Antarctic Micrometeorites Provide Clues to Solar System Formation

The extraction of clean snow from a trench near the CONCORDIA Antarctic station. Image courtesy of J. Duprat CSNSM-CNRS

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Researchers sifting through the pristine, cold snow in Antarctica have found micrometeorites that contain a bit of a surprise. The two micrometeorites, known as particles 19 and 119, contain extremely large amounts of carbon as well as excesses of deuterium. While this high organic content usually comes from distant interstellar space where molecular clouds gather to form new stars, other clues say these space rocks likely formed in our own solar system. This contradicts long-held notions that that all organic matter with extreme deuterium excesses have interstellar origins. Additionally, the meteorites could provide information about the protplanetary disk that formed our solar system.

(A) Backscattered scanning electron micrograph of particle 119. The carbon-rich areas appear dark (arrows); the bright inclusions are dominated by Fe-Ni sulfides and silicates. (B) High-resolution TEM image of particle 19. (C) Bright-field TEM image of particle 19. The lacey carbon film (13) is indicated as black arrows; the crystalline phases are Mgrich olivines (ol), Mg-rich pyroxenes (px), and Fe-Ni sulfides (S); OM, organic matter. Glassy aggregates (GEMS candidates) are highlighted in black squares (13). Image courtesy of Science/AAAS

Jean Duprat and colleagues working at the CONCORDIA polar station located in central Antarctica recovered the two micrometeorites from 40 to 55 year-old snow. In investigating their make-up to determine where they came from, the researchers identified crystalline materials embedded in particles 19 and 119 that indicate that they formed close to our sun, and much more recently than predicted.

Their findings imply that these well-preserved micrometeorites contain a record of the cold regions of our sun’s ancient proto-planetary disk, which eventually led to the formation of our solar system.

More studies of these and other meteorites could possibly reveal details of the first deliveries of organic materials to the primitive Earth.

The findings have been published in this week’s edition of Science.

Where In The Universe Challenge #103

Here’s this week’s Where In The Universe Challenge. You know what to do: take a look at this image and see if you can determine where in the universe this image is from; give yourself extra points if you can name the instrument responsible for the image. We’ll provide the image today, but won’t reveal the answer until tomorrow. This gives you a chance to mull over the image and provide your answer/guess in the comment section. Please, no links or extensive explanations of what you think this is — give everyone the chance to guess.

UPDATE: The answer has now been posted below.

This is an infrared image from Hubble of Uranus, taken way back in 1998. The rings really stand out in infrared, so we can see that the planet is surrounded by its four major rings — and if you look closely — by 10 of its 17 known satellites.

Also visible are clouds — about 20 in all, nearly as many clouds on Uranus as the previous total in the history of modern observations. The orange-colored clouds near the prominent bright band circle the planet at more than 300 mph (500 km/h). One of the clouds on the right-hand side is brighter than any other cloud ever seen on Uranus, at least back in 1998.

Credit for this image goes to Erich Karkoschka from the University of Arizona and, of course, NASA. See more about this image at the HubbleSite.

Check back later this week for another WITU challenge!

Successful Test for Orion Launch Abort System

NASA successfully tested the pad abort system developed for the Orion crew vehicle on Thursday morning at the White Sands Missile Range near Las Cruces, New Mexico. The 97-second flight test was the first fully integrated test of the Launch Abort System developed for Orion. “It was a big day for our exploration team,” said Doug Cooke, NASA’s Associate Administrator for Exploration following the test. “It looked flawless from my point of view. This is the first abort system the US has developed since Apollo, but it uses much more advanced technologies. It was a tremendous effort to get to this point, designing such a complex system, and we’ve been working on this for about 4 years. I appreciate the amount of dedication and focus from the team. It was beautiful, a tremendous team effort.”
Continue reading “Successful Test for Orion Launch Abort System”

Your Questions about Apollo 13 Answered by Jerry Woodfill

Now that our series on “13 Things That Saved Apollo 13” is complete, NASA engineer Jerry Woodfill has graciously agreed to answer questions from our readers. We have a lot of questions, so we will post some of Jerry’s answers today and more over the next few days.

Question from Daniel Roy: Did we ever find out why Apollo 13’s trajectory was too shallow on the way back in spite of TCMs? I have trouble believing that the low impulse/ slow venting/ random pointing from ruptured tanks could explain the delta V.

Jerry Woodfill: The shallowing trajectory resulted from the lunar lander’s cooling system discharging vapor during the coast back to Earth. It was not a result of residual release of remnant gases from service module damage. No Apollo mission returned to Earth with a LM attached except for Apollo 13. For that reason the slight but, nevertheless, noticed contribution to the shallowing entry angle had to be dealt with by the Apollo 13 retro. To this day, I find it remarkable that, though the retro did not know the source of the shallowing, he was certain it would cease after the last corrective compensating burn. And, of course it did, after the LEM was jettisoned.

Question from wjwbudro about how much residual power was provided by the fuel cells after the explosion

Jerry Woodfill: Your question about how much residual power the fuel cells contributed prior to employing the emergency (or some call them reenty batteries) launched me into some research about the chemistry of fuel cell operation. I’ve always shared that the reaction of hydrogen and oxygen produce electricity with two by-products extremely useful to human space exploration, breathable oxygen and water. Both oxygen and hydrogen must be present for the reaction to continue.

For Apollo 13, the sequence of the loss of the ability of the fuel cells to produce power relates to the loss of O2 and H2 entering them. Sy Liebergot has a wonderful CDROM where he deals with “how the data read.” Sy had to contend with analyzing what was going on (IN REAL TIME) with regard to the timing of loss of the O2 cryo-tanks, the fuel cells, etc. Google Sy on the Internet, and you’ll find a wealth of information discussing the issue. My admiration of how Sy dealt with such an overwhelming failure so masterfully continues 40 years after the event. But the bottom line is…no O2 into the cells no water, oxygen, or electrical power out. That was the reason for employing the emergency batteries. The fuel cells weren’t much help after because the rupture of the plumbing caused O2 tank One’s O2 to vent into space after O2 tank 2 exploded (I always say “exploded” though some disagree contending it to be a rapid heating of cryogenic O2 being vented into space, sort of like heating air in an empty sealed container until the vessel ruptures.)

Question from science teacher Christopher Becke from Warhill High School: What were the specs of the onboard computers, both in the LM and the Command Module? What was the clock speed and how much (and what type of) memory did they have? I’m trying to impress upon my students that their graphing calculators are more powerful than the computers that brought astronauts to the moon.

Jerry Woodfill: About a year ago, I felt like comparing Apollo 13’s computer to today’s state of the art. Besides the computers (CSM and LM), the only integrated circuit contained among the millions of spacecraft parts was an octal counter in my lunar lander’s caution and warning system’s brain known as the Caution and Warning Electronic Assembly or C&WEA for short. There was an excellent article I discovered at this link from the Download Squad.

Additionally, a wealth of information is given in the Apollo Experience Report which can be accessed at this link.

These documents are a national treasure for recreating the technical history of Apollo. I authored the warning system portion of the Apollo Experience Report on the lunar lander’s Caution and Warning System.

I recall that the strength of the Apollo computer, though it was a “lightweight” in RAM and Hard-Memory, was its “multi-tasking” ability. (Better than an iPhone, since Apple chose not to include that capability presently in mine.) However, when my warning system began to ring “Program Alarms,” (warnings, five of them to be exact) this multitasking capability proved altogether helpful in making Armstrong the first man on the Moon.

One of the Apollo Computer’s “subtasks” was akin to a kind of low level housekeeping info thing which generated an alarm. But the priority executive routine of providing landing control continued undisturbed. Ignoring the program alarms by Flight Controllers Steve Bales and John Garman was a huge reason Neil Armstrong was first on the Moon, that President Kennedy’s prediction and challenge was fulfilled in that decade, and, most importantly, for me…that I didn’t go down in engineering/aerospace infamy whose warning system sounded a “false-alarm” making Pete Conrad and Allan Bean the first men on the Moon on Apollo 12. Thanks Steve and John!

Question from Greg: Should NASA be spending more time reviewing the Apollo 13 mission and other mishaps in order to better anticipate and respond more effectively to new and unexpected mishaps in future missions?

Jerry Woodfill: The neat thing about every one of these questions is they launch potential investigations which can only help future space travelers. Whether it was Apollo One, Apollo 13, Challenger or Columbia, each tragedy resulted in fixing a later situation which might have been fatal if corrective steps had not been taken to learn from failure. This question is one that I’ve addressed extensively in unpublished books I’ve authored.

Now, regarding failure to fix potentially fatal items; yes, over the course of my 45 year career, it is easy to reflect and study failures after the fact and cite instances where people, groups, circumstances resulted in disaster and tragedy. I’m one of those guilty people. I should have done a better job with regard to the Apollo One warning system. Collectively, and, perhaps, individually, we share the burden of not having done a better job for Gus, Roger, and Ed.

Specifically, I remember the final review at North American of Spacecraft 012 where Ed, Gus, and Roger sat at the front of the conference room. They were included with a NASA review panel determining how to disposition “open items” or “squawks” needing fixing before or after shipment of their Apollo One spacecraft to the Cape.

My warning system was a problem for me because it became sort of the “wolf crying boy” who is always the one to aggravate those who want to ignore a root problem blaming it on the messenger. During the initial factory tests of this, the first of the litter of subsequent Apollo Command modules, there were dozens of times the alarm system sounded Master Alarms.

In summary, virtually none were the fault of the alarm system. But, nevertheless, it was blamed until I could find the actual culprit. Some said, “The electronics are simply too sensitive ringing alarms when all that has happened is a momentary switch actuation causing a brief electrical transient which triggers that Master Alarm.”

After dealing with all the culprits, I had only one unexplained alarm remaining. This was the one I was called to present to the board which included Ed, Gus and Roger. “Next item, O2 FLOW unexplained Caution and Warning Alarm.” It was July of 1966. My wife Betty and I had been married less than a month, and here I was dealing with a life-threatening situation.

To digress here, I think the movie APOLLO 13 would have been better served with this event as the opening scene because all the players in the Apollo program were involved. I remember Apollo 7 crewman Walt Cunningham, one of the Apollo One back-up astronauts along with Wally Schirra and Donn Eisele, rooting around in the Spacecraft 012 mockup. Walt emerged with some kind of handle he had accidentally severed from the ship’s interior. Amazed and disgusted, Walt held it up for all to see. Perhaps, that was a precursor for what was to follow?

My explanation was that the O2 Hi alarm was another of those momentary transient things. I shared that nonthreatening events like a routine turning on of the cyclic accumulator demanded added O2 flow into the cabin actuating the alarm. In fact, in route to the Moon, even a urine-dump would cause the O2 flow to increase ringing the alarm. (Later, that was one of my jobs, to indicate in Apollo 11’s check-list that an O2 Hi master alarm could be expected for that reason.) If it was a problem, it would surface once more during Cape testing and be dealt with then. My assessment was accepted by the board.

On January 27th, 1967, Ed, Gus, and Roger were hours into what was called a “plugs-out” test simulating a voyage to the Moon. Suddenly came the call, “We’ve got a fire in here!” In seconds three men perished. When Deke Slayton arrived later and surveyed the interior of Spacecraft 012, he looked up at the alarm panel. The O2 flow hi light was still on. Likely, the ECS (Environmental Control System) should have called for the high flow of Oxygen feeding the fire, but I will never know if it came on before the fire to warn the astronauts to take action. So that is why I cannot “white-wash” this question because it is simply these kinds of events that result in the failures we have experienced over the course of human space flight. Whenever one happens, it is because of people like me who should have done a better job.

Question from Dirk Alan: My question is about the free return trajectory. After rounding the moon, could a spacecraft head back to earth – travel round the earth and head back to the moon? Could it round the moon and head back to earth again and again ? I’m asking if a space station would be feasible in a circumlunar orbit re-supplied now and again with fuel for course corrections to shuttle between the earth and moon?

Jerry Woodfill: The short answer is yes to all of the above. For Apollo 13, the free return trajectory has been much discussed. I’ve often reflected about it, as well. In fact, the first consideration in the rescue was to return to the free return trajectory after the explosion. (BTW, I think I erred in my No. 12 submittal of the “13 Things..” in suggesting that a lander-less-Apollo 13 would have resulted in cremating the crew days later if the explosion had occurred in the circumstance at 55 hours 54 minutes 54 seconds. They were not in the free return mode at that time having departed from it by an earlier burn.)

In actuality, the crew, shortly after the explosion, used the lander’s descent engine to return to free-return. Recently, in conjunction with Apollo 13’s 40th anniversary, added study has been done. The investigation sought to determine how close Apollo 13 would have come to Earth based on its free-return orbit. Here is the link to a YouTube video summarizing the effort. It’s really neat!

Hey, I just listened once more and watched this again. Apparently, I was right predicting the crew without the lander would have been cremated after all, five weeks later in May of 1970. Don’t ascribe this to any talent I have. It’s just lucky. But watching the video will do much to answer every question you have above about space stations, etc. You might Google other terms like Hohmann Transfer Orbit, Aldrin Cycler Orbit, Libration Points, and Sling-Shot orbits. These are strategies in orbital mechanics considered when planning planetary exploration, manned and unmanned.

Questions from Gadi Eidelheit, Quasy and Tom Nicolaides about the Hatch That Would Not Close

Jerry Woodfill: I’ve shared the account of “the hatch that would not close” virtually every time I’ve shared the Apollo 13 story. ( This is approaching a 1000 talks. Do the math. Simply telling the story once a month for nearly 40 years adds up to nearly 500 times.) One man believed the inability to make the hatch close resulted from differential pressure between the vehicles. I tend to discount that because the hatch had been open for some time stabilizing the interior atmospheric pressure throughout the assemblage.

Others who have considered the problem, think that Jack Swigert and Jim Lovell’s belief that a meteor had punctured the LM caused Jack and Jim’s hasty efforts to be flawed and inexact. The misalignment in the hurried closing was responsible. This was addressed in one of the crew debriefs I reviewed several years ago.

Now, I just had the thought, “The Apollo 13 capsule is available at the Kansas Cosmosphere.” To my knowledge, no one since the rescue has actually tried to reproduce the hatch closing problem. But, again, I simply don’t know if that has been the case. (As we press on, I’m going to be honest about what I know and don’t know. This is one of those things I really can’t answer satisfactorily.)

From Hans-Peter Dollhopf: Question about Why an Apollo 13 Movie and not an Apollo 11 Movie:

Jerry Woodfill: Another question I wanted to address among those left at the close of each of the “13 Things…” articles concerns why a movie was made about Apollo 13 and not about Apollo 11. My thought is because of the circumstance of how the movie came into production. I have a close friend named Jerry Bostick. Jerry was the lead FIDO for Apollo 13. We knew one another through the local Methodist Church, too. Jerry’s son Mike was in one of the Sunday school class sessions I taught.

Well, Mike went on to work for Ron Howard as a producer for Universal Studios. Being familiar with the Apollo 13 rescue because his dad, Jerry Bostick, had played a key role, Mike suggested to Ron Howard that Universal buy the rights to Jim Lovell’s book LOST MOON, for a movie. Incidentally, Jerry Bostick is the source of the quote, “Failure is not an option.”

Google Jerry Bostick’s name, and you’ll be able to read the story. Now had Neil Armstrong’s child worked for Ron Howard, and, if Neil had written a book focused on Apollo 11, it might have competed for an academy award like Apollo 13. Incidentally, there are moments in Apollo 11’s mission just as perilous and potentially fatal as the Apollo 11 mission. Perhaps, Nancy will let me address them in another Universe Today series! I can count a half dozen so it won’t be “11 Things That Saved Apollo 11.”

Question: Didn’t the Soviets Plan also use LOR?

Jerry Woodfill: About the Soviet Direct Ascent approach. Prior to the dismantling of the “iron curtain” and the cooling of the “Cold War”, information about Soviet Manned Space endeavors was sketchy. I found, in 1977, that a Soviet rocket scientist had proposed a lunar orbit rendezvous technique in the early days of rocketry, even before Sputnik. Unfortunately, or fortunately, with regard to America’s efforts, his approach was not accepted initially. Earliest Soviet approaches, like America’s, tended toward the Direct Ascent scheme. Probably the same debate ongoing with American lunar planners existed in the Soviet Union.

The simplicity of a single vehicle based on a NOVA class booster led at the onset. Ultimately, perhaps, as Soviets studied America’s choice of LOR, and its LEM offspring, an approach similar to America’s was pursued. Nevertheless, the ultimate Soviet booster N-1 was much more powerful than the Saturn V. (10,000,000 pounds of first stage thrust versus approximately, 7,500,000.)

I was altogether astounded to discover the evolution of the Soviet approach when sketches, and even videos, were released with the collapse of the Soviet Union and its posture of manned space secrecy. But, I still contend, that the early focused efforts by NASA championed by Dr. Houbolt on the LOR lunar architecture won out over, I believe, tardy acceptance by the same in the Soviet Union. One of the finest compliments one receives is the adoption of a competitor’s approach. Simply comparing BURAN to the Space Shuttle tends to make this case as well.

Check back tomorrow for more answers from NASA engineer Jerry Woodfill.

13 Things That Saved Apollo 13, Part 13: The Mission Operations Team

The view in Mission Control after Apollo 13 landed safely. Credit: NASA.

The phrase “last but not least” was likely never more appropriate. Though this is the last article of our “13 Things That Saved Apollo 13” series, it might be the most important. “Each time I’ve heard Jim Lovell or Fred Haise speak of the rescue,” said NASA engineer Jerry Woodfill, “they have always expressed their gratitude to the folks on the ground who contributed to saving their lives.”

And it wasn’t just the astronauts who were grateful. As a testament to the appreciation the rest of the country felt, the Mission Operations Team for Apollo 13 — those who worked in the Mission Operation Control Room (MOCR – more commonly called Mission Control) and the Mission Evaluation Room (MER) — were awarded a Presidential Medal of Freedom.

“We fulfilled the latter part of President Kennedy’s mandate,” said Woodfill, “by returning them safely to Earth.”

The Presidential Medal of Freedom awarded to the Mission Operations Team of Apollo 13. Image courtesy Jerry Woodfill.

In previous articles in this series, we’ve highlighted just a few people who made significant – and some unsung – contributions to the Apollo 13 rescue. But likely every person who was part of the mission operations team made a contribution.

The words of President Richard Nixon as he presented the medal on April 18, 1970, perhaps say it best:

“We often speak of scientific ‘miracles’ – forgetting that these are not miraculous happenings at all, but rather the product of hard work, long hours and disciplined intelligence.

The men and Women of the Apollo XIII mission operations team performed such a miracle, transforming potential tragedy into one of the most dramatic rescues of all time. Years of intense preparation made this rescue possible. The skill coordination and performance under pressure of the mission operations team made it happen. Three brave astronauts are alive and on Earth because of their dedication and because at the critical moments the people of that team were wise enough and self-possessed enough to make the right decisions. Their extraordinary feat is a tribute to man’s ingenuity, to his resourcefulness and to his courage.”

Certificate given to Woodfill for the Congressional Medal of Freedom. Image courtesy Jerry Woodfill.

But, says Woodfill, it wasn’t just those whose names are listed on the initial award.

“There were a thousand more who never were named though their contribution was huge. I could write another hundred accounts of specific acts which, had they not been done, could have resulted in disaster. There was an unseen “cloud of helpers” whom I now know helped just as much as I did though they were never recognized. These folks weren’t even NASA employees or affiliated with the supporting contractors, Grumman (GAEC) or North American Aviation (NAA). Universe Today could go on for months, on a daily basis if I could add all these accounts. Studying something for 40 years brings forth this kind of thing.”

Employees at Johnson Space Center witnessing the President presenting the Presidential Medal of Freedom to the Apollo 13 Mission Operations Team (April 1970). Image courtesy Jerry Woodfill.

But since Apollo 13 happened 40 years ago, many of those involved are no longer alive. Woodfill said astronaut Jack Swigert is an example. A 40th anniversary celebration of the Apollo 13 mission at Johnson Space Center in April included a panel discussion with Jim Lovell, Fred Haise, Gene Kranz, Glenn Lunney, John Aaron, and was moderated by Jeffrey Kluger, co-author with Lovell of the book Lost Moon.

Read Woodfill’s account of the celebration on his website.

40th anniversary celebration of Apollo 13 at Johnson Space Center. Image courtesy Jerry Woodfill.

“During that two hour exchange, I added a half dozen more insights of unique things that saved Apollo 13,” said Woodfill. “But when the Q&A launched, I all but ran to the microphone to ask the first question: ‘Jim and Fred, could you comment on Jack Swigert’s contribution?’ Their remarks were gracious and appreciative, remembering their friend and crewmate. Neither they nor the country has forgotten Jack. He is the only astronaut to be honored by a statue in Congress, as he became an elected representative in Congress from the State of Colorado. Sadly, cancer took Jack’s life before he could serve. But I think if Jack could speak to us about his experience on Apollo 13, he might select the Mission Operations Team as well. In a sense, he represents all those no longer with us. They helped make it possible for Jim and Fred to have blessed us for the past 40 years with the altogether inspirational story of the rescue of Apollo 13.”

A plaque from the three Apollo 13 astronauts thanking the mission support teams. Note the panels of the caution and warning system above the signatures. 'That was my system,' said Woodfill. 'The alarm system personified what the team’s role was providing caution, warning, and assistance for the crew’s safety.' Image Courtesy Jerry Woodfill

So, while we have only scratched the surface among the many stories of Apollo 13’s rescue, surely there are thousands more tales of people being in the right place at the right time, decisions made years earlier that led to working at NASA, and chance meetings or discussions that opened up opportunities or jogged ideas for the rescue.

Jerry Woodfill and Fred Haise at the 40th anniversary celebration of Apollo 13 at JSC. Image courtesy Jerry Woodfill.

Jerry Woodfill is an example of such a story. He was attending Rice University on a basketball scholarship, a dream that inexplicably came true.

“However, my career as a college basketball player was as dismal as America’s early endeavors in space,” Woodfill admitted. “Sadly, I hold the record of the lowest shooting percentage in Rice University history…one out of eighteen shots! And the one shot I made at Baylor University with seconds left in the first half was a desperate 35 foot pass to our center under the basket. It sailed too high and went through the hoop. My only basket was actually a bad pass! In truth, I was zero for eighteen.”

He wasn’t doing very well in his classes, either. But then President John Kennedy came to Rice University to give a speech, a speech which helped launch the US to the Moon:

“But why, some say, the moon? Why choose this as our goal? And they may well ask why climb the highest mountain? Why, 35 years ago, fly the Atlantic? Why does Rice play Texas? We choose to go to the moon in this decade and do the other things, not because they are easy, but because they are hard, because that goal will serve to organize and measure the best of our energies and skills, because that challenge is one that we are unwilling to postpone, and one which we intend to win, and the others, too.”
John F. Kennedy, in his speech at Rice University, September 12, 1962

Inspired by Kennedy’s speech, Woodfill turned in his basketball shoes and focused on his studies of electrical engineering, hoping to become part of the space program to send people to the Moon – and return them safely to the Earth.

Yes, Woodfill become one of the half million Americans teaming up together to put the first men on the Moon.

And the rest is history.

Our extreme thanks to Jerry Woodfill for sharing his story, insights, and expertise as well as his warmth, humor and passion for NASA’s mission. “Godspeed to all you Apollo 13 rescuers, past and present, known and unknown!”

The “13 Things That Saved Apollo 13” series:

Introduction

Part 1: Timing

Part 2: The Hatch That Wouldn’t Close

Part 3: Charlie Duke’s Measles

Part 4: Using the LM for Propulsion

Part 5: Unexplained Shutdown of the Saturn V Center Engine

Part 6: Navigating by Earth’s Terminator

Part 7: The Apollo 1 Fire

Part 8: The Command Module Wasn’t Severed

Part 9: Position of the Tanks

Part 10: Duct Tape

Part 11: A Hollywood Movie

Part 12: Lunar Orbit Rendezvous

Part 13: The Mission Operations Team

Also:

Your Questions about Apollo 13 Answered by Jerry Woodfill (Part 1)

More Reader Questions about Apollo 13 Answered by Jerry Woodfill (part 2)

Final Round of Apollo 13 Questions Answered by Jerry Woodfill (part 3)

Never Before Published Images of Apollo 13’s Recovery

Listen to an interview of Jerry Woodfill on the 365 Days of Astronomy podcast.

New Image Reveals Thousands of Galaxies in Abell 315

Galaxy Cluster Abell 315 as seen by ESO's 2.2 meter telescope at La Silla. Credit: ESO/J. Dietrich

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In an image akin to the Hubble Deep Field, ESO’s La Silla Observatory in Chile stared at a patch of sky about as big as a full Moon and observed thousands of distant galaxies. The Wide Field Imager on ESO’s 2.2 meter telescope zeroed in on a large group of galaxies that are part of the massive galaxy cluster known as Abell 315. But there’s more in this image—including relatively close asteroids that show up as blue, green or red trails, which lie in the main asteroid belt, located between the orbits of Mars and Jupiter. Also, invisible dark matter is revealed in this image through its gravitational effects, noticeably visible on this galaxy cluster.

Of course, not all the galaxies seen here are the same distance from us. Some are relatively close, as it is possible to distinguish their spiral arms or elliptical halos if you zoom in on this larger image, especially in the upper part of the image. The more distant galaxies appear just like faint of blobs — their light has traveled through the Universe for eight billion years or more before reaching Earth.

The concentration of about a hundred yellowish galaxies is the Abell 315 galaxy cluster. The cluster is located in the constellation of Cetus (the Whale).

The galaxies in these clusters contribute to only ten percent of the mass, with hot gas in between galaxies accounting for another ten percent. The remaining 80 percent is made of dark matter that lies in between the galaxies.

We know the dark matter is there because of its effects: the enormous mass of a galaxy cluster acts on the light from galaxies behind the cluster like a cosmic magnifying glass, bending the trajectory of the light and thus making the galaxies appear slightly distorted. By observing and analyzing the twisted shapes of these background galaxies, astronomers can infer the total mass of the cluster responsible for the distortion, even when this mass is mostly invisible. However, this effect is usually tiny, and it is necessary to measure it over a huge number of galaxies to obtain significant results. In the case of Abell 315, the shapes of almost 10,000 faint galaxies in this image were studied in order to estimate the total mass of the cluster, which amounts to over a hundred thousand billion times the mass of our Sun.

For more information see the ESO release and additional images.

Shutdown of ‘Zombie’ Satellite Unsuccessful

Artist concept of the Galaxy 15 satellite in orbit. Credit: Orbital Sciences.

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A geostationary satellite that had its “brains fried” by a solar flare (love that description by our pal Ian O’Neill at Discovery Space) stopped communicating with ground controllers last month and remains out of control. While the Galaxy 15 communication satellite is still functional, its navigation and communications system are not. The instruments remain “on” but the satellite has drifted out of its assigned orbital slot and will soon be coming close to other satellites. While it likely won’t crash into other satellites, the rogue satellite can cause problems when it enters an orbital space occupied by other satellites by “stealing” their signal, thereby interrupting other vendor’s services to customers on Earth.

Space News reports that a satellite operating at full payload power that is no longer under control is unprecedented, and the company that operates the satellite, Intelsat, is seeking advice from other satellite operators and manufacturers.

Galaxy 15 satellite before launch in 2005. Credi: Orbital Sciences.

On May 3, Intelsat tried unsuccessfully to shut down the electronics payload so that it wouldn’t interfere with any other satellites. Earlier, Intelsat tried a fruitless effort of sending between 150,000 and 200,000 commands to the satellite to coax it back into service, and then on Monday tried to force the satellite to shut down its transponders, and ultimately the satellite’s payload.

Galaxy 15, which normally operates at 133 degrees west longitude 36,000 kilometers over the equator, is now closing in on the geostationary orbital slot just two degrees away occupied by another satellite using the same bandwidth (C-band) the AMC-11 spacecraft operated by SES World Skies. With its active payload, Galaxy 15 could cause potentially severe interference with the SES satellite during a two-week period starting around May 23, according to Space News.

Galaxy 15 relays Global Positioning System (GPS) navigation information to in-flight aircraft.

The various satellite companies are working together to figure out how to deal with the problem. Check out Space News for more information.

Latest Satellite Images of Oil Spill

Satellite image from the Aqua Satellite on May 4, 2010 showing the oil spill in the Gulf of Mexico. Credit: NASA/Goddard/MODIS Rapid Response Team

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NASA’s Aqua satellite flew over the oil slick in the Gulf of Mexico on May 4, at 18:50 UTC, or 2:50 p.m. EDT, and the Moderate Imaging Spectroradiometer, or MODIS, instrument captured this visible-light image. The bulk of the spill appears as a dull gray area southeast of the Mississippi Delta. The spill is the result of an explosion on April 20, 2010 which destroyed the Deepwater Horizon oil platform operating in the Gulf 80 kilometers (50 miles) offshore. Many of the workers on the platform were killed, and about 5,000 barrels of oil per day has been released into the water. The huge oil slick is being carried towards the Mississippi River Delta. Weather and currents have cooperated so far to keep the slick away from sensitive wetlands and wildlife areas along the Gulf Coast, and oil has come ashore in a few spots in Louisiana. However, the oil is expected to reach the Louisiana, Alabama, and Mississippi shores by Thursday, May 6, and cause considerable damage to property and endanger wildlife and habitats.

See more images below, including one from the International Space Station taken today.

The oil spill as seen from the International Space Station by astronaut Soichi Noguchi. Credit: NASA/JAXA/Noguchi

This image was taken on May 5 by astronaut Soichi Noguchi on board the ISS, and posted on Twitter.

A Envisat Advanced Synthetic Aperture Radar (ASAR) image from May 2, 2010. Credit: CLS

This image from ESA’s Envisat radar, shows sea surface roughness and current flow information. Not only could the slick head towards the US mainland, but there have been fears that the Loop Current in the Gulf of Mexico could catch the oil slick and drag it south towards coral reefs in the Florida Keys. If that were to happen, the oil could flow into the Gulf Stream and be carried up to the US East Coast.

But so far, the loop does not appear to be catching the oil slick.

The Deepwater Horizon oil spill (appearing as a dull gray color) is southeast of the Mississippi Delta in this May 1, 2010, image from NASA's MODIS instrument. Credit: NASA/Goddard/MODIS Rapid Response Team

Another MODIS image from May 1 shows the oil slick as a tangle of dull gray on the ocean surface, made visible to the satellite sensor by the sun’s reflection on the ocean surface. At this point, the oil slick was southeast of the Mississippi Delta.

Close-up view of the oil spill from the ASTER satellite from May 3, 2010. A new NASA satellite image shows the extent of the growing oil spill in the Gulf of Mexico. Image credit: NASA/GSFC/METI/ERSDAC/JAROS, and U.S./Japan ASTER Science Team

The Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) instrument on NASA’s Terra spacecraft captured this image of the growing oil spill in the Gulf of Mexico on May 1, 2010. The image is located at 29.0 degrees north latitude, 88.3 degrees west longitude and covers an area measuring 79.1 by 103.9 kilometers (49 by 64.4 miles), about 32 kilometers (20 miles) west of the mouth of the Mississippi River delta. No land is visible in the image.

The varying shades of white in the image reflect different thicknesses of oil (the whiter, the thicker the oil). The source of the oil spill is visible as the bright white area in the bottom center of the image. The thickest part of the spill extends vertically from it, appearing somewhat like the ash plume of an erupting volcano. The wispy patterns of the oil spill reflect the transport of the oil by waves and currents.

A wide angle view of the oil slick on April 29, 2010. Credit: NASA/Earth Observatory/Jesse Allen, using data provided courtesy of the University of Wisconsin’s Space Science and Engineering Center MODIS Direct Broadcast system.

Sources: NASA Earth Observatory, ESA

Opportunity’s Long and Winding Road to Endeavour Crater

Opportunity's view of the far-off rim of Endeavour Crater. Credit: NASA/JPL-Caltech/Cornell University

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Back in September of 2008, Mars Exploration Rover Principal Investigator Steve Squyres announced the Opportunity rover would head out to a large, faraway crater named Endeavour, and Squyres said he hoped to one day see the view from the rim. Well, Oppy has now provided an improved view OF the rim: off in the distance in the image above are the “Endeavour Hills,” the mounds which surround the perimeter of the crater, about 13 km (8 miles) away, along with the rim of an even more distant crater, Iazu, on the right.

As the crow flies, Endeavour is about 12 km away from Oppy’s starting point in 2008, Victoria Crater. But while the intrepid rover has already traveled 7 km towards Endeavour, it still has 12 km to go, as the route chosen to avoid potentially hazardous dune fields is more like 19km, as presently charted, said Guy Webster at JPL. You can see an example of Opportunity’s circuitous driving below.

Opportunity's tracks show how the rover avoided driving through potentially dangerous sand dunes. Credit: NASA/JPL/U of AZ

The original target timing for Opportunity reaching Endeavour was about two years, but since the science team has had the rover spend several weeks stopping at interesting targets of study along the way, the rover will definitely not make it to Endeavour by September 2010. It might take another year, or even two.

Additionally, it is now winter on Mars, and according to A.S.J. Rayl’s Rover Update from the Planetary Society, Opportunity is now roving for only about 30 minutes at a time, which enables it to cover only 30-to-50 meters on a drive sol. And, the rover is also taking Martian days off to re-charge its batteries. Record cold temps this winter (down to -37 C) on Mars is slowing the aging rover.

But back in March Oppy reached 20 kilometers (12.43 miles) of total driving in its 74 months on Mars. Pretty amazing for a piece of hardware that was supposed to last six months and drive about 600 meters. Later this month, Oppy will surpass the Viking Lander 1’s record of 6 years and 116 days to become the longest-lived robot on Mars. The Spirit rover has already surpassed that record, but it is unknown if the rover is only hibernating and we’ll hear from it when it warms up again, or if Spirit is no longer with us (sniff!).

Endeavour Crater is 21 kilometers (13 miles) in diameter, which is about 25 times wider than Victoria crater. The view in the top image is an area about 140 kilometers (about 90 miles) wide.

Orbital view of Opportunity's location from THEMIS. mage Credit: NASA/JPL-Caltech/Arizona State University

This view shows a top-down look at the area from orbit, and is a mosaic of daytime infrared images taken by the Thermal Emission Imaging System (THEMIS) camera on NASA’s Mars Odyssey orbiter.

Additionally, a new gif “movie” was released this week showing how Oppy emerged from Victoria crater about a year and a half ago. Click here to see it.

Sources: JPL, Mars Rover homepage, Planetary Society

Carnival of Space #152

This week’s Carnival of Space is hosted by Ryan Anderson over at Martian Chronicles.

Click here to read the Carnival of Space #152

And if you’re interested in looking back, here’s an archive to all the past Carnivals of Space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, let Fraser know if you can be a host, and he’ll schedule you into the calendar.

Finally, if you run a space-related blog, please post a link to the Carnival of Space. Help us get the word out.