Back to School Inspiration: Be That Light

Are you an educator, heading back to another year of teaching and need a little inspiration? — or do you know a teacher that is back in the classroom after summer break? Then this awesome little video is for you. It’s the latest from “Symphony of Science” and it features our friend Dr. Jeff Goldstein and a speech he made at the National Science Teachers Association Conference this year, “Science – It’s Not a Book of Knowledge … It’s a Journey.” Dr. Jeff is a science educator and planetary scientist and is the Director of National Center for Earth and Space Science Education. He is passionate about teaching and is admittedly “emotional about science,” as we all should be.

Here’s why he helped make this video: “Right now, in this very moment, we wanted to poetically and passionately reaffirm to teachers why they went into teaching, and for the millions of teachers across America, recognize their selfless and noble dedication to lighting the way. This is a heartfelt thank you to teachers for their unwavering dedication to the next generation.”

If you need more inspiration, see Dr. Jeff’s Blog on the Universe

Two Into The Blue: One Engineer’s Gemini Reflections

The Gemini Program taught NASA the essential basics of space flight. Robert L. Adcock was an engineer that participated on all ten flights. He has written these experiences down in Two into the Blue. Photo Credit: NASA.gov

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It is probably one of the least understood, but most crucial, (in terms of landing a man on the Moon) programs in U.S. space flight history. After just fifteen minutes in space (and all of it sub-orbital) President John F. Kennedy tasked NASA with sending astronauts to the lunar surface. NASA completed the Mercury Program and moved on to Gemini, which had a crew of two and would work to teach NASA the most basic elements of space flight.

Extravehicular activity (EVA), rendezvous and dealing with the microgravity environment were all issues tackled by NASA on the Gemini Program. Gemini was essentially NASA’s “classroom” – teaching the space agency the lessons needed to fly to the Moon.

Most books on Gemini follow the basic path, an overall of all spaceflight efforts and then a chronological history of the program and how it taught NASA how to live and work in space. Two into the Blue – breaks from this mold and tells the Gemini story from one engineer’s perspective, sharing along the way his thoughts and feelings during this time.

Two Into The Blue is published by Xlibris Corp and provides a fresh perspective on the Gemini missions. Image Credit: Xlibris Corp/NASA.gov

Two into the Blue is written by Robert L. Adcock, published by Xlibris Corp and weighs in at a light 142 pages. Adcock worked for about 36 years within the Aerospace Industry, his earliest experiences coincided with the development of rockets and the spacecraft that were among the first that the U.S. sent into orbit. Adcock grew up in Tennessee, graduated from the University with a BSEE and followed with a Doctorate in Business Administration that he received from Florida State in 1977.

Two into the Blue details Adcock’s experiences during this crucial time for the U.S. space program. The book is largely written from his perspective, telling his experiences during NASA’s Gemini years. Given that most books discussing the Mercury, Gemini and Apollo Programs are essentially identical in format makes Two into the Blue a welcome departure with new details and fresh stories. Adcock participated in some capacity every one of the Gemini Program’s ten flights.

Each of the Gemini missions was dedicated to techniques that would pave the way for the Apollo flights to the Moon. Without the Gemini series of missions, NASA would never have been able to learn all of the techniques needed to send a man to the Moon and return him safely to the Earth. Despite its vital role, Gemini is largely forgotten by most of the general public today. With NASA’s current future uncertain, this book allows one to look back to a time when the U.S. crewed space flight program’s future was bright.

Two into the Blue is a short read, but it is a great book for someone preparing to take a trip and who will be stuck in an airport or in a car. It’s also great for space enthusiasts seeking to find out more about the Gemini Program and the history that surrounded these important missions.

The Gemini Program followed the single-man Mercury flights, sending two astronauts to orbit and preparing NASA for trips to the Moon. Photo Credit: NASA.gov

Space Debris Problem Getting Worse, New Report Says

Space Debris in polar orbit. Image Credit: ESA

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In the movie WALL-E, the Earth is surrounded by a dense field of orbiting junk. The problem of space debris is not that bad yet, but is potentially heading in that direction. A new report released today by the National Research Council says the problem of space debris is getting worse and has passed a “tipping point.” The report says that while NASA has done a good job using their available resources to research the issue, decreased funding and increased responsibilities for the space agency is not a good combination for the future, and NASA has not been able to keep pace with increasing hazards posed by abandoned equipment, spent rocket bodies, and other debris orbiting the Earth.

“The current space environment is growing increasingly hazardous to spacecraft and astronauts,” said Donald Kessler, chair of the committee that wrote the report and retired head of NASA’s Orbital Debris Program Office. “NASA needs to determine the best path forward for tackling the multifaceted problems caused by meteoroids and orbital debris that put human and robotic space operations at risk.”

There’s enough debris currently in orbit to continually collide and create even more debris, raising the risk of spacecraft failures, the report notes. In addition, collisions with debris have disabled and even destroyed satellites in the past, as in the collision in 2009 between an Iridium satellite and a inoperative Russian satellite. Several recent near-misses of the International Space Station requiring evasive maneuvers and sending astronauts to the Soyuz vehicles as a precaution underscores the value in monitoring and tracking orbital debris as precisely as possible.

It is fitting that Kessler lead this committee: he laid out a scenario back in 1978 called the Kessler Syndrome where the amount and size of objects in Earth’s orbit could eventually become so large that they would continually collide with one another and create even more debris, eventually causing a “cascade” of collisions which could make low Earth orbit unusable for decades.

From the new report, it appears the Kessler Syndrome is not just an abstract event that might occur in the future. It’s happening now. The amount of debris is now growing exponentially, as just two collisions since January 2007 has doubled the total number of debris fragments in Earth’s orbit, according to the NRC report.

NASA had asked for the report; specifically, NASA’s chief of safety and mission assurance, Bryan O’Connor, asked the NRC in 2010 to independently examine the agency’s work on debris.

“We thank the National Research Council for their thorough review in this report,” said NASA spokeswoman Beth Dickey. “We will study their findings and recommendations carefully and use them to advise our future actions in this important area of work.”

The report, however, does not provide NASA with many specific ideas but says NASA should develop a formal strategic plan to better allocate its limited resources devoted to the management of orbital debris. In addition, removal of debris from the space environment or other actions to mitigate risks may be necessary.

For example, NASA should initiate a new effort to record, analyze, report, and share data on spacecraft anomalies. This will provide additional knowledge about the risk from debris particulates too small to be cataloged under the current system yet large enough to potentially cause damage.

The report also suggests more work internationally on this problem, since it is a global problem caused by other nations besides the US. Over the past decade and a half, the world’s major space agencies have been developing a set of orbital debris mitigation guidelines aimed at stemming the creation of new space debris and lessening the impact of existing debris on satellites and human spaceflight. Most agencies are in the process of implementing or have already implemented these voluntary measures which include on-board passive measures to eliminate latent sources of energy related to batteries, fuel tanks, propulsion systems and pyrotechnics.

But the growing number of developing countries that are launching using satellites, and they need to be encouraged to use these measures as well.

In addition, NASA should lead public discussion of orbital debris and emphasize that it is a long-term concern for society that must continue to be addressed.

Congress also needs to be aware of the problem and provide adequate funding for the issue.

You can read the report here. (free as a pdf download).

Sources: NRC press release, Washington Post

NASAs Lunar Mapping Duo Encapsulated and Ready for Sept. 8 Liftoff

Twin GRAIL Lunar Mappers being enclosed with payload fairing atop Delta II rocket. Spacecraft technicians monitor the movement of a section of the clamshell-shaped Delta payload fairing as it encloses NASA's twin Gravity Recovery and Interior Laboratory spacecraft at Space Launch Complex 17B on Cape Canaveral Air Force Station in Florida. Liftoff is slated for Sept. 8 at 8:37 a.m. EDT. Credit: NASA/Jim Grossmann

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NASA’s powerful lunar mapping duo of GRAIL spacecraft are now poised for liftoff in just one weeks time on Thursday, Sept. 8.

Mission managers held a Flight Readiness Review on Wednesday (Aug.31) and gave a tentative approval to begin fueling the Delta II rockets second stage on Sept. 2 and 3 after evaluating all issues related to the rocket, launch pad and payloads.

Launch preparations are proceeding on schedule towards an early morning lift off from the seaside Space Launch Complex 17B (SLC-17B) at Cape Canaveral Air Force Station, Florida. There are two instantaneous launch windows at 8:37:06 a.m. and 9:16:12 a.m. EDT lasting one second each.

“Launch vehicle and spacecraft closeouts will begin on Tuesday, and the Launch Readiness Review is also scheduled for Tuesday morning,” NASA KSC spokesman George Diller told Universe Today.

“This morning’s launch countdown dress rehearsal went fine.”

“Delta II 2nd stage fueling has been rescheduled for Friday and Saturday [Sept. 2 and 3]. Last evening a software error was found in the launch processing system data base. ULA (United Launch Alliance) decided they would like to look for any additional errors before the fueling begins. There is no impact to the launch date and currently no work is scheduled on Sunday or on Labor Day,” said Diller.

The launch period extends through Oct. 19, with liftoff occurring approximately four minutes earlier each day in case of a delay. The flight plan was designed to avoid a pair of lunar eclipses occurring on December 10th, 2011 and June 4th 2012 which would interfere with the missions operations and science.

The team is keeping a close watch on the weather as the season’s next Atlantic Ocean storm heads westwards. Katia has just been upgraded to Hurricane status and follows closely on the heels of the continuing vast destruction, misery and deaths caused by Hurricane Irene earlier this week.

“The preliminary weather forecast is favorable for launch day as long as the wind remains out of the west as is currently forecast for that time of the morning,” Diller told me.

Twin GRAIL Lunar Mappers are secured atop Delta II rocket and await enclose in the Delta payload fairing. The fairing will protect the spacecraft from the impact of aerodynamic pressure and heating during ascent and will be jettisoned once the spacecraft is outside the Earth's atmosphere. Credit: NASA/Jim Grossmann

The twin probes known as GRAIL-A and GRAIL-B (Gravity Recovery and Interior Laboratory) were encapsulated inside the clamshell like payload fairing on Aug. 23 The nearly identical spacecraft are mounted side by side and sit atop the Centaur upper stage.

The fairing shields the spacecraft from aerodynamic pressures, friction and extreme heating for the first few minutes of flight during ascent through the Earth atmosphere.

This Delta II Heavy booster rocket is the most powerful version of the Delta II family built by ULA. The booster’s first stage is augmented with larger diameter solid rocket motors.

GRAIL was processed for launch inside at the Astrotech payload processing facility in Titusville, Fla. See my GRAIL spacecraft photos from inside the Astrotech clean room facilities here.

“The GRAIL spacecraft inside the handling can departed Astrotech and arrived at the launch pad, SLC-17B on Aug. 18” said Tim Dunn, NASA’s Delta II Launch Director in an interview with Universe Today. “The spacecraft was then hoisted by crane onto the Delta II launch vehicle and the spacecraft mate operation was flawlessly executed by the combined ULA and NASA Delta II Team.”

An Integrated Systems Test (IST) of the mated booster and payload was completed on Aug. 22

Technicians prepare twin GRAIL spacecraft for enclosure in the Delta payload fairing. Credit: NASA/Jim Grossmann

The dynamic duo will orbit the moon in a tandam formation just 50 kilometers above the lunar surface with an average separation of 200 km. During the 90 day science phase the goal is to determine the structure of the lunar interior from crust to core and to advance understanding of the thermal evolution of the moon.

GRAIL-A & GRAIL-B will measure the lunar gravity field with unprecedented resolution up to 100 times improvement on the near side and 1000 times improvement for the far side.

NASA’s twin GRAIL Science Probes ready for Lunar Expedition
GRAIL B (left) and GRAIL A (right) spacecraft are mounted side by side on top of a payload adapter inside the clean room at Astrotech Space Operations facility. The spacecraft await lunar launch on Sept. 8, 2011. Credit: Ken Kremer

Read Ken’s continuing features about GRAIL

GRAIL Lunar Twins Mated to Delta Rocket at Launch Pad
GRAIL Twins ready for NASA Science Expedition to the Moon: Photo Gallery

Your Astrophotos of Comet Garradd

Astrophoto: Comet Garradd passing by M71 by Brian McGaffney
Comet Garradd passing by M71. Credit: Brian McGaffney

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We asked for ’em and you sent ’em in. Here are your photos of Comet Garradd, the best-looking comet in the sky right now, as it is brightening and moving faster as it gets closer to us and the Sun. This comet will reach perihelion on December 23, 2011. We start with Brian McGaffney who captured this photo of the Comet C/2009 P1 Garradd when it crossed star cluster M71. The image was taken from the Nutwood Observatory in Bancroft, Ontario on August 26th, 2011 at 11PM. Brian took the photo using an Apoggee U16M and a 14 inch astrograph and an ME mount.

But wait — there’s more!

Garradd and M71. Credit: Rich Richins. Click image to see larger version on Richard's website, Enchanted Skies.

Richard Richins sends us this image from his location in Las Cruces, New Mexico. Check out his website, Enchanted Skies.

Comet Garradd passing by the open cluster M71 on August 27, 2011. Credit: Efrain Morales Rivera. Click to view on Flickr

This image was taken on August 27, 2011 in Victoria, Aguadilla, Puerto Rico by Efrain Morales Rivera from the Jaicoa Observatory. “Comet Garradd’s tail is brushing along the core of cluster M71,” Effrain noted, adding the equipment he used was LX200ACF 12 inch. OTA, F6.3, CGE mount, ST2000xm Ccd, AO8, CFW9, Astronomik LRGB filterset.

Comet 2009 P1 Garradd+M71 Mercer. Credit: Leonard Ellul Mercer.

Leonard Ellul Mercer sent in this nice view from Malta in the Mediterranean Sea.

A set of 78 - 30 second exposures of Comet Garradd taken on August 4, 2011 by Suraky on Flickr.

Suraky on Flickr from British Columbia, Canada shares his first astrophotos shot from his new and improved darker backyard. This is a set of 78 – 30 second exposures taken between 1:16am and 2:40am GMT-7 on August 4, showing the motion of the comet across the sky during that time. Comet is magnitude 8.7, and 1.5AU from Earth. Two satellite traces also shown. Suraky used DeepSky Stacker, set to Maximum, “so it’s very noisy but it shows more of the comet tail.” There is also an inverted view available on Flickr. Equipment: Newtonian 190mm F5.3. LXD75 Mount. Canon T1i DSLR, ISO800

A collection of images of Comet Garradd from August 20, 2011 by Flickr user 37 Hz.

Flickr user 37Hz put together this collection of images from Saturday, August 20, 2011, taken from “Light polluted Zeist,” the Netherlands. 37Hz said, “Wouldn’t have found this comet without the “precise GOTO” function of my NexStar and the exact coordinates of the comet according to Carinasoft Voyager software.” Equipment: Celestron NexStar 5SE. Meade DSI II pro ccd camera, with about 10 seconds for each frame.

Comet Garradd on August 19, 2011 by jamieball833

jamieball833 submitted this image to Universe Today’s Flickr Group, saying “Now that the comet is at a distance of 1.394 AU from Earth and at magnitude 8.3 it is starting to get a little brighter!

Info:44 x 45 seconds, iso 1600 f/6.25

Right Ascension : 20h 25.8m
Declination : +17′ 34′

Comet Garradd C/2009 P1 passing M71 Cluster. Credit John Chumack.

Never failing to disappoint, John Chumack of Galactic Images got this great shot of Garradd, and also created a video, which we featured earlier this week.

Want to get your astrophoto featured on Universe Today? Join our Flickr group, post in our Forum or send us your images by email (this means you’re giving us permission to post them). Please explain what’s in the picture, when you took it, the equipment you used, etc.

Earth Could Spread Life Across The Milky Way

Panspermia Illustration Courtesy of Wikipedia

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Most of us are familiar with the concept of panspermia – where living organisms can be “seeded” from comet or asteroid impacts – but where does the life-giving content come from? According to a research group led by Mauricio Reyes-Ruiz from the National Autonomous University of Mexico, it just might come from Earth.

Inspired by the discovery of Moon and Mars rocks found on Earth from meteor strikes, the team began computer modeling of what might happen if pieces of Earth were transported across the Solar System via a collision scenario. The simulation involved 10,000 Earth particles moving over a period of 30,000 years. The amount of matter is tiny compared to the bulk our planet and it’s a blink of the eye in cosmic time, but scientists theorize that extreme lifeforms might be able to exist that long in space.

“The collision probability is greater than previously reported,” said Reyes-Ruiz. “It has been suggested that the ejection to interplanetary space of terrestrial crustal material, accelerated in a large impact, may result in the interchange of biological material between Earth and other Solar System bodies”

Could pieces of Earth really reach other planets? According to older theories, chances were good that some might reach the Moon or Venus, but gravity from the Sun and Earth makes reaching Mars improbable. However, the new simulations show a Mars impact – and even Jupiter – to be probable with the right ejection speeds. By involving slightly more particles at five times the rate of motion, the new results show the particles could even go beyond the Solar System. Oddly enough, the faster they moved, the lesser their chances of encountering the Moon and Venus became. Of the 10,242 tested, 691 particles ‘escaped’ out of the Solar System entirely, and six landed on Jupiter itself. Is this a Neil Young vision of flying Mother Nature’s silver seed to a new home?

Chris Shepherd of the Institute of Physics in London, who was not involved in the study, might agree with this conclusion. “This is an intriguing piece of work. The team have mapped out a really interesting scenario,” he said. One possible collision zone is Europa, the moon of Jupiter, and while the team did not simulate the number of particles that would specifically land there, many astronomers believe that it contains a large ocean, and could therefore support life.”

Original Story Source: Cosmos Magazine News Release. For Further Study: Dynamics of escaping Earth ejecta and their collision probability with different Solar System bodies.

“Impossible” Star Exists in Cosmic Forbidden Zone

This ancient star, in the constellation of Leo (The Lion), is called SDSS J102915+172927 and has been found to have the lowest amount of elements heavier than helium of all stars yet studied. It has a mass smaller than that of the Sun and is probably more than 13 billion years old. Credit: ESO/Digitized Sky Survey 2

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Astronomers say a newly found star should not exist and is in the “forbidden zone” of a widely accepted theory of star formation. The star, called SDSS J102915+172927, is composed almost entirely of hydrogen and helium, with only remarkably small amounts of other chemical elements in it. And how should this star be classified? We suggest either ‘easy listening’ or ‘jazz,’ as this star is certainly not heavy metal! But it may be one of the oldest stars ever found.

This faint star is located in the constellation of Leo (The Lion), and has the lowest amount of elements heavier than helium (what astronomers call “metals”) of all stars yet studied. It has a mass smaller than that of the Sun and is probably more than 13 billion years old.

“A widely accepted theory predicts that stars like this, with low mass and extremely low quantities of metals, shouldn’t exist because the clouds of material from which they formed could never have condensed,” said Elisabetta Caffau (Zentrum für Astronomie der Universität Heidelberg, Germany and Observatoire de Paris, France), lead author of the paper appearing in this week’s edition of Nature. “It was surprising to find, for the first time, a star in this ‘forbidden zone’, and it means we may have to revisit some of the star formation models.”

The team found the star with the X-shooter and UVES instruments on the Very Large Telescope. This allowed them to measure how abundant the various chemical elements were in the star. They found that the proportion of metals in SDSS J102915+172927 is more than 20,000 times smaller than that of the Sun.

“The star is faint, and so metal-poor that we could only detect the signature of one element heavier than helium — calcium — in our first observations,” said Piercarlo Bonifacio (Observatoire de Paris, France), who supervised the project. “We had to ask for additional telescope time from ESO’s Director General to study the star’s light in even more detail, and with a long exposure time, to try to find other metals.”

This picture shows the distribution of the light of different colours coming from the remarkable star SDSS J102915+172927 after it has been split up by the X-Shooter instrument on the ESO VLT. Credit: ESO/E. Caffau

The prevailing theory is that hydrogen and helium were created shortly after the Big Bang, together with some lithium, while almost all other elements were formed later in stars. Supernova explosions spread the stellar material into the interstellar medium, making it richer in metals. New stars form from this enriched medium so they have higher amounts of metals in their composition than the older stars. Therefore, the proportion of metals in a star tells us how old it is.

“The star we have studied is extremely metal-poor, meaning it is very primitive. It could be one of the oldest stars ever found,” adds Lorenzo Monaco from ESO, also involved in the study.

Also very surprising was the lack of lithium in SDSS J102915+172927. Such an old star should have a composition similar to that of the Universe shortly after the Big Bang, with a few more metals in it. But the team found that the proportion of lithium in the star was at least fifty times less than expected in the material produced by the Big Bang.

“It is a mystery how the lithium that formed just after the beginning of the Universe was destroyed in this star.” Bonifacio added.

Is this star one-of-a-kind? Probably not, the researchers say. “We have identified several more candidate stars that might have metal levels similar to, or even lower than, those in SDSS J102915+172927. We are now planning to observe them with the VLT to see if this is the case,” said Caffau.

Read the team’s paper (pdf file)

Source: ESO

Driving Miss Spirit…

Artist's impression of the Opportunity Rover, part of NASA's Mars Exploration Program. NASA/JPL-Caltech

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Are you ready to take a fun journey? One with a little Spirit? Then don’t miss the Opportunity to take the Mars Rover out for a drive. NASA has introduced a new website release which gives you page after page of awesome slideshows and entertaining text. If you’re looking for a great way to spend a few hours – be it by yourself or with kids – then you’ve got to visit “Explore Mars: Spirit’s Journey”. Here are just a few examples of what you’ll encounter…

“The first pictures I sent back showed a land of strange, dark rocks. People all over the world flocked to their televisions and the Web to see these pictures.”

“My team sent me to a football-sized rock called “Adirondack.” It had very little dust covering it. It also had a smooth surface, making it easier for me to put my arm right against it.”

“It was a rocky road to Bonneville, but worth it. Craters are good to study because they show deeper layers in their walls. The deeper the layer, the older the record of what Mars was like earlier in its history.”

“Once I got to the hills, my team faced a tough challenge. No robot had ever hiked up a hill and they didn’t know how they would get me up this massive summit.”

“After almost six months since landing, finally! Signs of past water! As I hiked up the hills, I came across a knobby looking rock. My team called it “Pot of Gold,” because this rock contains a mineral called hematite.”

But this isn’t all to the pages… just a few stops! In “Explore Mars: Spirit’s Journey” you will also find a virtual journey in 3D, an “All About Mars” program, more information on the Mars Rovers and even the opportunity to become a Martian! It’s a very entertaining way to spend some time. Enjoy!

ISS Crew Provides Light-Hearted Look at Current Space Flight Plight

What does the International Space Station crew think about the situation they face since the Progress cargo ship mishap? Astronaut Ron Garan wanted to do something light-hearted to let everyone know that “we are all in this together,” so he and his crewmates created a video. Garan said “Despite the seriousness of the possibilities, and while we are all in this period of uncertainty, it doesn’t mean we can’t still have a little fun.”

This video also provides an impromptu tour of the ISS and shows how big the space station is, as it takes fellow astronaut Mike Fossum a long time to find Garan.

It should be noted that they made this video before they got the news of the potential of having the ISS unmanned. “This would have serious implications, and we all hope that it does not come to that,” Garan wrote on his Fragil Oasis blog. You can read Garan’s entire commentary about the video at that link, and take a look around at his other postings, as well. Garan is doing a great job of sharing his experiences in space.

Hubble Movies “Star” Supersonic Jets

Astronomers have combined two decades of Hubble observations to make unprecedented movies revealing never-before-seen details of the birth pangs of new stars. This sheds new light on how stars like the Sun form. Credit: Hubble/ESA

[/caption]Don’t you know that you are a shooting star… Thanks to the NASA/ESA Hubble Space Telescope, an international team of scientists led by astronomer Patrick Hartigan of Rice University in Houston, USA, has done something pretty incredible. Using photos and information gathered from the last 14 years of observations, they’ve sewn together an unprecedented look at young jets ejected from three stars. Be prepared to be “blown” away…

The time-lapse sequence of “moving pictures” offers us an opportunity to witness activity that takes place over several years in just a few seconds. Active jets can remain volatile for periods of up to 100,000 years and these movies reveal details never seen – like knots of gas brightening and dimming – and collisions between fast-moving and slow-moving material. These insights allow scientists to form a clearer picture of stellar birth.

“For the first time we can actually observe how these jets interact with their surroundings by watching these time-lapse movies,” said Hartigan. “Those interactions tell us how young stars influence the environments out of which they form. With movies like these, we can now compare observations of jets with those produced by computer simulations and laboratory experiments to see which aspects of the interactions we understand and which we don’t understand.”

As a star forms in its collapsing cloud of cold gas, it gushes out streams of material in short bursts, pushing out from its poles at speeds of up to about 600,000 miles an hour. As the star ages, it spins material and its gravity attracts even more, creating a disc which may eventually become protoplanetary. The fast moving jets may be restricted by the neophyte star’s magnetic fields and could cease when the material runs out. However, by looking at this supposition in action, new questions arise. It would appear that the dust and gas move at different speeds.

“The bulk motion of the jet is about 300 kilometers per second,” Hartigan said. “That’s really fast, but it’s kind of like watching a stock car race; if all the cars are going the same speed, it’s fairly boring. The interesting stuff happens when things are jumbling around, blowing past one another or slamming into slower moving parts and causing shockwaves.”

But the “action” doesn’t stop there. In viewing these sequential shockwaves, the team was at a loss to understand the dynamics behind the collisions. By enlisting the aid of colleagues familiar with the physics of nuclear explosions, they quickly discovered a recognizable pattern.

“The fluid dynamicists immediately picked up on an aspect of the physics that astronomers typically overlook, and that led to a different interpretation for some of the features we were seeing,” Hartigan explained. “The scientists from each discipline bring their own unique perspectives to the project, and having that range of expertise has proved invaluable for learning about this critical phase of stellar evolution.”

Hartigan began using Hubble to collect still frames of stellar jets in 1994 and his findings are so complex he has employed the aid of experts in fluid dynamics from Los Alamos National Laboratory in New Mexico, the UK Atomic Weapons Establishment, and General Atomics in San Diego, California, as well as computer specialists from the University of Rochester in New York. The Hubble sequence movies have been such a scientific success that Hartigan’s team is now conducting laboratory experiments at the Omega Laser facility in New York to understand how supersonic jets interact with their environment.

“Our collaboration has exploited not just large laser facilities such as Omega, but also computer simulations that were developed for research into nuclear fusion,” explains Paula Rosen of the UK Atomic Weapons Establishment, a co-author of the research. “Using these experimental methods has enabled us to identify aspects of the physics that the astronomers overlooked — it is exciting to know that what we do in the laboratory here on Earth can shed light on complex phenomena in stellar jets over a thousand light-years away. In future, even larger lasers, like the National Ignition Facility at the Lawrence Livermore National Laboratory in California, will be able explore the nuclear processes that take place within stars.”

And all the world will love you just as long… as long as you are… a shooting star!

Original Story Source and Video Presentation: Hubble News. For further reading, Rice University News.