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February 12, 2014April 26, 2016 by Elizabeth Howell

Teamwork! Two Telescopes Combine Forces To Spot Distant Galaxy Clusters

Artist's impression of the Herschel Space Telescope. Credit: ESA/AOES Medialab/NASA/ESA/STScI

Doing something extraordinary often requires teamwork for humans, and the same can be said for telescopes. Witness the success of the Herschel and Planck observatories, whose data was combined in such a way to spot four galaxy clusters 10 billion years away — an era when the universe was just getting started.

Now that they have the technique down, astronomers believe they’ll be able to find about 2,000 other distant clusters that could show us more about how these collections of galaxies first came together.

Although very far away, the huge clumps of gas and dust coming together into stars is still visible, allowing telescopes to see the process in action.

“What we believe we are seeing in these distant clusters are giant elliptical galaxies in the process of being formed,” stated David Clements, a physicist at Imperial College London who led the research, referring to one of the two kinds of galaxies the universe has today. Elliptical galaxies are dominated by stars that are already formed, while spiral galaxies (like the Milky Way) include much more gas and dust.

Three false-color images of Herschel images identified by Planck. Infrared light is represented in three colors -- blue, green, and red -- that respectively show longer wavelengths. The green circle shows where Planck aimed. The co-ordinates show the location in right ascension and declination. Credit: D. Clements/ESA/NASA — Three false-color images of Herschel images identified by Planck. Infrared light is represented in three colors — blue, green, and red — that respectively show longer wavelengths. The green circle shows where Planck aimed. The co-ordinates show the location in right ascension and declination. Credit: D. Clements/ESA/NASA

This finding is yet another example of how the data from telescopes lives on, and can be used, long after the telescope missions have finished. Both Planck and Herschel finished their operations last year.

“The researchers used Planck data to find sources of far-infrared emission in areas covered by the Herschel satellite, then cross-referenced with Herschel data to look at these sources more closely,” the Royal Astronomical Society stated.

The two telescopes had complementary views, with Planck looking at the entire sky while Herschel surveyed smaller sections in higher resolution. By combining the data, researchers found 16 sources in total. A dozen of them were already discovered single galaxies, but four were the newly discovered galaxy clusters. Fresh observations were then used to figure out the distance.

You can read more details in the Monthly Notices of the Royal Astronomical Society or in preprint version on Arxiv.

Source: Royal Astronomical Society

February 10, 2014December 23, 2015 by Elizabeth Howell

How Massive Is A Neutrino? Cosmology Experiment Gives A Clue

Artist's conception of Planck, a space observatory operated by the European Space Agency, and the cosmic microwave background. Credit: ESA and the Planck Collaboration - D. Ducros

There have been a lot of attempts over the years to figure out the mass of a neutrino (a type of elementary particle). A new analysis not only comes up with a number, but also combines that with a new understanding of the universe’s evolution.

The research team investigated the mass further after observing galaxy clusters with the Planck observatory, a space telescope with the European Space Agency. As the researchers examined the cosmic microwave background (the afterglow of the Big Bang), they saw a difference between their observations and other predictions.

“We observe fewer galaxy clusters than we would expect from the Planck results and there is a weaker signal from gravitational lensing of galaxies than the CMB would suggest. A possible way of resolving this discrepancy is for neutrinos to have mass. The effect of these massive neutrinos would be to suppress the growth of dense structures that lead to the formation of clusters of galaxies,” the researchers stated.

The HST WFPC2 image of gravitational lensing in the galaxy cluster Abell 2218, indicating the presence of large amount of dark matter (credit Andrew Fruchter at STScI).

Neutrinos are a tiny piece of matter (along with other particles such as quarks and electrons). The challenge is, they’re hard to observe because they don’t react very easily to matter. Originally believed to be massless, newer particle physics experiments have shown that they do indeed have mass, but how much was not known.

There are three different flavors or types of neutrinos, and previous analysis suggested the sum was somewhere above 0.06 eV (less than a billionth of a proton’s mass.) The new result suggests it is closer to 0.320 +/- 0.081 eV, but that still has to be confirmed by further study. The researchers arrived at that by using the Planck data with “gravitational lensing observations in which images of galaxies are warped by the curvature of space-time,” they stated.

“If this result is borne out by further analysis, it not only adds significantly to our understanding of the sub-atomic world studied by particle physicists, but it would also be an important extension to the standard model of cosmology which has been developed over the last decade,” the researchers stated.

The research was done by the University of Manchester’s Richard Battye and the University of Nottingham’s Adam Moss. A paper on the work is published in Physical Review Letters and is also available in preprint version on Arxiv.

February 10, 2014December 23, 2015 by Elizabeth Howell

50 Years After Taking Over Earth, The Beatles’ Space Invasion Is Well Underway

Credit: Inside Science News Service and Amanda Page

As the Beatles strummed the opening notes to “All My Loving” on the Ed Sullivan Show 50 years ago yesterday, few could have imagined how wide-ranging that music would be. The broadcast gave birth to a global music phenomenon. And like all TV broadcasts of the day, the music carried out into space at the speed of light.

The Inside Science infographic above (see below for the full version) traces the history of the Beatles in relation to how far the broadcast travelled in that time. While those waves were washing out, er, across the universe, the Beatles have been taking over human space exploration in other ways. Below the jump are seven of the more memorable moments.

Rocking The Space Station With ‘Back at the ISS’

Technically speaking, this isn’t the Beatles, but it sure was inspired by them. ‘Back at the ISS’ — the remake of ‘Back in the U.S.S.R.’ by Dutch band Love & Mersey — is about a billion shades of awesome. Not only because of the lyrics, not only because of the high-energy space-themed video, but also because they sang in three languages. The song was released in March 2012 as a “rocking musical greeting” to Andre Kuipers (a European Space Agency astronaut) and the rest of the Expedition 30 crew days before the docking of the Automated Transfer Vehicle Edoardo Amaldi that month.

Beatles In The Sky With … Asteroids

Yup, there’s an asteroid named after the Beatles. Oh yeah, there are also asteroids named after members John Lennon, Paul McCartney, George Harrison and Ringo Starr.

Good Morning Good Morning wake-up calls

The Beatles have been used to wake up several shuttle crews, and also the Curiosity rover. Explained Eric Blood, Curiosity’s surface systems engineer: “She tends to be less cranky with a good wakeup song.”

Playing (And Drinking?) English Tea In Space

Here’s Paul McCartney in 2005 casually playing two tunes to the Expedition 12 crew — NASA astronaut Bill McArthur and Russian cosmonaut Valery Tokarev — during a live concert. It’s a bit hard to tell who had bigger stars in their eyes after the experience. “I told the audience ‘I think I need about 20 minutes to go have a lie down,’ McCartney stated in a NASA release from the time. “What do you do after that? We haven’t stopped talking about it since.”

Roll Over Beethoven: How The Beatles Almost Made Voyager’s ‘Golden Record’

Remember when scientists announced last year that Voyager 1 entered interstellar space? On board the spacecraft was a Golden Record intended to give aliens a glimpse into what Earth’s life is like. Included were songs from artists ranging from Bach to Blind Willie Johnson, but not the Beatles. They were almost included, though, as astronomer Carl Sagan (who chaired the selection committee) explained in his 1978 book Murmers of Earth. “We wanted to send ‘Here Comes The Sun’ by the Beatles, and all four Beatles gave their approval. But the Beatles did not own the copyright, and the legal status of the piece seemed too murky to risk,” he wrote.

Joining Mr. Mercury’s Light

There are so many earthly memorials to John Lennon after the singer’s untimely death in 1980, but late last year he got an extraterrestrial honor. Lennon was among 10 names approved for craters on the planet Mercury. “It’s unlikely that Mercury’s surface is populated with tangerine trees and marmalade skies, but the famous British musician who coined that phrase now has a physical presence on the planet closest to the Sun,” NASA said.

Sending Love To The Aliens With Jai Guru Deva Om

February 4, 2008 marked the first time NASA beamed any song into deep space, and what better choice than “Across The Universe”? The date marked the 40th anniversary of when the Beatles recorded the song, and came around the same time as the 45th anniversary of NASA’s Deep Space Network and the 50th anniversary of NASA’s first satellite, Explorer 1, among other milestones. In a statement, McCartney asked to “send my love to the aliens.”

What Beatles milestones in space have we missed? Let us know in the comments.

February 6, 2014December 23, 2015 by Elizabeth Howell

Milky Way-Mapping Telescope Nabs Its First Pictures In Space

The Large Magellanic Cloud is visible in this calibration image for the European Space Agency's Gaia telescope taken in 2014. Credit: ESA/DPAC/Airbus DS

From a lonely outpost in space, the European Space Agency’s Gaia telescope is getting ready to map out the Milky Way. It will take some time to calibrate the instruments to make sure they’re ready for work, however, and that’s why you’re looking at the image above.

Controllers aimed the telescope at the Large Magellanic Cloud, which is a satellite galaxy to our own Milky Way, and snapped this picture of star cluster NGC 1818.

“This test picture, taken as part of commissioning the mission to ‘fine tune’ the behaviour of the instruments, is one of the first proper ‘images’ to be seen from Gaia, but ironically, it will also be one of the last, as Gaia’s main scientific operational mode does not involve sending full images back to Earth,” ESA stated.

This is one crucial step along the road to making sure Gaia’s measurements are accurate. In the next five years, it will examine a billion stars (an astounding number, but still only 1 percent of the galaxy’s population). Gaia will build up a database of key stellar properties such as brightness, what it is made of and temperature.

For more information on Gaia, check out this past Universe Today story from its Dec. 19 launch as well as the official Gaia blog.

Source: ESA

January 18, 2014December 23, 2015 by Jason Major

Wake Up, Rosetta!

Artist's impression (not to scale) of the Rosetta orbiter deploying the Philae lander to comet 67P/Churyumov–Gerasimenko. Credit: ESA–C. Carreau/ATG medialab.

It’s being called “the most important alarm clock in the Solar System” — this Monday, January 20, at 10:00 GMT (which is 5:00 a.m. for U.S. East Coasters like me) the wake-up call will ring on ESA’s Rosetta spacecraft, bringing it out of hibernation after over two and a half years in preparation of its upcoming and highly-anticipated rendezvous with a comet.

The wake-up will incite the warming of Rosetta’s star trackers, which allow it to determine its orientation in space. Six hours later its thrusters will fire to stop its slow rotation and ensure that its solar arrays are receiving the right amount of sunlight. Using its thawed-out star trackers Rosetta will aim its transmitter towards Earth and, from 500 million miles (807 million km) away, will send a thumbs-up signal that everything is OK and it’s time to get back to work.

From that distance the transmission will take 45 minutes to reach us. Rosetta’s first signal is expected between 17:30 – 18:30 GMT (12:30 – 1:30 p.m. ET). Once we’re assured all is well, Rosetta has a very exciting year ahead!

After nearly a decade of soaring through the inner solar system, flying past Mars and Earth several times and even briefly visiting a couple of asteroids (2867 Steins on September 5, 2008 and 21 Lutetia on July 10, 2010) Rosetta is finally entering the home stretch of its mission to orbit the 4-km-wide comet 67P/Churyumov-Gerasimenko.

Once Rosetta enters orbit around the comet — the first time a spacecraft has ever done so — it will map its surface and, three months later in November, deploy the 220-lb (100-kg) Philae lander that will intimately investigate the surface of the nucleus using a suite of advanced science instruments. (Watch a video here of how all this will happen… using Legos!)

With Philae firmly attached to the comet, Rosetta will follow it around the Sun as it makes its closest pass in August 2015 and then heads back out towards the orbit of Jupiter. Rosetta will provide the most detailed observations ever of a comet’s composition and dramatic evolution as it encounters the heat and energy of our home star.

Of course, before all this can happen Rosetta first has to… WAKE UP! It entered hibernation in July 2011 and has remained silent in a slow spin ever since, with only its computer and some heaters kept running. Waking up from a 31-month nap can’t be easy, so ESA is inviting people around the world to help Wake Up Rosetta (and possibly even win a trip to Germany for the landing in November) by sharing their short movies of how best to awaken a sleeping spacecraft and sharing them to the contest page on Facebook or to Twitter, Vine, or Instagram with the #WakeUpRosetta hashtag.

See more about the contest below:

Video submissions to the Wake Up Rosetta video contest will be accepted until 17:30 GMT on Monday so if you haven’t already, get your cameras out and your imaginations going… this spacecraft isn’t going to wake itself! (Well, actually it kinda is but you can still show off your creativity!)

And even if you don’t send in a video, you can watch the live feed of Monday’s events from ESA starting at 09:15 GMT (4:15 a.m. ET) here and here. (Also follow @ESA_Rosetta on Twitter — currently it’s “still sleeping.”)

Want to find out where Rosetta is right now? Check out this cool interactive map from Daniel Scuka, Senior Editor of Spacecraft Operations at ESOC.

Rosetta launched on March 2, 2004 by an Ariane-5 G+ from Europe’s spaceport in Kourou, French Guiana. Read more on the mission page and the Rosetta blog here.

___________

UPDATE Jan. 20: Rosetta has awoken! This afternoon at 18:18 UTC, after 48 minutes of increasingly tense anticipation, a signal from the spacecraft was received by both NASA’s Deep Space Network in Goldstone, CA and the ground station in Canberra, Australia. Rosetta is up and running and so far seems to be in good condition — Go Rosetta and Philae! Read the full story here.

January 13, 2014December 30, 2015 by Jason Major

Watch Gaia Go From Lab to Launch in Two Minutes

In the early pre-dawn hours on December 19, 2013, with a rumble and a roar, a Soyuz rocket blazed through the clouds above the jungle-lined coast of French Guiana, ferrying ESA’s long-awaited Gaia spacecraft into orbit and beginning its mission to map the stars of the Milky Way. The fascinating time-lapse video above from ESA shows the Gaia spacecraft inside the clean room unfurling like a flower during its sunshield deployment test, the transfer of the Soyuz from the assembly building to the pad, and then its ultimate fiery liftoff.

That’s a lot going on in two minutes! But once nestled safely in its L2 orbit 1.5 million kilometers out, Gaia will have over five years to complete its work… read more here.

Credit: ESA–S. Corvaja, M. Pedoussaut, 2013. Source: ESA

December 30, 2013December 23, 2015 by Elizabeth Howell

Spider-Like Spacecraft Aims To Touch A Comet Next Year After Rosetta Reactivates

Artist's impression of Philae, the lander from the Rosetta spacecraft, descending to the surface of Comet 67P/Churyumov–Gerasimenko in November 2014. Credit: ESA–J. Huart, 2013

Watch out, you comet, Rosetta is on its way with a probe. The European Space Agency spacecraft is preparing to wake up in January from a nearly three-year-long hibernation period to ready for a close encounter with Comet 67P/Churyumov–Gerasimenko.

If all goes well, Rosetta should reach its destination in August and — after a couple of months in a mapping orbit — comes another exciting bit: the probe will deploy a spider-like lander called Philae on the surface in November. That will be the first time anything has soft-landed on a comet.

Philae has a ream of scientific instruments on board, most notably a drill that can penetrate as far as 20 centimeters (eight inches) into whatever lies below it. It can then pick up the samples and analyze them right on sight. This will allow the lander to learn more about what the comet’s surface and subsurface are made of, ESA says, and to figure out how its nucleus is constructed. (You can read more technical details here.)

A big concern, of course, is keeping Philae anchored on the low gravity of the comet (as was covered extensively in this past Universe Today story).

“As Philae touches down on the comet, two harpoons will anchor it to the surface; the self-adjusting landing gear will ensure that it stays upright, even on a slope, and then the lander’s feet will drill into the ground to secure it to the comet’s surface in the low gravity environment,” ESA wrote.

Artist's impression of the Rosetta spacecraft releasing its lander, Philae, above the surface of Comet 67P/Churyumov–Gerasimenko in November 2014. Credit: ESA–C. Carreau/ATG medialab — Artist’s impression of the Rosetta spacecraft releasing its lander, Philae, above the surface of Comet 67P/Churyumov–Gerasimenko in November 2014. Credit: ESA–C. Carreau/ATG medialab

But first comes Rosetta’s reactivation. ESA is so excited about this forthcoming milestone on Jan. 20 that it’s inviting the public to send in videos where people tell the spacecraft, essentially, to wake up after 31 months of hibernation. (The campaign is called “Wake Up, Rosetta”, and more contest details are here.)

What’s cute is that the official Rosetta Twitter account (@ESA_Rosetta) will become more exciting then as well. The last update, from Dec. 3, simply says “still sleeping” (as most of the updates do.) In response to someone asking the account to write something else this summer, the Twitter response was laconic: “A sleeping probe cannot tweet.”

But keep your eyes peeled even after the landing. Rosetta plans to stay with the comet as the icy body moves closer to the solar system, watching as the sun’s heat changes its surface. Read more about the mission here.

December 19, 2013December 23, 2015 by Jason Major

ESA’s Gaia Mission Launches to Map the Milky Way

Soyuz VS06, with Gaia space observatory, lifted off from Europe's Spaceport, French Guiana, on 19 December 2013. (ESA–S. Corvaja)

Early this morning, at 09:12 UTC, the cloudy pre-dawn sky above the coastal town of Kourou, French Guiana was brilliantly sliced by the fiery exhaust of a Soyuz VS06, which ferried ESA’s “billion-star surveyor” Gaia into space to begin its five-year mission to map the Milky Way.

Ten minutes after launch, after separation of the first three stages, the Fregat upper stage ignited, successfully delivering Gaia into a temporary parking orbit at an altitude of 175 km (108 miles). A second firing of the Fregat 11 minutes later took Gaia into its transfer orbit, followed by separation from the upper stage 42 minutes after liftoff. 46 minutes later Gaia’s sunshield was deployed, and the spacecraft is now cruising towards its target orbit around L2, a gravitationally-stable point in space located 1.5 million km (932,000 miles) away in the “shadow” of the Earth.

The launch itself was really quite beautiful, due in no small part to the large puffy clouds over the launch site. Watch the video below:

A global space astrometry mission, Gaia will make the largest, most precise three-dimensional map of our galaxy by surveying more than a billion stars over a five-year period.

“Gaia promises to build on the legacy of ESA’s first star-mapping mission, Hipparcos, launched in 1989, to reveal the history of the galaxy in which we live,” says Jean-Jacques Dordain, ESA’s Director General.

Soyuz VS06, with Gaia, lifted off from French Guiana, 19 December 2013. (ESA - S. Corvaja) — Soyuz VS06 with Gaia (ESA – S. Corvaja, 2013)

Repeatedly scanning the sky, Gaia will observe each of the billion stars an average of 70 times each over the five years. (That’s 40 million observations every day!) It will measure the position and key physical properties of each star, including its brightness, temperature and chemical composition.

By taking advantage of the slight change in perspective that occurs as Gaia orbits the Sun during a year, it will measure the stars’ distances and, by watching them patiently over the whole mission, their motions across the sky.

The motions of the stars can be put into “rewind” to learn more about where they came from and how the Milky Way was assembled over billions of years from the merging of smaller galaxies, and into “fast forward” to learn more about its ultimate fate.

“Gaia represents a dream of astronomers throughout history, right back to the pioneering observations of the ancient Greek astronomer Hipparchus, who catalogued the relative positions of around a thousand stars with only naked-eye observations and simple geometry. Over 2,000 years later, Gaia will not only produce an unrivaled stellar census, but along the way has the potential to uncover new asteroids, planets and dying stars.”

– Alvaro Giménez, ESA’s Director of Science and Robotic Exploration

Gaia will make an accurate map of the stars within the Milky Way from its location at L2 (ESA/ATG medialab; background: ESO/S. Brunier) — Gaia will make an accurate map of a billion stars within the Milky Way from its location at L2 (ESA/ATG medialab; background: ESO/S. Brunier)

Of the one billion stars Gaia will observe, 99% have never had their distances measured accurately. The mission will also study 500,000 distant quasars, search for exoplanets and brown dwarfs, and will conduct tests of Einstein’s General Theory of Relativity.

“Along with tens of thousands of other celestial and planetary objects,” said ESA’s Gaia project scientist Timo Prusti, “this vast treasure trove will give us a new view of our cosmic neighbourhood and its history, allowing us to explore the fundamental properties of our Solar System and the Milky Way, and our place in the wider Universe.”

Follow the status of Gaia on the mission blog here.

Source: ESA press release and Gaia fact sheet

Gaia's launch aboard an Arianespace-operated Soyuz on Dec. 19, 2013 from ESA's facility in French Guiana (ESA) — Gaia’s launch aboard an Arianespace-operated Soyuz on Dec. 19, 2013 from ESA’s facility in French Guiana (ESA)

December 18, 2013December 23, 2015 by Elizabeth Howell

Where Will ExoMars Land? Proposals Invited For Future Mars Rover And Lander

An artist's conception of the European Space Agency's ExoMars rover, scheduled to launch in 2018. Credit: ESA

Scientists, start your engines. The next few weeks will see a flurry of proposals come for the European Space Agency’s first rover mission on the Red Planet in 2018.

The ExoMars mission will see a lander and rover touch Mars, and what’s neat about this particular mission is the rover has a drill on board that can burrow as far down as 6 feet (2 meters) — a first on that planet. This means the mission would be well-suited to look for organic molecules, especially in light of the stunning findings Mars Curiosity scientists recently presented about a possibly life-friendly ancient lake on Mars.

Here, in ESA’s words, are what the site must accomplish:

The site must be ancient (older than 3.6 Ga)—from Mars’ early, habitable period: Pre- to late-Noachian (Phyllosian), possibly extending into the Hesperian;
The site must show abundant morphological and mineralogical evidence for long-duration, or frequently reoccurring, aqueous activity;
The site must include numerous sedimentary rock outcrops;
The outcrops must be distributed over the landing ellipse to ensure that the rover can get to some of them (typical rover traverse range is a few km);
The site must have little dust coverage.

If you’re well-versed in Red Planet geology, we’d love to hear your idea for possible sites. Feel free to leave your thoughts in the comments. For more information about the mission requirements, you can check out the ESA page, which details what proposals must contain.

November 29, 2013December 23, 2015 by Elizabeth Howell

Spacesuit Leak And Fist Pumps: Ride Along With Astronaut’s Eventful Space Station Mission

Expedition 36/37's Luca Parmitano, a European Space Agency astronaut, moments after landing Nov. 10, 2013. Credit: NASA/Carla Cioffi

The big news around astronaut circles these days is the assignment of Takuya Onishi — from the Japanese Aerospace Exploration Agency — to Expedition 48/49 around June 2016. Onishi is from the class of 2009, and we’re guessing he’d be sure to poll his classmates on how their mission training is going.

Well, another of the 2009 astronaut class — Luca Parmitano — just returned from six months in space. It was an eventful mission, with Parmitano facing down a scary water leak during a spacewalk, using the Canadarm to berth and let go of a cargo spacecraft, and then delighting the Internet with enthusiastic fist pumps just minutes after he landed.

Parmitano speaks about the science on station (up to 150 experiments at one time!) as well as what he was experiencing during the leak:

“We were starting our third task, and I felt some water on the back of my head,” he said in an undated video from orbit included in the new video. “And I realized it was cold water. It was not a normal feeling. So I called ground, and that point we called to terminate the EVA.”

But he made it back safely, and looks more than ready to take on another mission in this picture. The cause of the leak is still under investigation, and NASA is holding off on more spacewalks with American suits until they figure out what happened.

Parmitano’s mission also featured a unique collaboration with teenager Abby Harrison, who broadcasted her own question-and-answer sessions with him for the astronaut to reach a younger audience.