Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.3 4.3bsd-beta 6/6/85; site ucbvax.ARPA Path: utzoo!watmath!clyde!burl!ulysses!ucbvax!cit-vax.arpa!jon From: jon@CIT-VAX.ARPA (Jonathan P. Leech) Newsgroups: net.space Subject: Re: Voyager at Uranus Message-ID: <8510181908.AA22430@cit-vax.ARPA> Date: Fri, 18-Oct-85 15:08:17 EDT Article-I.D.: cit-vax.8510181908.AA22430 Posted: Fri Oct 18 15:08:17 1985 Date-Received: Tue, 22-Oct-85 04:58:59 EDT Sender: usenet@ucbvax.ARPA Organization: The ARPA Internet Lines: 52 Actually, having a Caltech ID would do you little good. During Saturn encounter, I found JPL was relatively tightly sealed (except to the press). Even if you could get in, the most interesting areas (Mission Operations and the press conferences in Von Karman Auditorium) are much more difficult, being filled with press types. However, during those encounters there were monitors placed all around Tech receiving real-time feed from JPL as the pictures came in. I suspect they'll do it again. There's no problem with access to Tech (only in wanting to stay...) Quoting from the document `Voyager Bulletin / Mission Status Report # 68, April 10, 1985': " ... Voyager 2 will make its closest approach to Uranus on January 24, 1986, passing within 110,000 kilometers (68,000 miles) of the planet's center." " Extended observations of Uranus will begin on November 4, 1985 and continue through Februrary 25, 1986. Future issues of the Voyager Bulletin will focus on preparations for the encounter, including the health of the spacecraft, science objectives for the encounter, and capabilities for sending and receiving data over large distances." " Uranus, its rings, and satellite orbits present a bull's-eye target to Voyager 2; the planet is tilted on its rotational axis and the illuminated pole presently points almost directly to the sun. This unique orientation means that significant events of the Uranus encounter, such as satellite encounters and ring plane crossing, will be compressed into about 5-1/2 hours, as compared to 35 hours for the approach to Jupiter's Galilean satellites and 13 days for the satellites out to Phoebe's orbit at Saturn." Current issues of this publication can probably be obtained by writing: Public Information Office F. E. Bristow, Manager Mail Code 180-200 Jet Propulsion Laboratory Pasadena, Ca. 91109 (818)-354-4321 Note that this address came from the Institute directory so I make no guarantees of its reliability. -- Jon Leech (jon@cit-vax.arpa) __@/