The solar probe Ulysses has circled the sun for more than 18 years–almost as long as the Greek hero Odysseus, also called Ulysses, was absent from home due to the Trojan War and his prolonged journey home–but the space probe doesn’t have a homecoming in its future. Ulysses will receive its final transmission tomorrow, as researchers say the scientific findings sent home by the failing spacecraft no longer justify the mission’s costs. After shut-off, Ulysses will continue to orbit the Sun, becoming in effect a man-made ‘comet’. “Whenever any of us look up in the years to come, Ulysses will be there, silently orbiting our star, which it studied so successfully during its long and active life” [SPACE.com], says mission manager Richard Marsden.
The craft has already exceeded expectations. In February 2008, mission engineers announced with great solemnity and with heaps of praise for the orbiter that the craft would fall silent within a few months. Its power supply had grown too weak to keep the craft’s fuel lines from freezing. Not so fast: Engineers figured out that they could keep the lines warm by firing the craft’s thrusters in short bursts every couple of hours [The Christian Science Monitor]. Using that clever fix, Ulysses soldiered on for another year.
(more…)
The sun has been surprisingly quiet lately, and until now astronomers couldn’t figure out why. An 11-year cycle governs solar flares and sunspots, and researchers knew that we were at the end of a cycle in a “solar minimum” or quiet period–but that somnolence has continued for an extra year beyond the point at which researchers expected sunspot activity to resume. Comments Australian astronomer Phil Wilkinson: “We have had a drought of sunspots…. This is the longest period the sun has been quiet since the start of the Space Age. Seeing the sun doing nothing is really exciting,” he said, adding it made physicists wonder how little they really understood [Sydney Morning Herald].
Now, new observations announced at a meeting of the American Astronomical Society reveal a possible explanation: “sluggish” solar jet streams 4,350 miles below the surface of the sun. Every 11 years, the sun simultaneously generates twin streams of plasma at each of its poles. Unlike the jet streams on Earth, the solar versions are magnetized and travel only toward the equator. This migration takes place very slowly–at about 10 kilometers per hour. For reasons still not understood, when the streams reach 22 degrees of latitude, north and south, they touch off a new solar cycle, and the sunspots reappear [ScienceNOW Daily News].
(more…)
A pair of solar observers known as the STEREO spacecraft have taken the first 3-D pictures of the sun’s powerful storms, during which billions of tons of charged particles erupt from the sun’s surface. The two spacecraft have taken up two positions about 100 million miles apart: Not unlike human eyes, the satellites’ two points of view allow for combination images that render scenes in three dimensions [National Geographic News].
Solar storms can have serious repercussions here on Earth. They can disrupt GPS signals and power grids, damage satellites, and bombard astronauts with solar radiation, experts said [National Geographic News]. But with the STEREO system, researchers say they can predict when a fierce storm will hit Earth 24 hours in advance (an improvement over previous 12-hour predictions). Says researcher Chris Davies: “That’s ample time to power down a satellite until the worst of the storm has passed; and if you’re an astronaut on the space station, you would have had plenty of time to get into an area that has much better shielding” [BBC News]. While STEREO is a temporary scientific research mission, researchers say it provides an example of how a “space weather” early-warning system would work.
(more…)
As the year 2008 draws to a close, the world’s timekeepers are giving us a little extra time to wrap up loose ends: They’re giving us one extra second, to be precise. The “leap second” must be added to keep atomic clocks ticking along in time to the planet’s rotation. So at precisely 23:59:60 at Greenwich, England, on New Year’s Eve, there will be a one-second void before the onset of midnight and the start of the New Year…. By the time the transition from 2008 to 2009 arrives in North America the Leap Second will have already been inserted into the world’s timescale [SPACE.com].
The adjustment is necessary because we have two different ways of measuring time. Traditionally, humankind has reckoned time by the spin of the Earth and its orbit around the sun. Under this astronomical arrangement, a second is one-86,400th of our planet’s daily rotation. But because of tidal friction and other natural phenomena, that rotation is slowing down by about two-thousandths of a second a day. Since the 1950s, however, atomic clocks — which are based on the unwavering motions of cesium atoms — have made it possible to measure time far more accurately, to within a billionth of a second a day [The New York Times]. To keep the two measurement systems in alignment, the atomic clocks have to add an extra second about every 500 days.
(more…)
Researchers have discovered the our planet’s atmosphere regularly expands and contracts in a short cycle of about nine days, and say that this “breathing” is caused by powerful gusts of solar wind. While researchers already knew that ultraviolet light from the sun can heat and swell the atmosphere, the discovery of short, cyclical fluctuations “was a surprising finding” that wasn’t correlated with any variation in solar UV flux [Science News], says atmospheric scientist Jeffrey Thayer.
The breathing cycle seems to reach its peak when solar features called coronal holes are facing Earth. These dark spots in the sun’s corona—a sort of solar atmosphere—are areas where the sun’s magnetic field has been blown open by pressurized solar wind, sending the “winds” toward Earth at high speed. As the fast winds streaming from coronal holes approach Earth, they cause gases in our upper atmosphere to heat up and expand, then cool down and contract, changing the upper atmosphere’s density [National Geographic News].
(more…)
A starlit sky may look serene, but those stars are actually quivering and quaking; now, researchers have recorded the stellar vibrations of distant stars for the first time. The pulsations reflect changes in temperature caused when roiling heat makes the outer surface of the star vibrate. Portions of the surface expand and cool, while others contract and get warmer [New Scientist].
The initial discovery of oscillations in our Sun in the late 1970’s led to the creation of “solar seismology,” which has since been used to measure the movement and transport of heat around the Sun. Solar seismology led to rapid progress in understanding the Sun’s internal structure, but eventually researchers hit a wall [COSMOS]. For accurate measurements, researchers need a long stretch of uninterrupted observations, which is impossible from ground-based telescopes.
(more…)
The solar wind, a steady stream of charged subatomic particles that stream out from the sun at a speed of one million miles per hour, has dwindled to its weakest state since recording began, researchers say. While researchers already knew that solar winds fluctuate in 11-year cycles, the current doldrums trump the declines seen over the past 50 years. “We know that the sun has been this cool before, this inactive before,” said [physicist] Nancy Crooker…. “But that was prior to the Space Age, so we didn’t have actual physical measurements until now” [SPACE.com].
The data was collected by the first solar explorer, the Ulysses probe, which was launched in 1990 as a joint venture between NASA and the European Space Agency. The 17-year-old space probe, which circles the sun from a distance of about 337 million miles, has been studying the environment above and below the poles of the sun. It is just months away from shutting down because of freezing fuel [AP].
(more…)
