Can Solar Flares Hurt Astronauts?

Expedition 29 astronaut Ron Garan looks down on the coast of Australia from the safety of the ISS. (NASA)

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Solar flares, coronal mass ejections, high-energy photons, cosmic rays… space is full of various forms of radiation that a human wouldn’t want to be exposed to for very long. Energized particles traveling into and through the body can cause a host of nasty health problems, from low blood count to radiation sickness to cataracts and cancer… and potentially even death. Luckily Earth’s magnetic field and atmosphere protects us on the surface from much of this radiation, but what about the astronauts aboard the Space Station? How could events such as today’s powerful near-X-class solar flare and last week’s CME affect them, orbiting 240 miles above Earth’s surface?

Surprisingly, they are safer than you might think.

M8.7-class solar flare erupting on the Sun's northeastern hemisphere at 03:49 UT on Jan. 23, 2012. (Courtesy NASA/SDO and the AIA team. Edited by J. Major.)

The M8.7-class flare that erupted from the Sun early on Jan. 23 sent a huge wave of high-energy protons Earthward, creating the largest solar storm seen since 2005.  The cloud of energetic particles raced outwards through the Sun’s atmosphere at speeds well over a million miles per hour, blowing past our planet later the same day. (More slower-moving charged particles will impact the magnetosphere in the coming days.) We are safe on Earth but astronauts exposed to such radiation could have faced serious health risks. Fortunately, most solar protons cannot pass through the hull of the Space Station and so as long as the astronauts stay inside, they are safe.

Of course, this is not the case with more dangerous cosmic rays.

According to the NASA Science site:

Cosmic rays are super-charged subatomic particles coming mainly from outside our solar system. Sources include exploding stars, black holes and other characters that dwarf the sun in violence. Unlike solar protons, which are relatively easy to stop with materials such as aluminum or plastic, cosmic rays cannot be completely stopped by any known shielding technology.

Even inside their ships, astronauts are exposed to a slow drizzle of cosmic rays coming right through the hull. The particles penetrate flesh, damaging tissue at the microscopic level. One possible side-effect is broken DNA, which can, over the course of time, cause cancer, cataracts and other maladies.

In a nutshell, cosmic rays are bad. Especially in large, long-term doses.

Now the astronauts aboard the ISS are still well within Earth’s protective magnetic field and so are shielded from much of the cosmic radiation that passes through our solar system daily. And, strangely enough, when solar flares occur – such as today’s – the amount of cosmic radiation the ISS encounters actually decreases.

Why?

The solar particles push them away.

Decrease in cosmic radiation during a CME recorded in 2005.

In an effect known as the “Forbush decrease”,  magnetically-charged particles ejected from the Sun during flares and CMEs reduce the amount of cosmic radiation the ISS experiences, basically because they “sweep away” other charged particles of more cosmic origin.

Because cosmic rays can easily penetrate the Station’s hull, and solar protons are much less able to, the irony is that astronauts are actually a degree safer during solar storms than they would be otherwise.

And it’s not just in low-Earth orbit, either: Wherever CMEs go, cosmic rays are deflected. Forbush decreases have been observed on Earth and in Earth orbit onboard Mir and the ISS. The Pioneer 10 and 11 and Voyager 1 and 2 spacecraft have experienced them, too, beyond the orbit of Neptune. (via NASA Science.)

Due to this unexpected side effect of solar activity it’s quite possible that future manned missions to the Moon, Mars, an asteroid, etc. would be scheduled during a period of solar maximum, like the one we are in the middle of right now. The added protection from cosmic rays would be a big benefit for long-duration missions since we really don’t know all the effects that cosmic radiation may have on the human body. We simply haven’t been traveling in space long enough. But the less exposure to radiation, the better it is for astronauts.

Maybe solar storms aren’t so bad after all.

Read more about solar radiation and the Forbush decrease on NASA Science here.

Young Magnetic Star Possesses Precise Carbon Dioxide Ring

Artist's conception image of a young star surrounded by a disk (made up of rings) (Credits: NASA/JPL-Caltech)

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Catching a ring – or accretion disk – around a star isn’t unusual. However, catching a sharply defined carbon-dioxide ring around a young, magnetic star that’s precisely 1 AU away with a width 0.32 AU or less might raise a few eyebrows. This isn’t just any disk, either… It’s been likened as a “rope-like structure” and there’s even more to the mystery. It’s encircling a Herbig Ae star.

Discovered with the European Southern Observatory’s Very Large Telescope, the edges of this accretion disk are uniquely crisp. Located in the constellation of Centaurus at about 700 light years distant, V1052 (HD 101412) is a parent star with an infrared excess. “HD 101412 is most unusual in having resolved, magnetically split spectral lines which reveal a surface field modulus that varies between 2.5 to 3.5 kG.” says C.R. Cowley (et al). Previous studies “have surveyed molecular emission in a variety of young stellar objects. They found the emission to be much more subdued in Herbig Ae/Be stars than their cooler congeners, the T Tauri stars. This was true for HD 101412 as well, which was among the 25 Herbig Ae/Be stars they discussed. One exception, however, was the molecule CO2, which had a very large flux in HD 101412; indeed, only one T Tauri star had a higher CO2 flux.”

It’s not unusual for carbon dioxide to be found near young stars, but it is a bit more normal for it to be distributed throughout the disk region. “It’s exciting because this is the most constrained ring we’ve ever seen, and it requires an explanation,” explains Cowley, who is professor emeritus at the University of Michigan and leader of the international research effort. “At present time, we just don’t understand what makes it a rope rather than a dish.”

Because V1052 itself is different could be the reason. It is hypothesized the magnetic fields may be holding the rings in the disk structure at a certain distance. The idea has also been forwarded that there may be “shepherding planets”, much like Saturn’s ring structure, which may be the cause. “What makes this star so special is its very strong magnetic field and the fact that it rotates extremely slow compared to other stars of the same type,” said Swetlana Hubrig, of the Leibniz Institute for Astrophysics Potsdam (AIP), Germany.

One thing that is certain is how clean and well-defined the disk lines are centered around the Earth/Sun distance. This accords well with computer modeling where “A wider disk will not fit the observations.” These observations – and the exotic parent star – have been under intense scrutiny since 2008 and the findings have been recently published on-line in Astronomy and Astrophysics. It’s work that helps deepen the understanding of the interaction between central stars, their magnetic fields, and planet-forming disks. It also allows for fact finding when it comes to diverse systems and better knowledge of how solar systems form… even unusual ones.

“Why do turbulent motions not tear the ring apart?” Cowley wondered. “How permanent is the structure? What forces might act to preserve it for times comparable to the stellar formation time itself?”

When it comes to Herbig Ae stars, they are not only rare, but present a rare opportunity for study. In this case, it gives the team something to be quite excited about.

“This star is a gift of nature,” Hubrig said

Original Story Source: Leibniz Institute for Astrophysic News Release. For Further Reading: The narrow, inner CO ring around the magnetic Herbig Ae star, HD 101412.

Opportunity arrives at Greeley Haven – 5th Winter Haven Worksite on Mars

Opportunity Mars Rover at Winter Haven Worksite at Endeavour Crater. NASA’s Opportunity rover has parked near this spot at the “Greeley Haven” worksite where the robot will spend her 5th Martian Winter Haven since landing 8 years ago in January 2004. This mosaic of images was snapped in December 2011 and shows the view from the Cape York Ridge at the western rim of Endeavour Crater looking south along the crater rim to a future area that Opportunity will drive to and explore next spring. Credit: NASA/JPL/Cornell/ Marco Di Lorenzo/Kenneth Kremer

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NASA’s seemingly indestructible Opportunity rover has arrived at the breathtaking location where she’ll be working through her unfathomable 5th Martian Winter. The Opportunity Mars Exploration Rover has not only endured, but flourished for 8 years of unending “Exploration & Discovery” on the Red Planet despite having an expected lifetime at landing of just 3 months, way back in January 2004.

Opportunity is parked at a northward facing outcrop dubbed “Greeley Haven” where she can soak up the sun and juice her innards throughout the utterly harsh and Antarctic-like temperatures on tap for the next few months that threaten to kill her each and every Martian day. See our mosaic above around the Greeley Haven area.

Science team members told Universe Today that the rover is sitting at Greeley Haven because the site offers a roughly 15 degree tilt that will maximize the electric output from the life-giving solar arrays and also allow the robot to carry out a vigorous science campaign during the seasonal Martian winter season that officially begins in March.

Greeley Haven is a located at the northern tip of the “Cape York” segment of the western rim of the vast crater named Endeavour, some 14 miles (22 km) wide that’s loaded with a bountiful variety of rocks and soil that neither Opportunity nor her twin Spirit have ever touched and drilled into before and stem from an earlier epoch when liquid water flowed eons ago and perhaps may have been more favorable to sustaining life.

“Opportunity is currently sitting on Saddleback at Greeley Haven, an outcrop of impact breccias on Cape York, Endeavour crater’s rim,” Ray Arvidson told Universe Today. Arvisdon is the mission’s deputy principal investigator, of Washington University in St. Louis.

“Her northerly tilt is about ~15 degrees which is enough to have a vibrant winter campaign. The Martian southern winter solstice occurs at the end of March. A few months after that date we will drive her off the outcrop and further explore Cape York.”

Approaching 'Greeley Haven' on Endeavour Rim
Opportunity captured this view of a northward-facing outcrop, "Greeley Haven," where the rover will work during its fifth Martian winter. This southward-looking image was taken on Sol 2790 on Mars (Nov. 29, 2011). The rover team chose this designation as a tribute to the influential planetary geologist Ronald Greeley (1939-2011), who was a member of the science team for the Mars rovers and many other interplanetary missions. Credit: NASA/JPL-Caltech

“Greeley Haven” is named in tribute to planetary Geologist Ronald Greeley (1939-2011) who was a beloved member of the rover science team and a host of other NASA planetary missions. He taught at Arizona State University and inspired several generations of students and planetary scientists until his recent death on Oct. 27, 2011.

“We’ll hunker down at Greeley Haven as long as we need to, and we’ll do good science while we’re there,” Steve Squyres of Cornell University, Ithaca, N.Y., told Universe Today. Squyres is the Principal Investigator for Opportunity.

Opportunity is collecting a high resolution 360 degree panorama to commemorate Greeley.

Throughout the past 4 Martian winters, Opportunity had continued to traverse without pause. But this winter time it’s different because the solar panels are significantly more coated with an obscuring layer of dust hindering their energy output.

So the rover is parked with a tilt for her 5th Martian winter, mimicking the successful strategy power boosting used by Spirit to survive 3 harsh Martian winters.

And there is a silver lining to sitting mostly still that enables a chance to determine what’s at the core of the Red Planet, a key fact we don’t know.

“This winter science campaign will feature two way radio tracking with Earth to determine the Martian spin axis dynamics – thus the interior structure, a long-neglected aspect of Mars,” Arvidson told me.

I asked Squyres for a progress update and how long would the data collection require ?

Squyres replied that the experiment has already begun and added – “Hard to say how long. It’s months, as opposed to weeks or years, but it depends very much on data quality and the amount of data we get per week. We’re very early in the experiment now… we’ll just see how it goes.”

Locator Map for 'Greeley Haven' on Endeavour Crater Rim
Opportunity will spend its fifth Martian winter working at Greeley Haven on the western rim of Endeavour Crater. Credit: NASA/JPL-Caltech/UA

Voyager Mission Is Cooling Its Jets

Artist's concept of NASA's Voyager spacecraft. Image credit: NASA/JPL-Caltech

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Or, more appropriately, Voyager 1 is cooling its instruments. To help conserve power, the mission managers at NASA have decided to cut the electricity to a heating element – one that’s part of the nearby infrared spectrometer that’s not been in operation for some 14 years. This power cut will lower the temperature of the ultraviolet spectrometer by about 23 degrees Celsius (41 degrees Fahrenheit)… a temperature that’s mild compared to the below minus 79 degrees Celsius (minus 110 degrees Fahrenheit) that the instrument has dropped to in previous times. It’s not a drastic measure, however, but all part of a crucial plan to manage electrical power to keep the spacecraft operational and transmitting data for another 13 years.

Just because the power is cut back doesn’t mean the instrument quit working. At the present, the spectrometer is continuing to gather and transmit data. The resilient system was designed to work in temperatures as frosty as minus 35 degrees Celsius (minus 31 degrees Fahrenheit) and has even operated beyond the call of duty when heaters were switched off over the last 17 years. While it was taking a chance that the equipment might malfunction, the engineering team was confident since the spectrometer has worked at minus 56 degrees Celsius (minus 69 degrees Fahrenheit.) since 2005. “The spectrometer is likely operating at a temperature somewhat lower than minus 79 degrees Celsius, or minus 110 degrees Fahrenheit,” says the team. “But the temperature detector does not go any lower.”

While it has been awhile since Voyager 1’s encounter with Jupiter and Saturn which made the spectrometer busy, that doesn’t mean its data will be disregarded. Both scientists and mission management specialists will continue to monitor performance levels and an international team of scientists will further review spectrometer data.

Live long and prosper, Voyager!

Original Story Source: JPL News Release.

Carnival of Space #233

This week’s Carnival of Space is hosted by Bill Dunford at Riding with Robots on the High Frontier.

Click here to read the Carnival of Space #233, a variety of space news and images from around the web.

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, sign up to be a host. Send and email to the above address

Stunning Auroras From Around the World (January 22-23, 2012)

This photo was taken on January 22, 2012 in Fairbanks North Star Borough County, Alaska, US, using a Nikon D5000. The explodey look is due to perspective from looking right up the magnetic field lines. The aurora in the middle of the explosion is pointing straight down at the camera. Credit: Jason Ahrns

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On January 22nd 2012, skywatchers in the northern hemisphere were rewarded with amazing displays of aurora. The cause of these displays was a Kp level 5.67 geomagnetic storm originating from solar activity on the 19th of January, produced visible aurorae throughout the northern hemisphere and viewers as far south as northeast England had great auroral views.

Here is a selection of aurora images and videos taken during the event.

More below!

Aurora over Donegal, Ireland. Credit: Brendan Alexander

Brian Horisk adventureart.co.uk hills near Dundee

Callum - Aberdeen
Looking north from the science operations center at Poker Flats, Alaska. Credit: Jason Ahrns.
David Woodford
Gerry Mcgegor - over looking John O'Groats & orkney's
Gillian C - Edinburgh
Graham Scott - Aberdeenshire
Lawrie Dryden - Kinloss
Corinne Mills - Near Dundee Scotland
Andrew Smith - St Mary's Lighthouse Whitley Bay England
Brian Smith - Clackmannanshire Scotland
Graham Scott - Aberdeenshire
Jon Porter Kielder - Northumberland England
Alan Rowe
Dean Mann - Nethybridge Highlands
Ben Hurst - Dundee
David Breen - Newcastle Upon Tyne England
David Breen - Newcastle Upon Tyne England
Aurora Webcam Sweden http://www.auroraskystation.com/live-camera/9/
Lee Jennings Cresswell Beach Northumberland England
Lee Jennings Cresswell Beach Northumberland England

Key Step in Evolution Replicated by Scientists – With Yeast

Sacharomyces cerevisiae yeast cells. Credit: Wikimedia Commons

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One of the great puzzles in science has been the evolution of single-celled organisms into the incredibly wide variety of flora and fauna that we see today. How did Earth make the transition from an initially lifeless ball of rock to one populated only by single-celled organisms to a world teeming with more complex life?

As scientists understand it, single-celled organisms first began evolving into more complex forms more than 500 million years ago, as they began to form multi-cellular clusters. What isn’t understood is just how that process happened. But now, biologists are another step closer figuring out this puzzle, by successfully replicating this key step – using an ingredient common in the making of bread and beer – ordinary Brewer’s yeast (Saccharomyces cerevisiae). While helping to solve evolutionary riddles here on Earth, it also by extension has bearing on the question of biological evolution on other planets or moons as well.

The results were published in last week’s issue of the Journal Proceedings of the National Academy of Sciences (PNAS).

Yeasts are a microscopic form of fungi; they are uni-cellular but can become multi-cellular through the formation of a string of connected budding cells, like in molds. The experiments were based on this fact, and were surprisingly simple, they just hadn’t been done before, according to Will Ratcliff, a scientist at the University of Minnesota (UMN) and a co-author of the paper. “I don’t think anyone had ever tried it before,” he said, adding: “There aren’t many scientists doing experimental evolution, and they’re trying to answer questions about evolution, not recreate it.”

Sam Scheiner, program director in NSF’s Division of Environmental Biology, also adds: “To understand why the world is full of plants and animals, including humans, we need to know how one-celled organisms made the switch to living as a group, as multi-celled organisms. This study is the first to experimentally observe that transition, providing a look at an event that took place hundreds of millions of years ago.”

It’s been thought that the step toward multi-cellular complexity was a difficult one, an evolutionary hurdle that would be very hard to overcome. The new research however, suggests it may not be that difficult after all.

It took the first experiment only 60 days to produce results. The yeast was first added to a nutrient-rich culture, then the cells were allowed to grow for one day. They were then stratified by weight using a centrifuge. Clusters of yeast cells landed on the bottom of the test tubes. The process was then repeated, taking the cell clusters and re-adding them to fresh cultures. After sixty cycles of this, the cell clusters started to look like spherical snowflakes, composed of hundreds of cells.

The most significant finding was that the cells were not just clustering and sticking together randomly; the clusters were composed of cells that were genetically related to each other and remained attached after cell division. When clusters reached “critical mass,” some cells died, a process known as apoptosis, which allows the offspring to separate.

This then, simply put, is the process toward multi-cellular life. As described by Ratcliff, “A cluster alone isn’t multi-cellular. But when cells in a cluster cooperate, make sacrifices for the common good, and adapt to change, that’s an evolutionary transition to multi-cellularity.”

So next time you are baking bread or brewing your own beer, consider the fact that those lowly little yeast cells hold a lot more importance than just a useful role in your kitchen – they are also helping to solve some of the biggest mysteries of how life started, both here and perhaps elsewhere.

NOAA: Largest Solar Radiation Storm Since 2005 Now in Progress

X-Ray image from a GOES satellite at 14:12 UTC on January 23, 2012. Credit: NOAA

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Earth’s magnetic field is already full of activity from an Earth-directed Coronal Mass Ejection (CME) last week. But all indications are another blast is headed our way from the strongest solar radiation storm since September, 2005. NOAA says the storm is currently in progress and continues to get stronger, with a very fast CME headed towards Earth. Sunspot 1402 erupted, producing a long-duration M9-class solar flare. “Geomagnetic storming is a near certainty from this event,” reported NOAA. The associated solar flare peaked at about 0400 UTC on January 23 (11pm Jan 22 EST).”

A computer model just released by NOAA’s Space Weather Prediction Center forecasts the storm will arrive sometime on January 24, at about 14:18 UT (+/- 7 hours), as the CME is traveling at approx. 2,200 km per second. Click here to see the animated model.

We’ve already shown you a video of the auroral activity going on yesterday and will soon post a gallery of beautiful aurorae from around the world. And it looks like we’ll likely have more photos to share in the coming week! And NASA says skywatchers should be on the lookout for aurora in lower than normal latitudes. Scientists are also predicting that Mars will get hit too, several hours after Earth. At this point, there’s no way to predict the possible effect on Earth-orbiting satellites for communications, GPS, etc, or the effect on Mars spacecraft.

These kinds of events can cause problems for spacecrafts in geosynchronous, polar and other orbits passing could be affected by the cloud’s arrival. In addition, strong geomagnetic storms are possible, so high-latitude sky watchers should be alert for aurorae.

Below is a video from the Solar Dynamics Observatory of the event:

Gabby Giffords To Resign From Congress

U.S. Congresswoman Rep. Gabrielle Giffords (D) announced today, Sunday Jan. 22, that she will step down from Congress later this week to continue recuperating from critical brain injuries she suffered during a deadly assassination attempt a year ago in Tucson, Arizona.

She announced the resignation on her official congressional website and in a poignant YouTube video message (see above) to her constituents saying that she will “do what is best for Arizona” as she recovers from the shooting attack that happened 1 year ago on Jan. 8, 2011 in her Arizona district.

One of her last official acts will be to attend the State of the Union Address by President Obama on Tuesday, January 24 at the Capitol in Washington, D.C.

Giffords is submitting letters of resignations to House Speaker John Boehner and Arizona Gov. Jan Brewer. Brewer will call a special primary and general election to fill her seat for the remainder of her term which expires at the end of 2012. The primary election will be held within about 60 days. She represented the 8th Congressional District in southern Arizona.

“Gabby Giffords embodies the very best of what public service should be. She’s universally admired for qualities that transcend party or ideology – a dedication to fairness, a willingness to listen to different ideas, and a tireless commitment to the work of perfecting our union. That’s why the people of Arizona chose Gabby – to speak and fight and stand up for them,” President Obama said in a statement issued Sunday evening. “Gabby’s cheerful presence will be missed in Washington. But she will remain an inspiration to all whose lives she touched – myself included. And I’m confident that we haven’t seen the last of this extraordinary American.”

“I salute Congresswoman Giffords for her service, and for the courage and perseverance she has shown in the face of tragedy. She will be missed,” House Speaker John Boehner said in a statement issued Sunday.

Before the shooting she was considered to be a rising star in Congress.

Giffords was shot in the head at point blank range. Six people were killed including a 9 year old girl and a Federal Judge and 13 others were wounded.

The 41 year old congresswoman is resigning in order to continue her recovery from the gunshot wounds she suffered a year ago while conducting a ‘meet-and-greet’ with her constituents at a shopping center in Tucson. She has been undergoing intensive rehabilitation over the past year.

U.S. Congresswoman Rep. Gabrielle Giffords of Arizona announced on Jan. 22, that she will step down from Congress. This still image is from her official video announcement.

“I have more work to do on my recovery, so to do what is best for Arizona, I will step down this week,” Congresswoman Giffords says in the heartfelt two minute video message to her constituents.

“A lot has happened over the past year,” she said in halting words. “We cannot change that. But I know on the issues we fought for, we can change things for the better. Jobs, border security, veterans. We can do so much more by working together.”

The video features footage of Giffords before and after the attack, some of it quite graphic.

“I don’t remember much from that horrible day, but I will never forget the trust you placed in me to be your voice,” Giffords goes on to say. “Thank you for your prayers and for giving me time to recover. I have more work to do on my recovery. So to do what is best for Arizona, I will step down this week.”

Giffords was first elected to the U.S. House of Representatives in November 2006. She was last re-elected in November 2010 and now will not seek re-election this fall.

Gabby Giffords was a strong supporter of NASA and America’s space program.

Gabby Giffords and Mark Kelly

She is married to veteran Astronaut Mark Kelly, who commanded the last mission of Space Shuttle Endeavour in May 2011, STS-134. Kelly recently resigned from NASA to continue helping Gabby in her recovery.

The shooting happened as Kelly was in the final stages of training for the STS-134 mission. Kelly temporarily interrupted his training to be with his wife who was in critical condition.

Space Shuttle Endeavour launches on May 16, 2011 from the Kennedy Space Center with veteran Shuttle Commander Mark Kelly, husband of Congresswoman Gabrielle Giffords. Credit: Ken Kremer

Gabby Giffords has made a remarkable recovery and she continues to improve and inspire all of us every day. She faces a long road of recovery ahead that will require all her efforts to continue making progress.

“Every day my spirit is high. I will return. Thank you !” – Giffords signs off

Solar Storm Sparks Stunning Aurora

The Earth-directed solar storm we alerted readers to this week has hit, with reports of auroral activity in Russia, Denmark, Scotland, England, and Norway. Helge Mortensen from Tromvik, Norway captured this stunning video. According to Spaceweather.com, the coronal mass ejection (CME) hit Earth’s magnetic field at 0617 UT on Jan. 22nd.

There’s also a live aurora webcam you can watch via this link

Check out the likelihood of seeing aurorae where you live at the NOAA Auroral Activity webpage, which includes maps for both northern and southern hemispheres.