Note: The file you are viewing is a single HTML file from who knows where in cyberspace. That means that links and images within the file are not included with the single file and will not likely work. If the original site is still in esistence and can be found, this paricluar file will ultimately be replaced with a link back to its origin. In the meantime, the file is here for its text value only.


S&T's Weekly News Bulletin

August 1, 1995


Comet Hale-Bopp

On the morning of July 23rd, two amateurs discovered a new comet just south of the Sagittarius Teapot near the globular cluster M70. Alan Hale in Cloudcroft, NM, and Thomas Bopp near Stanfield, AZ, were both using 16-inch reflectors. They described the comet as a tailless, 11th-magnitude glow. Thanks to hundreds of positional observations, Brian Marsden of the IAU's Central Bureau for Astronomical Telegrams has calculated that Comet Hale-Bopp is a whopping 7 astronomical units from the Sun -- well beyond Jupiter, and farther away than any comet discovered by amateurs before. The fact that it can be seen at all suggests it may be experiencing an outburst, which might be making it appear 5 to 10 magnitudes brighter than it otherwise would be.

Meanwhile, Warren Offutt, a New Mexico neighbor of Hale, used his 24-inch reflector and a CCD to record a "spiral coma," an appearance typical of Comet Schwassmann-Wachmann 1 after its own outburst. Moreover, Offutt says the new comet has shrunk and dimmed a little in the past week. Sky & Telescope columnist John Bortle notes that when a comet undergoes an outburst, a second flare-up sometimes occurs about 30 days later. Bortle was intrigued by Hale-Bopp's fan-shaped head when he observed it on July 31st.

According to Marsden the comet will reach perihelion in March or April of 1997, just inside the Earth's orbit. It will grace the predawn sky for northern observers that spring, but how bright it will get is still anybody's guess. For now it's magnitude 10 or 11 and crossing Sagittarius. Here are Hale-Bopp's coordinates (equinox 2000) for 0 hours Universal Time:

           R.A.  (2000)  Decl.
           =====================
August  1  18h 38.0m    -31d 55'
August  6  18h 34.7m    -31d 46'
August 11  18h 31.7m    -31d 35'


 

Saturn's New Moons

When Earth passed through the ring plane of Saturn on May 22nd, observers Amanda Bosh and Andrew Rivkin used the Hubble Space Telescope to detect two, and perhaps four, new satellites of Saturn. These objects are too close to Saturn and too faint to be seen near the bright ring system ordinarily. But the rings' edge-on geometry made their discovery possible. Two of the sightings could be of two known moons, Atlas and Prometheus, but the Hubble locations don't correspond to where their orbits predict they should be. The others, which are 17th and 18th magnitude, are clearly new objects. An image from HST's May 22nd run appears on page 11 of Sky & Telescope's July issue.

Meteors this week

The coming week features a pair of lesser meteor showers with radiants in the southern sky. The South Delta Aquarid shower comes to a slow maximum at 5h Universal time on July 29th (the night of July 28th), which is during the dark of the Moon this year. Peaking one day later is the Alpha Capricornid shower, which though generally weak has a high proportion of bright meteors.

Galileo burns! (again)

The Galileo spacecraft, having been freed of its atmospheric probe just two weeks ago, fired its engine for 306 seconds on July 27th. The result was a velocity change of 225 km per hour -- not much compared to its cruising speed but enough to ensure that the spacecraft will not plunge along with the probe into Jupiter's atmosphere next December 7th. On that date the main spacecraft will fire the engine again, this time much longer, to slip into orbit around the giant planet.
Weekly News Bulletin main page.
SKY Online home page.

Copyright © 1995 Sky Publishing Corporation, All Rights Reserved.
This material may not be reproduced in any form without permission.
For more information contact Sky Publishing Corp., P.O. Box 9111, Belmont, MA 02178-9111, USA. Phone: +1-617-864-7360. Fax: +1-617-576-0336 (editorial only), +1-617-864-6117 (all other).

Disclaimer: The file contained in the box above or displayed in a separate window from a link in the box above is NOT owned nor implied to be owned by BeYoND THe iLLuSioN. Most files at BeYoND THe iLLuSioN are originally from public Bulletin Board Systems (BBS) which were popular in the days before the Internet or from gopher, web, and FTP sites from the early days of the Internet which no longer exist today. Essentially, all files were acquired from the public domain in one for or another.

However, there have been occasions when copyright protected material has appeared on BeYoND THe iLLuSIoN without permission of the copyright holder. In these instances, we have and will continue to remove the copyright protected file as soon as it is brought to our attention. This can now be done using our Report Copyright Material form. Fill out the form, and the webmaster will be notified of the situation.

There are also times when files found on BeYoND THe iLLuSioN have a real home somewhere else on the Internet. In these instances, we will gladly replace the file with a link to its true home whenever it is brought to our attention. If you know of the true home of any of these files, you can use our Report Original URL form to bring it yo our attention.