Flipside of the SunSpaceScience.com; Feb. 15, 2001; NASA Science News: "The Sun Does a Flip"
Spectrographs at the National Solar Observatory on Kitt Peak have detected a sudden flip in the orientation of the Sun's magnetic field. Just a few months ago our star's northern hemisphere was home to its north magnetic pole. Now it hosts the south pole! Is this a sign of impending doom? No, but it's a sure sign that solar maximum has arrived. "This always happens around the time of solar maximum," says solar physicist David Hathaway. "The magnetic poles exchange places at the peak of the sunspot cycle. In fact, it's a good indication that Solar Max is really here." Like clockwork the magnetic pole flip happens at the peak of every 11-year sunspot cycle; the north magnetic pole is expected to revert back to the northern hemisphere in 2012. These field changes are felt throughout the solar system because the magnetic field of the Sun forms a bubble called the heliosphere that extends beyond the orbit of Pluto. This year solar astronomers will have the best seat in the solar system to study the magnetic flip -- courtesy of the Ulysses spacecraft. A joint venture of the European Space Agency and NASA, Ulysses flies 2.2 AU over the Sun's poles every six years. In 1994 and 1996 the spacecraft made important discoveries as it swung by the solar poles during the sunspot minimum. Having just swung by the south pole of the Sun, the craft will observe the north polar region this fall. With those observations completed the craft will have gathered data over the course of a full solar cycle. |
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Donut in the ForestNASA-GSFC; Feb. 22, 2001; Press Release: "Dusty Space Donut Caught with Surprise Companion"
The old saying about not being able to see the forest because of the trees holds true in astronomy. If you could selectively eliminate most of the trees you'd be able to detect objects hidden in the forest. To this end astronomers have attached an interferometer aperture mask on the 10-m Keck telescope's secondary mirror that blocks 90% of the light collected. Interference patterns made through the mask are recorded by the Near Infrared Camera and computer processed to construct an image with four times greater resolution, for small fields of view, than the Hubble Space Telescope. When this setup was aimed at a massive (5x size of our Sun) young (1-million years old) star called LkHa101 (522 light-years away in Perseus) astronomers saw details in the cloud of material surrounding the star and a companion star orbiting 2.6 billion miles away. The circular cloud appears about 10 AU in diameter in the computer images, but cooler dust that does not glow in the spectral range of the camera makes the physical cloud larger. At the center of the cloud the heat from LkHa101 burns off the in-falling material and creates a "donut hole" of radius 316-million miles around the star.
Prior to the use of the interferometer aperture mask the companion star and central hole were undetectable. "We've seen the donut hole for the first time, and it's a lot bigger than people thought," said NASA Goddard's Dr. William Danchi. Dr. John Monnier of the Harvard-Smithsonian Center for Astrophysics adds: "These images allow us to look back in time to understand better the origins of our Sun and Solar system." The donut of material around the star would be expected to form planets -- though LkHa101's expected life-span is only 100-million years. Currently the star burns energy at a rate that would make it 40,000 brighter than our Sun at the same distance. Dr. Peter Tuthill of Sydney University in Australia makes it clear that this is only the first step in clearing the forests: "The interferometer technology demonstrated by our aperture mask lets us detect extraordinarily fine detail, and is a first step in projects that will combine light from an array of telescopes to image planets around distant stars." Dr. Tuthill is the primary author of a paper published in the February 22 issue of Nature that describes the findings concerning LkHa101. Drs. Danchi and Monnier are co-authors of the study. Image Credits: National Science Foundation, NASA and Harvard-Smithsonian Center for Astrophysics |
Life Recipe Ingredients Found in FranceSpaceDaily.com; Feb. 27, 2001; TerraDaily: "Meteorite Analysis Suggests Comets Delivered Life's Key Ingredients" France, with its passion for combining ingredients in pursuit of the perfect recipe, is also the home of a cometary meteorite containing the amino acid ingredients for the recipe of life on Earth. Though the 1864 Orgueil meteorite, named after the town near the landing site, had previously been studied, Scripps Institute of Oceanography (San Diego) scientists re-examined it using state-of-the-art instruments to search for amino acids -- fundamental protein components required for life.
"We found that the amino acids in Orgueil are abiotic. They were formed without the help of biology, only chemical reactions." -- Oliver Botta of the Scripps Institute
A fresh piece of the interior of the meteorite contained a simple mixture of amino acids. The carbon isotope ratio in the sample indicated that the chemicals were not the result of contamination on the ground. "We found that the amino acids in Orgueil are abiotic. They were formed without the help of biology, only chemical reactions," said Oliver Botta of the Scripps Institute. "We think these amino acids were synthesized in space."
Scientists had previously believed that a large variety of amino acids were required to form life, but recent research indicates only a few different types of these chemicals are required for life to arise. The amino acids in the meteorite may have been of the type that helped generate life on Earth. So the question remained: from what type of body did the meteorite originate from? The Orgueil contents appear to have been synthesized from components that included hydrogen cyanide: a chemical that was recently observed in the comets Hale-Bopp and Hyakutake. And unlike asteroid derived meteorites that were studied and found to contain upward of 70 amino acids, the Orgueil appears to be comprised of only two. A 1938 Tanzania meteorite named Ivuna was studied and found to have similar properties to Orgueil. "This suggested to us that what we may be seeing in Orgueil and Ivuna are the products of reactions that once took place in the nucleus of a comet," said Scripp Institute's Jeffrey Bada. "If it’s true, this would be the first time that a meteorite from the nucleus of a comet has been identified," added Scripps Daniel Glavin. "There is really a lot we don’t understand about the chemistry of a comet nucleus and this would be our first insight."The Orgueil meteorite researchers believe that comet derived meteorites brought the ingredients of life to Earth. The results of the study were published in the Feb. 27 issue of the Proceedings of the National Academy of Sciences. |
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First Flamer of 2001European Space Agency; Feb. 23, 2001; Press Release: "SOHO Analyses a Kamikaze Comet"
While not unusual for comet hunters in far-flung parts of the globe to discover the same comet, it is would seem unusual to hear that they used the same observation instrument. But not so unusual when the instrument is the ubiquitous Internet. Comet C/2001 C2 (SOHO) has been credited to Sebastian Hoenig of Germany and Xing Ming Zhou of China who both discovered if on Feb. 6 by studying images from the SOHO spacecraft that are posted daily for comet hunters to peruse. Comet C/2001 C2 is a "sungrazer" believed to be a fragment of a large body that broke up long ago. But don't expect the comet to make an Earth-visible appearance anytime soon: the smallish comet flew close enough to the Sun to be evaporated a day after discovery on Feb. 7. The SOHO ultraviolet coronagraph instrument imaged ultraviolet light from hydrogen atoms that billowed from the comet as the Sun's heat decomposed the water ice in the nucleus. It was estimated that 100-kg of water evaporated every second from the tiny 10-20 meter comet nucleus. It was also imaged by the visible-light coronagraph on SOHO.Images of the comet are not just of passing interest. The images shown here were taken an hour apart and yield valuable information about the comet and solar wind. The ultraviolet inset images show the comet at 2.7 and 1.6-million km from the Sun's surface. It is superimposed on a visible light coronagraph image of the Sun. The white ring on the coronagraph mask indicates the disk of the visible Sun. The blowup shows a gas tail one-half million km long. At that distance the comet was moving though a tenuous solar wind. The image closer to the Sun is interpreted as showing a much denser solar wind. This latest comet imaged by SOHO was just one of nearly 300 comets discovered by the spacecraft since 1996. |
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