Posted on by Nancy Atkinson

The 2012 Nobel Prize in Physics, Explained

This hot-off-the-press video from the science-explainer folks at Sixty Symbols does a great job of detailing the science of the work by Serge Haroche of France and American David Wineland, which won them 2012 Nobel Prize in physics today. Their experiments on quantum particles have already resulted in ultra-precise clocks and may one day help lead to computers that can work faster than those in use today.

The video also shows how expectations were that the prize might go to the teams at the Large Hadron Collier for the discovery of what they called a “Higgs-like boson” — a particle that resembles the long sought-after Higgs.
Continue reading “The 2012 Nobel Prize in Physics, Explained”

Posted on by Nancy Atkinson

Watch Live: Felix Baumgartner’s Record Breaking Jump Attempt

UPDATE: The launch/jump attempt for Felix Baumgartner and the Red Bull Stratos mission on October 9 has been aborted due to winds at the launch site in Roswell, New Mexico. At first, there was a 5 hour weather delay, then a radio system malfunction which was fixed, and then the winds became too high. Winds have to relatively benign for the huge balloon to take off. The balloon used for this mission is three times larger than any other human balloon flight.

Felix Baumgartner will leap from nearly 37 km (23 miles, 120,000 feet), attempting to not only break the sound barrier with his body, but also break the record for the longest freefall

We’ll provide updates and post the live video feed for future attempts. The weather for the rest of the week remains “iffy,” however.

Posted on by Nancy Atkinson

Last Night’s View: Skies Filled with Stunning Aurora

The Aurora Borealis fills nearly the entire sky in Cleary Summit, Alaska. Credit: Jason Ahrns on Flickr.

With just a glancing blow from a coronal mass ejection (CME) this week, skywatchers in the northern latitudes have been enjoying some beautiful views of the Aurora Borealis. Here are a few stunning views from last night (October 8-9, 2012), including this jaw-dropping aurora that filled the entire sky for Jason Ahrns in Cleary Summit, Alaska. “This lens has a near-180 degree field of view from corner to corner – this swirl covered the entire sky, and put off enough light to read the focus indicator on my lens,” Jason wrote on Flickr.

See more below:

This view is from Kilmany, Scotland. “You could see the rays moving left – so stunning,” said photographer Corinne Mills.

This view came from the AuroraMAX camera in Yellowknife, NWT taken at 00:53 MDT on October 9, 2012. Credit: AuroraMAX.

“I’ve been tracking aurora activity all day and it peaked again tonight,” writes photographer Gareth Paxton on Flickr. “There was a substantial glow in the sky – this was taken from Linlithgow (Scotland).”

Northern lights over Ottawa, Canada. Credit: FailedProtostar on Flickr.

Stunning view from Saskatoon, Saskatchewan. Credit: Colin Chatfield.

Another beauty by Jason Arhns in Alaska, which he calls a “ghost flame.” Credit: Jason Arhns

Green aurora over Ulverston, Cumbria, UK. Credit: Raymond Gilchrist on Flickr.

Posted on by Jason Major

Curiosity Finds…SOMETHING…on Martian Surface

While scooping its first samples of Martian soil, NASA’s Curiosity rover captured the image above, which shows what seems to be a small, seemingly metallic sliver or chip of… something… resting on the ground. Is it a piece of the rover? Or some other discarded fleck of the MSL descent mechanisms? Or perhaps an exotic Martian pebble of some sort? Nobody knows for sure yet, but needless to say the soil samples have taken a back seat to this new finding for the time being.

See a ChemCam image of the object below.

ChemCam shot of a recently spotted unknown object on Mars. (NASA/JPL-Caltech)

The ChemCam image, although monochrome, reveals some interesting and curiously organic-looking edges on the object… although it could be a bit of something that came loose from the rover itself. Perhaps a bit of plastic wrap or tape from a cable? Or a flake of metal from the back shell?

Or, as MSNBC’s Alan Boyle jokingly (?) suggested, another piece of “Martian macaroni”?

The MSL mission page states:

Curiosity’s first scooping activity appeared to go well on Oct. 7. Subsequently, the rover team decided to refrain from using the rover’s robotic arm on Oct. 8 due to the detection of a bright object on the ground that might be a piece from the rover. Instead of arm activities during the 62nd Martian day, or sol, of the mission, Curiosity is acquiring additional imaging of the object to aid the team in identifying the object and assessing possible impact, if any, to sampling activities.

Stay tuned for more info on this intriguing news as it’s available!

Image: NASA/JPL-Caltech

P.S. Of course, the now-famous “Sarcastic Rover” had something to say about it on Twitter:

Posted on by Nancy Atkinson

Recent UK Fireball Could Not Have “Skipped” Around the World, New Analysis Says

The meteoroid seen over the UK on September 21, 2012 has created quite a sensation – make that a several sensations. First, the bright object(s) in the night sky were seen across a wide area by many people, and the brightness and duration – 40 to 60 seconds reported and videoed by some observers – had some experts wondering if the slow moving light-show might have been caused by space junk. But analysis by satellite tracker Marco Langbroek revealed this was likely an Aten asteroid, asteroid which have orbits that often cross the Earth’s orbit, but their average distance from the Sun is less than 1 AU, the distance from the Earth to the Sun.

Atens are fairly unusual, making this a rather unique event. But then came another analysis that seemed to be so crazy, it might have been true: this meteoroid may have skipped like a stone in and out of Earth’s atmosphere, where it slowed enough to orbit the Earth until appearing as another meteor over Canada, just a few hours after it was seen over the UK and northern Europe.

How amazing that would have been! And there was much speculation about this possibility. But, it turns out, after more details emerged and further investigation ensued, it is not possible that the space rock could have boomeranged around the world and been seen in again 2½ hours later over Canada. However, the current thinking is that at least one or two of the largest pieces retained enough velocity that they went into an elliptical Earth orbit, and went perhaps a half an orbit around Earth.

“At first it seemed natural to consider a possible dynamical linkage (between the UK and Canadian meteors), partly because the precise location and time over Quebec/Ontario was not well-known early on,” said aerospace engineer and meteor expert Robert Matson, in an email to Universe Today. Matson worked extensively with Esko Lyytinen, a member of the Finnish Fireball Working Group of the Ursa Astronomical Association, to analyze the possible connection between the September 21 UK fireball, and the Quebec fireball that followed about 2½ hours later.

At first, the time of the fireball sighting over southeastern Canada and northeastern USA was in doubt, but two Canadian all-sky cameras from the Western Meteor Physics Group captured the meteor, providing an accurate time.

“And once I triangulated the location to a spot between Ottawa and Montreal, a linkage to the UK fireball was no longer possible due to the longitude mismatch,” Matson said.

Additionally, the 153-minute time difference between meteors places a strict limit on the maximum longitude difference for a “skipping” meteoroid of roughly 38 degrees. This would put the final perigee well off the coast of Newfoundland, south of Greenland, Matson added.

More facts emerged, putting a death knoll on the connection between the two.

“Independent of the longitude mismatch, triangulation of the Canadian videos revealed that the entry angle was quite steep over Quebec – quite at odds with what an orbiting remnant from a prior encounter would have had,” Matson said. “So the meteors are not only unrelated, their respective asteroid sources would have been in different solar orbits.”

Image of fireball taken on Feb. 25, 2004 by the Elginfield CCD camera from the University of Western Ontario.

Another duo of astronomers from the British Astronomical Association, John Mason and Nick James concurred, also noting the shallow angle of the UK fireball, in addition to its slow speed. “We get velocities of 7.8 and 8.5 km/s and a height of 62 km ascending,” they wrote in the BAA blog. “These velocities and the track orientation and position are not at all consistent with ongoing speculation that there is a connection between this fireball and a fireball seen in south-eastern Canada/north-eastern USA 155 minutes later.”

But did parts of the meteoroid survive and skip out of the atmosphere? “Nearly all of the fragments of the meteoroid did just come in for good during and shortly after the UK passage, but at least one or two of the largest pieces retained enough velocity that they went into elliptical earth orbit,” Matson said. “The perigee of that orbit was a little over 50 km above the UK. The apogee would have been half an orbit later, possibly thousands of kilometers above the South Pacific, south of New Zealand.”

Just how high the apogee altitude was depends on how much the meteoroid decelerated over the UK, Matson added.

“This is why Esko, myself and others are very interested in determining the velocity of those fragments after they passed through perigee,” he said. “Below 7.9 km/sec, and they never get back out of the atmosphere; between 7.9 and 11.2 km/sec, they go into orbit — and we believe a couple of the biggest pieces were in the lower half of this range.”

But Matson said that if any remnant or remnants of the UK fireball did “skip” out of the atmosphere, they certainly had to come back in for good somewhere on the planet. “It is even remotely possible that it happened over Quebec,” Matson said. “But the laws of orbital mechanics do not allow an aerobraked fragment of the UK meteoroid to reenter over Quebec only 2½ hours later. It would have to be more than 4 hours later to line up with Quebec.”

The most likely scenario, Matson said, is that the surviving portion(s) of the UK meteoroid came in for good less than 2½ hours later, with the only possible locations during that window being the North Atlantic, Florida, Cuba, Central America, the Pacific, New Zealand, Australia, the Indian Ocean, the Arabian Peninsula, Turkey or southern Europe. Of these, the northern hemisphere locations would be favored.

So perhaps we haven’t heard the last of this meteoroid!

As crazy as the bouncing bolide sounds, it has happened in the past, according to Kelly Beatty at Sky and Telescope, who mentioned at least one instance where a large meteoroid streaked across the sky and then returned to interplanetary space. This sighting took place over the Rocky Mountains in broad daylight on August 10, 1972, and the meteoroid came as close as 35 miles (57 km) above Earth’s surface before skipping out into space. Beatty added that its velocity was too fast to become captured and return again.

You can read more analysis of the UK fireball being an Aten asteroid by Phil Plait at Bad Astronomy

Hat tip: Luke Dones

This article was updated on 10/9/12

Posted on by Tammy Plotner

Weekly SkyWatcher’s Forecast: October 8-14, 2012

Messier 73 - Credit: Palomar Observatory, courtesy of Caltech

Greetings, fellow SkyWatchers! With early evening dark skies, this is a perfect opportunity to take on some more serious studies. We’ll start off BIG… and work down to the really small. (Think Hickson Compact Groups.) There’s even a meteor shower this week! Now, get out your telescopes and get ready, cuz’ I’m waitin’ in the backyard and lookin’ for the “Double Dark”…

Monday, October 8 – Today marks the birthday of Ejnar Hertzsprung. Born 1873, Hertzsprung was a Danish astronomer who first proved the existence of giant and dwarf stars in the early 1900s. His discoveries included the relationship between color and luminosity, which wasn’t truly recognized until it was recovered by Henry Russell. Now it is a familiar part of all our studies as the Hertzsprung-Russell diagram. His use of absolute magnitudes will come into play tonight as we have a look at the age-old mystery of M73.

Located about three fingerwidths north-northwest of Theta Capricorni (RA 58.9 Dec -12 38), this 9th magnitude open cluster consisting of four stars was discovered by Charles Messier on October 4, 1780. He described it as a “Cluster of three or four small stars, which resembles a nebula at first glance…” Hotly debated as to whether or not the grouping is a genuine cluster or simply an asterism, it was also included in J. Herschel’s catalog (GC 4617) and given the NGC 6994 designation by Dreyer. In 1931 Collinder cataloged M73 as Cr 426, with an estimated distance of 12,000 light-years. Still, the debate about its authenticity as a physically related group continued.

At least two stars show the same proper motion, leading scientists to believe M73 may be the remnant of a much older and now dispersed cluster – or simply two related stars. Of the 140 stars investigated in the region, 24 may be real members, including those in Messier’s original observation. Thanks to the work of Hertzsprung and Russell, these candidates fall within the color-magnitude diagram of a 2 to 3 billion year old cluster with Messier’s suspect four being evolved giants. The most recent data indicates M73 may simply be an asterism – sharing no common proper motion, but until more studies are undertaken you can enjoy this unusual Messier in even a small telescope!

Tuesday, October 9 – Tonight is the peak of the Draconid meteor shower whose radiant is near the westering constellation of Hercules. This particular shower can be quite impressive when comet Giacobini-Zinner passes near Earth. When this happens, the fall rate jumps to 200 per hour and has even been known to reach 1000. So what am I going to tell you about this year? Comet Giacobini-Zinner reached perihelion on July 2nd of 2005, passing with 8 million kilometers of Earth, but has now greatly distanced itself from our solar system. Chances are the Draconids will only produce around 3 to 5 per hour, but no one knows for sure!

While we’re out, let’s take the time to have a peek at M72, just about a degree and a half west (RA 20 53.5 Dec -12 32) of last night’s target M73.

Originally found by Mechain on the night of August 29-30, 1780, this class IX globular cluster is one of the faintest and most remote of the Messiers, and Charles didn’t catalog it until over a month after its discovery. At around magnitude 9, this 53,000 light-year distant globular will be not much more than a faint round smudge in smaller aperture, but will take on a modicum of resolution in larger telescopes. Well beyond the galactic center and heading toward us at 255 kilometers per second, M72 is home to 42 variables and the average magnitude of its members is around 15. While mid-sized scopes will pick up a graininess in the texture of this globular, notice how evenly the light is distributed, with little evidence of a core region. Be sure to write down your observations!

Wednesday, October 10 – Today in 1846, William Lassell was busy at his scope as he made a new discovery – Neptune’s moon Triton! Although our everyday equipment can’t “see” Triton, we can still have a look at Neptune which is also hanging out in tonight’s study constellation of Capricornus. Try checking astronomy periodicals or many great on-line sites for accurate locator charts.

Tonight let’s head to the eastern portion of Capricornus and start by identifying Zeta about a fistwidth southwest of the eastern corner star – Delta. Now look southeast about 2 fingerwidths and identify 5th magnitude star 41. About one half degree west is our target we’ll be revisiting this evening, M30 (Right Ascension: 21 : 40.4 – Declination: -23 : 11).

At near magnitude 8, this class V globular cluster is well suited to even binoculars and becomes spectacular in a telescope. Originally discovered by Messier in August 1764 and resolved by William Herschel in 1783, some of M30?s most attractive features are the branches of stars which seem to radiate from its concentrated core region. Estimated to be around 26,000 light-years away, you’ll find it fairly well resolved in large aperture, but take time to really look. The dense central region may have already undergone core collapse – yet as close as these stars are, very few have collided to form x-ray binaries. For the smaller scope, notice how well M30?s red giants resolve and be sure to mark your notes!

Thursday, October 11 – Tonight is time for a telescopic challenge – a compact galaxy group. You’ll find it less than half a degree southeast of stellar pair 4 and 5 Aquarii (RA 20 52 26.00 Dec -05 46 19.1).

Known as Hickson 88, this grouping of four faint spiral galaxies is estimated to be around 240 million light-years away and is by no means an easy object – yet the galactic cores can just be glimpsed with mid-sized scopes from a very dark site. Requiring around 12.5? to study, you’ll find the brightest of these to be northernmost NGC 6978 and NGC 6977. While little detail can be seen in the average large backyard scope, NGC 6978 shows some evidence of being a barred spiral, while NGC 6977 shows the even appearance of a face-on. Further south, NGC 6976 is much smaller and considerably fainter. It is usually caught while averting and studying the neighborhood. The southernmost galaxy is NGC 6975, whose slender, edge-on appearance makes it much harder to catch.

Although these four galaxies seem to be in close proximity to one another, no current data suggests any interaction between them. While such a faint galaxy grouping is not for everyone, it’s a challenge worthy of seasoned astronomer with a large scope! Enjoy…

Friday, October 12 – Today in 1891, the Astronomical Society of France was established. Exactly one year later in 1892, astronomy great E. E. Barnard was hard at work using the new tool of photography and became the first to discover a comet – 1892 V – in this way!

Not only did Barnard use photography for comets, but his main interest of study was details within the Milky Way. Tonight let us take out binoculars or a telescope at the widest possible field of view and have a look at two such regions in the westering Aquila – The “Double Dark Nebula.”

Just northeast of Altair is bright star Gamma Aquilae, and about a fingerwidth west is a pair of Barnard discoveries: B142 and B143 – two glorious absences of stars known as interstellar dust clouds. B143 is no more than a half degree in size and will simply look like a blank area shaped like a horseshoe, with its extensions point toward the west. Just south is B142, an elongated comma shape, which seems to underline its companion.

Located anywhere from 1000 to 3000 light-years away, these non-luminous clouds of gas and dust are a very fine example of Barnard’s passion. Do not be upset if you don’t see them on your first attempt – for the chances are if you are seeing “nothing,” you are looking in the right place!

Saturday, October 13 – Today marks the founding of the British Interplanetary Society in 1933. “From imagination to reality,” the BIS is the world’s oldest established organization devoted solely to supporting and promoting the exploration of space and astronautics.

Tonight we’ll do them proud as we go back for another look at the mighty M2. You’ll find it located about three fingerwidths north-northeast of Beta Aquarii (RA 33.5 Dec 00 49).

At slightly dimmer than 6th magnitude, this outstanding globular cluster is just inside that region where it can’t quite be viewed unaided, but even the smallest of binoculars will pick it out of a relatively starless field with ease. Holding a Class II designation, it was first discovered by Maraldi on September 11, 1746 and rediscovered independently by Messier exactly 14 years later. At a distance of roughly 37,500 light-years, it is estimated to contain in the neighborhood of 150,000 stars.

Even a small telescope will reveal M2’s rich and concentrated core region and slight ellipticity. Not bad for a 13 billion year old group of stars! As aperture increases, some of the brightest stars will begin to resolve, and in larger telescopes it will approach total resolution. You might well note a dark area in the northeastern section, and several more located throughout the splendid field. Feast your eyes on one of the finest in the skies!

Sunday, October 14 – Before we leave Cygnus for the year, try your luck with IC 5070 (Right Ascension: 20 : 50.8 – Declination: +44 : 21), also known as the “Pelican Nebula.” You’ll find it just about a degree southeast of Deneb and surrounding the binary star 56 Cygni.

Located around 2000 light-years away, the Pelican is an extension of the elusive North American Nebula, NGC 7000. Given its great expanse and faintness, catching the Pelican does require clean skies, but it can be spotted best with large binoculars. As part of this huge star forming region, look for the obscuring dark dust cloud Lynds 935 to help you distinguish the nebula’s edges. Although it is every bit as close as the Orion Nebula, this star hatchery isn’t quite as easy!

Now let’s give deep sky a rest as we travel to the northwest corner of Capricornus and have a look just south of Alpha at beautiful Beta.

Named Dabih, this lovely white 3rd magnitude star has a very easily to split 6th magnitude companion which will appear slightly blue. Over 100 times brighter than our own Sun, the primary star is also a spectroscopic triple – one whose unseen companions orbit in a little over 8 days and 1374 days. Oddly enough the B star is also a very tight binary as well – yet the two major stars of this system are separated by about a trillion miles! If you have a large aperture telescope – power up. According to T. W. Webb, a 13th magnitude unrelated double is also found in between the two brighter stars. No matter if you chose binoculars or a telescope, I’m sure you’ll find the 150 light-year trip worth your time to add to your doubles list!

Until next week? Wishing you clear skies!

Posted on by Fraser Cain

Virtual Star Party – Oct. 7, 2012: West Coast Edition

Only the West Coast of North America was represented in our Virtual Star Party this week. We had astronomers in Oregon, California and Nevada. But we also a great night, with dozens of observed objects, including Comet 168P/Hergenrother.

Click here to see all the pictures from last night’s observing session.

Astronomers: Gary Gonella, Roy Salisbury, Bill McLaughlin, and Stuart Forman.

Bringing the Science: Dr. Thad Szabo and Scott Lewis

Host: Fraser Cain

We hold our Virtual Star Party every Sunday night when it gets dark on the West Coast, and broadcast live on Google+. Circle the Virtual Star Party page on G+ to get a notification of the event.

Posted on by Nancy Atkinson

Voyager 1 May Have Left the Solar System

Number of particles from the Sun hitting Voyager 1. Credit: NASA

While there’s no official word from NASA on this, the buzz around the blogosphere is that Voyager 1 has left the Solar System. The evidence comes from this graph, above, which shows the number of particles, mainly protons, from the Sun hitting Voyager 1 across time. A huge drop at the end of August hints that Voyager 1 may now be in interstellar space. The last we heard from the Voyager team was early August, and they indicated that on July 28, the level of lower-energy particles originating from inside our Solar System dropped by half. However, in three days, the levels had recovered to near their previous levels. But then the bottom dropped out at the end of August.

The Voyager team has said they have been seeing two of three key signs of changes expected to occur at the boundary of interstellar space. In addition to the drop in particles from the Sun, they’ve also seen a jump in the level of high-energy cosmic rays originating from outside our Solar System.

The third key sign would be the direction of the magnetic field. No word on that yet, but scientists are eagerly analyzing the data to see whether that has, indeed, changed direction. Scientists expect that all three of these signs will have changed when Voyager 1 has crossed into interstellar space.

“These are thrilling times for the Voyager team as we try to understand the quickening pace of changes as Voyager 1 approaches the edge of interstellar space,” said Edward Stone, the Voyager project scientist for the entire mission, who was quoted in early August. “We are certainly in a new region at the edge of the solar system where things are changing rapidly. But we are not yet able to say that Voyager 1 has entered interstellar space.”

Stone added that the data are changing in ways that the team didn’t expect, “but Voyager has always surprised us with new discoveries.”

Voyager 1 launched on Sept. 5, 1977, is approximately 18 billion kilometers (11 billion miles) from the Sun. Voyager 2, which launched on Aug. 20, 1977, is close behind, at 15 billion km (9.3 billion miles) from the Sun.

Sources: NASA, Eric Berger/ Houston Chronicle, Scientific American

Posted on by Ken Kremer

Scooping Mars – Shaken Not Stirred ! – Color Video

Image Caption: Scooping Mars at ‘Rocknest’ mosaic shows a before and after view of the spot where Curiosity dug up her 1st Martian soil sample on Sol 61 (Oct 7. 2012). Navcam camera mosaic at left shows the arm at work during scooping operations. Image at right shows the tiny scooped trench measuring about 1.8 inches (4.5 centimeters) wide. See NASA JPL scooped sample vibration video below. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo

“Here’s the scoop: I like my regolith shaken!” tweeted NASA’s Curiosity Mars rover a short while ago in a nod to the 50th anniversary of the premiere of the 1st James Bond action flick.

And the “proof” is in the video as they say. See below a short NASA video clip showing the 1st Martian material collected using the small table spoon sized scoop on Curiosity’s robotic arm and subsequently being vibrated inside the scoop after it was lifted from the ground of Gale Crater this past weekend on Sol 61, Oct. 7, 2012.

Scooping Mars at ‘Rocknest’ mosaic above shows a before and after view of the spot where Curiosity was working at on Sol 61.

“So excited to dig in! One scoop of regolith ripple, coming right up!” she tweeted in the midst of the action.


Video Caption: This 256 frame video clip of Mastcam images shows the 1st sample of Martian material being vibrated inside Curiosity’s table spoon sized scoop on Oct. 7, 2012. Credit: NASA/JPL-Caltech/MSSS

Yeah baby ! Just as the rover’s science and engineers announced last week, the 6 wheeled mega robot Curiosity scored a major success by scooping up her very first sample of windblown Martian sand from the ‘Rocknest’ ripple she arrived at just last week.

The plan ahead is to use the collected “Red Planet” material to cleanse the interior of the rover’s sample-handling system of a residual layer of oily contamination of “Home Planet” material that could interfere with unambiguously interpreting the results.

For sure the science team doesn’t want any false positives with respect to any potential detection of the long sought organic compounds that could shed light on whether a habitant supporting Martian microbes ever existed in the past or present.

The newly collected material will be vibrated at 8 G’s and then be fed into Curiosity’s Collection and Handling for In-Situ Martian Rock Analysis (CHIMRA) device on the robotic arm turret.

Curiosity’s motorized scoop measures 1.8 inches (4.5 centimeters) wide, 2.8 inches (7 centimeters) long. The images reveal the scoop left behind a small hole about 1.8 inches (4.5 centimeters) wide.

Image Caption: Sol 61 Navcam raw image shows the hole dug up by Curioisty’s scoop on Oct. 7, 2012 Credit: NASA/JPL-Caltech

Image Caption: Mastcam 100 telephoto close up image of Rocknest trench on Sol 61. Credit: NASA/JPL-Caltech/MSSS

At last week’s Oct. 4 media briefing, the rover team said they would make three deliveries of scooped soil to cleanse out the sample acquisition system over the next two week or so before pouring sieved Mars material into the SAM and Chemin analytical chemistry labs on the rover’s deck for detailed evaluation of the elemental and mineralogical composition.

Ken Kremer

Posted on by Nancy Atkinson

Baumgartner in Final Preparations for Supersonic Freefall Attempt on October 9

Skydiver, pilot and BASEjumper Felix Baumgartner will attempt to break the sound barrier in freefall on Tuesday, October 9, 2012, jumping from a capsule lifted by a giant balloon to 36,576 meters (120,000 feet). This is something that Baumgartner has been preparing for over the past five years, but his team says the time period he now finds himself — the last few hours before takeoff — might be the most challenging of all.

“I’ll probably feel the most anxious when I’m trying to sleep in the hours before I start getting ready –when everything’s quiet and it’s just me and my thoughts,” 43-year old Baumgartner admitted. “Once my day begins, I’ll have a lot to do and my mind will have something to focus on.”

The target time for the launch of the balloon and capsule is 12:00 GMT/ 8 am EDT/5 am PDT on October 9. To watch it live, tune into http://youtube.com/redbull or http://redbullstratos.com/

Here’s how Baumgarter is spending the final 24 hours before the jump from the edge of space:

Launch Minus 24 Hours: Baumgartner started the day with a light cardio-based workout, mostly to “relax and loosen up,” according to Red Bull High Performance Director Andy Walshe.

Pilot Felix Baumgartner and girlfriend Nicole Oetl pose for a photograph during the preparations for the flight of the Red Bull Stratos mission in Roswell, New Mexico. Credit: Red Bull Stratos.

Minus 18h30: Rest and relaxation. His family has arrived at the New Mexico launch site and he will spend time with them, as well as reading messages of support that have been pouring in from around the world and drawing in his sketchbook – a pastime that he says helps to clear his mind. In the back of his mind he is always reviewing his checklists for the mission, his team says.

Minus 13h30: Baumgartner will join members of the crew for a light early dinner, but the food on his plate will be unique. For at least 24 hours before his jump, he must stick to a low-fiber diet prescribed by the mission’s medical team. It is vital for him to eat only foods that will clear his system quickly, without leaving residue that could create gas: a condition that can cause problems in the low-pressure of the stratosphere because it can expand in the body and cause serious discomfort.

Minus 12h00: Baumgartner will attempt to get to sleep early – before the Sun has even set. But whether he sleeps or tosses and turns all night — like Charles Lindbergh did before his historic flight across the Atlantic in 1920 – only Baumgarter knows.

Minus 4h30: “When I need to be ready, I’m always ready,” Baumgartner often says. And while he will try to sleep as long as possible, he’ll need to rise four to five hours before dawn to be ready for the intense day ahead.

Minus 3h30: Baumgartner will arrive at the launch site, accompanied by his team, which includes Col. Joe Kittinger, whose freefall record Baumgarter is trying to break. Kittinger, a retired Air Force officer, jumped from 31,500 meters (31.5 km, 19.5 miles, 102,000 ft) in 1960. Now 83, Kittinger has been assisting Baumgartner in preparations for the jump.

Minus 4h00: Baumgartner will head to the runway where, as is habitual for the experienced pilot before
every flight, he will conduct a meticulous inspection of the capsule.

Minus 2h30: Baumgartner will undergo a final medical check and a compact, state-of-the-art physiological monitoring system will be strapped to his chest to be worn under his pressure suit throughout the mission.

Minus 2h00: Life Support Engineer Mike Todd will dress Baumgartner in his suit, a painstaking process, and Baumgartnerwill ‘pre-breathe’ oxygen for two hours to eliminate nitrogen from his bloodstream, which could expand dangerously at altitude.

Minus 0h30: Baumgartner will be strapped into his capsule chair to conduct final instrument checks as
directed by Mission Control. Then Capsule Engineer Jon Wells will seal the clear acrylic door. For several more long minutes of anticipation, Baumgartner will await countdown and, finally, launch.

Here’s a video that shows what the ascent and jump might be like:

Source: Red Bull Stratos