We’re getting a lot of visitors to our site today, many searching for information about earthquakes, tsunamis, and the ‘SuperMoon’ phenomenon. Just to be clear, the Moon did not cause the earthquake in Japan. Several scientists have posted articles online today clarifying the topic, and all of them, in no uncertain terms, agree that the the upcoming perigee of the Moon — where it is closer than usual in its orbit to Earth — had nothing to do with the earthquake and ensuing tsunami. Tammy discussed this yesterday, but as we often do, we’ll also point you in the direction of an article by astronomer Phil Plait about this topic, and another by Ben Goldacre, who completely debunks an article that appeared in the Daily Mail about the possibility of a connection between the two events.
In addition, Dr. Jim Garvin, chief scientist at NASA’s Goddard Space Flight Center, has provided some answers to questions about the ‘supermoon’ phenomenon, below:
Question: What is the definition of a supermoon and why is it called that?
Garvin: ‘Supermoon’ is a situation when the moon is slightly closer to Earth in its orbit than on average, and this effect is most noticeable when it occurs at the same time as a full moon. So, the moon may seem bigger although the difference in its distance from Earth is only a few percent at such times.
It is called a supermoon because this is a very noticeable alignment that at first glance would seem to have an effect. The ‘super’ in supermoon is really just the appearance of being closer, but unless we were measuring the Earth-Moon distance by laser rangefinders (as we do to track the LRO [Lunar Reconnaissance Orbiter] spacecraft in low lunar orbit and to watch the Earth-Moon distance over years), there is really no difference. The supermoon really attests to the wonderful new wealth of data NASA’s LRO mission has returned for the Moon, making several key science questions about our nearest neighbor all the more important.
Question: Are there any adverse effects on Earth because of the close proximity of the moon?
Garvin: The effects on Earth from a supermoon are minor, and according to the most detailed studies by terrestrial seismologists and volcanologists, the combination of the moon being at its closest to Earth in its orbit, and being in its ‘full moon’ configuration (relative to the Earth and sun), should not affect the internal energy balance of the Earth since there are lunar tides every day. The Earth has stored a tremendous amount of internal energy within its thin outer shell or crust, and the small differences in the tidal forces exerted by the moon (and sun) are not enough to fundamentally overcome the much larger forces within the planet due to convection (and other aspects of the internal energy balance that drives plate tectonics). Nonetheless, these supermoon times remind us of the effect of our ‘Africa-sized’ nearest neighbor on our lives, affecting ocean tides and contributing to many cultural aspects of our lives (as a visible aspect of how our planet is part of the solar system and space).
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.”
At the end of the movie “Apollo 13,” when the character of Jim Lovell says “I look up at the Moon and wonder, when will we be going back, and who will that be?” he probably didn’t have anything like the Google Lunar X PRIZE in mind. Similarly, when the GLXP was announced back in 2007, the founders had no idea that nearly 30 teams would be vying for the $30 million in incentive prizes to return to the Moon’s surface with a robotic craft.
Will Pomerantz, the former Senior Director of Space Prizes from the X PRIZE Foundation recalled an advisory committee meeting several years ago before the prize was announced. “We went around the room and asked everyone to estimate how many teams are going to compete in this,” Pomerantz said. “The answers ranged from zero on the low end to maybe a dozen or fifteen at the absolute max and that probably came either for myself or from Peter Diamandis, our founder. The fact that we have almost thirty blows us away, and we couldn’t be more thrilled.”
The X PRIZE Foundation recently announced the official roster of 29 teams that will attempt to send a robot to the Moon that travels at least 500 meters and transmit video, images, and data back to the Earth. The organization says this signifies a “new era of exploration’s diverse and participatory nature.”
The teams are headquartered all over the world — seventeen different headquarter nations — and most of the teams are actually multinationals, so team members are working in almost seventy different countries on every continent except for Antarctica.
“This is going to be the first time anything has been on the lunar surface since the final Soviet robotic mission in 1976,” Pomerantz said and those of us in the states really haven’t seen any data directly from the lunar surface since 1972, so we think that there’s at a ton to be learned scientifically, but also there’s a huge inspirational factor there for people to be able to see those images again.”
Of course, the robotic missions being designed are much less complicated and expensive than a human mission to the Moon.
The concepts range from snake-like robots that slither along the surface to ball-shaped vehicles that can shift their mass internally move along the lunar surface to small robotic vehicles – “not too much bigger than the cell phone you’ve got your pocket,” Pomeranzt said – to rovers that look very much NASA- or ESA-designed vehicles. Others won’t rove at all, but reignite their engines to take off and fly to another location. This may allow them to explore totally different types of terrain that is totally inaccessible to a rover.
The landing sites that the various teams are shooting for differ as well. “Essentially everyone is going on the near side for obvious communication reasons,” Pomerantz said. “Almost everyone is going in a fairly low latitude and going in the equatorial zones.”
There are bonus prizes of several million additional dollars for teams that can go to particular sites, such the South Pole, where they could possibly confirm the findings at the LCROSS impact site, or if they go back to visit one of the Apollo landing sites or one of the sites of a non-human mission.
“I know that causes some concern for some people,” Pomerantz said. “People very rightly want to make sure that we are being respectful of those treasured historical sites. But I think it is important to recognize that no one values those sites more than the men and women around the world who are dedicating their careers to getting back to the surface of the Moon. They absolutely understand that those are our valuable treasures that need to be respected but they also understand that there’s an enormous amount to be gained from going back and respectfully revisiting the. There is some very interesting science that we can do by going back and seeing how the site and how those materials have changed over the past forty years.”
Why offer a prize to return to the Moon?
“We want to open the space frontier in the way similar to what we did it for the first X PRZE, the Ansari X PRIZE,” Pomerantz said. “We want to make space exploration and lunar exploration in particular radically cheaper. We think when you create a much lower price point, when you bring the price of missions down to a tenth to what it historically has been or even a hundredth of what it historically has been, you’re opening it up to a huge variety of new customers, new science communities, new industries that just can’t exist at the current price points.”
All the teams have to come up with their own funding.
“This is really a cash on delivery kind of model,” Pomerantz said. “But we don’t want to pay people to try. There are enough other people out there that are funding people to try new things. We want to reward people upon success. That means that no matter how crazy an idea might seem today, if it happens to be the best one, then we’ll reward it.”
Right now, the prize money is set to expire by the end of 2015, but the GLXP organizers are quite confident that at least one of the 29 teams will successfully reach the Moon before then. And obviously, NASA is confident, as well, as the space agency is offering a program called the Innovative Lunar Demonstration and Data Program, which is essentially $30 million dollars worth of data purchases from commercial efforts that reach the Moon.
“This is NASA saying for first time ever we are able to buy data about conducting lunar missions and about the Moon itself, rather than having to go out and pay for the acquisition of that data directly on the hopes that it will work,” Pomerantz said. “This is a great buy for NASA and I think they are getting a tremendous value and is a great way for teams to show their investors and supporters that, hey we’ve got a willing customer here. And NASA is not afraid of us; this isn’t an ‘us versus them competition.’ This is an area where our success is their success and vice versa.
Pomerantz is leaving the X PRIZE Foundation to begin work with Virgin Galactic. “I’ve loved every minute of being with the X PRIZE, but this was an opportunity just too good to pass up and I’m extremely excited about it even though I’m sad to be leaving X PRIZE.”
Take a gander at this brand new image of the Moon from the Lunar Reconnaissance Orbiter, which is one of the largest and highest resolution images ever compiled of the near-side of the Moon. For two weeks in mid-December 2010, LRO’s orbit allowed the spacecraft to remain looking straight down. Gathering over 1,300 images during this time, LRO’s imaging run allowed the team to compile a monstrous 24,000 x 24,000 pixel mosaic from the Wide Angle Camera (WAC), with a resolution of approximately 145 meters per pixel. The detail is nothing short of spectacular.
Follow-up observations of a potential ‘skylight’ in a lava tube on the Moon has revealed a cavernous lunar pit in the Marius Hills region, with a view of the interior and bottom of the pit. The sun angle, camera angle and lighting conditions were just right for the Lunar Reconnaissance Orbiter camera to look all the way down to the floor of the pit. And this is no small hole in the ground — the LRO team says this pit is about 65 meters in diameter! This latest image confirms this object is actually a subsurface cave; a lava tube close to the surface where part of it has collapsed. These lava tubes could be great locations for lunar bases that could protect human explorers from dangers such as cosmic rays, meteorite impacts, and the extreme temperature differences between the lunar day and night.
This is the fourth time that this particular lunar pit has been imaged. Since LRO is constantly orbiting the Moon and it completes a full cycle of lunar imaging each month, the team can do follow up observations of previous discoveries and re-image targets under different lighting conditions.
Previous images had revealed the dark, cave-like entrance, and another showed part of the pit wall.
For this fourth imaging run, the spacecraft slewed 43° to the east and the solar incidence angle was 34° from vertical. This was just the right angle so that if there actually was an open lava tube extending horizontally its floor would be illuminated.
The LROC team hit paydirt (or pay-regolith, if you will).
With LRO’s Narrow Angle Camera, the team was able to image a few meters under the overhang to show the interior of this sublunarean void. With this oblique angle, they were also able to capture the layered nature of the mare bedrock in the pit walls. These exposed layers give scientists important clues as to how the vast mare were deposited.
The collection of images now verifies this is actually a cavernous subsurface cave. These pits had been predicted to exist, based on the understanding of the geomorphology of mare deposits and lava flow behavior on Earth, but never directly imaged before.
The LROC team will be presenting their findings about this pit and others that have been imaged at the Lunar and Planetary Science Conference. You can read their abstract here. (pdf file).
Shortly after the loss of the Space Shuttle Challenger in 1986, seven craters on the eastern rim of the Apollo basin were named after the crew: Gregory Jarvis, Christa McAuliffe, Ronald McNair, Ellison Onizuka, Judith Resnik, Dick Scobee, Michael Smith. The Lunar Reconnaissance Orbiter Wide Angle Camera recently took this image of the region. Below is a video from the Kaguya spacecraft flying over the area.
According to OnOrbit, the crater “Onizuka” is incorrectly identified in this video. Rather, “Onizuka” is the crater next and to the right of the one labeled in the video as “The Onizuka”.
The Apollo Basin is not where I would have guessed — the area around the Moon’s equator on the near side where all the Apollo landings took place — but instead is a 524 km-diameter impact basin located within the center of the the giant South Pole-Aitken basin, (36°S, 209°E).
How often have you heard (or thought) the sentiment that all NASA really needs is a President who will issue a bold challenge for the space agency, like Kennedy did in 1961, initiating the Apollo program to the Moon? Can we ever expect to witness such a call to action again?
“It is very unlikely,” said space historian and author Andrew Chaikin, who believes Apollo was an historical anomaly. “I think for many decades people saw Apollo as a model for how to do a space program; that you get a President to get up and make a challenge and the country follows along and does great things. But that was only true that one time in the context of the Cold War.”
We went to the Moon when we did not because we were a nation devoted to exploration, Chaikin believes, but because it seemed a politically important course of action in the context of our Cold War with the Soviet Union. “Once that was accomplished, then that political imperative evaporated,” he said.
Likely, we won’t hear any bold space-related challenge in tonight’s State of the Union Address by President Obama. Given the state of the economy, NASA might be facing a cut or freeze on their budget, a fact which might emphasize how unique an event the Apollo program ended up to be.
“What is required now is the development of technologies that will allow us to explore space in a sustainable way,” said Chaikin, author of “A Man on the Moon: The Voyages of the Apollo Astronauts,” who I interviewed for the NASA Lunar Science Institute podcast, “a way that won’t break the bank and will allow us to do more and more with reliable transportation systems that get us up into low Earth orbit. Then perhaps we can build the machines that can actually be stored in space to allow us to venture beyond low Earth orbit to the Moon and even further, to Mars and other destinations in the solar system.”
Chaikin said he’s actually very excited about the work being done in the private sector, such as by SpaceX, one of several commercial space companies trying to develop new transportation systems to provide sustainable hardware and sustainable architecture. “That can allow us to really get back in the game of exploring, not only with robots as we have been doing all along, but with humans again,” Chaikin said.
But Apollo’s uniqueness doesn’t mean it wasn’t important, or hasn’t left a lasting legacy for human spaceflight, and the human race in general.
“Simply put Apollo was the opening act in a story that has no end,” Chaikin said. “It’s a story of human beings leaving their home planet and venturing out into the universe, and as far as we go into space in some distant epoch, when we are living in other star systems and venturing throughout the galaxy, Apollo will have been the first step, so it is absolutely monumental when you look at it in that scale. I think Apollo is a lasting inspiration about what humans can accomplish when they work together.”
Apollo also showed people that anything was possible. “There was a phrase that went into our language after Apollo, and that was ‘If we can put a man on the Moon, why can’t we…’ fill in the blank,” said Chaikin. “The spirit that humans can overcome monumental challenges by working together, I think, is a valid legacy of Apollo culturally.”
Chaikin said Apollo was also important because of the technology development it spurred.
“A lot of the challenges that Apollo presented forced the industries to accelerate their development,” he said, “particularly in microelectronics. It is not that NASA invented all of the microelectronics that we use today but rather that the requirements of building a moon-ship and cramming it with all of the electronics that it needed to do its job required the electronics industry to miniaturize at a faster pace, it required the development of computers that could fit on a spacecraft, it required all kinds of analytical techniques and real-time tracking of the spacecraft as it went to and from the Moon. The legacy today is all the communications technologies and information processing technology that we are surrounded by. That really got an amazing jump start as part of the Apollo program.”
And Apollo also affected our culture, in unique ways we observe even today. How often have you seen the “Earthrise” image taken by Apollo 8 or the picture of Buzz Aldrin standing on the Moon or other Apollo-related imagery in non-space-related venues?
“We got to a place where humans had never been before,” Chaikin said, “and the other lasting legacy is the view that we got from that ‘mountaintop,’ of our Earth as a very precious oasis of life in space, and a world that really is to be cherished and protected.”
We knew even as it was happening, Chaikin said, that seeing our world floating alone in space was perhaps the most profound impact of the voyage.
“In fact, if you look at the front page of the New York Times the very day after Frank Borman and his crew became the first humans to orbit the Moon,” Chaikin said, “you will see an essay by a poet named Archibald MacLeish talking about the impact of that view and the perspective of us as ‘brothers in the eternal cold riding on spaceship Earth.’ So this is one of the things sets Apollo apart from other earlier explorations is that we were experiencing it as it happened through live television and we were actually absorbing and processing the impact in real time.”
But then, humans being as attention-challenged as we are, it didn’t take very long for all of it to become old hat and to kind of recede into history. “And that is where we are today,” Chaikin said.
That being said, Chaikin does not see the Moon as a “been there, done that” world.
“As you know, we’ve been finding frozen water at the poles of the Moon and this is a completely different view of the Moon than we had 40 years ago,” Chaikin said. “And there are more and more intricacies that we are finding all the time. The Moon itself is a Rosetta Stone for deciphering the history of the solar system, and is profoundly valuable world for us on so many levels. And it is a spectacular place. The Apollo astronauts – I’ve spent hours talking to all of them about the Moon, about the experience of being on the Moon and they just say it is a spectacular place.”
“It is too bad that the political impetus for going to the Moon was so short-lived because it was part of the Cold war,” Chaikin continued, “and looking back we can see why that was the case. It is too bad we lost interest in the Moon and it has taken us so long to turn our attention back to the Moon and all it has to offer.”
Listen to the entire interview with Chaikin on the NLSI podcast, which can also be heard on the 365 Days of Astronomy podcast.
For more information about Andrew Chaikin, see his website, andrewchaikin.com
When people look out of the corner of their eyes, they often don’t see things very clearly. But that’s not the case for the Lunar Reconnaissance Orbiter’s cameras. Occasionally LRO’s cameras are commanded to look off to the side at extreme angles, and the results, thought not frequent, are incredible. This stunning image of the central uplifts inside of Aitken Crater was taken on January 11, 2011. Here, LROC was looking over the southwest ridge of its central peak, and in the distance the lower portion of the northeastern walls of Aitken crater itself is just visible. To quote the Fred Haise character in the movie Apollo 13, this image makes me tempted to take a spacecraft down and “do some prospecting.” …
Mostly, LRO looks straight down for its images, but has collected a limited number of these oblique views of the lunar surface. They are very useful for engineering purposes, but also provide a unique view for visualizing key geologic features on the lunar surface — like Aitken. And usually, they are beautiful shots.
Aitken Crater(~135 km in diameter) is of interest because it is is one of the most geologically diverse settings on the farside. The floor of the crater is covered in mare basalt, which are quite rare on the lunar farside, and lunar scientists are still trying to figure out why. Aitken is also on the northern rim of the great South Pole-Aitken basin, the oldest and largest impact basin on the Moon and one of the oldest and largest impact basins in the whole Solar System! Further exploration of the South Pole-Aitken basin is one of the highest priorities for planetary science in the next decade.
A new study reveals that the water within the Apollo Moon rocks – and within the Moon itself — likely came from comets bombarding the nascent lunar surface, shortly after it formed following an impact event with a young Earth and Mars-sized protoplanet. The recent findings of abundant water at the lunar poles by the LCROSS impactor and across the Moon’s surface by various spacecraft have turned the long-standing notion of a dry Moon on its head, and the past year and a half, researchers have been trying to determine where this unexpected water came from.
“The water we are looking at is internal,” said Larry Taylor from the University of Tennessee, Knoxville, a member of an international team. “It was put into the moon during its initial formation, where it existed like a melting pot in space, where cometary materials were added in at small yet significant amounts.”
Using secondary ion mass spectrometry, the researchers measured the water signatures within rocks returned from the Apollo 11, 12, 14, and 17 missions that landed on the moon between 1969 and 1972. They found the chemical properties of the lunar water were very similar to signatures seen in three different comets: Hyakutake, Hale-Bopp and Halley.
The team found significant water in the lunar mineral apatite from both mare and highlands rocks, which indicates “a role for water during all phases of the Moon’s magmatic history,” the team wrote in their paper. “Variations of hydrogen isotope ratios in apatite suggest sources for water in lunar rocks could come from the lunar mantle, solar wind protons and comets. We conclude that a significant delivery of cometary water to the Earth–Moon system occurred shortly after the Moon-forming impact.”
Even though comet impacts may also have created the Earth’s oceans, Taylor said the water signatures from the mass spectrometer show that the water on the Earth and Moon are different, as apatite has a ratio of the deuterium and hydrogen that are distinctive from those in normal Earth water.
“The values of deuterium/hydrogen (D/H) that we measure in apatite in the Apollo rock samples is clearly distinguishable from water from the Earth, mitigating against this being some sort of contamination on Earth,” said James Greenwood of Wesleyan University, who led the research team.
Initially after the Apollo program, the Moon was believed to extremely dry. Many of the rocks returned by the astronauts and also the Soviet Luna program contained trace water or minor hydrous minerals, but those signatures were attributed to terrestrial contamination since most of the boxes of the Apollo program used to bring the Moon rocks to Earth leaked. This led the scientists to assume that the trace amounts of water they found came from Earth air that had entered the containers. The assumption remained that, outside of possible ice at the moon’s poles, there was no water on the moon.
Forty years later, a trio of spacecraft found evidence of water across the surface of the Moon: The Chandrayaan-1 spacecraft’s Moon Mineralogy Mapper (M Cubed) found that infrared light was being absorbed near the lunar poles at wavelengths consistent with hydroxyl- and water-bearing materials. A spectrometer on the re-purposed Deep Impact probe showed strong evidence that water is ubiquitous over the surface of the moon, and archival data from a Cassini Moon flyby also agreed with the finding that water appears to be widespread across the lunar surface.
“This discovery forces us to go back to square one on the whole formation of the Earth and moon,” said Taylor. “Before our research, we thought the Earth and moon had the same volatiles after the Giant Impact, just at greatly different quantities. Our work brings to light another component in the formation that we had not anticipated — comets.”
Taylor added that the existence of hydrogen and oxygen – water – on the moon can literally serve as a launch pad for further space exploration.
“This water could allow the moon to be a gas station in the sky,” said Taylor. “Spaceships use up to 85 percent of their fuel getting away from Earth’s gravity. This means the moon can act as a stepping stone to other planets. Missions can fuel up at the moon, with liquid hydrogen and liquid oxygen from the water, as they head into deeper space, to other places such as Mars.”