Lunar Farside Gets Highest Resolution Look Yet from LRO

The lunar farside as never seen before! LROC WAC orthographic projection centered at 180° longitude, 0° latitude. Credit: NASA/GSFC/Arizona State University.

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The first time humans were able to catch a glimpse of the far side of the Moon was back in 1959 when the Soviet Luna 3 spacecraft sent back 29 grainy images taken during its successful loop around the Moon. “What a surprise – the farside was a different world, geologically,” said Mark Robinson, principal investigator for the camera on board the Lunar Reconnaissance Orbiter. “Unlike the widespread maria on the nearside, basaltic volcanism was restricted to a relatively few, smaller regions on the farside, and the battered highlands crust dominated.”

Since then, just a handful of spacecraft have taken images of the far side of the Moon, but now, Robinson has had a hand in creating the most detailed view yet of the farside of the Moon. A mosaic of the far side released today is comprised of over 15,000 Wide Angle Camera images acquired between November 2009 and February 2011.


“This WAC mosaic provides the most complete look at the morphology of the farside to date, and will provide a valuable resource for the scientific community,” Robinson wrote on the LROC website. “And it’s simply a spectacular sight!”

And how!

Every month, as LRO circles the Moon, the WAC gathers images to provide nearly complete coverage of the Moon under unique lighting. This mosaic knits together images all with similar lighting. As an added bonus the orbit-to-orbit image overlap provides stereo coverage, and even more images will be released on March 15.

“As the mission progresses, and our knowledge of the lunar photometric function increases, improved and new mosaics will be released!” Robinson said. “Work your way around the Moon with these six orthographic projections constructed from WAC mosaics.”

Click here for more stunning, high resolution views of the Moon.

Source: LROC

Grieving Glory — And Will The Taurus XL Fly Again?

Orbital Sciences Taurus rocket. Credit: NASA

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Last week’s loss of the $420 million Glory satellite has sent NASA into an intensive investigation to find out why two climate change missions in a row — flying aboard the same type of rocket — crashed due to what apparently was a similar technical glitch. Orbital Sciences out of Dulles, Va. is the company that designed the Taurus XL rocket that hosted both Glory and the Orbiting Carbon Satellite that crashed in 2009. They insisted last week that they’ll bounce back with the Taurus. But they may not be bouncing back on a NASA mission. Joy Bretthauer, NASA’s Glory program executive, acknowledged that the Orbiting Carbon Observatory 2, which will launch in 2013, is contracted to fly on none other than a Taurus XL. That may not stand, she said: “The bottom line is NASA will not fly in a launch vehicle that we do not have confidence in.”

Meanwhile, scores of researchers who poured their hearts into the mission are working to cope with the loss. Greg Kopp, the Boulder, Colorado-based principal investigator on the Total Irradiance Monitor that was supposed to fly aboard Glory, gave a thorough debriefing about his experience for the radio program Colorado Matters, on Colorado Public Radio out of Denver. It airs today.

Rich Straka, deputy general manager for operations for the Orbital Sciences launch systems group,  said during a NASA press briefing that the problem with both launches had to do with a protective covering called a clamshell fairing, held onto the vehicle with frangible, or breakable, joints meant to explosively fracture when commanded to do so.

“The fairing is then in two halves and there are piston pushers that push the fairing off,” Straka explained.

But in neither launch — the OCO in 2009 or Glory last week — did the fairing come off the rocket. In both cases, it stayed put and weighed the satellite down, preventing its flight toward orbit.

“We went into this flight confident that we had nailed the fairing issue,” said Ron Grabe, executive vice president and general manager of Orbital Sciences’ launch systems group. “We went so far as to completely change out the initiation system to a system that we use on one of our other vehicles, and in the intervening years that system flew successfully three times.”

Specifically, the company had previously used a hot gas system to drive the pistons that would push the fairing halves apart. But they traced the OCO launch loss to an initiation failure in the hot gas system. Orbital Sciences redesigned the Taurus XL rocket to use a cold gas system, starting with a pressurized bottle of nitrogen, just like the one in use on their Minotaur rocket.

NASA’s Bretthauer said she and others in the agency are heavy-hearted, but also baffled that their review of the OCO failure didn’t rule out the same mishap for Glory.

“We really thought we had it right,” she said. “We obviously never would have launched if we had not strongly believed the OCO failure had been mitigated.”

Kopp, a solar physicist at CU Bouder’s Laboratory for Atmospheric and Space Physics (LASP), said Bretthauer herself has asked a key question during early meetings to investigate the Glory failure: If a thorough investigation by both NASA and Orbital Sciences missed a key problem, how can we trust the process the second time around?

Meanwhile, Kopp and others are regrouping to see how much of Glory’s science can be salvaged. His instrument, the TIM, was supposed to continue an ongoing measure of the sun’s energy reaching Earth, to try to better understand the sun’s role in climate change. For now, older instruments like SORCE are carrying the torch. And it’s possible that development of missions currently in the pipeline — like the Joint Polar Satellite System (JPSS), a collaboration between NASA and NOAA — might be sped up to fill in the gaps.

More information: See also NASA’s Glory and OCO pages, a previous story about the Glory mission, and two stories about the OCO crash in 2009, here and here. This story is cross-posted at anneminard.com.

Massive 8.9 Earthquake Hits Japan; Tsunamis Predicted for Pacific Basin

Seismology
Earthquake map from the USGS of recent quake activity around Japan. Credit: USGS

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An 8.9-magnitude earthquake struck off the coast of northern Japan on March 11, one of the strongest to ever hit Japan. The massive quake has triggered tsunamis not only in Japan, but around the Pacific Basin. Walls of water and debris have inundated coastal areas of Japan, and tsunami warnings were issued for at least 20 countries and numerous Pacific islands, including coastal Russia, the western coast of Canada and the US, the Marcus Islands, Taiwan, Guam and the Hawaiian Islands, where a full coastal evactuation has been taking place throughout early Friday morning. Strong aftershocks, as strong as 6.5-magnitude continue to shake the region, (the latest U.S. Geological Survey map, above, shows 95 recent quakes in the area) and at least one nuclear power plant in Japan may be encountering problems. Images coming from Japan show widespread damage from both the quakes and the tsunamis.

The USGS reported that the epicenter of the earthquake was 373 kilometers (231 miles) northeast of Tokyo and 130 km (80 miles) east of Sendai, Honshu. Police reports from Sendai say that so 200-300 bodies have been recovered, but the total death toll will likely be much, much higher. Reports say this is the 6th largest earthquake ever monitored, and the largest in Japan in over 140 years.

Tokyo did not suffer much damage, but in northern Japan, many areas were devastated. Compounding the damage was a wall of water that rushed inland of the island nation, leveling houses and washing away boats, cars and other debris. Click here to see some shocking images from the New York Times.

Reports says Japan is evacuating thousands of people from nearby a nuclear power plant, but the current condition of the reactor core is unknown at this time. Four reactors are located near the Earthquake area. The reactors were shut down, and no leaks have been found so far, but the cooling system for the reactors may not be working correctly.

Reports via Twitter say the roof may have collapsed at JAXA Tsukuba Space Center.

Tsunami waves have now begun to wash ashore in the Hawaiian Islands. The first waves are not necessarily the strongest; waves are predicted to be 2-3 meters (6-8 ft.) in Hawaii. Tsunamis are very hard to predict, and the USGS says wave heights can vary widely.

Get the latest on the tsunami predictions from NOAA’s Pacific Tsunami Warning Center.

See this Google Map, overlaid with NOAA-predicted tsunami times.

Callan Bentley at the AGU Blogosphere has a good overview of earthquake and tsunami dynamics.

Predicted tusnami map from the March 11 earthquake. Credit: CNN

Endeavour’s Final Rollout

Endeavour begins her journey out to the launch pad under a clear, cold Florida sky. Photo Credit: Ken Kremer/www.rittenhouseastronomicalsociety.org/Dr.Kremer/K.htm

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CAPE CANAVERAL – The youngest orbiter in NASA’s shuttle fleet headed to Launch Complex 39A at Kennedy Space Center in Florida for the last time on Friday, Mar. 10. The shuttle started its slow trek out to the launch pad around 8 p.m. EST. Endeavour is being prepared for the STS-134 mission which is scheduled to launch on Apr. 19 at 7:48 p.m. EST.

The space shuttle Endeavour rolled out to Launch Complex for the final time at 7:56 p.m. EST. Photo Credit: Jason Rhian

Endeavour was wheeled out of NASA’s massive Vehicle Assembly Building (VAB) on top of the crawler-transporter. This huge, tracked vehicle moves at a blistering pace of about a mile an hour. Therefore it took Endeavour several hours to reach LC39A. What is known as “Rollout” had been slated to occur the day prior, but a front of nasty weather blew in and shuttle managers decided to push the trip back a day.

The STS-134 will be Endeavour’s 25th and final mission. It is a resupply flight to the International Space Station. Its payload consists of the Alpha Magnetic Spectrometer -02 (AMS-02) as well as the Express Logistics Carrier-3.

Endeavour, bathed in golden light, awaits her final trip out to the launch pad. Photo Credit: Ken Kremer/www.rittenhouseastronomicalsociety.org/Dr.Kremer/K.htm

“As exciting as it will be to fly this mission, what’s even more exciting is the science that this flight will bring to the International Space Station,” said STS-134 Pilot Greg Johnson. “I have no doubt that the AMS-02 will teach us new things about how the universe works and it may even show us new particles that we didn’t even know existed.”

Commander Mark Kelly will lead the crew of six, Johnson is the pilot and the Mission Specialists will be Mike Fincke, Andrew J. Feustel, Greg Chamitoff and European astronaut Roberto Vittori.

STS-134 Pilot Greg Johnson talks to reporters about his views on the upcoming STS-134 mission. Photo Credit: Jason Rhian

For a while it was uncertain whether-or-not Mark Kelly, the mission’s commander would be on this historic flight. His wife, Congresswoman Gabrielle Giffords, was severely injured when she was shot in the head by alleged gunman Jared Lee Loughner. NASA named Rick Sturckow as the mission’s backup commander. However, Kelly announced later that he would remain the mission’s commander and resumed training with his crewmates. By all accounts, it was Giffords that encouraged him to continue and it appears that she will back at Kennedy Space Center when the mission launches.

“While all of us that have worked on Endeavour are a little sad that this is her final mission, we remained focused on conducting her last flight as safely as possible,” said Endeavour’s Flow Director, Dana Hutcherson.

Reflected in the waters of the Kennedy Space Center turn basin, Endeavour heads out for her date with history. Photo Credit: Ken Kremer/www.rittenhouseastronomicalsociety.org/Dr.Kremer/K.htm

Endeavour was constructed after the loss of Challenger in 1986. The orbiter first flew in 1992. After the STS-134 mission concludes there will only be one flight remaining in the shuttle program, STS-135, currently slated for a June 28 launch. It has been hinted that Endeavour might end up staying at Kennedy Space Center – at the Kennedy Space Center Visitor Complex. However, an official announcement has yet to be made.

Endeavour is the youngest orbiter in the shuttle fleet, this resupply flight to the International Space Station will be the last mission of its 19-year career. Photo Credit: Jason Rhian

New Amazingly Life-like Android Better Than Star Trek’s Data

Henrik Scharfe and his look-alike, the Geminoid DK. Credit: Geminoid DK

Even though the Star Trek character “Data” was played by a human, this new android might be more life-like. Watch the video, and I think you’ll agree that it is hard to tell (at first) that this is a robot. It’s called Geminoid DK, built by the Intelligent Robotics lab at Osaka University and designed by professor Hiroshi Ishiguro. Just like Data was modeled after his creator Doctor Noonian Soong, the Geminoid DK is created in the likeness of professor Henrik Scharfe of Aalborg University in Denmark. Not sure if it can whistle or if it remembers every fact to which it is exposed, but Geminoid DK has a better hairdo (and beard) than Data, and it can smile.


“All of the movements and expressions of Geminoid DK are remote controlled by an operator with a computer, who uses a motion-capture system that tracks facial expressions and head movements. Turn your head and the Geminoid does the same; move your mouth and the android follows suit,” IEEE Spectrum reports.

The Geminoid is going to be used for researching “emotional affordances” in human-robot interaction, the novel notion of “blended presence,” as well as cultural differences (from different continents) in the perception of robots.

This is the third in a series of life-like robots built by Ishiguro – the first was made to look like Ishiguro himself, the second resembled a young Japanese model. Ishiguro and Sharfe are working together on this latest robot project.

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For more info see the Geminoid DK website.

Source: IEEE Spectrum via EarthSKy Blog

Runaway Star Creates Quite a Shock

A fast-moving star, Alpha Camelopardalis, creates a stunning bow shock in this new image from WISE. Credit: NASA/JPL-Caltech/WISE Team

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Faster than a speeding bullet, this supergiant star looks like it might be wearing a red cape. Alpha Camelopardalis, the bright star in the middle of this image, is a runaway star, moving at incredible speeds – astronomers believe could be zooming along at somewhere between 680 and 4,200 kilometers per second (between 1.5 and 9.4 million miles per hour). The speed of this star is so fast, a huge bow shock is being created as the star moves through space. Alpha Cam’s bow shock can’t be seen in visible light, but WISE’s infrared detectors allow us to see this arc of heated gas and dust around the star.

Runaway stars are kicked into motion either through the supernova explosion of a companion star or through gravitational interactions with other stars in a cluster. The WISE team explains the bow shock:

“Because Alpha Cam is a supergiant star, it gives off a very strong wind. The speed of the wind is boosted in the forward direction the star is moving in space. When this fast-moving wind slams into the slower-moving interstellar material, a bow shock is created, similar to the wake in front of the bow of a ship in water. The stellar wind compresses the interstellar gas and dust, causing it to heat up and glow in infrared.”

Just as astronomers aren’t quite sure about the speed Alpha Cam is traveling, its distance is also somewhat uncertain, but it is probably somewhere between 1,600 and 6,900 light-years away. It is located in the constellation Camelopardis, near Ursa Major. (Right ascension: 4h 54m 03.0113s, declination: +66° 20′ 33.641”)

The colors used in this image represent specific wavelengths of infrared light. Stars are seen primarily in blue and cyan (blue-green), because they are emitting light brightly at 3.4 and 4.6 microns. Green represents 12-micron light, primarily emitted by dust. The red of the blow shock represents light emitted at 22 microns.

Source: WISE

James Elliot, Discoverer of Uranus Ring System, Dies

James Elliot, 1943–2011

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Astronomer James Elliot, a professor at MIT, has passed away at the age of 67. Elliot was part of a team of astronomers from Cornell University that discovered the rings around the planet Uranus in 1977. Elliot specialized in the techniques of planetary astronomy, particularly stellar occultations, to probe planetary atmospheres and the physical properties of small bodies in the outer solar system and beyond. Of particular interest to him was Pluto, Triton, Kuiper Belt objects and extrasolar planets. Steve Tilford from Steve’s Astro Corner knew Elliot personally and has written a very nice retrospective on Elliot’s life.

March 19, 2011… “SuperMoon” or “SuperHype”?

Full Moon Schedules
Credit: JPL/NASA

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I mean no disrespect for those who enjoy the study of astrology. Some of the greatest astronomers of the past were also astrologers. To practice either line requires a deep understanding of our solar system, its movements and the relationship to the celestial sphere. The only thing I have difficulty swallowing is how a perfectly normal function could wreak havoc on planet Earth. Does an astrological prediction of an upcoming “Extreme SuperMoon” spell impending disaster – or is it just one more attempt to excite our natural tendencies to love a good gloom and doom story? That’s what I set about to find out…

On March 19, 2011 the Moon will pass by Earth at a distance of 356,577 kilometers (221,567 miles) – the closest pass in 18 years . In my world, this is known as lunar perigee and a normal lunar perigee averaging a distance of 364,397 kilometers (226,425 miles) happens… well… like clockwork once every orbital period. According to astrologer, Richard Nolle, this month’s closer than average pass is called an Extreme SuperMoon. “SuperMoon is a word I coined in a 1979 article for Dell Publishing Company’s HOROSCOPE magazine, describing what is technically termed a perigee-syzygy; i.e. a new or full Moon (syzygy) which occurs with the Moon at or near (within 90% of) its closest approach to Earth (perigee) in a given orbit.” says Richard. “In short, Earth, Moon and Sun are all in a line, with Moon in its nearest approach to Earth.”

Opinions aside, it is a scientific fact when the Moon is at perigee there is more gravitational pull, creating higher tides or significant variations in high and low tides. In addition, the tidal effect of the Sun’s gravitational field increases the Moon’s orbital eccentricity when the orbit’s major axis is aligned with the Sun-Earth vector. Or, more specifically, when the Moon is full or new. We are all aware of Earth’s tidal bulges. The average tidal bulge closely follows the Moon in its orbit, and the Earth rotates under this tidal bulge in just over a day. However, the rotation drags the position of the tidal bulge ahead of the position directly under the Moon. It produces torque… But is it above average torque when the Moon is closer? It you ask a geologist, they’ll tell you no. If you ask an astronomer, they’ll tell you that just about any cataclysmic Earth event can be related to stars. But if you ask me, I’ll tell you that you should draw your own opinion. Even the American Meteorlogical Society states: “Tidal forces contribute to ocean currents, which moderate global temperatures by transporting heat energy toward the poles. It has been suggested that in addition to other factors, harmonic beat variations in tidal forcing may contribute to climate changes.”

Credit: Richard Nolle
“SuperMoons are noteworthy for their close association with extreme tidal forces working in what astrologers of old used to call the sublunary world: the atmosphere, crust and oceans of our home planet – including ourselves, of course. From extreme coastal tides to severe storms to powerful earthquakes and volcanic eruptions, the entire natural world surges and spasms under the sway of the SuperMoon alignment – within three days either way of the exact syzygy, as a general rule.” says Nolle. “Obviously it won’t be the case that all hell will break loose all over the world within a few days either side of the SuperMoons. For most of us, the geocosmic risk raised by SuperMoon alignments will pass with little notice in our immediate vicinity. This is a rather roomy planet, after all. But the fact remains that a SuperMoon is planetary in scale, being a special alignment of Earth, Sun and Moon. It’s likewise planetary in scope, in the sense that there’s no place on Earth not subject to the tidal force of the perigee-syzygy.”

If you take the time to really look at Nolle’s work, you’ll find that he does not believe earthquakes and volcanic eruptions go wandering all over the planet. They happen in predictable locations, like the infamous “Ring of Fire” around the Pacific plate. “If you’re in (or plan to be in) a place that’s subject to seismic upheaval during a SuperMoon stress window, it’s not hard to figure out that being prepared to the extent that you can is not a bad idea. Likewise, people on the coast should be prepared for extreme tidal surges. Severe storms on the other hand can strike just about anywhere, so it behooves us all to be ready for rough weather when a SuperMoon alignment forms.”

Does this mean I’m about to buy into astrology? Not hardly. But what I do believe in is respect for other’s work and opinions. It’s very obvious that Nolle has done his astronomy homework – as well as paying close attention to current political and social situations. “That said, there’s no harm in making sensible preparations for this year’s SuperMoons.” quips Richard. “The worst that can happen, if the worst doesn’t happen, is that you end up with a stock of fresh batteries and candles, some extra bottled water and canned goods, maybe a full tank of gas and an evacuation bag packed just in case. (The US Department of Homeland Security has a detailed evacuation kit inventory that, to quote them, “could mean the difference between life and death”.) And maybe you’ll think twice about being in transit and vulnerable to the weather hazards and delays that are so common during SuperMoon alignments. These are the kind of sensible precautions that can make a big difference if the worst does come to pass.”

What do I believe will happen during an Extreme SuperMoon? I think if we aren’t having two snowstorms followed by a nocturnal tornado and then chased down by a week of flooding in Ohio, that the March Worm Moon will appear to be about 30% brighter and about 15% larger than a “normal” full Moon. If I were an astrophotographer, I’d be getting out my camera (and hip waders) to do a few comparison shots with upcoming full Moons. But considering all things are equal?

I think I’ll just stay home.

Be sure to visit Richard Nolle’s page SuperMoon for more insight!

Astronomers Continue to Monitor Asteroid Apophis

Apophis (circled) in a composite of five exposures taken on January 31 with the University of Hawaii 2.2-meter telescope on Mauna Kea. Image by D. Tholen, M. Micheli, G. Elliott, UH Institute for Astronomy.

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Asteroid Apophis continues to be an object of interest for astronomers. Even though the possibility of an Earth impact by the now-famous asteroid has been ruled out during its upcoming close encounter on April 13, 2029, this close flyby will significantly change Apophis’s orbit, and astronomers are uncertain how that could affect future encounters with our planet. For that reason, astronomers have been eager to obtain new data to further refine the details of the 2029 encounter. However, for three years, the asteroid’s orbit had it “hiding” behind the Sun, but it has now emerged. This newest image of Apophis was taken on January 31, 2011, using the University of Hawaii’s 2.2-meter telescope on Mauna Kea, and astronomers from UH at Manoa say they will make repeated observations of this potentially dangerous near-Earth asteroid.

Astronomers measure the position of an asteroid by comparing with the known positions of stars that appear in the same image as the asteroid. As a result, any tiny error in the catalog of star positions, due for example to the very slow motions of the stars around the center of our Milky Way galaxy, can affect the measurement of the position of the asteroid.

“We will need to repeat the observation on several different nights using different stars to average out this source of imprecision before we will be able to significantly improve the orbit of Apophis and therefore the details of the 2029 close approach and future impact possibilities,” said astronomer David Tholen, one of the co-discoverers of Apophis, who made the latest observations along with graduate students Marco Micheli and Garrett Elliott.

They obtained the new images when the 270-meter (900-foot) diameter asteroid was less than 44 degrees from the sun and about a million times fainter than the faintest star that the average human eye can see without optical aid.

The astronomers will be taking advantage of Apophis’s position for the next few months, as its elliptical orbit around the Sun will take it back into the sun’s glare this summer, making observations – and measurements of its position – impossible. However, in 2012, Apophis will again become observable for approximately nine months. In 2013, the asteroid will pass close enough to Earth for ultraprecise radar signals to be bounced off its surface.

“Radar observations are important because we can estimate orbital parameters and provides us lots of information about an asteroid’s surface features and internal structure, and how they may have formed,” said Lance Benner, an astronomer at JPL, who specializes in radar imaging of near-Earth asteroids. “We need to know these things if we are going to deflect one of these.” Speaking at the American Geophysical Union conference in 2009, Benner said radar is the most powerful astronomical technique for both finding new asteroids and measuring their orbits.

“We can measure their velocity to less than 1mm per second, and do this up to 20 million kilometers from earth. Radar helps us compute the trajectory much farther into the future – even up to 300 years, giving us much more advance notice.” Benner said they can routinely image asteroids at 7.5 meters per pixel, and a new system at the Goldstone radar facility will be able to get the resolution down to 1 meter per pixel.

On April 13, 2029, Apophis will come closer to Earth than the geosynchronous communications satellites that orbit Earth at an altitude of about 36,000 km (22,000 miles). Astronomers say Apophis will then be briefly visible to the naked eye as a fast-moving starlike object.

Source: University of Hawaii Institute for Astronomy

Where In The Universe Challenge #140

It’s time once again for another Where In The Universe Challenge. Name where in the Universe this image was taken and give yourself extra points if you can name the telescope or spacecraft responsible for the image. Post your guesses in the comments section, and check back on later at this same post to find the answer. To make this challenge fun for everyone, please don’t include links or extensive explanations with your answer. Good luck!

UPDATE: The answer has been posted below.

This is the nebula BFS 29 surrounding the star CE-Camelopardalis, as seen by the WISE spacecraft. This nebula can be found hovering in the band of the night sky comprising the Milky Way. “BFS” stands for Blitz, Fich, and Stark — the three astronomers who identified and cataloged this nebula back in 1982. The “29” means that it’s the 29th object in their catalog. Learn more about this image on the WISE website.