Lis’s team found just one signal at a single frequency, the wide bandwidth of Z-Spec enabled Bradford and his colleagues to discover water emission at many frequencies. These multiple water transitions allowed Bradford’s team to determine the physical characteristics of the quasar’s gas and the water’s mass.
A Space Shuttle On the Sun, One Last Time
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If you’re like me, you were probably wondering if photographer Thierry Legault would have the opportunity to photograph space shuttle Atlantis in orbit during the final mission of the shuttle program. Regular UT readers will recall that Legault has taken several amazing images of the space shuttle and International Space Station from the ground with his specialized equipment, with many spectacular views of the spacecraft transiting across the face of the Sun or the Moon. It took a mad dash across Europe, but he was successful in chasing down the shuttle, capturing it crossing the face of the Sun several times, and once — just in the nick of time (above) — just minutes before the Atlantis’ final deorbit burn.
“I went to Czech Republik, then Germany and now I’m in Netherlands, on my way back to Paris,” Legault said in a note he sent to Universe Today. “The last transit has been taken Thursday morning, just 21 minutes before the deorbit burn, therefore there are chances that is the last image of a space shuttle in orbit.”
Earlier in the mission, he was able to catch the ISS and shuttle just 50 minutes after Atlantis undocked from the station, so his images capture historic moments of the final shuttle mission.
In addition, this stunning view shows Atlantis docked to the ISS:
Legault said this solar transit of Atlantis docked to the ISS was taken on July 15th from France (Caen, Normandy). Transit duration: 0.7s. ISS distance to observer: 520 km. Speed in orbit: 7.5km/s (27000 km/h or 17000 mph).
Four images of Atlantis crossing the face of the Sun taken on July 21st 2011 at 08:27:48 UT, and combined into one image. The images were taken just 21 minutes before Atlantis’ deorbit burn, from the area of Emden, NW Germany. Transit duration: 0.9s. Distance to observer: 566 km. Speed in orbit: 7.8 km/s.
Solar transit taken on July 19th at 7:17 UT from Czech Republik (North of Praha), showing Atlantis and the ISS side by side, 50 minutes after undocking. Transit duration: 1s. ISS distance to observer: 676 km.
Many thanks to Thierry Legault for sharing his images with Universe Today, and taking us along on the ride of his travels across Europe to capture the final space shuttle mission in a way that only he can!
Hoping Forward At The End Of The Shuttle Era
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CAPE CANAVERAL Fla. — The last space shuttle mission, STS-135, ended with the landing of the shuttle Atlantis at Kennedy Space Center’s Shuttle Landing Facility at 5:57 a.m. EDT. The air was thick with both humidity and mosquitoes. It was also a day thick with loss. The United States, for the foreseeable future, has lost the ability to launch massive payloads, such as the International Space Station’s Kibo module, into orbit. Lost the capabilities that a manned spacecraft with a robot manipulator system or RMS affords. Lost the ability to chase down wayward satellites, repair them on-orbit or return them to Earth for more intensive work. Lost, at least for the time being, its leadership position in terms of space flight – that position now belongs to Russia with its human-rated Soyuz Spacecraft and unmanned Progress Cargo vessels.
NASA is working to put a positive spin on this new era. The space agency hopes that small, commercial space firms will provide the nation with the capacity to send men and material to orbit as it works to travel beyond low-Earth-orbit (LEO) once again. Only time will tell how successful this direction will be, but there are positive signs that NASA might be on the right path. Following the space program for decades – you learn to hedge your bets. Today’s SpaceX is tomorrow’s Constellation Program.
Twin sonic booms shake me out of my revelry as the shuttle announces its return home. Then, a couple minutes later, there is the roar of the approaching orbiter. This sound comes not from shuttle, but rather from the sound of air being forcibly moved out of the shuttle’s path. I had set up two mini-camcorders to capture the landing, but had decided not to take any pictures. I took a moment, for myself, to watch as the shuttle roared past and landed.
There were a number of events held later in the day to commemorate the occasion. It struck me as odd that folks, some of whom would be in the unemployment line the following day, were celebrating. I decided to skip these events – I’ll celebrate when this nation regains the ability to launch astronauts into LEO. NASA Administrator Charlie Bolden worked to reassure everyone that all was well, given that he mistakenly said that the crew of STS-134 returned today – his words were not that reassuring.
With luck, when the U.S. does return to space again, it will do so on a multitude of different craft, with a multitude of different abilities – and hopefully launch vehicles. If these spacecraft are as different from one another as Boeing’s CST-100 is from Sierra Nevada Corporation’s Dream Chaser – that will be a very good thing – it will mean that many of the capabilities lost today will be replaced, albeit on completely separate vehicles.
That said, we are now entering an undiscovered country, one that NASA has never delved into before. Near the end of Apollo, the shuttle program was approved. With the end of the shuttle program here – NASA has no established human space flight program, it has initiatives, but no umbrella program, no clear path. That said, there are some potentially amazing things on the horizon – but they exist primarily on paper or on PowerPoint. Until they are fleshed out, until they fulfill their promises – today was a day of loss. Like the shuttle program, today was a mixed bag. One filled with hope for what might come, but uncertainty with what the future holds.
These are my personal reflections on the end of the shuttle program. They do not represent the opinions of Universe Today. These thoughts come from following and covering the space program for the last two decades and are not in favor of any one group’s position. I do not work to tell people things I think they want to hear – but what I feel they need to hear. I appreciate and welcome a mature debate with respect given by all sides for everyone’s point of view.
Caught In The Web… Space Spider!
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Look, he’s crawling up my wall… Black and hairy, very small… Now he’s up above my head… Hanging by a little thread. Nope. It’s not Boris the Spider, it’s spiral galaxy IC 342 and it’s hanging out in the constellation of Camelopardalis. Thanks to NASA’s Spitzer Space Telescope, we’re able to peer through the dust clouds and sneak a peek at this arachnid appearing beastie.
Residing at an approximate distance of 10 million light-years, this impressive grand design spiral is difficult for details because it’s located directly behind the disk of the Milky Way from our point of view. Tiny particles of interstellar dust, which measure just a fraction of a micron across, approximate the blue wavelength of light. These vast areas composed of silicates, carbon, ice, and/or iron compounds dim the light in a process called extinction – but using infrared vision can even the score. Line-of-sight stars from our galaxy appear blue/white and the blue haze around the galaxy’s nucleus is from IC 342’s collective starlight. Its gangly arms glow a soft crimson and clumps of newly forming stars radiate red.
It’s small wonder the core of IC 342 appears so spooky. According to research, it has undergone a recent burst of star formation activity and is close enough to have gravitationally influenced the evolution of the local group of galaxies and the Milky Way. Can you observe Boris yourself? Absolutely. You’ll find this magnitude 9 critter located along the galactic equator at RA 03h 46m 48.5s – Dec +68 05′ 46″. But beware… Its low surface brightness means you’ll need a rich field telescope and good, dark skies.
Creepy, crawly… Creepy, crawly… Creepy, creepy, crawly, crawly…
Original News Source: JPL / Spitzer News.
Elliptical Galaxies Don’t Act Their Age…
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Thanks to images taken with the MegaCam camera mounted on the Canada-France-Hawaii Telescope (CFHT, CNRC/CNRS/University of Hawaii), researchers are beginning to see that elliptical galaxies just aren’t acting their age. Their initial studies are showing signs of recent merging – meaning that many could be as much as five times younger than previously thought.
We’ve been studying massive elliptical galaxies for a long time and their stripped down stellar population has always led astronomers to assume most were in the 7 to 10 billion year old age bracket. However, astronomers from CNRS, CEA, CFHT, and the Observatoire de Lyon – all members of the Atlas3D international collaboration – have been sneaking a peak at the galactic fountain of youth. According to observations done on two elliptical galaxies (NGC 680 & NGC 5557), it would appear they’ve undergone a spiral galaxy merger… one that’s happened as recently as 1 to 3 billion years ago.
“Such age estimate is based on the presence of ultra faint filaments in the distant outskirts of the galaxies. These features called tidal streams in the astronomers parlance are typical residuals from a galaxy merger.” says the CFH team. “They are known not to survive in this shape and brightness for more than a few billion years, hence the new age estimate of the resulting elliptical galaxies. These structures were detected for the first time thanks to a very-deep imaging technique boosting the capabilities of CFHT’s wide-field optical imager MegaCam.”
The Atlas3D team isn’t stopping with these results and they’re looking at a survey of more than one hundred elliptical galaxies close to the Milky Way. When the samples are gathered and compared, they’ll look for more faint extended features that could spell a recent merger. It could mean we need to rethink our standard model for elliptical galaxies formation!
Maybe even ask ’em for ID…
Original News Source: CFH News.
Forever Blowing Bubbles…
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Thanks to ESO’s Hidden Treasures 2010 astrophotography competition, Manu Mejias, from Argentina compiled the data to give us a view of a cosmic superbubble that staggers the imagination with its size. Spanning around around 325 by 250 light-years across, we’d never realize the true nature of this phenomenon if it wasn’t so far away.
Officially designated as LHA 120–N 44, this sprawling complex of hot gases makes its home in the Large Magellanic Cloud. Skirting its edge is young star cluster, NGC 1929, whose intense ultra-violet radiation paints the visible portrait of stellar winds in action. To give you a good idea of just how big this super-bubble really is, take a look at this awesome map from Atlas Of The Universe.
Can you conceive of a nebula so large that it stretched from Cassiopeia to Vela in one direction and far further than Ursa Major to Phoenix in the other? Like a bracelet around the arm of the Milky Way, it would be so huge we probably wouldn’t even be aware it was there. Now that’s a super superbubble!
Picture a soapy mixture being stretched to the breaking point… the massive stars embedded in the nearby clusters going supernova – creating shockwaves and expelled gases. Like the child blowing the bubble, the stellar winds continued to expel, clearing the center of material. At the perimeters, new stars are continuing to form where the gases are compressed. It’s the nature of the beast… cosmic recycling in action.
Many thanks go to Manu Mejias for taking a look at a really BIG picture!
Original Story Source: ESO Photo Release. And thanks to Richard Powell of Atlas Of The Universe.
Pan-STARRS Discovers two Super Supernovae
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Supernovae are the brightest phenomenon in the current universe. As massive stars die as supernovae, they briefly outshine the rest of the stars in their galaxy and are visible, at least once the light gets there, from across the universe. Until recently, astronomers thought they pretty much had supernovae figured out; they could either form from the direct collapse of a massive core or the tipping over the Chandrasekhar limit as a white dwarf accreted neighbor. These methods seemed to work well until astronomers began to discover “ultra-luminous” supernovae beginning with SN 2005ap. The usual suspects could not produce such bright explosions and astronomers began looking for new methods as well as new ultra-luminous supernovae to help understand these outliers. Recently, the automated sky survey Pan-STARRS netted two more.
Since 2010, the Panoramic Survey Telescope & Rapid Response System (Pan-STARR) has been conducting observations atop Mount Haleakala and is controlled by the University of Hawaii. Its primary mission is to search for objects that may pose a threat to Earth. To do this, it repeatedly scans the northern sky, looking at 10 patches per night and cycling through various color filters. While it has been very successful in this area, the observations can also be used to study objects that change on short timescales such as supernovae.
The first of the two new supernovae, PS1-10ky was already in the process of exploding as Pan-STARRS came into operation, thus, the brightness curve was incomplete since it was discovered near peak brightness and no data exists to catch it as it brightened. However, for the second, PS1-10awh, the team caught while in the process of brightening and have a complete light curve for the object. Combining the two, the team, led by Laura Chomiuk at the Harvard-Smithsonian Center for Astrophysics, was able to get a full picture of just how these titanic supernovae behave. And what’s more, since they were observed with multiple filters, the team was able to understand just how the energy was distributed. Additionally, the team was able to use other instruments, including Gemini, to get spectroscopic information.
The two new supernovae are very similar in many regards to the other ultra-luminous supernovae discovered previously, including SN 2010gx and SCP 06F6. All of these objects have been exceptionally bright with little absorption in their spectra. What little they did have was due to partially ionized carbon, silicon, and magnesium. The average peak brightness was -22.5 magnitudes where as typical core collapse supernovae peak around -19.5. The presence of these lines allowed astronomers to measure the expansion velocity for the new objects as 40,000 km/sec and place a distance to these objects as around 7 billion light years (previous ultra-luminous supernovae like these have been between 2 and 5 billion light years).
But what could power these leviathans? The team considered three scenarios. The first was radioactive decay. The violence of supernovae explosions injects atomic nuclei with additional protons and neutrons creating unstable isotopes which rapidly decay giving off visible light. This process is generally implicated in the fading out of supernovae as this decay process withers out slowly. However, based on the observations, the team concluded that it should not be possible to create sufficient amounts of the radioactive elements necessary to account for the observed brightness.
Another possibility was a rapidly rotating magnetar underwent a rapid change in its rotation. This sudden change would throw off large large chunks of material from the surface which could, in extreme cases, match the observed expansion velocity of these objects.
Lastly, the team considers a more typical supernova expanding into a relatively dense medium. In this case, the shockwave produced by the supernova would interact with the cloud around the star and the kinetic energy would heat the gas, causing it to glow. This too could reproduce many of the observed features of the supernova, but had the requirement that the star shed large amounts of material just before exploding. Some evidence is given for this as being a common occurrence in massive Luminous Blue Variable stars observed in the nearby universe. The team notes that this hypothesis may be tested by searching for radio emission as the shockwave interacted with the gas.
Amazing Image: ISS Crew Captures Shuttle Atlantis’ Last Brilliant Trip Through the Atmosphere
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Simply incredible. Atlantis on its way home taken by the Expedition 28 crew of the space station. Via the NASA_Johnson Twitpic page.
Guest Post: End of an Era: Space Shuttle Program (1981 – 2011)
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Editor’s Note: Ray Sanders from the “Dear Astronomer” website sent us his observations of the end of the space shuttle era.
When space shuttle Atlantis touched down in Florida earlier this morning, it marked the end of the Shuttle era. Soon the magnificent “flying bricks” as they are commonly nicknamed will be museum exhibits.
I’ll be able to tell my soon-to-be-born daughter about how I used to watch the shuttle launches when I was her age – much like my father told me about seeing Apollo launches when he was a kid. Having watched the first shuttle launch (I was a little young for the Enterprise rollout), seeing the Challenger explosion on live television with the rest of my 4th grade class, the launch of the Hubble Space Telescope, construction of the ISS (Originally U.S space station Freedom), the loss of Columbia and too many other missions to list, you could say I grew up with the shuttle program – those birds are very much a part of
the fabric of my life.
Being the little space dweeb that I was ( and still am?) I enjoyed launching my Estes space shuttle rocket (along with my SR-71, Saturn V and V2 models) and had just about every space-themed Lego kit known to exist. Despite the space toys and my extreme interest in space (and astronomy) as a kid, I never got a chance to go to space camp – something I’ll make sure my daughter goes to if she’s interested. My hopes are that when she’s old enough to appreciate it, there will be a form of space exploration that captivates her as much as the shuttles did during their time.
To a certain degree, I envy those a bit older than myself who were lucky to watch the lunar landings in the late 60?s and early 70?s. I write this on the 42nd anniversary of Apollo 11, when the human race first stepped on the moon. I’m sure space enthusiasts a bit older than I am were a bit dismayed about the end of Apollo and had lingering questions about whether or not the fancy new “space shuttles” would even get off the ground. Fast forward through thirty years of the shuttle program and an entirely new generation sits at the precipice, asking the very same question: “where do we go from here?”