Giant Ultraviolet Rings Found Around Ancient Galaxies

Astronomers have found unexpected rings and arcs of ultraviolet light around a selection of galaxies, four of which are shown here as viewed by NASA's and the European Space Agency's Hubble Space Telescope. Image credit: NASA/ESA /JPL-Caltech/STScI/UCLA

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Title this ‘Zombie Galaxies’ or ‘Night of the Living Galaxies.’ Astronomers have found mysterious, giant loops of ultraviolet light around old, massive galaxies, which were presumed to be “dead,” and these galaxies seem to have come back to life. Somehow these “over-the-hill galaxies” have been infused with fresh gas to form new stars that power these truly gargantuan rings, some of which could encircle several Milky Way galaxies.

The discovery of these rings implies that old bloated galaxies that were once devoid of star-making can be reignited with star birth, and that galaxy evolution does not proceed straight from the cradle to the grave.

“In a galaxy’s lifetime, it must make the transition from an active, star-forming galaxy to a quiescent galaxy that does not form stars,” said Samir Salim, lead author of a recent study and a research scientist in the department of astronomy at Indiana University, Bloomington. “But it is possible this process goes the other way, too, and that old galaxies can be rejuvenated.”

Using two orbiting observatories, NASA’s Galaxy Evolution Explorer and Hubble Space Telescope, the astronomers surveyed a vast region of the sky in ultraviolet light. GALEX picked out 30 elliptical and lens-shaped “early” galaxies with puzzlingly strong ultraviolet emissions but no signs of visible star formation, and Hubble was used to take a closer look.

What Hubble showed shocked the astronomers. Three-quarters of the galaxies were spanned by great, shining rings of ultraviolet light, with some ripples stretching 250,000 light-years. A few galaxies even had spiral-shaped ultraviolet features.

“We haven’t seen anything quite like these rings before,” said Michael Rich, co-author of the paper and a research astronomer at UCLA. “These beautiful and very unusual objects might be telling us something very important about the evolution of galaxies.”

But astronomers are unsure where the gas for this galactic resurrection came from and how it has created rings. One possibility is that a smaller galaxy merged with a big, old one, bringing in fresh gas to spawn hordes of new stars, and could in rare instances give rise to the ring structures as well.

But the researchers have their doubts about this origin scenario. “To create a density shock wave that forms rings like those we’ve seen, a small galaxy has to hit a larger galaxy pretty much straight in the center,” said Salim. “You have to have a dead-on collision, and that’s very uncommon.”

Another option that the astronomers like better is that the rejuvenating spark could have come from a gradual sopping-up of the gas in the so-called intergalactic medium, the thin soup of material between galaxies. This external gas could generate these rings, especially in the presence of bar-like structures that span some galaxies’ centers.

Ultimately, more observations will be needed to show how these galaxies began growing younger and lit up with humongous halos. Salim and Rich plan to search for more evidence of bars, as well as faint structures that might be the remnants of stellar blooms that occurred in the galaxies’ pasts. Rather like recurring seasons, it may be that galaxies stirred from winter can breed stars again and then bask in another vibrant, ultraviolet-soaked summer.

The study detailing the findings appeared in the April 21 issue of the Astrophysical Journal.

Source: JPL

Ambitious Survey Spots Stellar Nurseries

VISTA Magellanic Cloud Survey view of the Tarantula Nebula. Credit: ESO/M.-R. Cioni/VISTA Magellanic Cloud survey. Acknowledgment: Cambridge Astronomical Survey Unit

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ESO’s VISTA telescope has begun a new survey of the Magellanic Cloud, and this spectacular image of the Tarantula Nebula is a taste of great things to come from this near-infrared scan of the more interesting galaxies in our neighborhood. This panoramic near-infrared view captures the nebula itself in great detail as well as the rich surrounding area of sky. “This view is of one of the most important regions of star formation in the local Universe — the spectacular 30 Doradus star-forming region, also called the Tarantula Nebula,” said the leader of the survey team, Maria-Rosa Cioni from the University of Hertfordshire. “At its core is a large cluster of stars called RMC 136, in which some of the most massive stars known are located.”

VISTA is a new survey telescope at the Paranal Observatory in Chile, and is equipped with a huge camera that detects light in the near-infrared part of the spectrum, revealing a wealth of detail about astronomical objects that gives us insight into the inner workings of astronomical phenomena. Near-infrared light has a longer wavelength than visible light, fortunately, it can pass through much of the dust that would normally obscure the views that our eyes can see. This makes it particularly useful for studying objects such as young stars that are still enshrouded in the gas and dust clouds from which they formed. Another powerful aspect of VISTA is the large area of the sky that its camera can capture in each shot.
The VISTA Magellanic Cloud Survey is one of six huge near-infrared surveys of the southern sky that will take up most of the first five years of operations of VISTA.

This project will scan a vast area — 184 square degrees of the sky (corresponding to almost one thousand times the apparent area of the full Moon) including our neighboring galaxies the Large and Small Magellanic Clouds. The end result will be a detailed study of the star formation history and three-dimensional geometry of the Magellanic system.

“The VISTA images will allow us to extend our studies beyond the inner regions of the Tarantula into the multitude of smaller stellar nurseries nearby, which also harbor a rich population of young and massive stars,” said Chris Evans who is part of the VMC team. “Armed with the new, exquisite infrared images, we will be able to probe the cocoons in which massive stars are still forming today, while also looking at their interaction with older stars in the wider region.”

The wide-field image shows a host of different objects. The bright area above the centre is the Tarantula Nebula itself, with the RMC 136 cluster of massive stars in its core. To the left is the NGC 2100 star cluster. To the right is the tiny remnant of the supernova SN1987A (eso1032). Below the centre are a series of star-forming regions including NGC 2080 — nicknamed the “Ghost Head Nebula” — and the NGC 2083 star cluster.

See more images, zoomable images, and movies of the Tarantula Nebula at the ESO website.

WISE Cryostat is Depleting

An image released in August 2010 from WISE image of the Small Magellanic Cloud. Image credit: NASA/JPL-Caltech/WISE Team

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NASA’s Wide-field Infrared Survey Explorer, or WISE, is losing its cool. The spacecraft is running out of the frozen coolant needed to keep its heat-sensitive instrument chilled, and will only be in operation for 2-3 more months. While the spacecraft was designed to be rather short-lived – 7 to 10 months — it still is sad to see the mission winding down. But WISE has completed its primary mission, a full scan of the entire sky in infrared light, which was accomplished by July 17, 2010. The mission has taken more than 1.5 million snapshots so far, uncovering hundreds of millions of objects, including asteroids, stars and galaxies. It has discovered more than 29,000 new asteroids to date, more than 100 near-Earth objects and 15 comets.

The telescope has two coolant tanks that keep the spacecraft’s normal operating temperature at 12 Kelvin (minus 438 degrees Fahrenheit). The outer, secondary tank is now depleted, causing the temperature to increase. One of WISE’s infrared detectors, the longest-wavelength band most sensitive to heat, stopped producing useful data once the telescope warmed to 31 Kelvin (minus 404 degrees Fahrenheit). The primary tank still has a healthy supply of coolant, and data quality from the remaining infrared detectors remains high.

WISE is continuing a second survey of about one-half the sky as originally planned. It’s possible the remaining coolant will run out before that scan is finished. Scientists say the second scan will help identify new and nearby objects, as well as those that have changed in brightness. It could also help to confirm oddball objects picked up in the first scan.

NASA is hoping to find more Near Earth Objects with WISE’s remaining days of operations.
“WISE’s prime mission was to do an infrared background map,” said Lindley Johnson, program executive for the Near-Earth Objects Observation program at NASA, speaking at a workshop this week to define objectives for exploring asteroids. “But we realized in talking with scientists that it would also make a good asteroid detector by comparing images. It has done a good job of finding a lot of objects for us.”

Source: NASA

Breathtaking Galaxy Amid the Dense Coma Cluster

A majestic face-on spiral galaxy located deep within the Coma Cluster of galaxies. Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)

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The Coma Cluster is a huge, densely populated cluster, with thousands of galaxies closely bunched together. Amid the bedlam of ellipticals, lenticulars and irregulars is this majestic face-on spiral galaxy known as NGC 4911. Hubble stared long and deep to get this highly detailed image of this particular galaxy located deep within the Coma Cluster. Data from three different years and 28 hours of exposure time were combined to capture this breathtaking look at spiral arms, glowing newborn star clusters and iridescent pink clouds of hydrogen, meaning there is ongoing star formation.

The Coma Cluster lies 320 million light-years away in the northern constellation Coma Berenices. As usual for clusters like this, there are only a few young spirals galaxies, and Hubble magnificently captured one of them in all its glory, using long exposure times with the Wide Field Planetary Camera 2 and the Advanced Camera for Surveys.

Source: HubbleSite

Universe Today Welcomes Spacevidcast


You may have noticed a couple of recent posts that included videos from the great folks at Spacevidcast. Universe Today is proud to announce that Spacevidcast will now be a regular feature here on UT, so we hope you’ll enjoy all the additional content and videos you’ll see from Spacevidcast — which has the stated (and honorable!) goals of educating “the planet on the values of space flight” and to “open up the cosmos and truly make space commonplace for everyone on the planet.”

In addition to the features you’ll see on Universe Today, Spacevidcast also does daily on-demand episodes, weekly live shows and live HD coverage of major space events. So check out Spacevidcast’s site for more information. And give Benjamin and Cariann Higginbotham and their team a warm, Universe Today welcome!

Interview with Elon Musk

SpaceX founder, CEO and CTO Elon Musk sat down with the Spacevidcast team for about 20 minutes to talk about space and SpaceX. This is the 10 minute SpacePod edition which has a little under 1/2 the interview available. We chat about the Falcon X, the future of space and why he built SpaceX.

Former NASA Administrator O’Keefe in Alaska Plane Crash

Former NASA Administrator Sean O'Keefe. Credit: NASA

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Update: (2:30 pm EDT) Good news: Keith Cowing at NASA Watch reports that according to a family source both Sean O’Keefe and his son Jonathan Kevin survived the plane crash but they are both rather banged up. Unfortunately, former Sen. Stevens was killed.

Former NASA Administrator Sean O’Keefe was on board a plane believed to be carrying nine people that crashed in Southwest Alaska late Monday, August 9. Rescue crews were trying to reach the wreckage early this morning, and the National Transportation Safety Board told the Associated Press that five of the nine people aboard the plane are believed to have been killed. Former U.S. senator Ted Stevens was also believed to be on board. CNN also reported that five people were killed and two were seriously injured.

Rescue crews were trying to reach the wreckage early Tuesday, but were hampered by bad weather, the AP reported. A National Transportation Safety Board investigative team has been dispatched from Washington.

The Anchorage Daily News was the first to report that friends of Stevens, 86, think he was aboard the aircraft. The friends said Stevens had been planning to visit a lodge owned by the same telecommunications company that owned the small plane, the newspaper said. It reported that Stevens’s wife was with a longtime family friend, trying to confirm Stevens’ whereabouts.

O’Keefe, 54, was NASA’s tenth administrator and served from December 2001 to February 2005. His tenure was marked by a mix of triumph and tragedy, ranging from the tremendous success of the Mars Exploration Rovers to the Space Shuttle Columbia accident. He currently is the chief executive of defense contractor EADS North America. A spokesman for EADS said O’Keefe was a passenger on the plane, but added that no further information about O’Keefe’s status was available.

Keith Cowing at NASAWatch reported that O’Keefe’s son was with him on the plane.

The National Guard was called to the area about 20 miles north of Dillingham at about 7 p.m. Monday after a passing aircraft saw the downed plane, but severe weather has hampered search and rescue efforts.

The National Weather Service reported rain and fog at Dillingham, with low clouds and limited visibility early Tuesday.

Conditions ranged from visibility of about 10 miles reported at Dillingham shortly before 7 p.m. Monday to 3 miles, with rain and fog, reported about an hour later, according to the agency.

The aircraft is a 1957 DeHavilland DHC-3 Otter.

Reports say there were people who were on the scene — “good Samaratans” — helping the crash victims.

We’ll provide more information as it becomes available.

Historic ISS Spacewalk Unsuccessful, Astronauts To Try Again

Astronauts Wheelock and Caldwell Dyson conducted an eight hour, 3 minute-long spacewalk to replace a balky coolant pump. Credit: NASA

Expedition 24 Flight Engineers Douglas Wheelock and Tracy Caldwell Dyson battled with a balky ammonia pump on a spacewalk that lasted for eight hours and 3 minutes.  Sadly their efforts were in vain.  A line connected to the pump began leaking ammonia forcing mission managers on the ground to reevaluate the situation.  They decided to leave the pump where it is for the time being.  The coolant problem has caused the International Space Station (ISS) to run at a diminished capacity since the pump began acting up.

The spacewalk marked the sixth-longest in human spaceflight history and the longest at the space station without a space shuttle present.  For Wheelock it was his fourth spacewalk, it was Caldwell Dyson’s first.  The pair wrapped up their first attempt at 3:22 p.m. EDT.  Teams monitoring on the ground wanted to review the situation further before the next spacewalk, currently scheduled for Wednesday, Aug. 11, takes place. 

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Meanwhile all of the crew members are perfectly safe and the space station itself is operating at a normal capacity (many science experiments have been shut down to avoid overheating).  Engineers also powered down and adjusted other systems on the station to avoid any complications.  The ammonia pump failed last week and is one of two located on the space station’s S1 Truss element.

There are currently two additional spacewalks planned to address this problem.  The next one is currently scheduled to take place no-earlier than Wednesday, Aug. 11.

Carnival of Space #166

This week’s Carnival of Space is hosted by Jason Perry over at Gish Bar Times.

Click here to read the Carnival of Space #166.

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 Fraser know if you can be a host, and he’ll schedule you into the calendar.

Finally, if you run a space-related blog, please post a link to the Carnival of Space. Help us get the word out.

View From Space: Huge Piece of Glacier Breaks Off Greenland

Enormous chuck of ice breaks off the Petermann Glacier in Greenland. Credit: NASA.

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A huge ice island four times the size of Manhattan– and half as thick as the Empire State Building is tall– has broken off from one of Greenland’s two main glaciers. On August 5, 2010, an enormous chunk of ice, roughly 97 square miles (251 square kilometers) in size, broke off the Petermann Glacier, along the northwestern coast of Greenland. Satellite images, like this one from NASA’s Aqua satellite show the glacier lost about one-quarter of its 70-kilometer (40-mile) long floating ice shelf. Located a thousand kilometers south of the North Pole, the now-separate ice island contains enough fresh water to keep public tap water in the United States flowing for 120 days, said scientists from the University of Delaware who have been monitoring the break.

While thousands of icebergs detach from Greenland’s glaciers every year, the last time one this large formed was in 1962. The flow of sea water beneath Greenland’s glaciers is a main cause of ice detaching from them.

This movie made from another satellite — Envisat from the European Space Agency – shows the giant iceberg breaking off.

Time-series animation based on Envisat Advanced Synthetic Aperture Radar (ASAR) data from 31 July, 4 August, and 7 August 2010 showing the breaking of the Petermann glacier and the movement of the new iceberg towards Nares Strait. Credits: ESA

The animation above was created by combining three Advanced Synthetic Aperture Radar (ASAR) acquisitions (31 July, 4 August and 7 August 2010) taken over the same area. The breaking of the glacier tongue and the movement of the iceberg can be clearly seen in this sequence.

The Petermann glacier is one of the largest glaciers connecting the Greenland inland ice sheet with the Arctic Ocean. Upon reaching the sea, a number of these large outlet glaciers extend into the water with a floating ‘ice tongue’.
The ice tongue of the Petermann glacier was the largest in Greenland. This tide-water glacier regularly advances towards the ocean at about 1 km per year. During the previous months, satellite images revealed that several cracks had appeared on the glacier surface, suggesting to scientists that a break-up event was imminent.

Scientists say it’s hard to tell if global warming caused the event. Records on the glacier and sea water below have only been kept since 2003. The first six months of 2010 have been the hottest globally on record.

Sources: NASA, ESA