‘NASA Johnson Style’ Parodies ‘Gangnam Style’ Music Video

Check this out and get in the groove to enjoy some really cool fun from NASA

NASA interns and NASA astronauts have joined forces to create a very humorous and entertaining music video parody of the “Gangnam Style” mega hit by international pop sensation PSY – It’s called “NASA Johnson Style” and its New!

A team of interns from NASA’s Johnson Space Center (pictured below) in Houston created original lyrics, convinced several initially incredulous astronauts to dance along and shot the video at several NASA centers. Then they integrated the whole kit and kaboodle with the “Gangnam Style” instrumental track. Scotty would be proud of the intricate engineering demanded to pull this off – but where are the tribbles !

Image caption: Mike Massimino (center) poses with the intern video team after filming at JSC. Photo credit: Nicole Cloutier

The video features a fun loving crew of NASA astronauts including Mike Massimino, who deftly repaired the Hubble Space Telescope twice among other things, Clayton Anderson and Tracy Caldwell Dyson who lived and worked for many months aboard the International Space Station, and Mike Coats, a Shuttle commander and the retiring Director of the Johnson Space Center.

The video also features actual footage from the International Space Station , Apollo Moonwalks, Curiosity on Mars, Dawn at Vesta, Houston Mission control, the SLS and Orion Crew vehicle as well as real research labs and scientists here on Earth. So it’s fun and meant to be educational as well.

“Gangnam Style” by the Korean singing star PSY is the most popular YouTube music ever and is enjoyed by millions more every day since it was released last summer. It has spawned numerous other parodies.

And in case you missed last summer’s mega hit parody straight from the Red Planet – click on this: “We’re NASA and We Know It (Mars Curiosity)” – Note: this is NOT a NASA production

Now, turn up the volume and enjoy some light hearted cheer in this Holiday season.

Ken Kremer

Hubble Census Unveils Galaxies Shining Near Cosmic Dawn

This new image of the Hubble Ultra Deep Field (HUDF) 2012 campaign reveals a previously unseen population of seven faraway galaxies, which are observed as they appeared in a period 350 million to 600 million years after the Big Bang. Credit: NASA, ESA, R. Ellis (Caltech), and the UDF 2012 Team

Astronomers using NASA’s Hubble Space Telescope have spotted some of the most distant, dim and ancient galaxies ever detected in a new survey. The images, taken with Hubble’s Wide Field Camera 3 (WFC 3) looks further back in time than any previous Hubble observation, providing information about the conditions in the early Universe.

“This is like a scientific version of the story of Genesis,” said astronomer Avi Loeb from Harvard University.

The seven distant galaxies represent a previously unseen population of galaxies that formed more than 13 billion years ago, when the Universe was less than 3 percent of its present age. In these deepest images to date from Hubble, astronomers were able to take a sample of the amount of galaxies at the time. The results show a smooth decline in the number of galaxies with increasing look-back time to about 450 million years after the Big Bang.

The data provides the first reliable census of this uncharted period of cosmic history, according to the scientists. As astronomers look even deeper into the Universe, galaxy numbers appear to drop off smoothly leading them to believe that the “cosmic dawn” was gradual, not a dramatic event.

“Observations of the microwave afterglow from the Big Bang tell us that reionization happened more than about 13 billion years ago,” said Brant Robertson of the University of Arizona in Tucson, a member of the survey team. “Our data confirms that reionization was a drawn-out process occurring over several hundred million years with galaxies slowly building up their stars and chemical elements. There wasn’t a single dramatic moment when galaxies formed; it was a gradual process.”

These galaxies were found as part of an ambitious Hubble survey of an intensively studied patch of sky known as the Ultra Deep Field (UDF), which was originally taken in 2003-2004, focusing in on a small area in the sky in the constellation Fornax. In the new 2012 campaign, called UDF 2012, a team of astronomers led by Richard Ellis of the California Institute of Technology used the WFC3 to peer deeper into space in near-infrared light than any previous Hubble observation. The observations were made over a period of six weeks during August and September 2012, and the first scientific results are now appearing in a series of scientific papers. The UDF 2012 team is publicly releasing these unique data, after preparing them for other research groups to use.

“Hubble is achieving just great science,” said John Grunsfeld, former astronaut and NASA’s associate administrator for science, speaking at a briefing about the new survey. “This is an origins story, where we’re going back to the beginning, back to the first stars that appeared in the Universe. This validates that when we get James Webb Space Telescope online it will have a lot to look at and a lot to do.”

The James Webb Space Telescope is slated to launch in 2018.

Astronomers detected seven galaxies in the time period 400-600 million years after the Big Bang. All extremely distant, they ranged in distance with redshifts from 8.6 to nearly 12.

Astronomers study the distant universe in near-infrared light because the expansion of space stretches ultraviolet and visible light from galaxies into infrared wavelengths, a phenomenon called “redshift.” The more distant a galaxy, the higher its redshift.

Notably, one of the galaxies may be a distance record breaker, observed 380 million years after the birth of our universe in the Big Bang, corresponding to a redshift of 11.9. This is the galaxy UDFj-39546284, which was previously detected and was originally suggested as the most distant object ever found nearly two years ago by Hubble. Later observations put it at a redshift of 10.3, but the newly refined observations put it even more distant.

A timeline of the Universe and our observations of it. Credit: University of Arizona.

Scientists think that the universe began with the Big Bang about 13.7 billion years ago. Hydrogen formed about 400,000 years later but with no stars, spacetime was dark. About 200 million years later, hydrogen clouds collapsed forming the first stars and galaxies; what astronomers call the “cosmic dawn.” Light from these new stars began breaking down hydrogen into protons and electrons during a time period called cosmic reionization. In the present universe, scientists see galaxies growing in mass and size with the synthesis of elements, leading to the formation of complex molecules including the components to create life. Our Sun and solar system formed just over 4 billion years ago.

“The team pushed Hubble to its limits. This is probably the farthest back Hubble can look, according to the study leader, Richard Ellis. “We are pushing Hubble well beyond what it was designed to do.”

Read more about the findings and the HUDF 2012 Campaign at the HubbleSite.

Read the team’s paper: The Abundance of Star-Forming Galaxies in the Redshift Range 8.5 to 12: New Results from the 2012 Hubble Ultra Deep Field Campaign

Additional Sources: CalTech ESA Hubble

Gigantic Plasma Jets Pour From the Heart of Hercules A

Combined Hubble (optical) and VLA (radio) images show enormous radio jets shooting out from the galaxy Hercules A

Combined Hubble (optical) and VLA (radio) images show enormous radio jets shooting out from the galaxy Hercules A

Talk about pouring your heart out! Astronomers using Hubble’s Wide Field Camera 3 and the recently-upgraded Karl G. Jansky Very Large Array (VLA) radio telescope in New Mexico have identified gigantic jets of plasma, subatomic particles and magnetic fields blasting out of the center of Hercules A, a massive galaxy 2 billion light-years away.

The image above is a combination of optical images from Hubble and radio data gathered by the multi-dish VLA. If our eyes could see in the high-energy spectrum of radio, this is what Hercules A — the otherwise ordinary-looking elliptical galaxy in the center — would really look like.

(Of course, if we could see in radio our entire sky would be a very optically busy place!)

Also known as 3C 348, Hercules A is incredibly massive — nearly 1,000 times the mass of our Milky Way galaxy with a similarly scaled-up version of  a supermassive black hole at its center. Due to its powerful gravity and intense magnetic field Hercules A’s monster black hole is firing superheated material far out into space from its rotational poles. Although invisible in optical light, these jets are bright in radio wavelengths and are thus revealed through VLA observations.

Traveling close to the speed of light, the jets stretch for nearly 1.5 million light-years from both sides of the galaxy. Ring-shaped structures within them suggest that occasional strong outbursts of material have occurred in the past.

Announced on November 29, these findings illustrate the combined imaging power of two of astronomy’s most valuable and cutting-edge tools: Hubble and the newly-updated VLA. The video below shows how it was all done… check it out.

Read more on the NRAO press release here.

Image credits: NASA, ESA, S. Baum and C. O’Dea (RIT), R. Perley and W. Cotton (NRAO/AUI/NSF), and the Hubble Heritage Team (STScI/AURA). Source: NRAO.

Unraveling the Secrets of Type Ia Supernovae: a New Two-Minute Thesis

The folks over at PHD Comics have put together a new video in their Two-Minute Thesis series, this one featuring Ph.D candidate Or Graur of the University of Tel Aviv and the American Museum of Natural History discussing the secret lives — and deaths — of astronomers’ “standard candles” of universal distance, Type Ia supernovae.

Judging distances across intergalactic space isn’t easy, so in order to figure out how far away galaxies are astronomers have learned to use the light from Type Ia supernovae, which flare up with the brilliance of 5 billion Suns… and rather precisely so.

Type Ia supernovae are thought to be created from a pairing of two stars: one super-dense white dwarf which draws in material from a binary companion until a critical mass — about 40% more mass than the Sun – is reached. The overpacked white dwarf suddenly undergoes a rapid series of thermonuclear reactions and explodes in an incredibly bright outburst of material and energy.

But exactly what sorts of stellar pairs lead to Type Ia supernovae and how frequently they occur aren’t known, and that’s what Ph.D candidate Or Graur is aiming to learn more about.

Read more: A New Species of Type Ia Supernova?

“We don’t really know what kind of star it is that leads to these explosions, which is kind of embarrassing,” says Graur. “The companion star could be a regular star like our Sun, a red giant or supergiant, or another white dwarf.”

Because stars age at certain rates, by looking deeper into space with the Hubble and Subaru telescopes Graur hopes to determine how often and when in the Universe’s history Type Ia supernovae occur, and thus figure out what types of stars are most likely responsible.

“My rate measurements favor a second white dwarf as the binary companion,” Graur says, “but the issue is far from settled.”

Watch the video for the full story, and visit PHD TV and PHD Comics for more great science illustrations.

Video: PHDComics. Animation: Jorge Cham. Series Producer: Meg Rosenburg. Inset image: merging white dwarfs causing a Type Ia supernova. (NASA/CXC/M Weiss)

Holiday Gift Idea: Hubble Star Cards

Universe Today writer John Williams is a busy guy. Not only does he write about space and astronomy, he also has his own graphic design and web company called TerraZoom, is the curator of the award winning Starry Critters website, and is a NASA/JPL Solar System Ambassador. A couple of years ago John created a card game called Hubble Star Cards, and the game won a Hubble Gold Star award in 2010 from NASA and the Institute for Global Environmental Strategies (IGES) for its inspiring use of the amazing imagery from the Hubble Space Telescope. As the description says, “the vivid, stunning images motivate and engage children of all ages to learn about objects in space.”

Hubble Star Cards are now available in a high-quality, stunningly beautiful printed card set.

The cards are a just a bit larger than a normal card deck, at 3 inches by 5×5 inches, so the beautiful Hubble images are bigger and better.

They sell for $24.95, but Universe Today readers can get 15% off using UNIVERSE as a coupon code. Check them out at the Hubblestarcards.com website.

“Hubble has a unique ability to draw the public into exploring space,” says John. “Through beautiful images of planets, star clusters, pillars of dust, and galaxies, Hubble provides a crucial stepping stone in the process of scientific inquiry. Hubble Star Cards create a hand-held experience that opens the door to new questions and answers. You can actually hold the Universe, all of creation, in the palm of your hand and have fun learning about it at the same time.”

The game includes 60 cards categorized by planets, planetary nebulae, supernovae remnants, nebulae, star clusters and galaxies. The cards include an image, a basic description, a key to the type of object, location in the sky, constellation, and distance from Earth. Possible games include War, Go Fish, Sorting, Distances and Matching. Although targeted for students 8 and older, preschoolers have played many of the games just by using the amazing imagery as a guide.

Get more info about the Hubble Star Cards here.

Watch Live Webcast: What Does Hubble’s Deepest Image of the Universe Reveal?

This image, called the Hubble eXtreme Deep Field (XDF), combines Hubble observations taken over the past decade of a small patch of sky in the constellation of Fornax. With a total of over two million seconds of exposure time, it is the deepest image of the Universe ever made, combining data from previous images including the Hubble Ultra Deep Field (taken in 2002 and 2003) and Hubble Ultra Deep Field Infrared (2009). The image covers an area less than a tenth of the width of the full Moon, making it just a 30 millionth of the whole sky. Yet even in this tiny fraction of the sky, the long exposure reveals about 5500 galaxies, some of them so distant that we see them when the Universe was less than 5% of its current age. The Hubble eXtreme Deep Field image contains several of the most distant objects ever identified. Credit: NASA

Astronomers using the Hubble Space Telescope recently released the deepest image of the sky ever obtained which reveals the faintest and most distant galaxies ever seen. The Hubble eXtreme Deep Field (XDF) is like a time machine, allowing us to see at how some galaxies looked just 450 million years after the Universe’s birth in the Big Bang.

Want to know more? The Kavli Foundation is hosting a live Q&A webcast on October 4 from 18:00- 18:30 UTC (11-11:30 am PDT) to provide the public a chance to ask questions of leading scientists about the image and the science behind it. Pascal Oesch, a Hubble Fellow at the University of California at Santa Cruz, and Michele Trenti, a researcher at the Kavli Institute for Cosmology, Cambridge at the University of Cambridge in the U.K., will discuss the image and answer questions about how the image was created and what it reveals about the early Universe. Watch the webcast below or at this link. Viewers may submit questions to the two Hubble researchers via Twitter using #KavliAstro or email to [email protected].

Lead image caption: The Hubble eXtreme Deep Field (XDF). Credit: NASA, ESA, G. Illingworth, D. Magee, and P. Oesch (University of California, Santa Cruz), R. Bouwens (Leiden University), and the HUDF09 Team

Weekly Space Hangout – Sept. 27, 2012

This was an action-packed episode of the Weekly Space Hangout. Lots of stories, very little time.

Participants: Mike Wall, Alan Boyle, Ian O’Neill, Nancy Atkinson, Jason Major

Host: Fraser Cain

Want to watch us record the show live? Point your browser at next week’s event page to put the recording right into your calendar.

Hubble’s View of Messier 68: Like Diamonds in the Sky

If you’ve ever looked at Messier 68 through a telescope, you know what a delightful view it is. But the Hubble Space Telescope offers a spectacular, diamond-studded picture of this crowded stellar encampment, a spherical, star-filled region of space known as a globular cluster. This beautiful grouping of stars has been performing a type of stellar dance for perhaps 10 million years.

At a distance of approximately 33,000 light-years, the M68 globular cluster contains at least 2,000 stars that are visible, including 250 giants and 42 variables. It spans 106 light years in diameter.

Mutual gravitational attraction among a cluster’s numerous stars keeps stellar members in check, allowing globular clusters to hang together for many billions of years.

Astronomers can measure the ages of globular clusters by looking at the light of their constituent stars.

The chemical elements leave signatures in this light, and the starlight reveals that stars of globular clusters typically contain fewer heavy elements, such as carbon, oxygen and iron, than stars like the Sun.

Since successive generations of stars gradually create these elements through nuclear fusion, stars having fewer of them are relics of earlier epochs in the Universe.

Indeed, the stars in globular clusters rank among the oldest on record, dating back more than 10 billion years.

More than 150 of these objects surround our Milky Way Galaxy. On a galactic scale, globular clusters are not all that big. In Messier 68’s case, its stars span a volume of space with a diameter of little more than a hundred light-years. The disc of the Milky Way, on the other hand, extends over some 100,000 light-years or more.

Image caption: The globular cluster Messier 68. Credit: ESA/Hubble & NASA

Source: ESA

Fifth Moon Found Around Pluto

This just in! Astronomers working with the Hubble Space Telescope have spotted a new moon around distant Pluto, bringing the known count up to 5. The image above was released by NASA just minutes ago, showing the Pluto system with its newest member, P5.

This news comes just a couple of weeks shy of the one-year anniversary of the announcement of Pluto’s 4th known moon, still currently named “P4”.

The news was shared this morning by an undoubtedly excited Alan Stern of the Southwest Research Institute (SwRI) on Twitter.

Astronomers estimate P5 to be between 6 and 15 miles (9.6 to 24 km) in diameter. It orbits Pluto in the same plane as the other moons — Charon, Nix, Hydra and P4.

“The moons form a series of neatly nested orbits, a bit like Russian dolls,” said team lead Mark Showalter of the SETI Institute.

A mini-abstract of an upcoming paper lists image sets acquired on 5 separate occasions in June and July. According to the abstract, P5 is 4% as bright as Nix and 50% as bright as P4.

The satellite’s mean magnitude is V = 27.0 +/- 0.3, making it 4 percent as bright as Pluto II (Nix) and half as bright as S/2011 (134340) 1. The diameter depends on the assumed geometric albedo: 10 km if p_v = 0.35, or 25 km if p_v =0.04. The motion is consistent with a body traveling on a near-circular orbit coplanar with the other satellites. The inferred mean motion is 17.8 +/- 0.1 degrees per day (P = 20.2 +/- 0.1 days), and the projected radial distance from Pluto is 42000 +/- 2000 km, placing P5 interior to Pluto II (Nix) and close to the 1:3 mean motion resonance with Pluto I (Charon).

The new detection will help scientists navigate NASA’s New Horizons spacecraft through the Pluto system in 2015, when it makes an historic and long-awaited high-speed flyby of the distant world.

See the news release from NASA here.

(H/T to Ray Sanders at DearAstronomer.com)

Top image: NASA, ESA and M. Showalter (SETI Institute)

The Last Outbursts of a Dying Star

As stars approach the inevitable ends of their lives they run out of stellar fuel and begin to lose a gravitational grip on their outermost layers, which can get periodically blown far out into space in enormous gouts of gas — sometimes irregularly-shaped, sometimes in a neat sphere. The latter is the case with the star above, a red giant called U Cam in the constellation Camelopardalis imaged by the Hubble Space Telescope.

From the Hubble image description:

U Cam is an example of a carbon star. This is a rare type of star whose atmosphere contains more carbon than oxygen. Due to its low surface gravity, typically as much as half of the total mass of a carbon star may be lost by way of powerful stellar winds. Located in the constellation of Camelopardalis (The Giraffe), near the North Celestial Pole, U Cam itself is actually much smaller than it appears in Hubble’s picture. In fact, the star would easily fit within a single pixel at the center of the image. Its brightness, however, is enough to saturate the camera’s receptors, making the star look much bigger than it really is.

The shell of gas, which is both much larger and much fainter than its parent star, is visible in intricate detail in Hubble’s portrait. While phenomena that occur at the ends of stars’ lives are often quite irregular and unstable, the shell of gas expelled from U Cam is almost perfectly spherical.

Image credit: ESA/NASA