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A Bright Comet Is Coming
Washington DC (SPX) Jan 11, 2007 If you watch the morning or evening sky these days and have a clear view of the horizon, you will be able to spot a bright object with a prominent tail. That object is comet C/2006 P1 (Comet McNaught). It was discovered on August 7th, 2006 by the hugely successful comet discoverer Rob McNaught. At time of discovery, the comet was a very faint object, but the predicted perihelion distance (closest distance to the sun) of just 0.17 astronomical units (the average distance between the Earth and sun, about 150 million kilometers) indicated that the object has the potential to become very bright indeed. Nobody really knows just what this comet will look like at its closest point to the sun and that is where SOHO comes in! The LASCO instrument aboard SOHO has the ability to watch comets as they get extremely close to the sun. Fortunately for us, C/2006 P1 is going to pass right through the LASCO C3 field of view in less than a weeks' time! As soon as SOHO's cameras capture the comet, we will post images and further information to the SOHO website. In the meantime, you may enjoy looking at some photographs and checking out the links below for further information. The image to the left shows the expected track of the comet through SOHO's coronagraph LASCO C3. The comet will appear in the field of view of C3 at around 10:00 UT (05:00 EDT) on January 12th (a few hours before perihelion) in the upper-left of the images and travel almost vertically down, exiting C3's field of view in the lower left at roughly 03:00 UT on January 16th. Recent estimates of the comet's maximal brightness have ranged widely from magnitude +2.1 (about as bright as Polaris, the North Star) to a super-bright -8.8 (about 40 times brighter than Venus)! The lower the magnitude number, the brighter the object. The brightest stars in the sky are categorized as zero or first magnitude. Negative magnitudes are reserved for the most brilliant objects: the brightest star is Sirius (-1.4); the full Moon is -12.7; the Sun is -26.7. Current estimates put comet McNaught at magnitude 0 to -1, and it is still brightening. It could be -2 or -3 by the time it reaches LASCO's field of view. This means it will be brighter than comet NEAT or comet 96P/Machholz. In other words, this could be the brightest and most spectacular comet that SOHO has ever seen! Related Links McNaught gallery on Spaceweather.com The Iron and Ice Of Our Solar System
New Evidence Of Extrasolar Asteroid Belt
Los Angeles CA (SPX) Jan 10, 2007Providing the best evidence yet for an asteroid belt beyond the solar system, new measurements pinpoint the location of such a disk of warm dust surrounding the star Zeta Leporis. As the January 6, 2007 issue of Science News reports, this dust lies about the same distance from Zeta Leporis as the solar system's asteroid belt lies from the sun. Margaret M. Moerchen and Charles M. Telesco and their colleagues at the University of Florida in Gainesville report these findings in an upcoming Astrophysical Journal Letters. |
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