How to Handle Moon Rocks and Lunar Bugs: A Personal History of Apollo’s Lunar Receiving Lab

Apollo 11 crew in quarantine talking with President Richard Nixon. Credit: NASA

50 lbs. of moon rocks. That’s how much weight was allocated for the Apollo 11 astronauts to bring back lunar samples to Earth. But this would be the first time materials from another world would be brought to our planet. What should be done with these alien rocks, and could they possibly be a threat to life as we know it?

What started out as a seemingly straightforward idea of building a facility to store and study rocks from the Moon ended up becoming a power struggle between engineers building the facility and scientists who wanted to study the rocks and those who wanted to save the world from biological disaster — not to mention even more squabbling between the various governmental agencies and politicians. In the middle of it all was James McLane, Jr. one of the engineers tasked with the early planning for the Manned Spaceflight Center –now known as Johnson Space Center in Houston — and in particular, he led a group to determine the requirements and design concept of NASA’s Lunar Receiving Laboratory.

James C. McLane Jr. in 1971.  Photo courtesy of James McLane Jr.
James C. McLane Jr. in 1971. Photo courtesy of James McLane Jr.

“We started the Manned Spaceflight Center from scratch and a cadre of people envisioned what we should have for the space program’s ground facilities,” said McLane, in an interview from his home with Universe Today. “A whole range of facilities were recommended. For a year or so I went from one design review to another to add my two bits as to how things might be done. The new facilities included a big manned centrifuge, electronics labs, and a thermal vacuum lab with a couple of very big space simulation chambers to test the Apollo spacecraft and its onboard crew under conditions similar to those to be found during the lunar missions. There was just about everything you could think of that was needed to support the Apollo program.”

While engineers at the MSC were intent on designing unique, world-class facilities (as well as rockets and spacecraft to take humans to the moon) scientists were excited about the prospect of researching pristine lunar materials.

Lunar Receiving lab concept drawing. Credit: NASA
Lunar Receiving lab concept drawing. Credit: NASA

During this time, a couple of young MSC scientists, chemist Don Flory and geologist Elbert King had been given responsibility of designing the airtight sample return containers in which lunar samples would be brought back to Earth. But, said McLane, no one had given much thought as to how the rocks should be handled or stored once they were brought back to Earth. “There really wasn’t much direction on what should be done after we got them back to Earth,” he said. “Oh, there were scientific committees of course, but for some reason this was down low on their priority list. I think they were thinking more about the research they were going to do with the rocks.”

But one day Flory and King showed up in their boss’s office and said since they had the responsibility for the container they were a little concerned what would be done with it after the astronauts returned the samples. They suggested that, at least, the containers ought to be opened in a vacuum chamber.

“They asked, ‘Does anyone around the Center have a small vacuum chamber where we can open these boxes?’ And that started the whole business of what would happen to the lunar samples and what was required to do that,” said McLane. “A small office was setup under the Assistant Director of Engineering, Aleck Bond, and I was assigned to head it. We were charged with determining what was needed to receive, protect, catalog, and distribute the materials collected from the surface of the moon. We were guided and assisted by a committee appointed by NASA headquarters, consisting mostly of people who had been selected, or expected to be selected as principal investigators for some of the many examinations and experiments proposed for the lunar samples.”

The initial plan called for a clean room approximately “ten feet by ten feet by seven feet” where the sample box could be opened under vacuum conditions and repackaged for distribution to various researchers.

But some NASA officials concluded just a single room wouldn’t be sufficient, and quickly came up with a plan for a 2,500 square foot research facility where the lunar samples would not only be stored, but studied as well. After more discussion, an 8,000 square-foot version was proposed.

Scientists in the Lunar Receiving Laboratory. Credit: NASA
Scientists in the Lunar Receiving Laboratory. Credit: NASA

Working with the scientific advisory committee to develop a workable plan for the ever-growing and changing proposed facility turned out to be an interesting challenge for McLane and his team.

“The biggest challenges were political,” McLane said. “All the scientists involved in studying the samples had laboratories of their own. They didn’t want to do anything unless it was going to benefit their facility back home. Others were suspicious that we were trying to appropriate activities that weren’t in the Manned Spacecraft Center’s charter at the expense of other NASA Centers. So, it was difficult to get everybody to cooperate and agree on just on the initial receiving procedure. A few of the experiments such as those to determine low level radiation properties of the samples were very time dependant. Thus it became evident that the facility and equipment required to perform those experiments would have to be located very near the point where the samples were first available. That point was Houston, and it particularly rankled some of the scientists to see new state-of-the-art facilities and equipment being located at Houston rather than at their home laboratories.”

“I had never worked with high level scientists before, and our advisory committee usually consisted of people who were at the level of principal assistants to Nobel Prize winners,” McLane continued.”Overall, it was a great group to work with, with one important exception. They each reserved the right to change his mind. It was not unusual for us to settle a contentious issue only to have it brought up again some weeks later. This caused some real schedule problems, but the instigator would plead ’Well, I was just wrong before’, or ‘I changed my mind’, often ignoring schedule and reality.

For example, one issue was whether to use glove boxes or use a closed container with mechanical manipulators (McLane equated them to the toy grappling machines in restaurants, only a little fancier) to work with the moon rocks. It took many discussions and debates to decide, and the decision would make a big different on what direction the engineers needed to go for building the lab, and they had a limited amount of time to decide.

McLane was also surprised about all the different scientific speculation that took place. “Some of the leading scientists of this country thought the moon was covered with several hundred feet of lunar dust and thought that when we landed on the moon the spacecraft would sink into the dust,” he said. “Fortunately that didn’t happen. Others thought the rocks on the moon, sitting in hard vacuum and bombarded with radiation and meteorites, that when first exposed to air they might catch on fire or explode. The speculations by good, smart, reputable people were just unlimited. But I guess they were trying to think of all the possibilities. We were fortunate that no one forced us to plan for any of these extreme speculations. Overall, our advisors did a good job of things.”

The Lunar Receving Lab shortly after it was built. Credit: NASA
The Lunar Receving Lab shortly after it was built. Credit: NASA

But then at one of the meetings in Washington to meet with advisors at NASA Headquarters, a scientist from the Public Health Service showed up and asked how NASA was going to protect against contamination of the Earth by lunar microorganisms.

McLane said the initial reaction by everyone else was, “What?”

For a couple of years a small group of scientists (which included a young and relatively unknown scientist named Carl Sagan) had been discussing the remote possibility that lunar samples brought back to Earth might contain deadly organisms that could destroy life on Earth. Even the spacecraft and the astronauts themselves could possibly bring back non-terrestrial organisms that could be harmful. Several governmental agencies, including the Department of Agriculture, the US Army, and the National Institute of Health got wind of this idea — and perhaps blew it a little out of proportion — and NASA was forced to take action to prevent a possible biological disaster.

“The ‘lunar bugs’ as we called them,” said McLane, “well, nobody really believed there was life on the Moon, especially something that might affect people – make them sick or kill off our civilization, that sort of thing.”

McLane said that the first time Deke Slayton, head astronaut at the time, heard about this, he just about “flew out the window.”

“He said, ‘No way is somebody going to step in and put these restraints on the program. It’s difficult enough to just fly to the moon without all these precautions about contamination.’ But NASA had meetings with the Surgeon General of the US, and he took the attitude, ‘How much is the Apollo program going to cost – $20 billion or so? I don’t think it is outlandish to set aside one percent of that to guard against great catastrophe on Earth.'”

“We said that we would take on the challenge of guarding against organisms, but the Surgeon General would have to justify it to the Congress, about the increased costs to the program,” McLane recalled. “And he did. So that got settled. We developed a scheme and it was approved. Everyone had to accept it, there wasn’t any choice.”

That changed the entire complexion of what McLane and his team had to accomplish before astronauts could go to the Moon. What started out a just a small clean room would now have to be a research lab, plus a quarantine facility. Plans for the facility grew to an 86,000 square foot structure that would cost over $9 million.

Lunar Receiving Lab.  This drawing illustrates the complex design of the LRL, with its several different components including Lunar Sample Laboratory, Astronaut Reception Area, Radiation Laboratory, and Support and Administration. Credit: NASA
Lunar Receiving Lab. This drawing illustrates the complex design of the LRL, with its several different components including Lunar Sample Laboratory, Astronaut Reception Area, Radiation Laboratory, and Support and Administration. Credit: NASA


“We had to devise all the precautions,” said McLane, “as well as the facilities and procedures for quarantine of the astronauts, as well as accepting the samples and initiating tests on the rocks that had to be done quickly behind absolute biological barriers to test for any contamination before anything could be distributed to the scientific community. It was very interesting work.”

The LRL had accommodations for all the people and equipment that needed to be quarantined. “The astronauts were picked up in the ocean and they had to wear a special suit that was supposedly impervious to ‘lunar bugs,'” McLane said. “The astronauts were put into a modified Grumman Airstream trailer and delivered to Houston, trailer and all, waving at everyone through the windows, and talking to the president. They were taken to the Lunar Receiving Lab and placed in quarantine. It was comfortable in there, but the astronauts didn’t particularly like being in quarantine. We tried to limit the number of people who went into quarantine with them, but inevitably there were a few people– mostly ambitious secretaries and that sort of thing— who intentionally violated procedure and exposed themselves to the hypothetical lunar bugs and had move into the quarantine quarters.” The astronauts stayed in quarantine for three weeks.

First lunar samples arrive from Apollo 11.  Credit: NASA
First lunar samples arrive from Apollo 11. Credit: NASA

By the time Apollo 11 launched McLane had moved on to other projects. “My part of the organization was the engineering directorate, and I was only charged with determining the requirements for the facility and staffing the facility,” he said. “Once we reached the point where the design had come along and the staffing was pretty well up, leading the lab required someone with an interest in science as opposed to engineering.”

But he watched with interest as the first mission to the Moon unfolded. He even had a place in the Mission Control VIP viewing gallery for the launch, sitting just behind science-fiction writer Arthur C. Clarke.

Of course, it was determined that there were no “lunar bugs” and the quarantine requirement was dropped after Apollo 14. But the LRL safely stored, distributed and allowed for study of the lunar samples. In 1976 a portion of the samples were moved to Brooks Air Force Base in San Antonio, Texas for second-site storage.
The LRL building is currently occupied by NASA’s Life Sciences division. It contains biomedical and environment labs, and is used for experiments involving human adaptation to microgravity.

James C. McLane Jr today.  Photo courtesy of James McLane Jr.
James C. McLane Jr today. Photo courtesy of James McLane Jr.

The lessons learned from creating the LRL will certainly be used in preparing for the first Mars sample return mission. Now, 86 years of age, will McLane offer any words of advice?

“The best that I hear now is that the techniques of isolation we used wouldn’t be adequate for a sample coming back from Mars,” he said, “so somebody else has a big job on their hands.”

McLane will be attending a special Apollo 11 celebration at Johnson Space Center – “just for the old timers,” he said.

For more information on the history of the Lunar Receiving Lab, see NASA’s “Lunar Receiving Laboratory Project History.”

Additional source: “Moon Rocks and Moon Germs: A History of NASA’s Lunar Receiving Laboratory,” Astronautics and Aeronauts, Winter 2001.

Plane of the Ecliptic

Solar eclipse. Credit: NASA

[/caption]

Plane of the ecliptic, also known as the ecliptic plane, is a phrase you will often hear in astronomy. A basic definition is that the plane of the ecliptic is the plane of the Earth’s orbit, but that does not mean much to most people. Space is a three-dimensional vacuum, which you can think of as a kind of pool with the planets suspended in it. The Earth orbits the Sun on a particular angle and its orbit is elliptical in shape. The orbit is often shown as an ellipse made of dotted lines with the Sun at its center. If you made this ellipse a solid surface and extended it infinitively, then you would have the plane of the ecliptic. Actually our entire Solar System can be thought of as flat because all of the planets’ orbits are near or on this plane.

The ecliptic plane is used as the main reference when describing the position of other celestial objects in our Solar System. The angle between the plane of the ecliptic and the plane of an orbit is called the inclination. Until it was stripped of its status as a planet, Pluto was the planet with the most extreme inclination – 17°. Mercury is the only other planet with a significant inclination of 7°. There is also a 7° inclination between the plane of the Sun’s equator and the ecliptic plane. There are other celestial bodies that have a much greater inclination than any of the planets, such as Eris with a 44° inclination or Pallas with a 34° inclination.

The ecliptic plane got its name from the fact that a solar eclipse can only happen when the Moon crosses this plane to block out the Sun. Our Moon crosses the ecliptic about twice a month. A solar eclipse occurs when a new Moon crosses the ecliptic, and a lunar eclipse occurs when a full Moon crosses it.

Seasons on Earth are caused by our planet’s axial tilt of 23.5°, which causes variations in the amount of sunlight different parts of the Earth receive. This goes for all the other planets too. For example, Uranus rotates on its side with an axial tilt of 97.8°, which results in extreme variations in its seasons. The eclipse is also home to the constellations of the zodiac. There are twelve constellations in the zodiac, which are important symbols in astrology and can also be found in the Chinese calendar.  Here’s a list of all the zodiac symbols.

Universe Today has a number of articles including Virgo one of the zodiac signs and axial tilt.

You should also check out these articles on the ecliptic plane and ecliptic facts for more information.

Do not forget to tune into Astronomy Cast’s episode about the planet’s orbits.

Reference:
NASA: The Path of the Sun, the Ecliptic

Minor Planets

Main Belt Asteroids
Ceres, the recently promoted dwarf planet in the asteroid belt is still too small to be easily seen by Hubble credit: NASA/ESA/STScI

[/caption]
Minor planet is a term used to refer to a celestial object – that is not a planet or comet – which orbits the Sun. Found in 1801, Ceres, also known as a dwarf planet, was the first minor planet discovered. The term minor planet has been in use since the 1800’s. Planetoids, asteroids, and minor planets have all been used interchangeably, but the situation became even more confusing when the International Astronomical Union (IAU) committee reclassified minor planets and comets into the new categories of dwarf planets and small solar system bodies. At the same time, the IAU created a new definition of what a planet is, and Pluto was reclassified as a dwarf planet. Hydrostatic equilibrium – the ability to maintain a roughly spherical shape – is what separates dwarf planets from the more irregularly shaped small solar system bodies. The names become even more confusing because the IAU still recognizes the use of the term minor planets.

Minor planets are extremely common with over 400,000 registered and thousands more found each month. Approximately 15,000 minor planets have been given official names while the rest are numbered. When asteroids were first discovered, they were named after characters from Greek and Roman mythology like Ceres was. At first, astronomers thought that the asteroids, especially Ceres and Pallas were actually planets. Astronomers also created symbols for the first asteroids found. There were symbols created for 14 asteroids and some of them were very complex like Victoria’s symbol, which looks like a plant with three leaves growing out of an off center starburst. Soon, astronomers ran out of mythological names and started christening asteroids after television characters, famous people, and relatives of discoverers. Most names were feminine, attesting to an unnamed  tradition. As the numbers ran into the thousands, scientists started using their pets as inspiration. After an asteroid was named 2309 Mr. Spock, pet’s names were banned. That did not stop the oddness though because names such as 9007 James Bond and 6402 Chesirecat have been suggested and actually accepted.

There are a number of different categories that minor planets fall into including asteroids, Trans-Neptunian objects, and centaurs. There  are various types of asteroids, although most of them can be found in the asteroid belt, which is the region of space between Mars and Jupiter. Trans-Neptunian objects are celestial bodies found orbiting beyond Neptune, and centaurs are celestial bodies with unstable orbits located between Jupiter and Neptune. The categories also overlap, making classifying things a nightmare. For example, Ceres is a dwarf planet and minor planet, additionally it can also be classified as an asteroid.

Universe Today has a number of articles including astronomers find new minor planet and why Pluto is no lone a planet.

You can also check out these articles on asteroids and the solar system.

Astronomy Cast has an episode on the asteroid belt you will want to listen to.

Reference:
Wikipedia

Habitable Planet

Habitable zone

[/caption]
The term “habitable planet” seems rather broad. Does it mean that it is habitable for humans? Is it merely capable of supporting some other form of life? Quite simply, planetary habitability refers to a planet’s ability to both develop and sustain life.

Unfortunately, scientists have had to base their calculations for a habitable planet on Earth’s characteristics and do some guesswork. Some of the factors that astronomers look at when evaluating a planet’s habitability are mass, surface characteristics, orbit, rotation, and geochemistry.

One of the most basic assumptions that astronomers make when searching for a habitable planet is that it has to be terrestrial. This means that the planet is composed mostly of rock and metal and has a solid surface. A gas giant on the other hand has no solid surface, which makes it an unlikely candidate for supporting life. Mass is also an important factor, because low mass planets have too little gravity to keep their atmosphere. They also do not have live volcanoes and other geologic activity, which helps temper the surface to support life, because they lose energy as a result of a small diameter. Planets with high orbital eccentricity – the irregularity of the orbit – have a greater fluctuation in surface temperatures because they are closer to the Sun at some points and much further away at other points in the orbit. In order to be habitable, a planet has to have a moderate rotation. If there is no axial tilt then there are no change of seasons, and if the axial tilt is too severe than the planet will have a difficult time achieving homeostasis – balance. Another assumption astronomers make when determining planetary habitability is that life on other planets will also be carbon-based. The four elements most important for life are oxygen, nitrogen, carbon, and hydrogen. With so many considerations, it is not surprising that scientists have a difficult time determining whether a planet can sustain life.

Astronomers are searching for habitable planets in other solar systems too. They have started by searching in the habitable zones of other solar systems. A habitable zone is the region in space with conditions most favorable for supporting life. Astronomers are unsure exactly what the extent of the habitable zone of our Solar System is. Earth is located in the center of it, but it may even extend as far as Mars, and it almost reaches Venus. The habitable zone and planetary habitability focus on carbon-based life, so they do not help predict other forms of life.

Universe Today has a number of articles you should take a look at including the habitable zone and number of habitable planets.

You should also check out habitable planets and habitable planets are common.

Astronomy Cast has an episode on the search for water on Mars, which tells why finding water is a clue to finding life.

“That’s the Way It Is” — Apollo Supporter Walter Cronkite Dies


Newscaster Walter Cronkite has passed away at the age of 92. He was admired and known for his enthusiastic coverage NASA’s space missions, from the early Mercury launches, through the ground-breaking Gemini missions, to the subsequent moon landings — which at times left him speechless — and the space shuttle program.
Continue reading ““That’s the Way It Is” — Apollo Supporter Walter Cronkite Dies”

Solar Cycle Triggers La Nina, El Nino-like Climate Shifts

[/caption]

Researchers have discovered a link between the 11-year solar cycle and tropical Pacific weather patterns that resemble La Niña and El Niño events.

When it comes to influencing Earth’s climate, the Sun’s variability pales in recent decades compared to greehouse gases — but the new research shows it still plays a distinguishable part.

The total energy reaching Earth from the sun varies by only 0.1 percent across the solar cycle. Scientists have sought for decades to link these ups and downs to natural weather and climate variations and distinguish their subtle effects from the larger pattern of human-caused global warming.

Co-authors Gerald Meehl and Julie Arblaster, both affiliated with the National Center for Atmospheric Research in Boulder, Colorado, analyzed computer models of global climate and more than a century of ocean temperature records. Arblaster is also affiliated with the Australian Bureau of Meteorology.

In the new paper and a previous one with additional colleagues, the researchers have been able to show that, as the sun’s output reaches a peak, the small amount of extra sunshine over several years causes a slight increase in local atmospheric heating, especially across parts of the tropical and subtropical Pacific where Sun-blocking clouds are normally scarce.

That small amount of extra heat leads to more evaporation, producing extra water vapor. In turn, the moisture is carried by trade winds to the normally rainy areas of the western tropical Pacific, fueling heavier rains.

As this climatic loop intensifies, the trade winds strengthen. That keeps the eastern Pacific even cooler and drier than usual, producing La Niña-like conditions.

“We have fleshed out the effects of a new mechanism to understand what happens in the tropical Pacific when there is a maximum of solar activity,” Meehl said. “When the sun’s output peaks, it has far-ranging and often subtle impacts on tropical precipitation and on weather systems around much of the world.”

The result of this chain of events is similar to a La Niña event, although the cooling of about 1-2 degrees Fahrenheit is focused further east and is only about half as strong as for a typical La Niña.

True La Niña and El Nino events are associated with changes in the temperatures of surface waters of the eastern Pacific Ocean. They can affect weather patterns worldwide.

Although the Pacific pattern in the new paper is produced by the solar maximum, the authors found that its switch to an El Niño-like state is likely triggered by the same kind of processes that normally lead from La Niña to El Niño.

The transition starts when the changes of the strength of the trade winds produce slow-moving off-equatorial pulses known as Rossby waves in the upper ocean, which take about a year to travel back west across the Pacific.

The energy then reflects from the western boundary of the tropical Pacific and ricochets eastward along the equator, deepening the upper layer of water and warming the ocean surface.

As a result, the Pacific experiences an El Niño-like event about two years after solar maximum — also about half as strong as a true El Niño. The event settles down after about a year, and the system returns to a neutral state.

“El Niño and La Niña seem to have their own separate mechanisms,” Meehl said, “but the solar maximum can come along and tilt the probabilities toward a weak La Niña. If the system was heading toward a La Niña anyway,” he adds, “it would presumably be a larger one.”

The study authors say the new research may pave the way toward predictions of temperature and precipitation patterns at certain times during the approximately 11-year solar cycle.

In an email, Meehl noted that previous work by his team and other research groups has shown that “most of the warming trend in the first half of the 20th Century was due to an increasing trend of solar output, while most of the warming trend in the last half of the 20th Century and ever since has been due to ever-increasing GHG (greenhouse gas) concentrations in the atmosphere from the burning of fossil fuels.”

The new paper appears this month in the Journal of Climate, a publication of the American Meteorological Society. (Sorry, it’s not yet available online.)

Source: Eurekalert

Ancient Domes Reveal 3.45-billion-year-old Life History

[/caption]

Ancient, dome-like rock structures contain clues that life was active on Earth 3.45 billion years ago, according to new research — and the findings could help shed light on life’s history on Earth and other planets, including Mars.

Abigail Allwood, who studies planetary habitability at NASA’s Jet Propulsion Laboratory, led the research. She and her colleagues studied stromatolites, which are dome- or column-like sedimentary rock structures formed in shallow water, layer by layer, over long periods of geologic time.

Geologists have long known that the large majority of the relatively young stromatolites they study—those half a billion years old or so—have a biological origin; they’re formed with the help of layers of microbes that grow in a thin film on the seafloor.Close-up, cross-section view of the interior of a domical stromatolite. The black layers are the "cooked" organic remains of Early Archean microbial mats.  Credit: Abigail Allwood

The microbes’ surface is coated in a mucilaginous substance to which sediment particles rolling past get stuck.

“It has a strong flypaper effect,” said John Grotzinger, a Caltech geologist and a study co-author. In addition, the microbes sprout a tangle of filaments that almost seem to grab the particles as they move along. “The end result,” Grotzinger explains, “is that wherever the mat is, sediment gets trapped.”

So in a young stromalite, dark bands like those seen in the close-up cross section at left indicate organic material. But 3.45 billion years ago, in the early Archean period of geologic history, things weren’t quite so simple.

“Because stromatolites from this period of time have been around longer, more geologic processing has happened,” Grotzinger says. Pushed deeper toward the center of Earth as time went by, these stromatolites were exposed to increasing, unrelenting heat. This is a problem when it comes to examining the stromatolites’ potential biological beginnings, he explains, because heat degrades organic matter. “The hydrocarbons are driven off,” he says. “What’s left behind is a residue of nothing but carbon.”

As such, geologists debate whether or not the carbon found in these ancient rocks is diagnostic of life.

Allwood and her team turned to the texture and morphology of the rocks themselves, from samples gathered in Western Australia. The samples, says Grotzinger, were “incredibly well preserved.” Dark lines of what was potentially organic matter were “clearly associated with the lamination, just like we see in younger rocks. That sort of relationship would be hard to explain without a biological mechanism.”

Allwood set about trying to find other types of evidence. She looked at what she calls the “microscale textures and fabrics in the rocks, patterns of textural variation through the stromatolites and—importantly—organic layers that looked like actual fossilized organic remnants of microbial mats within the stromatolites.”

She saw “discrete, matlike layers of organic material that contoured the stromatolites from edge to edge, following steep slopes and continuing along low areas without thickening.” She also found pieces of microbial mat incorporated into storm deposits, which disproved the idea that the organic material had been introduced into the rock more recently, rather than being laid down with the original sediment.

“In addition,” Allwood notes, “Raman spectroscopy showed that the organics had been ‘cooked’ to the same burial temperature as the host rock, again indicating the organics are not young contaminants.”

Allwood said she, Grotzinger, and their team have collected enough evidence that it’s no longer a great leap to accept the stromatolites as biological in origin. And the researchers say the implications of the findings don’t stop at life on Earth.

“One of my motivations for understanding stromatolites,” Allwood says, “is the knowledge that if microbial communities once flourished on Mars, of all the traces they might leave in the rock record for us to discover, stromatolite and microbial reefs are arguably the most easily preserved and readily detected. Moreover, they’re particularly likely to form in evaporative, mineral-precipitating settings such as those that have been identified on Mars. But to be able to interpret stromatolitic structures, we need a much more detailed understanding of how they form.”

Both images courtesy of Abigail Allwood.

Source: Eurekalert, a media service of the American Association for the Advancement of Science (AAAS). The research appeared in online June 10 and in print June 16 in the Proceedings of the National Academy of Sciences (PNAS).

LRO Images Apollo Landing Sites (w00t!)

The Apollo 14 landing site imaged by LRO. Credit: NASA

[/caption]

As anticipated, NASA released images of the Apollo landing sites taken by the Lunar Reconnaissance Orbiter (LRO). The pictures show the Apollo missions’ lunar module descent stages sitting on the moon’s surface, as long shadows from a low sun angle make the modules’ locations evident. Also visible are the tracks left where the astronauts walked repeatedly in a “high traffic zone” and perhaps by the Modularized Equipment Transporter (MET) wheelbarrow-like carrier used on Apollo 14. Wow.

As a journalist, I (most of the time) try to remain objective and calm. But there’s only one response to these images: W00T!


Apollo 11 landing site as imaged by LRO. Credit: NASA
Apollo 11 landing site as imaged by LRO. Credit: NASA

These first images were taken between July 11 and 15, and the spacecraft is not yet in its final mapping orbit. Future LROC images from these sites will have two to three times greater resolution.
Apollo 15 site by LRO. Credit: NASA
Apollo 15 site by LRO. Credit: NASA

These images are the first glimpses from LRO,” said Michael Wargo, chief lunar scientist, NASA Headquarters, Washington. “Things are only going to get better.”

The Japanese Kaguya spacecraft previously took images of some of the Apollo landing sites, but not at a high enough resolution to show any of the details of the lander or any other details. But here on these images, the hardware is visible. “It’s great to see the hardware on the surface, waiting for us to return,” said Mark Robinson, principal investigator for LRO.

Robinson said the LROC team anxiously awaited each image. “We were very interested in getting our first peek at the lunar module descent stages just for the thrill — and to see how well the cameras had come into focus. Indeed, the images are fantastic and so is the focus.”

Apollo 16 by LRO. Credit: NASA
Apollo 16 by LRO. Credit: NASA

The Lunar Reconnaissance Orbiter Camera, or LROC, was able to image five of the six Apollo sites, with the remaining Apollo 12 site expected to be photographed in the coming weeks.

The spacecraft’s current elliptical orbit resulted in image resolutions that were slightly different for each site but were all around four feet per pixel. Because the deck of the descent stage is about 12 feet in diameter, the Apollo relics themselves fill an area of about nine pixels. However, because the sun was low to the horizon when the images were made, even subtle variations in topography create long shadows. Standing slightly more than ten feet above the surface, each Apollo descent stage creates a distinct shadow that fills roughly 20 pixels.

Apollo 17 LRO. Credit: NASA
Apollo 17 LRO. Credit: NASA

The image of the Apollo 14 landing site had a particularly desirable lighting condition that allowed visibility of additional details. The Apollo Lunar Surface Experiment Package, a set of scientific instruments placed by the astronauts at the landing site, is discernable, as are the faint trails between the module and instrument package left by the astronauts’ footprints.
Zoomed in Apollo 14 image by LRO. Credit: NASA
Zoomed in Apollo 14 image by LRO. Credit: NASA

Source: NASA

Chandrayaan-1 Rescued from Failure

India Moon Mission
Artist concept of Chandrayaan-1 orbiting the moon. Credit: ISRO

[/caption]
The Chandrayaan 1 spacecraft, India’s moon orbiting satellite was almost lost earlier this year, Indian Space Research Organization revealed, as the star tracking system overheated and malfunctioned. The system helps determine and maintain the spacecraft’s orientation. Engineers were able to patch in the gyroscopes and another instrument to help maneuver the spacecraft, but they are not sure how long this jury-rigged system will work. At this point, determining the spacecraft’s future might be difficult, and differing statements from various officials reflect that.

“We are not sure how long we will be able to sustain it. The life of Chandrayaan-I designed for two years may be reduced,” said ISRO spokesman S. Satish.

ISRO chief Madhavan Nair said the star tracking system cannot be recovered, but he dismissed suggestions that the sensor’s failure might reduce the life span of the spacecraft.

“The life (of the spacecraft) is not dependent on this instrument. This instrument is used only for orientation of the spacecraft,” he said. “The sensor cannot be recovered at this stage and we hope that the remaining part of this mission will be completed.”
Chandrayaan-1's first picture of the moon.  Credit:  ISRO

Chandrayaan-1 launched in October 2008 and suffered from overheating shortly after it began operations in lunar orbit in November, but the ISRO was able to change the spacecraft’s orientation and cut down on the amount of time the instruments were used to compensate.

In May 2009, however, officials unexpectedly raised the orbit of the spacecraft. At that time officials said they had completed mission objectives from 100 km above the moon and raised the height of the spacecraft to 200 km to enable imaging lunar surface with a wider swath. But reports say that May is when the star tracker system malfunctioned, as well.

Nair said the star sensor is suspected to have failed because of “excessive radiation” from the Sun. He said gyroscopes are not susceptible for the kind of radiation that the sensor was subjected to. “So, we hope it will survive the remaining mission duration”.

He added more than 90 percent of the two-year mission’s objectives have already been achieved.

ISRO Scientists hope the Chandrayaan project will boost India’s capacity to build more efficient rockets and satellites, especially through miniaturization, and open research avenues for young Indian scientists. India plans to follow the Chandrayaan, which means “moon craft” in Sanskrit, by landing a rover on the moon in 2011.

Source: The Hindu

Weekend SkyWatcher’s Forecast: July 17-19, 2009

Greetings, fellow SkyWatchers! It’s a picturesque weekend to get up early as the Moon heads for the Pleiades and on towards a close encounter with Venus. With plenty of dark skies to go around and the random meteor rate a little higher than usual, why not spend some time with the constellation of Lupus? No telescope or binoculars? No problem. There’s also plenty of things to do over the next few days that only requires just your eyes and a little knowledge of the skies. I’ll see you in the backyard…

robertsFriday, July 17, 2009 – This date marks the 1904 passing of Isaac Roberts, an English astronomer who specialized in photographing nebulae. Since many deep sky objects are far too faint to be seen with the human eye, photography soon became a great way of studying them, but as the Earth moved, long exposure photography became problematic as the image also moved and blurred. Roberts’ developed a telescope/camera combination which would track, allowing for a long exposure times and perfected images. As an ironic twist, this is also the date on which a star was first photographed at Harvard Observatory!

Tonight let’s have a look at a real little power punch globular cluster located in northern Lupus— NGC 5824. Although it’s not an easy star hop, you’ll find it about 7 degrees southwest of Theta Librae,
and exactly the same distance south of Sigma Librae (RA 15 03 58 Dec –33 04 04). Look for a 5th magnitude star in the finderscope to guide you to its position southeast.

ngc_5824

As a Class I globular cluster, you won’t find any others that are more concentrated than this. Holding a rough magnitude of 9, this little beauty has a deeply concentrated core region that is simply unresolvable. Discovered by E.E. Barnard in 1884, it enjoys its life in the outer fringes of its galactic halo about 104 light-years away from Earth and contains many recently discovered variable stars. Oddly enough, this metal-poor globular may have been formed by a merger. Research on GC 5824’s stellar population leads us to believe that two less dense and differently aged globulars may have approached one another at a low velocity and combined to form this ultra-compact structure. Be sure to mark your observing notes on this one! It also belongs to the Bennett catalog and is part of many globular cluster lists.

Saturday, July 18, 2009 – Celestial scenery alert! Get up before dawn to witness the Moon graze by the Pleiades. For some observers, the pair will be separated by around half a degree; it will be an occultation event for others. Still not enough? Then be sure to look for the twin red pair of Mars and Aldebaran spaced equidistant to the Moon’s south!

alpha_draconisTonight let’s begin with the 1689 birth of Samuel Molyneux. This British astronomer and his assistant were the first to measure the aberration of starlight. What star did they choose? Alpha Draconis, which oscillated with an excursion of 39’’ from its lowest declination in May. Why choose a single star during an early dark evening? Because Alpha Draconis—Thuban—is far from bright. At magnitude 3.65, Thuban’s ‘‘alpha’’ designation must have come from a time when it, not Polaris, was the northern celestial pole star. If you’re aware that the two outer stars of the ‘‘dipper’’ point to Polaris, then use the two inner stars to point to Thuban (RA 14 04 23 Dec +64 22 33). This 300-light-year distant white giant star is no longer main sequence, a rare binary type.

ngc_6124Now head to binary Eta Lupi, a fine double star resolvable with binoculars. You’ll find it by staring at Antares and heading due south two binocular fields to center on bright H and N Scorpii—then one binocular field southwest. Now hop 5 degrees southeast (RA 16 25 18 Dec – 40 39 00) to encounter the fine open cluster NGC 6124. Discovered by Lacaille, and known as object I.8, this 5th magnitude open cluster is also Dunlop 514, Melotte 145, and Collinder 301. Situated about 19 light years away, it shows a fine, round, faint spray of stars to binoculars and is resolved into about 100 stellar members to larger telescopes. Although NGC 6124 is low for northern observers, it’s worth the wait to try at culmination. Be sure to mark your notes because this delightful galactic cluster is also a Caldwell object and counts for a southern skies binocular award.

pickeringSunday, July 19, 2009 – Want a picturesque sight before dawn? Then look for the close pairing of Venus and the Moon. Which has the greater crescent? This probably would have interested Edward Charles Pickering, who was born on this date in 1864. Pickering was the director of Harvard College Observatory for 42 years and published the first all-sky photographic map in 1902. While at Harvard, he recruited many women to work for him, including Annie Jump Cannon, Henrietta Swan Leavitt, and Antonia Maury. These women were called “Pickering’s Harem” by the scientific community – but don’t you believe any crap for one instant. In those days, it was incredibly difficult for a woman to have her academic work recognized and Edward Pickering was one of the very few men open-minded enough to realize just what these women astronomers could achieve and allow them the chance to do it!

Tonight for unaided observers, let’s begin by identifying Zeta Ophiuchi, the centermost in a line of stars marking the edge of the constellation of Ophiuchus, about a handspan north of Antares. As a magnificent 3rd magnitude blue-white Class O, this hydrogen-fusing dwarf is eight times larger than our own Sun. Hanging out some 460 light-years away, it is dulled by the interstellar dust of the Milky Way and would shine two full magnitudes brighter if it were not obscured. Zeta is a ‘‘runaway star’’—a product of a one-time supernova event of a double-star system. Now roughly halfway through its 8 million-year life span, the same fate awaits this star! Nowpoint binoculars or small scopes about three finger-widths south to have a look at Phi Ophiuchi. This is a spectroscopic double star, but it has several delightful visual companions!

Almost in between these two bright stars is our telescopic target for tonight—M107. Discovered by Pierre Mechain in 1782, and added to the catalog in 1947, it’s probably one of the last of the Messier objects to be discovered and wasn’t resolved into individual stars until studied by Herschel in 1793.

m107

M107 isn’t the most impressive of globulars, but this Class X is notable as a faint, diffuse area with a core region in binoculars and is surprisingly bright in a small telescope. It’s a curious cluster, for some believe it contains dark, dust-obscured areas, which make it unusual. Located around 21,000 lightyears away, this little beauty contains around 25 known variable stars. Visually, the cluster begins to resolve around the edges to mid-aperture, and the structure is rather loose. If sky conditions permit, the resolution of individual chains at the globular’s edges makes this globular well worth a visit!

This week’s awesome images are (in order of appearance): Isaac Roberts (historical image), NGC 5824, Alpha Draconis, NGC 6124 (credit—Palomar Observatory, courtesy of Caltech), Edward Pickering (historical image) and M107 (credit—Palomar Observatory, courtesy of Caltech). We thank you so much!