First Images in a New Hunt for Dark Energy

Zoomed-in image from the Dark Energy Camera of the barred spiral galaxy NGC 1365, about 60 million light-years from Earth. (Dark Energy Survey Collaboration)

The ongoing search for dark energy now has a new set of eyes: the Dark Energy Camera, mounted on the 4-meter Victor M. Blanco telescope at the National Science Foundation’s Cerro Tololo Inter-American Observatory in Chile. The culmination of eight years of planning and engineering, the phone-booth-sized 570-megapixel Dark Energy Camera has now gathered its very first images, capturing light from cosmic structures tens of millions of light-years away.

Eventually the program’s survey will help astronomers uncover the secrets of dark energy — the enigmatic force suspected to be behind the ongoing and curiously accelerating expansion of the Universe.

Zoomed-in image from the Dark Energy Camera of the Fornax cluster

“The Dark Energy Survey will help us understand why the expansion of the universe is accelerating, rather than slowing due to gravity,” said Brenna Flaugher, project manager and scientist at Fermilab.

Read more: Polar Telescope Casts New Light on Dark Energy

The most powerful instrument of its kind, the Dark Energy Camera will be used to create highly-detailed color images of  a full 1/8th of the night sky — about 5,000 square degrees — surveying thousands of supernovae, galactic clusters and literally hundreds of millions of galaxies, peering as far away as 8 billion light-years.

The survey will attempt to measure the effects of dark energy on large-scale cosmic structures, as well as identify its gravitational lensing effects on light from distant galaxies. The images seen here, acquired on September 12, 2012, are just the beginning… the Dark Energy Survey is expected to begin actual scientific investigations this December.

Full Dark Energy Camera composite image of the Small Magellanic Cloud

“The achievement of first light through the Dark Energy Camera begins a significant new era in our exploration of the cosmic frontier,” said James Siegrist, associate director of science for high energy physics with the U.S. Department of Energy. “The results of this survey will bring us closer to understanding the mystery of dark energy, and what it means for the universe.”

Read more on the Symmetry Magazine article here, and you can also follow the Dark Energy Survey on Facebook here. (The Fermilab press release can be found here.)

Images: Dark Energy Survey Collaboration. Inset image: the 4-meter Blanco Telescope dome at CTIO (NOAO)

The Dark Energy Survey is supported by funding from the U.S. Department of Energy; the National Science Foundation; funding agencies in the United Kingdom, Spain, Brazil, Germany and Switzerland; and the participating DES institutions.

 

Curiosity Captures a Martian Eclipse

Yes, Mars gets eclipses too! This brief animation, made from ten raw subframe images acquired with Curiosity’s Mastcam on September 13 — the 37th Sol of the mission — show the silhouette of Mars’ moon Phobos as it slipped in front of the Sun’s limb.

The entire animation spans a real time of about 2 minutes.

As a moon Phobos really is an oddity. In addition to its small size – only 8 miles (13 km) across at its widest – and irregular shape, it also orbits its parent planet at a very low altitude, only 5,840 miles (9,400 km) and thus needs to travel at a relatively high velocity in order to even stay in orbit. Phobos actually orbits Mars over three times faster than Mars rotates, appearing to rise in Mars’ western sky. And its orbit is so low that it can’t even be seen from the polar regions!

Since Phobos, and its even more petite sibling Deimos, are so small, the Mars rovers won’t ever see a total solar eclipse. In fact these events are often referred to as transits rather than actual eclipses.

This isn’t the first time an eclipse was captured by a Mars Exploration Rover; Opportunity witnessed a similar partial eclipse of the Sun by Phobos in December 2010, and Spirit caught a lunar (or “Phobal?”) eclipse on camera back in 2005, when the moon passed into the shadow of Mars.

Curiosity’s find was no accident, either, as mission engineers had the Mastcam already positioned to capture the event. Preparation really pays off!

See the latest images and news from the MSL mission here.

Images: NASA/JPL-Caltech/Malin Space Science Systems. Animation by Jason Major. Inset image: Phobos as seen by Mars Express ESA/DLR/FU Berlin (G. Neukum)

UPDATE 9/19/12: See a close-up animation of the eclipse event here.

Farewell to a Hero: Photos From Armstrong’s Burial at Sea

Armstrong’s burial service aboard the USS Philippine Sea on September 14, 2012 (NASA/Bill Ingalls)

Earlier today, Friday, September 14, 2012, Neil A. Armstrong’s burial at sea service was held aboard the USS Philippine Sea (CG 58) in the Atlantic Ocean. Armstrong, the first man to walk on the moon during the 1969 Apollo 11 mission, died Saturday, August 25. He was 82.

An icon of exploration for all of humanity, he will be missed by millions and remembered forever. Godspeed, sir, and thank you.

See more photos below.

US Navy personnel carry the cremated remains of Apollo 11 astronaut Neil Armstrong

Members of the US Navy ceremonial guard hold an American flag over Armstrong’s remains

A US Navy firing squad fires three volleys in honor of Neil Armstrong

US Navy Lieutenant Commander Paul Nagy and Carol Armstrong, wife of Neil Armstrong, commit the remains of Neil Armstrong to the sea

US Navy Captain Steve Shinego presents the US flag to Carol Armstrong as Neil’s son, Eric “Rick” Armstrong, looks on.

All photos credit NASA/Bill Ingalls.

See more photos from the service on the Flickr set here.

Neil Alden Armstrong, 1930 – 2012.

Sonic-Powered Levitation Allows for Zero-G Drug Research

It’s not special effects: researchers at the U.S. Department of Energy’s Argonne National Laboratory in Illinois have developed a way to cancel out the effects of gravity, allowing liquids to be held without containers. The effect is created using sound waves emitted by an acoustic levitator — an instrument designed by NASA for simulating microgravity.

Watch the video. It’s the coolest thing you’ll see all week.

This accomplishes more than just a neat effect; by keeping liquids in place without the need for a physical container, pharmaceutical research can be performed while the drugs are still in their purest, “amorphous” state.

“Most drugs on the market are crystalline – they don’t get fully absorbed by the body and thus we aren’t getting the most efficient use out of them,” said Yash Vaishnav, Argonne Senior Manager for Intellectual Property Development and Commercialization.

When solutions come in contact with the interior surfaces of their containers, evaporation takes place, which can lead to crystallization. In order to find a way to hold liquids without anything coming in contact with them (a tricky task while under the effect of Earth’s pesky gravity) ANL X-ray physicist Chris Benmore looked to NASA’s acoustic levitator.

Using two sets of sound waves emitted at 22khz and precisely aimed at each other, a “standing wave” is established at their center. The resulting acoustic force is strong enough to counter the downward tug of gravity at certain points (at least as far as droplets of liquid are concerned.)

The liquid drugs can then be studied without the problem of crystallization, making this technological parlor trick a powerful analytical tool for pharmaceutical researchers. The ultimate goal is to learn how to reduce the amount of a particular drug but still retain the desired effects — with less of the undesired ones.

Read more here on the Argonne National Lab site.

The nation’s first national laboratory, Argonne conducts leading-edge basic and applied scientific research in virtually every scientific discipline. With employees from more than 60 nations, Argonne is managed by UChicago Argonne, LLC for the U.S. Department of Energy’sOffice of Science.

In Fact It’s Cold As Hell: Mars Isn’t As Earthlike As It Might Look

The slopes of Gale Crater as seen by Curiosity are reminiscent of the American southwest (NASA/JPL-Caltech)

“Mars ain’t no kind of place to raise your kids; in fact it’s cold as hell” sang Elton John in “Rocket Man”, and although the song was released in 1972 — four years before the first successful landing on Mars — his weather forecast was spot-on. Even though the fantastic images that are being returned from NASA’s Curiosity rover show a rocky, ruddy landscape that could easily be mistaken for an arid region of the American Southwest one must remember three things: this is Mars, we’re looking around the inside of an impact crater billions of years old, and it’s cold out there.

Mars Exploration Program blogger Jeffrey Marlow writes in his latest “Martian Diaries” post:

Over the first 30 sols, air temperature has ranged from approximately -103 degrees Fahrenheit (-75 Celsius) at night to roughly 32 degrees Fahrenheit (0 Celsius) in the afternoon. Two factors conspire to cause such a wide daily range (most day-night fluctuations on Earth are about 10 to 30 degrees Fahrenheit). The martian atmosphere is very thin; with fewer molecules in the air to heat up and cool down, there’s more solar power to go around during the day, and less atmospheric warmth at night, so the magnitude of temperature shifts is amplified. There is also very little water vapor; water is particularly good at retaining its heat, and the dryness makes the temperature swings even more pronounced. 

In that way Mars is like an Earthly desert; even after a blisteringly hot day the temperatures can plummet at night, leaving an ill-prepared camper shivering beneath the cold glow of starlight. Except on Mars, where the Sun is only 50% as bright as on Earth and the atmosphere only 1% as dense, the nighttime lows dip to Arctic depths.

“Deserts on Earth have very extreme temperature ranges,” says Mars Science Laboratory Deputy Project Scientist, Ashwin Vasavada. “So if you take a desert on Earth and put it in a very thin atmosphere 50% farther from the Sun, you’d have something like what we’re seeing at Gale Crater.”

And although the afternoon temperatures in Gale may climb slightly above freezing that doesn’t mean liquid water will be found pooling about in any large amounts. Curiosity’s in no danger from flash floods on Mars… not these days, anyway.

With atmospheric pressure just above water’s thermodynamic triple point, and temperatures occasionally hovering around the freezing point, it is likely that local niches are seeing above-zero temperatures, and Vasavada acknowledges, “liquid water could exist here over a tiny range of conditions.” But don’t expect a Culligan water plant in Gale Crater any time soon. “We wouldn’t expect for Curiosity to see liquid water, because it would evaporate or re-freeze too quickly,” explains Vasavada. “With so little water vapor in the atmosphere, any liquid water molecules on the surface would quickly turn to gas.”

So when on Mars, drink your coffee quickly. (And pack a blanket.)

“Gale Crater may look like the dusty, basaltic basins of the American southwest, but one look at the thermometer will send you running for the winter coat.”

– Jeffrey Marlow, Martian Diaries

Read Marlow’s full article here.

Image: Sunset on Mars seen by the MER Spirit from Gusev Crater in 2005 (NASA/JPL-Caltech)

50 Years Ago Today, We Chose to Go to the Moon

“We set sail on this new sea because there is new knowledge to be gained, and new rights to be won, and they must be won and used for the progress of all people.”
– John F. Kennedy, September 12, 1962

On this day, 50 years ago, on a warm, sunny morning in Houston, Texas, President John F. Kennedy delivered a now-famous speech to 40,000 spectators at Rice University, a speech that supported the United States’s commitment to step beyond the boundaries of our world, to go beyond low-Earth orbit and eventually, successfully (and indeed before the decade was out!) land men on the Moon and return them safely to Earth.

It was an inspiring speech, both for the nation’s newly-developed space industry as well as for the entire country. (Would that we saw more overt dedication to space exploration from our leaders today!) This video from Rice University, itself celebrating its 100th anniversary in October, gives some insight into the events of that day in September of 1962, the small moments that led up to it and the large ones that followed.

From the Rice news release by Jade Boyd:

JFK’s 1962 moon speech still appeals 50 years later

Few moments in Rice’s history are as well known or oft remarked upon as the 1962 speech in which President John F. Kennedy boldly declared, “We choose to go to the moon!”

The speech marked a turning point for Rice, the city of Houston, the nation and the world. Globally, the space race played out against the backdrop of the Cold War, and in the U.S. the space program shared headlines with the Vietnam War and the struggle for civil rights. In Houston, NASA would pump more than $1 billion into the local economy in the 1960s and help the city blossom into the nation’s fourth-largest metropolis.

In a tribute to Apollo 11 astronaut Neil Armstrong this week, Rice alum Paul Burka ’63, executive editor of Texas Monthly magazine, published the verbatim text of Kennedy’s speech in his blog. Burka, who was at Rice Stadium that day, said the speech “speaks to the way Americans viewed the future in those days. It is a great speech, one that encapsulates all of recorded history and seeks to set it in the history of our own time. Unlike today’s politicians, Kennedy spoke to our best impulses as a nation, not our worst.”

Kennedy spoke at the stadium at 10 a.m. Sept. 12. It was a warm, sunny day, and fall classes were not yet under way. Rice’s incoming freshmen were on campus for orientation, but many of the estimated 40,000 spectators were Houston school children, said Rice Centennial Historian Melissa Kean.

Kennedy told the audience that the United States intended to take the lead in spaceflight, both to ensure that the Soviet Union did not base strategic weapons in space and because space exploration “is one of the great adventures of all time, and no nation which expects to be the leader of other nations can expect to stay behind in the race for space.”

The best-known line from the speech — “We choose to go to the moon!” — earned a thunderous ovation, in part because of Kennedy’s clever oratory. He played to the hometown crowd with the preceding line, “Why does Rice play Texas?” — a line that Kennedy jotted between the lines of the typed copy prepared by White House aide Ted Sorensen.

In its front-page coverage of the speech, the Rice Thresher made note of this line and others. The paper reported that the speech capped a two-day visit to Houston in which Kennedy toured facilities at the Manned Spacecraft Center (now Johnson Space Center), and the Thresher referred to the costly nature of the space program by citing the $5.4 billion annual NASA budget, a figure Kennedy also used in the speech.

The number impressed chemist Robert Curl ’54, one of many faculty members at the stadium.

“I came away in wonder that he was seriously proposing this,” said Curl, Rice’s Pitzer-Schlumberger Professor Emeritus of Natural Sciences and professor emeritus of chemistry. “It seemed like an enormous amount of money to spend on an exploration program. It was an impressive amount of money back then, and if you adjust for inflation, the Apollo program cost more than the LHC today.”

Curl said Kennedy’s vision paid off for NASA and Houston when Apollo 11 landed on the moon less than eight years later.

Another Rice faculty member in attendance was Ron Sass, fellow in global climate change at Rice’s Baker Institute for Public Policy and the Harry C. and Olga K. Wiess Professor Emeritus of Natural Sciences.

Sass and Curl each said Kennedy’s speech seemed no more remarkable at the time than the 1960 speech by President Eisenhower at Autry Court. Today, Eisenhower’s speech is largely forgotten, and Kennedy’s is still frequently cited in the news.

Sass said part of the enduring appeal of Kennedy’s speech is the magnitude of what he proposed, something Sass said he has come to appreciate more with age.

“It didn’t seem outlandish to me at the time,” Sass said. “I was young, and I thought you could do just about anything.”

“If this capsule history of our progress teaches us anything, it is that man, in his quest for knowledge and progress, is determined and cannot be deterred. The exploration of space will go ahead, whether we join in it or not, and it is one of the great adventures of all time, and no nation which expects to be the leader of other nations can expect to stay behind in the race for space.”
– President John F. Kennedy

For a full transcript of JFK’s speech, click here.

Video and inset image: Rice University. Apollo 11 liftoff: NASA

Watch Jupiter Get Hit in the Original HD Video

Caught on webcam by amateur astronomer George Hall in Dallas, Texas, the impact on Jupiter that occurred yesterday at 6:35 a.m. CT can be clearly seen in the brief video above as a bright flash along the giant planet’s left side.

According to Hall on his website the video was captured with a 12″ LX200GPS, 3x Televue Barlow, and Point Grey Flea 3 camera using Astro IIDC software.

Great catch, George! Currently this is the only video footage we’ve seen of this particular event. Also, tonight at 10 p.m. ET / 7 p.m. PT the SLOOH Space Camera site will broadcast a live viewing of Jupiter to search for any remaining evidence of an impact. Tune in here.

Video © George Hall. All rights reserved, used with permission.

A Memorial to 9/11… on Mars

Today, on the 11th anniversary of the World Trade Center attack, countless hearts and minds will be reflecting upon a day that changed our world forever and remembering those who lost their lives in the tragic collapse of the twin towers. Memorial events will be held in many locations around the planet… and even, in a small yet poignant way, on another planet. For, unknown to many, two pieces of the World Trade Center are currently on the surface of Mars: one affixed to the rover Spirit, now sitting silently next to a small rise dubbed “Home Plate”, and the other on its sister rover Opportunity, still actively exploring the rim of Endeavour crater.

Even more than scientific exploration tools, these rovers are also interplanetary memorials to all the victims of 9/11.

(The following is a repost of an article first featured on Universe Today in 2011, on the 10th anniversary of 9/11.)

In September of 2001 workers at Honeybee Robotics in lower Manhattan were busy preparing the Rock Abrasion Tools that the twin rovers Spirit and Opportunity would each be equipped with, specialized instruments that would allow scientists to study the interiors of Martian rocks. After the World Trade Center attacks occurred, the company wanted a way to memorialize those who had lost their lives.

Through what was undoubtedly some incredibly skillful use of contacts, Honeybee founder and MER science team member Stephen Gorevan – on a suggestion by JPL engineer Steve Kondos and with help from the NYC mayor’s office and rover mission leader Steve Squyres – was able to procure two pieces of aluminum from the tower debris. These were fashioned into cylindrical cable shields by a contracted metal shop in Round Rock, Texas, and had American flags adhered to each by Honeybee engineer Tom Myrick.

The image above, taken in 2004, shows the cable shield with American flag on the Rock Abrasion Tool attached to Spirit. At right is an image of the flag shield on Opportunity, acquired on September 11, 2011.

The rovers were launched in the summer of 2003 and have both successfully operated on Mars many years past their planned initial mission timelines. Spirit currently sits silent, having ceased communication in March 2010, but Opportunity is still going strong in its exploration of the Martian surface.

“It’s gratifying knowing that a piece of the World Trade Center is up there on Mars. That shield on Mars, to me, contrasts the destructive nature of the attackers with the ingenuity and hopeful attitude of Americans.”

– Stephen Gorevan, Honeybee Robotics founder and chairman

These memorials will remain on Mars long after both rovers have ceased to run, subtle memorials to thousands of lives and testaments to our ability to forge ahead in the name of hopefulness and discovery.

Original source: OnOrbit.com

Image credit: NASA / JPL-Caltech

Photo of Manhattan taken from orbit on September 11, 2001. (NASA)

STEREO Spots a CME Soaring Into Space

Press “play.” Say “wow.”

The enormous eruption of a solar prominence and resulting coronal mass ejection (CME) back on August 31 that was captured in amazing HD by NASA’s Solar Dynamics Observatory was also spotted by the Sun-flanking STEREO-B spacecraft, which observed the gigantic gout of solar material soaring away from the Sun.

This video shows the eruption as it passes across the fields of view of several of STEREO-B’s cameras over the course of 48 hours.

According to NASA’s Goddard Space Flight Center, “while CMEs are routinely seen in the Heliographic Imager (HI) telescopes, it’s very rare for prominences to stay visible for so long. The HI1 field of view ranges from 4 to 24 degrees away from the Sun. To get a sense of scale, we know the Sun is roughly 860,000 miles wide — and look how far the prominence holds together. And this CME is so bright it initially saturates the COR1 telescope.”

The bright spot in the red (COR2) field of view is the planet Venus.

Coronal mass ejections are huge bubbles of gas bounded by magnetic field lines that are ejected from the Sun over the course of several minutes — sometimes even hours. If they are directed toward Earth, the cloud of charged solar particles can interact with our magnetosphere and cause anything from increased auroral activity to radio interference to failure of sensitive electromagnetic equipment.

Particularly long filaments like the one that caused the August 31 CME have been known to collapse with explosive results when they hit the stellar surface.

The CME did not travel directly toward Earth but did connect with Earth’s magnetosphere with a glancing blow, causing bright aurorae to appear around the upper latitudes on the night of September 3.

Image: NASA/STEREO/GSFC

Clay Deposits Don’t Prove Existence of Ancient Martian Lakes

HiRISE image of branching features in the floor of Antoniadi Crater thought to contain clay material. (NASA/JPL/University of Arizona)

In the hunt for evidence of a warmer, wetter past on Mars, clay deposits have been viewed as good indications that stable liquid water existed on its surface for some time — perhaps even long enough to allow life to develop. But new research conducted here on Earth shows that some clays don’t necessarily need lakes of liquid water to form. Instead they can be the result of volcanic activity, which is not nearly so hospitable to life.

A research team led by Alain Meunier of the Université de Poitiers in France studied lavas containing iron and magnesium — similar to ancient clays identified on the surface of Mars — in the French Polynesian atoll of Moruroa. The team’s findings show that the same types of clay outcrops can be caused by the solidifying of water-rich magma in a volcanic environment, and don’t require Earthlike aquatic conditions at all.

The results also correlate to the deuterium-to-hydrogen (D/H) ratio within clays found in Martian meteorites.

Read: Life from Mars Could Have Polluted Earth

“To crystallize, clays need water but not necessarily liquid water,” said Alain Meunier to the Agençe France-Presse (AFP). “Consequently, they cannot be used to prove that the planet was habitable or not during its early history.”

Additionally, the clay deposits found on Mars can be several hundred meters thick, which seems to be more indicative of upwelling magma than interactions with water.

“[This] new hypothesis proposes that the minerals instead formed during brief periods of magmatic degassing, diminishing the prospects for signs of life in these settings,” wrote Brian Hynek from the Department of Geological Sciences at the University of Colorado, in response to the paper by Meunier et al. which was published in the September 9 edition of the journal Nature Geoscience.

This does not necessarily mean that all Martian clays weren’t formed in the presence of water, however. Gale Crater — where NASA’s Curiosity rover is now exploring — could very well have been the site of a Martian lake, billions of years in the past. Clays found there could have been created by water.

Read: Take a Trip to Explore Gale Crater

According to Bethany Ehlmann of the California Institute of Technology, co-author of the study, “there are particular characteristics of texture” to clays formed under different conditions, and “Gale is a different flavor of Mars.”

Perhaps Curiosity will yet discover if Gale’s original flavor was more cool and wet than hot and spicy.

Read more on New Scientist and Cosmos Magazine.

Inset image: Moruroa Atoll (NASA)