Pulsar Sets New Speed Record

A pulsar may have been spotted racing through space at over 6 million miles per hour (9.65 million km/h), setting a new speed record for these curious cosmic objects. If observations are what they appear to be, astronomers will have to recalculate the incredible forces created by supernova explosions.

Seen in observations made with 3 different telescopes — NASA’s Chandra X-ray Observatory, ESA’s XMM-Newton, and the Parkes radio telescope in Australia — the x-ray-emitting object IGR J11014-6103 appears to be racing away from the remnants of a supernova in the constellation Carina, 30,000 light-years from Earth.

The comet-shaped object is thought to be a pulsar, the rapidly-spinning, superdense remains of a star. The facts that it’s dim in optical and infrared wavelengths and hasn’t changed in x-ray brightness between XMM-Newton observations in 2003 and Chandra measurements in 2011 support the claim.

IGR J11014’s comet-like shape may be the result of its breakneck speed through space as its pulsar wind nebula gets blown back by the high-energy bow shock created at the forefront of its passage.

Pulsar wind nebulae are the results of charged particles streaming out from the pulsar itself. The particles, traveling at nearly light-speed, are rapidly decelerated by the interstellar medium and create a visible shock wave. In the case of IGR J11014, the pulsar wind is formed into a “tail” by its bow shock — effectively a sonic boom in front of it.

Further observations will be needed to confirm that IGR J11014 is indeed a pulsar, especially considering that actual pulsations have not yet been detected. If it is a pulsar, and is really traveling at the record-breaking speeds it appears to be — between 5.4 and 6.5 million miles per hour, more than 12 times faster than the Sun travels around the center of the galaxy — a new model of supernova explosions may be required.

Read more on the Chandra news release here.

Image: X-ray: NASA/CXC/UC Berkeley/J.Tomsick et al & ESA/XMM-Newton, Optical: DSS; IR: 2MASS/UMass/IPAC-Caltech/NASA/NSF. Video: NASA/CXC/A. Hobart.

Super Secret Spy Satellite Soars Spectacularly to Space on Delta 4 Heavy Booster

Image caption: An upgraded Delta 4 Heavy rocket and super secret spy satellite roar off pad 37 on June 29, 2012 from Cape Canaveral, Florida. Credit: Ken Kremer

A super secret spy satellite for the National Reconnaissance Office (NRO) soared spectacularly to space today (June 29) aboard a Delta 4 Heavy Booster – America’s most powerful rocket following the retirement of NASA’s venerable Space Shuttle Orbiters.

Liftoff of the mammoth Delta 4 Heavy rocket – composed of a trio of liquid fueled common core boosters – finally came at 9:15 a.m. EDT about 3 hours late after a variety of technical issues halted the countdown three times at less than 4 minutes from liftoff from Space Launch Complex 37 on Cape Canaveral Air Force Station, Florida.

Heavy rains and flooding from Tropical Storm Debby had forced a 1 day launch delay from June 28.

The 232 foot tall United Launch Alliance (ULA) Delta lifted off into a magnificent clear blue sky atop the rumbling thunder of three upgraded boosters strapped together side by side and it gradually arced over to the East on the way to orbit.

Both side attached boosters jettisoned as planned. After the second stage engine ignited and the payload fairing separated, the flight went into a preplanned communications black out for the remainder of the flight to orbit and the entire intelligence mission ahead for the hush, hush NROL-15 satellite.

“Today’s successful launch of the NROL-15 mission is the third of four launches for the NRO this year and the second EELV launch for the NRO in just nine days,” said Jim Sponnick, ULA vice president, Mission Operations. “We congratulate the combined NRO , U.S. Air Force and ULA team along with our mission partners for their continued focus on mission success as we deliver the critical capabilities to support the soldiers, sailors, airmen and Marines.”

Just last week on June 20, a ULA Atlas 5 booster lofted the secret NROL-38 satellite for the NRO.

This was only the 6th launch of the Delta 4 Heavy booster and the inaugural flight featuring the upgraded RS-68A Liquid Hydrogen/Liquid Oxygen first stage engines. Each improved engine delivers some 797,000 pounds of thrust vs 758,000 pounds in the prior version – an increase of 39,000 pounds. A single RL 10 engine powered the second stage.

“The upgraded Delta IV Heavy vehicle was developed with an extremely thorough and comprehensive system engineering process by the ULA and Pratt-Whitney Rocketdyne teams, along with substantial involvement by our U.S. government customers,” said Sponnick. “Congratulations to the entire team on today’s successful inaugural flight of the upgraded Delta IV Heavy launch vehicle and the RS-68A engine.”

Ken Kremer

Smoking Wildfires Seen From Space

Wildfires continue to rage across the western United States, burning forests and property alike, and even the most remote have sent up enormous plumes of smoke that are plainly visible to astronauts aboard the Space Station.

The photo above was taken by an Expedition 31 crew member on June 27, showing thick smoke drifting northeast from the Fontenelle fire currently burning in Wyoming. More plumes can be seen to the north.

Utah’s Great Salt Lake can be seen at the bottom right of the image. Its two-tone coloration is due to different species of algae that live in the lake, which is split by the physical barrier of a railroad causeway.

You can watch a video of the wildfires in the west taken from the ISS here, and see more “fire and smoke” news and images from space here.

Image: NASA

Oldest Impact Crater on Earth Discovered in Greenland

Artistic expression of large meteorite impact
An artistic expression of how a large meteorite impact into the sea might have looked in the first second of the impacting. We do not know if the area that was hit was actually covered by water or if there was just a sea nearby. Source: Carsten Egestal Thuesen, GEUS

With shifting continents, rain, and wind, finding traces of ancient impact craters on Earth has been, literally, astronomically low. Now, an international team of scientists say they have found a massive impact crater in Greenland a billion years older than other known asteroid impact on Earth.

Scientists found the remains of the giant 100-kilometer (62 mile) wide crater near the Maniitsoq region of West Greenland and they believe it’s three billion years old. The largest and previously oldest known crater is the 300 kilometer-wide Vredefort crater in South Africa. Tipped on its side, the edges of the Maniitsoq crater would extend from the surface of the Earth to the edge of space.


“This single discovery means that we can study the effects of cratering on the Earth nearly a billion years further back in time than was possible before,” according to Dr. Iain McDonald of the School of Earth and Ocean Sciences at Cardiff University, who was part of the team.

Finding the crater wasn’t an easy task. Today, the Moon still shows marks of the massive bombardment that took place between three and four billion years ago. The early Earth, with its greater gravitational attraction, would have experienced even more collisions. But the land around Maniitsoq has been eroded over the eons to expose crust that originally was 25 kilometers (16 miles) below the surface. Effects of the immense shockwave produced on impact penetrated deep into the crust and remain visible.

Evidence at that depth had never been observed before, says McDonald. “The process was rather like a Sherlock Holmes story,” said McDonald. “We eliminated the impossible in terms of any conventional terrestrial processes, and were left with a giant impact as the only explanation for all of the facts.”

Only about 180 impact craters have been discovered on Earth. Around 30 percent of them contain important natural resources, including nickel, gold, oil and natural gas. It was during an exploration of natural resources that evidence for the crater was discovered. “It has taken us nearly three years to convince our peers in the scientific community,” said McDonald. “But the mining industry was far more receptive. A Canadian exploration company has been using the impact model to explore for deposits of nickel and platinum metals at Maniitsoq since the autumn of 2011.”

The international team, led by Adam Garde, a senior research scientist at the Geological Survey of Denmark and Greenland, or GEUS, contains members from Cardiff, Lund University in Sweden, and the Institute of Planetary Science in Moscow. Their work was recently published in the jounal Earth and Planetary Science Letters.

Image caption: An artistic expression of how a large meteorite impact into the sea might have looked in the first second of the impacting. We do not know if the area that was hit was actually covered by water or if there was just a sea nearby. Source: Carsten Egestal Thuesen, GEUS

Map caption: Black circle on map shows the location of the meteorite impact structure near the town Maniitsoq in Greenland.

Read more about the Maniitsoq structure.

Video: Kennedy Space Center 50th Anniversary

On July 1, 1962, the Launch Operations Center in Florida officially became operational. The name was later changed to John F. Kennedy Space Center in honor of the president and his vision of Americans visiting the Moon. This video looks back at the many launches and space exploration highlights that occurred at KSC, so enjoy this look back from where many journeys to space began. If you are going to be near KSC during the US’s 4th of July holiday, NASA is hosting some special events in commemoration of the 50th anniversary. The KSC Visitor Complex is offering rare behind-the-scenes tours for its 50th anniversary year, including one taking visitors inside the massive, 525-foot-tall Vehicle Assembly Building, where the Apollo rockets and space shuttles were assembled.

You can find out more info about the events at the KSC Visitor’s Center website

First Light Image for NuSTAR

Here is the first image taken by the newest space mission, NuSTAR, or the Nuclear Spectroscopic Telescope Array, the first space telescope with the ability to see the highest energy X-rays in our universe and produce crisp images of them.

“Today, we obtained the first-ever focused images of the high-energy X-ray universe,” said Fiona Harrison, the mission’s principal investigator. “It’s like putting on a new pair of glasses and seeing aspects of the world around us clearly for the first time.”

With the successful “first light” images, the mission will begin its exploration of the most elusive and energetic black holes — as well as other areas of extreme physics in our cosmos — to help in our understanding of the structure of the universe.

The first images show Cygnus X-1, a black hole in our galaxy that is siphoning gas off a giant-star companion. This particular black hole was chosen as a first target because it is extremely bright in X-rays, allowing the NuSTAR team to easily see where the telescope’s focused X-rays are falling on the detectors.

NuSTAR launched on June 13 and its lengthy mast, which provides the telescope mirrors and detectors with the distance needed to focus X-rays, was deployed on June 21. The NuSTAR team spent the next week verifying the pointing and motion capabilities of the satellite, and fine-tuning the alignment of the mast.

The mission’s primary observing program is expected to start in about two weeks. But before it does, the team will continue tests and point the NuSTAR at two other bright calibration targets: G21.5-0.9, the remnant of a supernova explosion that occurred several thousand years ago in our own Milky Way galaxy; and 3C273, an actively feeding black hole, or quasar, located 2 billion light-years away at the center of another galaxy. These targets will be used to make a small adjustment to place the X-ray light at the optimum spot on the detector, and to further calibrate and understand the telescope in preparation for future science observations.

Other targets for the mission include the burnt-out remains of dead stars, such as those that exploded as supernovae; high-speed jets; the temperamental surface of our sun; and the structures where galaxies cluster together like mega-cities.

“This is a really exciting time for the team,” said Daniel Stern, the NuSTAR project scientist. “We can already see the power of NuSTAR to crack open the high-energy X-ray universe and reveal secrets that were impossible to get at before.”

Lead image caption: NASA’s Nuclear Spectroscopic Telescope Array, or NuSTAR, has taken its first snapshots of the highest-energy X-rays in the cosmos (lower right), producing images that are much crisper than previous high-energy telescopes (example in upper right). NuSTAR chose a black hole in the constellation Cygnus (shown in the skymap on the left) as its first target due to its brightness. Image credit: NASA/JPL-Caltech

Galactic Gong – Milky Way Struck and Still Ringing After 100 Million Years

Small Magellanic Cloud
Small Magellanic Cloud

When galaxies collide, stars are thrown from orbits, spiral arms are stretched and twisted, and now scientists say galaxies ring like a bell long after the cosmic crash.

A team of astronomers from the United States and Canada say they have heard echoes of that ringing, possible evidence of a galactic encounter 100 million years ago when a small satellite galaxy or dark matter object passed through the Milky Way Galaxy; close to our position in the galaxy, as if a rock were thrown into a still pond causing the stars to bounce up and down on the waves. Their results were published in the Astrophysical Journal Letters.

“We have found evidence that our Milky Way had an encounter with a small galaxy or massive dark matter structure perhaps as recently as 100 million years ago,” said Larry Widrow, professor at Queen’s University in Canada. “We clearly observe unexpected differences in the Milky Way’s stellar distribution above and below the Galaxy’s midplane that have the appearance of a vertical wave — something that nobody has seen before.”

Astronomers took observations from about 300,000 nearby stars in the Sloan Digital Sky Survey. Stars move up and down at 20-30 kilometers per second while see-sawing around the galaxy at 220 kilometers per second. By comparison, the International Space Station putters around Earth at 7.71 kilometers per second; Voyager 1, the fastest man-made object, currently is leaving the solar system at about 17.46 kilometers per second. Widrow and colleagues at the University of Kentucky, The University of Chicago and Fermi National Accelerator Laboratory found that the positions of nearby stars is not quite as regular as previously thought. The team noticed a small but statistically significant difference in the distribution of stars above and below the midplane of the Milky Way.

“Our part of the Milky Way is ringing like a bell,” said Brian Yanny, of the Department of Energy’s Fermilab. “But we have not been able to identify the celestial object that passed through the Milky Way. It could have been one of the small satellite galaxies that move around the center of our galaxy, or an invisible structure such as a dark matter halo.”

Susan Gardner, professor of physics at the University of Kentucky added, “The perturbation need not have been a single isolated event in the past, and it may even be ongoing. Additional observations may well clarify its origin.”

Other possibilities considered for the variations were the effect of interstellar dust or simply the way the stars were selected in the survey. But as those events failed to explain fully the observations, the astronomers began to explore possible recent events in the history of the galaxy.

More than 20 visible satellite galaxies circle the Milky Way. Invisible satellites made up of dark matter, hypothetical matter that cannot be seen but is thought to make up a majority of the mass of the Universe, might also orbit our galaxy. Scientists believe that most of the mass orbiting the galaxy is in the form of dark matter. Using computer simulations to explore the effects of a small galaxy or dark matter structure passing through the disk of the Milky Way, the scientists developed a clearer picture of the see-saw effects they were seeing.

In terms of the nine-billion lifetime of the Milky Way Galaxy, the effects are short-lived. This part of the galaxy has been “ringing” for 100 million years and will continue for 100 million years more as the up-and-down motion dissipates, say the astronomers – unless we are hit again.

Image caption: The Small Magellanic Cloud is one of 20 visible satellite galaxies that orbit the Milky Way Galaxy. Astronomers report that a smaller counterpart or dark matter object passed through the Milky Way near our position about 100 million years ago.

Meteorite Crashes Into London Cab


Londoners awoke this morning to news of a meteorite which struck a taxi in the heart of the city’s busy shopping district Covent Garden. Witnesses were left stunned by what looked like a scene straight out of a science fiction film. An incident team arrived almost immediately to cordon off the meteorite and keep the public at a safe distance.

No one was injured as a result of the incident, but it’s a cosmic harbinger of things to come…

Of course, the “things to come” turn out to be 4 weeks of science programs on Eden TV’s Science Month, which starts up in July.

The incident was in fact a well-orchestrated publicity stunt by the UK’s Eden TV (Sky 532 Virgin 208). Science Month will run all day every day during the month of July. Highlights in the first week include Wonders of the Universe (Monday 2 July at 9pm), Finding Life Beyond Earth (Monday 2 July at 10pm), The Code (Wednesday 4 July at 10pm) and Deadliest Volcano (Thursday 5 July at 7pm).

Sure, after all’s said and done it was a PR stunt. But it was a cool PR stunt (even if not quite scientifically accurate!)

Come on, we all know that meteorites aren’t steaming hot when they land. 😉

Robots Tested in Sample Return Challenge

Caption: Participants in NASA’s Sample Return Robot Challenge. Credit: NASA

Editor’s note: This guest post was written by Andy Tomaswick, an electrical engineer who follows space science and technology.

Picking up rocks can be harder than you’d think. That is one of the lessons to take away from the recently completed Sample Return Robot Challenge hosted by NASA and the Worchester Polytechnic Institute (WPI).

The challenge offered a $1.5 million prize to the robot that could complete a series of automated search and retrieve missions while also meeting NASA’s technical standards for the design of the robot. NASA intended to farm the technologies developed for the competition for design ideas for a possible future Mars sample return mission.

Many NASA employees got to see the technologies first hand at the competition in Massachusetts on a weekend in June. Lori Garver, NASA’s deputy administrator, spoke at a pre-event ceremony followed by a chance for the teams to show off their robots to local high school students, with some 7,000 people in total attending the event.

The actual challenge started off with a test to see if the teams complied with the design regulations handed out by NASA. Five of the six teams that showed up for he event failed to meet the standards, with Team SpacePRIDE from Graniteville, South Carolina the only team to successfully do so. The main difficulty for most teams dealt with a safety-related pause switch which required all moving parts to immediately suspend its movement upon triggering that switch. This would, in theory, save any innocent bystanders from the wrath of an autonomous robot that is not yet subject to the Three Laws of Robotics. Despite the switch not functioning as intended on most robots, all the teams were allowed to participate in the actual event, and the competition went on as planned.

However, the task proved too much for any robot, as none were able to successfully collect the samples needed to meet the challenge’s requirements in the time allotted. The teams did display one of the strengths of the open challenge type format: they all brought very unique ideas to bear on solving the automated problem. Team SpacePRIDE drew particular attention by having a three-robot system, with two smaller scout rovers and one larger collector rover. All of the teams had plenty of feedback to give to the NASA sponsors, and all of the competitors seemed to enjoy themselves as well.

That feedback lies at the real heart of the Centennial Challenge competitions that NASA has been hosting. Even if no one wins the prizes on offer, the challenges themselves draw interest from students around the country as well as spawn ideas from the teams. The good thing about no one completing the challenge this year is that next year the $1.5 million pot is still up for grabs, assuming NASA agrees to sponsor the event again.

Source: NASA Sample Return Robot Challenge Concludes, Team SpacePRIDE

Mighty Delta 4 Heavy Rocket and Clandestine Satellite Poised at Pad

Image caption: The Delta 4 Heavy rocket and Super secret payload stand poised for launch at 6:13 a.m. EDT on June 29, 2012 following retraction of the mobile service tower. Credit: Ken Kremer

A mighty triple-barreled Delta 4 Heavy rocket with a clandestine military satellite perhaps the size of Hubble was unveiled this evening (June 28) at a seaside launch pad at Cape Canaveral, Florida.

The 232 foot tall rocket is poised to blast off at 6:13 a.m. EDT from Space Launch Complex 40 at Cape Canaveral Air Force Station. The exact launch window, like everything else about the classified mission and the NROL-15 spy satellite is top secret.

The mobile service tower was retracted from around the absolutely gorgeous white and orange colored rocket starting around 8:30 p.m. and the super secret spy satellite being launched for the National Reconnaissance Office (NRO) – see my photos.

The launch was delayed a day by the lingering devastation caused by Tropical Storm Debby.

Image caption: Delta 4 Heavy rocket and top secret NRO payload are poised for launch on June 29. Credit: Ken Kremer/www.kenkremer.com

The United Launch Alliance Delta 4 Heavy is flying for the first time with upgraded RS-68A first stage engines, each of which delivers 720,000 pounds of thrust.

This will be the 6th launch of the Delta 4 Heavy – now the most powerful rocket in the US fleet following the shutdown of NASA’s Space Shuttle Program.

As of 12:45 a.m. June 29 , the countdown is now underway ! Fueling will commence shortly. Stay tuned for a post – launch report

Ken Kremer