Archive for goddard space flight center

Young Planet around TW Hydrae Challenges Theories on How Planets Form – Sci

A new study published in the Astrophysical Journal (arXiv.org version) provides evidence that an extrasolar planet may be forming quite far from a small red dwarf star known as TW Hydrae.

TW Hydrae protoplanetary disk (NASA / ESA / J. Debes, STScI / H. Jang-Condell, University of Wyoming / A. Weinberger, Carnegie Institution of Washington / A. Roberge, Goddard Space Flight Center / G. Schneider, University of Arizona, Steward Observatory / A. Feild, STScI, AURA)

TW Hydrae protoplanetary disk (NASA / ESA / J. Debes, STScI / H. Jang-Condell, University of Wyoming / A. Weinberger, Carnegie Institution of Washington / A. Roberge, Goddard Space Flight Center / G. Schneider, University of Arizona, Steward Observatory / A. Feild, STScI, AURA)

TW Hydrae is located some 176 light-years away in the constellation Hydra. It is only about 55% of the mass of the Sun.

The study authors led by Dr Glenn Schneider from the University of Arizona used NASA’s Hubble Space Telescope to detect a deficit of material in the TW Hydrae’s protoplanetary disk at about 80 AUs (astronomical units), or 7.5 billion miles. If the planet orbited in our Solar System, it would be roughly twice Pluto’s distance from the Sun.

Astronomers’ models indicate that the depression is about 20 AUs wide, just slightly wider than necessary for a planet-opening gap and consistent with a planet of between 6 and 28 Earth masses. The feature is seen at all wavelengths indicating it is structural and not a local compositional difference. The astronomers believe the evidence is strong for planet formation causing the gap.

“TW Hydrae is between 5 and 10 million years old, and should be in the final throes of planet formation before its disk dissipates,” said study co-author Dr Alycia Weinberger of the Carnegie Institution.

“It is surprising to find a planet only 5 to 10% of Jupiter’s mass forming so far out since planets should form faster closer in. In all planet formation scenarios, it’s difficult to make a low-mass planet far away from a low mass star.”

The goal of the study was to understand not only whether planets have formed, but also what conditions can result in planet formation and what chemical constituents are available for new planets. Models showed that the disk was brighter than expected, which indicates that very small dust grains are being lifted high above the midplane. This is surprising because observations with radio telescopes have previously shown that the disk contains dust that has conglomerated into pebbles.

The scientists designed the observations to be able to detect large water ice grains in the surface layer of the disk. These grains weren’t seen, which probably means that they have grown and sunk to the midplane of the disk where they can aggregate into water-rich planets.

Planet formation far away from a small parent star is at odds with the conventional planet-making dogma. Under the most accepted scenario, planets form over tens of millions of years from the slow accretion of dust, rocks, and gas. That happens most easily close to the central star, where orbital timescales are short. Even under a disk instability scenario, in which planets can collapse quickly from the disk, it’s not clear such a low mass planet could form.

“Typically, you need pebbles before you can form a planet. So, if there is a planet in the gap and there is no dust larger than a grain of sand farther out, we have provided a challenge for traditional planet formation models,” concluded study lead author Dr John Debes from the Space Science Telescope Institute.

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Bibliographic information: John H. Debes et al. 2013. The 0.5-2.22 μm Scattered Light Spectrum of the Disk around TW Hya: Detection of a Partially Filled Disk Gap at 80 AU. ApJ 771, 45; doi: 10.1088/0004-637X/771/1/45

Article source: http://www.sci-news.com/astronomy/article01156-planet-tw-hydrae.html

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NASA’s Asteroid Sample Return Mission Moves into Development

RELEASE
:
13-143

NASA’s Asteroid Sample Return Mission Moves into Development

WASHINGTON — NASA’s first mission to sample an asteroid is moving ahead into development and testing in preparation for its launch in 2016.

The Origins-Spectral Interpretation Resource Identification Security Regolith Explorer (OSIRIS-REx) passed a confirmation review Wednesday called Key Decision Point (KDP)-C. NASA officials reviewed a series of detailed project assessments and authorized the spacecraft’s continuation into the development phase.

OSIRIS-REx will rendezvous with the asteroid Bennu in 2018 and return a sample of it to Earth in 2023.

“Successfully passing KDP-C is a major milestone for the project,” said Mike Donnelly, OSIRIS-REx project manager at NASA’s Goddard Space Flight Center in Greenbelt, Md. “This means NASA believes we have an executable plan to return a sample from Bennu. It now falls on the project and its development team members to execute that plan.”

Bennu could hold clues to the origin of the solar system. OSIRIS-REx will map the asteroid’s global properties, measure non-gravitational forces and provide observations that can be compared with data obtained by telescope observations from Earth. OSIRIS-REx will collect a minimum of 2 ounces (60 grams) of surface material.

“The entire OSIRIS-REx team has worked very hard to get to this point,” said Dante Lauretta, OSIRIS-REx principal investigator at the University of Arizona in Tucson. “We have a long way to go before we arrive at Bennu , but I have every confidence when we do, we will have built a supremely capable system to return a sample of this primitive asteroid.”

The mission will be a vital part of NASA’s plans to find, study, capture and relocate an asteroid for exploration by astronauts. NASA recently announced an asteroid initiative proposing a strategy to leverage human and robotic activities for the first human mission to an asteroid while also accelerating efforts to improve detection and characterization of asteroids.

NASA’s Goddard Space Flight Center in Greenbelt, Md. will provide overall mission management, systems engineering and safety and mission assurance. The University of Arizona in Tucson is the principal investigator institution. Lockheed Martin Space Systems of Denver will build the spacecraft. OSIRIS-REx is the third mission in NASA’s New Frontiers Program. NASA’s Marshall Space Flight Center in Huntsville, Ala., manages New Frontiers for NASA’s Science Mission Directorate in Washington.

For more information on OSIRIS-REx, visit:

http://www.nasa.gov/mission_pages/osiris-rex/index.html

and

http://osiris-rex.lpl.arizona.edu/

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Article source: http://www.nasa.gov/home/hqnews/2013/may/HQ_13-143_OSIRIS-Rex.html

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NASA fast-motion video of sun: ‘Violent dance’

The sun is ramping up toward solar maximum — the white-hot peak of activity in an 11-year cycle — and NASA has been snapping images of the phenomenon every 12 seconds for three years.

The space agency put together a three-minute video showing images taken by the Solar Dynamic Observatory since spring 2010. As the Los Angeles Times’ Deborah Netburn reported last month, the NASA video stitches together two SDO images per day over the three-year period.

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Alex Young, a heliophysicist at Goddard Space Flight Center, narrates the video to point up some of the sun’s best-of moments in that time frame. The video shows the whirling, boiling mass of gases that is our nearest star. It also shows a partial eclipse by the moon, the largest flare of this solar cycle and the every-100-years Transit of Venus.

Young told The Times on Friday that, from a historical point of view, this is scientists’ moment in the sun: “Combining all the extremely detailed data that we have … scientists now have the most complete view of the sun in history.”

The SDO has provided virtually uninterrupted multi-wavelength views of the star by way of three instruments, he said.

According to Goddard, the observatory has regularly captured solar flares and coronal mass ejections in action. This space weather may hurl radiation and solar material toward the Earth, where it can cause radio blackouts and, in extreme cases, disrupt power. It can also interfere with satellites in space.

“SDO’s glimpses into the violent dance on the sun help scientists understand what causes these giant explosions — with the hopes of some day improving our ability to predict this space weather,” an online posting from the space center said.

Images provided by the SDO have been stable, according to the center, despite the fact that the craft orbits the Earth at 6,876 mph and the Earth orbits the sun at 67,062 mph. 

Young said that as scientists “combine all these amazing data with data from upcoming missions such as IRIS, we move one step closer to piecing together the puzzle that is the sun. Understanding the solar cycle is one of these pieces.”

The scientist said that all of the SDO images were exciting to him as a heliophysicist, but that his personal favorite was the Transit of Venus. The transit was a once-in-a-lifetime occurrence, when Venus moved between the sun and the Earth and viewers saw a tiny dot floating across the surface of the sun over several hours.

“I was able to observe that rare event both with SDO and in person from the top of Mauna Kea, Hawaii, while I was on my honeymoon,” he said

ALSO:

Space station has sprung a leak

Comet of the century? This could fizzle

Watch: Astronaut wrings out washcloth in space

 

Article source: http://www.latimes.com/news/science/sciencenow/la-sci-sn-solar-maximum-nasa-video-20130510,0,7791678.story

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NASA’s GROVER Debuts On Greenland’s Ice Sheet

NASA’s GROVER Debuts On Greenland’s Ice Sheet

NASA’s new Earth-bound rover began testing on the Greenland ice sheet this week.

GROVER, which stands for both Greenland Rover and Goddard Remotely Operated Vehicle for Exploration and Research, is an autonomous, solar-operated robot that carries a ground-penetrating radar to examine the layers of Greenland’s ice sheet. Its findings will help scientists understand how the massive ice sheet gains and loses ice.

The GROVER team, led by glaciologist Lora Koenig from NASA’s Goddard Space Flight Center in Greenbelt, Md., arrived in Summit Camp, the highest spot in Greenland, on May 6, 2013. After loading and testing the rover’s radar and fixing a minor communications glitch, the team began the robot’s tests on the ice on May 8, defying winds of up to 23 mph (37 kph) and temperatures as low as minus 22 F (minus 30 C).

The GROVER tests will continue through June 8. GROVER, a prototype, was first developed in 2010 and 2011 during summer engineering boot camps at Goddard, before further refinement, with NASA funding, at Boise State University. Its trial in Greenland will also serve as a test of using rovers in harsh polar regions to gather data.

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Image Credit: Lora Koenig / NASA Goddard

Article source: http://www.nasa.gov/multimedia/imagegallery/image_feature_2506.html

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Saving Fermi: NASA’s system for avoiding collisions with space junk

In late March last year, the people operating the Fermi Gamma-ray Space Telescope got a bit of a scare. Their hardware was one week away from a close encounter with a defunct Russian spy satellite. A week might seem like short notice for one-of-a-kind hardware like Fermi, but in some ways the team was lucky to have any warning at all. Prior to 2007, NASA didn’t even have a policy in place to identify threats to unmanned hardware.

That has now changed. Thanks to cooperation between the military and the Goddard Space Flight Center, everything that can possibly get out of the way of space junk is regularly tracked for potential collision risks. That system is what alerted Fermi’s controllers to the danger and allowed them to use on-board thrusters for something they were never designed to do: move the satellite safely out of the way.

Tracking threats

The technical term for the risk identification process is “conjunction assessment,” or CA. This process involves taking the latest tracking information, calculating orbits, and figuring out whether two objects are likely to be in the same place at the same time. This may seem like an easy problem—after all, it’s just math—but there are a lot of potential complications. One is simply the ever-expanding catalog of junk in the relevant orbits (primarily low-Earth and geostationary), some of it caused by collisions between two existing pieces of junk. Another is the fact that these orbits aren’t stable. The atmosphere may be sparse at these altitudes, but it’s still there, and it creates varying amounts of drag on things in orbit.

Finally, tracking junk is not a matter of knowing precisely where everything is at all times. The measurements come with uncertainties and aren’t constantly updated, so these uncertainties can grow with time. At best, you can typically only calculate the probability of a collision rather than getting a binary yes-or-no answer.

The Goddard Space Flight Center started this sort of monitoring in 2004, but things were formalized in 2007 when NASA issued its first formal policy. If the hardware was in or near low-Earth or geosynchronous orbit and it had the capability to maneuver in orbit, it needed to have conjunction assessments performed. To make sure these assessments were good, NASA entered into an agreement with the Department of Defense, which has a group (USSTRATCOM) that tracks space objects. With this policy in place, Goddard expanded its service, offering to perform assessments for any unmanned NASA hardware.

The system is heavily automated, performing daily downloads of the latest tracking data and running analyses out to one week for low-Earth orbits and 10 days for geosynchronous ones. Goddard staff perform a more detailed analysis every Monday, Wednesday, and Friday. The software collection uses Matlab, a commercial software package, to run three different types of collision probabilities (2-D, Monte Carlo, and nonlinear). Other commercial software is used to visualize any potential collisions identified by the software.

Potential collisions are flagged for monitoring if there’s simply a high probability of conjunction. Typically, the probability goes down after a couple of additional days of tracking, but in rare cases this doesn’t happen (and, in a few, the probability went up with further monitoring). When the probability doesn’t go down, the software can calculate a maneuver that will reduce the probability of collision to an acceptable level. The solution will take into account other potential hazards as well as mission requirements—some Earth-monitoring satellites can’t orbit above a certain altitude and still perform their jobs.

Saving Fermi

This is the system that alerted Fermi controllers that they might experience a close encounter with Cosmos 1805, a defunct Russian spy satellite. The expected distance between the two: about 200 meters. For context, the Russian satellite that wiped out an Iridium communication satellite had been expected to pass nearly 600m from it. That and a relative speed of over 40,000 kilometers an hour would be enough to make anyone nervous.

Fermi doesn’t actually need to change its orbit in order to function. Eric Stoneking, Fermi’s lead engineer for its attitude control systems, said the telescope normally functions in one of two modes. In one, the satellite remains stationary and lets its low-Earth orbit sweep its field of view in order to survey the entire sky. When it is imaging a specific object or event, Fermi rotates in synchrony with its orbit in order to remain pointed at the same location in the sky. Stoneking told Ars that these changes are all done using reaction wheels, the same pointing devices that direct hardware like the Hubble Space Telescope (and Kepler, where their failures are putting the mission at risk).

Since it’s mostly just scanning the sky, “Fermi has no orbit maintenance needs,” Stoneking said. Despite that, it does have on-board thrusters. NASA requires its satellites to have what is termed “de-orbit capability.” Basically, they have to be able to be sent into the atmosphere to burn up safely rather than falling in an uncontrolled manner or staying in orbit and contributing to the junk problem. To deorbit at the end of its mission, Kepler had onboard thrusters.

The problem is that they were only meant to be fired once, after the mission was over. Firing them earlier made people a bit nervous, both because of a history of past problems that occurred while powering up thrusters for the first time—hardware has been lost due to leaks or even explosions—and because of what Stoneking called “the natural inclination to think things over before doing something that can’t be undone.” Nevertheless, given the 1,400kg threat zooming at it, the Fermi team worked with the Goddard collision assessment group to plan a maneuver that would get it safely out of the way.

Over several days, the risk of a collision did not go away and the team decided to move Fermi. This required stowing the telescope’s solar panels and communication antenna, which could have been damaged by the propellant, and using the reaction wheels to point it in the intended direction of travel. When those were done, it only took a one-second firing to move Fermi safely out of the way. With the burn done, the process was reversed in less than an hour and Fermi was back in operation.

Even Fermi’s future death was unaffected. “We fired the thrusters for about a second total,” Stoneking told Ars. “For deorbit, we’ll fire them for well over half an hour.”

Article source: http://arstechnica.com/science/2013/05/saving-fermi-nasas-system-for-avoiding-collisions-with-space-junk/

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Satellite Animation Shows Smoke from California’s Springs Fire


On May 3, 2013, the NOAA GOES infrared and visible imagery were combined to create an animation that showed the plume of smoke from the fire. The smoke plume is seen blowing west and out over the eastern Pacific Ocean. The animation runs 17 seconds and shows the smoke plume from May 3 at 1415 to 2000 UTC (10:15 a.m. to 4 p.m. EDT) was created by the NASA GOES Project, located at NASA’s Goddard Space Flight Center, Greenbelt, Md.

According to Reuters news, the Springs Fire has now consumed as much as 28,000 acres of brush in the coastal area located northwest of Los Angeles. The fire started on Thursday, May 2, and by Sunday, May 5, the weather allowed firefighters to put containment lines around the fire.

NOAA’s GOES-15 or GOES-West satellite sits in a fixed orbit that continually monitors the weather over the western U.S.

Text: Robert Gutro
NASA’s Goddard Space Flight Center, Greenbelt, MD

Article source: http://www.nasa.gov/mission_pages/fires/main/20130506-CA-Springs.html

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Fermi, Swift see “shockingly bright” burst

Views of gamma-ray burst 130427AA record-setting blast of gamma rays from a dying star in a distant galaxy has wowed astronomers around the world. The eruption, which is classified as a gamma-ray burst (GRB) and designated GRB 130427A, produced the highest-energy light ever detected from such an event.

“We have waited a long time for a gamma-ray burst this shockingly, eye-wateringly bright,” said Julie McEnery from NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “The GRB lasted so long that a record number of telescopes on the ground were able to catch it while space-based observations were still ongoing.”

Just after 3:47 a.m. EDT on Saturday, April 27, Fermi’s Gamma-ray Burst Monitor (GBM) triggered on an eruption of high-energy light in the constellation Leo. The burst occurred as NASA’s Swift satellite was slewing between targets, which delayed its Burst Alert Telescope’s detection by less than a minute.

Fermi’s Large Area Telescope (LAT) recorded one gamma ray with an energy of at least 94 billion electron volts (GeV), or some 35 billion times the energy of visible light, and about three times greater than the LAT’s previous record. The GeV emission from the burst lasted for hours, and it remained detectable by the LAT for the better part of a day, setting a new record for the longest gamma-ray emission from a GRB.

The burst subsequently was detected in optical, infrared, and radio wavelengths by ground-based observatories, based on the rapid accurate position from Swift. Astronomers quickly learned that the GRB was located about 3.6 billion light-years away, which for these events is relatively close.

Gamma-ray bursts are the universe’s most luminous explosions. Astronomers think most occur when massive stars run out of nuclear fuel and collapse under their own weight. As the core collapses into a black hole, jets of material shoot outward at nearly the speed of light.

The jets bore all the way through the collapsing star and continue into space, where they interact with gas previously shed by the star and generate bright afterglows that fade with time.

If the GRB is near enough, astronomers usually discover a supernova at the site a week or so after the outburst.

“This GRB is in the closest 5 percent of bursts, so the big push now is to find an emerging supernova, which accompanies nearly all long GRBs at this distance,” said Neil Gehrels from Goddard.

Ground-based observatories are monitoring the location of GRB 130427A and expect to find an underlying supernova by midmonth.

Article source: http://www.astronomy.com/~/link.aspx?_id=2a8103b1-c869-4612-ac1c-8b77d106a7bc

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NASA’s next rover target after Mars? Greenland

From May 3 to June 8, the Goddard Remotely Operated Vehicle for Exploration and Research will travel to the highest part of the ice-locked landmass to examine the record of changes contained in the ice sheet’s frigid layers.

The 6-foot-tall GROVER weighs in at 800 pounds and rolls around on modified snowmobile tracks at an average speed of 1.2 miles per hour. Because it’s powered by solar panels, it doesn’t pollute the air — and because the summer sun doesn’t fall beneath the horizon, the rover can operate day and night.

Human explorers often search such extreme environments in person, said Lora Koenig, a Goddard glaciologist GROVER science adviser, who has crossed “hundreds of kilometers” of western Antarctica doing similar research. But unlike humans, robots don’t need to take a break on the ice.

“We have to make camps, take time out to eat, make water — and all the living on the ice sheet takes a lot of time,” Koenig said in an interview shortly before boarding a plane to Greenland. “The robot, even though it’ll go slower, should be able to gather more data because it can operate 24 hours a day.”

Research with a rover is less expensive than most other methods, including human exploration and aircraft surveys.

The rover will send radar waves through the ice, which will bounce off buried features and give the scientists a picture of the story contained in its layers of compacted snow. For scientists studying climate change, this is crucial data: Greenland began making the news last summer when scientists realized that higher temperatures were causing melting across 97% of the ice sheet.

GROVER was designed by teams of students in 2010 and 2011 at an engineering boot camp at NASA’s Goddard Space Flight Center in Greenbelt, Md.

One of the graduate students, Gabriel Trisca, said that GROVER could be a useful platform for all kinds of science instruments, not just radar. 

“It would be just a matter of getting one instrument and plugging it in,” Trisca said as he and fellow Boise State University graduate student Mark Robertson headed to the airport. “I hope there are other projects that can benefit from an autonomous vehicle like this, that can be controlled via satellite from anywhere in the world.”

Follow me on Twitter @aminawrite.

Article source: http://www.latimes.com/news/science/sciencenow/la-sci-nasa-rover-grover-greenland-ice-mars-20130503,0,5267625.story

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NASA Hubble Space Telescope questions answered by Jennifer Wiseman


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April 28, 2013 |
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NASA - National Aeronautics and Space AdministrationGreenbelt, MD – NASA’s Jennifer Wiseman is the senior project scientist for the Hubble Space Telescope at NASA’s Goddard Space Flight Center in Greenbelt, MD, where the mission is managed.

The following questions and answers were provided in April 2013 about the history and the status of the Hubble.

Jennifer Wiseman is a senior astrophysicist at the NASA Goddard Space Flight Center, where she serves as the Senior Project Scientist for the Hubble Space Telescope. (Credit: NASA)

Jennifer Wiseman is a senior astrophysicist at the NASA Goddard Space Flight Center, where she serves as the Senior Project Scientist for the Hubble Space Telescope. (Credit: NASA)

Can you provide some basic information about the Hubble?

The Hubble Space Telescope was launched in 1990, aboard a NASA space shuttle. It is a satellite orbiting the Earth every 90 minutes.

Instruments like cameras and spectrographs on board observe objects in space, getting a clear view because the telescope is above the Earth’s atmosphere and clouds. The telescope transmits its observations to receivers on the ground, and then scientists and the public can view the images and analyze the data.

What is Hubble’s Lifetime?

The Hubble Space Telescope floats against the background of Earth after a week of repair and upgrade by Space Shuttle Columbia astronauts in 2002. (Credit: NASA/STSCI)

The Hubble Space Telescope

When Hubble was originally launched, the goal was for the telescope to operate at least 15 years, but possibly much longer. It has now been in operation 23 years, and we anticipate several more years of good operation.

The reason it could last so long is that the telescope was designed to be visited by astronauts every few years. The astronauts have been able to put in new instruments, repair other malfunctioning instruments, and refurbish the telescope five times since launch, making it like a new telescope each time.

How is Hubble Functioning Now (April 2013)?

Hubble is working very well right now; in fact, with new instruments installed just four years ago (2009) during the last astronaut servicing mission, Hubble has become more scientifically powerful than ever.

We expect the telescope to keep working well for years leading up to (and hopefully beyond) the launch of the next major flagship space telescope, the James Webb Space Telescope, which is scheduled for launch in 2018.

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Can you cite some of Hubble’s most astounding discoveries?

Some of the most profound discoveries include these:

  • Hubble measured the expansion rate of the universe, and helped us determine the age of the universe to be about 13.7 billion years.
  • Hubble also was used to study the expansion history of the universe, including observations that, along with ground-based telescope observations, led to the discovery that the expansion of the universe is accelerating due to the mysterious “dark energy” phenomenon.
  • Hubble was the first telescope to analyze the chemical makeup of the atmosphere of a planet outside our solar system.
  • Hubble was used to determine that most galaxies have powerful black holes at their centers, including our own Milky Way galaxy.
  • Hubble images showed that young stars are encircled by flattened dusty disks, the region where planets are forming.
  • Hubble has discovered several previously unknown moons of Pluto.

Where can I find images and more information about Hubble and its discoveries?

You can find spectacular images and information about the Hubble Space Telescope at http://hubblesite.org or www.nasa.gov/hubble.

For Hubble Factoids, visit:
www.nasa.gov/mission_pages/hubble/story/index.html

For the Hubble story, visit:
www.nasa.gov/mission_pages/hubble/story/the_story.html


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Article source: http://www.clarksvilleonline.com/2013/04/28/nasa-hubble-space-telescope-questions-answered-by-jennifer-wiseman/

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NASA Probes Near Sun Safe from Triple Solar Eruption




A coronal mass ejection is heading toward Mercury. The CME exploded from the sun on April 20, 2013.


This image of a coronal mass ejection (CME) was captured on April 20, 2013. The CME is headed in the direction of Mercury. The large bright spot on the left is Venus.
CREDIT: ESANASA/SOHO


Two NASA spacecraft are safe and sound, after the sun unleashed three intense back-to-back solar eruptions in their direction, scientists say.

NASA’s Messenger spacecraft in orbit around Mercury and the Stereo-A, which studies the sun from Earth orbit, suffered no damage from the passing solar storms.

On April 20, the sun fired off a solar eruption that sent huge wave of plasma and charged particles, called a coronal mass ejection (CME), toward Mercury. The next day, the sun unleashed two more CMEs in the same direction, and managers from both the Messenger and Stereo missions were alerted of the potential hazards should the CMEs hit or pass closely to the probes.

But, it appears both spacecraft made it through unscathed.

“The CME did pass by Stereo-A — we can see it in the data,” said C. Alex Young, a solar astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Md. “Other than that, we didn’t see anything out of the ordinary.”

In severe cases, CMEs can scramble a spacecraft’s onboard electronics, but these particular eruptions were not very strong, Young explained. Still, spacecraft manufacturers are mindful of the amount of radiation their hardware will likely be exposed to in space.

“These spacecraft, while they certainly can be affected by spaceweather, they’re generally made to withstand reasonable amounts of radiation,” Young told SPACE.com.

Start the Quiz

This image, captured by NASA's Solar Dynamics Observatory (SDO) on March 10, 2012, shows an active region on the sun, seen as the bright spot to the right. Designated AR 1429, the spot has so far produced three X-class flares and numerous M-class flares.

This image, captured by NASA's Solar Dynamics Observatory (SDO) on March 10, 2012, shows an active region on the sun, seen as the bright spot to the right. Designated AR 1429, the spot has so far produced three X-class flares and numerous M-class flares.

Stereo-A is one of a pair of twin space probes tasked with monitoring solar weather events. The Stereo spacecraft (short for Solar Terrestrial Relations Observatory) were both launched in 2006.

NASA’s Messenger spacecraft has been orbiting Mercury since March 2011. The mission completed its first full map of Mercury’s surface last month.

The sun’s activity ebbs and flows on an 11-year cycle, and solar weather events are expected to increase this year as the current cycle ramps up toward the solar maximum. The current solar weather cycle is known as Solar Cycle 24.

Follow Denise Chow on Twitter @denisechow. Follow us @SpacedotcomFacebook or Google+. Originally published on SPACE.com.

Article source: http://www.space.com/20840-sun-eruptions-nasa-spacecraft-mercury.html

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