by Dr. Whitney Shane, MIRAs Charles Hitchcock Adams Fellow |
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Fixed Stars Fortunately not all strong radio sources are so faint optically. Most of them are either old supernovae or the centers of galaxies. A rewarding example of the first is the Crab Nebula (Messier 1), which radio astronomers call Taurus A. It is visible virtually all night during the fall months. The second strongest radio source is Cygnus A, which is an example of a galaxy. It is in the evening sky during the fall, but dont bother to look for it as it is also extremely faint. When first identified in 1954 it was thought to be a pair of colliding galaxies, but it is probably more accurately described as a large galaxy capturing a small satellite. The large galaxy must have a black hole in its center, and the tidal disturbance of the capture is allowing material to fall into this gravitational trap, producing the observed energy. Because of its great distance, this turns out to be a remarkably powerful radio source. The best nearby example of such a galaxy is Centaurus A, which is quite bright, but located, unfortunately for us, in the southern sky. Collisions do not seem to be necessary to create strong radio sources. Virgo A (Messier 87), which will become visible in the morning sky toward the end of fall, looks much like an ordinary elliptical galaxy, although a jet extending out from the center is visible on photographs. Actually, it is a huge radio source, and it appears that the nucleus is sending out powerful streams of very energetic charged particles in opposite directions. These interact with a magnetic field to produce the radio energy. Even the nucleus of our own Galaxy is a strong radio source, part of the complex source Sagittarius A. There is probably also a black hole here into which a small amount of matter is falling. This seems to be the rule for large galaxies. Unfortunately Sagittarius A is hidden from our optical view by very heavy obscuration. Planets Venus will be very prominent and high in the morning sky through the whole quarter. It will reach maximum elongation at the end of October, but will still be well above the horizon at dawn at the end of the year. Mars will not be favorably located for observation, remaining fairly low in the south-western sky during the whole quarter. A lunar occultation on December 12 will unfortunately not be visible from the western U.S. Jupiter, on the other hand, is well placed for observation, passing opposition on October 23. A day later it will be found 4 degrees north of the full moon. It will continue moving west until it reaches its stationary point in the second half of December. Saturn is currently following Jupiter across the sky, and a few degrees to the north. It will pass opposition on November 6 and will thus be well placed for observation during the whole quarter. The current series of occultations of Uranus and Neptune continue, and one of these, the occultation of Uranus on October 19, will be visible from our region. Meteor Showers Eclipses |
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Go back to Fall 1999 Newsletter index | MIRA home mira@mira.org © 1999 MIRA Last updated 2/8/01 by et |
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