Return-path: X-Andrew-Authenticated-as: 7997;andrew.cmu.edu;Ted Anderson Received: from beak.andrew.cmu.edu via trymail for +dist+/afs/andrew.cmu.edu/usr11/tm2b/space/space.dl@andrew.cmu.edu (->+dist+/afs/andrew.cmu.edu/usr11/tm2b/space/space.dl) (->ota+space.digests) ID ; Tue, 3 Jul 1990 02:24:31 -0400 (EDT) Message-ID: Precedence: junk Reply-To: space+@Andrew.CMU.EDU From: space-request+@Andrew.CMU.EDU To: space+@Andrew.CMU.EDU Date: Tue, 3 Jul 1990 02:23:36 -0400 (EDT) Subject: SPACE Digest V12 #7 SPACE Digest Volume 12 : Issue 7 Today's Topics: Re: Reflections on (Edwin P.) Hubble and NASA Re: RE Hubble Space Telescope Update - 06/28/90 Unexplained Circles Administrivia: Submissions to the SPACE Digest/sci.space should be mailed to space+@andrew.cmu.edu. Other mail, esp. [un]subscription notices, should be sent to space-request+@andrew.cmu.edu, or, if urgent, to tm2b+@andrew.cmu.edu ---------------------------------------------------------------------- Date: 2 Jul 90 19:26:08 GMT From: usc!jarthur!bridge2!3comvax!michaelm@ucsd.edu (Michael McNeil) Subject: Re: Reflections on (Edwin P.) Hubble and NASA ron@mlfarm.uucp (Ronald Florence) writes: >fax0112@uoft02.utoledo.edu writes: >>Lets draw a lesson from Hubble himself. He first studied law and >>passed the bar. He then enlisted and became an officer. Later >>he turned Yerkes, 'a moribund institution', into a major research >>center and made many famous discoveries. Pretty good for such a >>humble start in the wrong direction. > >Hubble's autobiography shouldn't be trusted any more >than his British accent, which was pure affectation. Yerkes was >hardly a "moribund" institution before Hubble's arrival. Under Hales >it was probably the premier institution for astronomical research in >the United States. Hubble dismissed the work of Shapley and his other >predecessors at Mount Wilson as "of no significance" which is >remarkably like the NASA press releases which described the Hubble >Space Telescope as the most important event in astronomy since Galileo. Edwin Hubble made two outstanding discoveries in his life -- he discovered that the Milky Way isn't the only galaxy in the universe, and he discovered that the universe as a whole is expanding. (For a while after the former discovery, galaxies like the Milky Way were termed "island universes," a phrase I always thought quite romantic.) Most people would be satisfied with one Columbus- or Galileo-caliber discovery. Personally, I'm willing to forgive a little "affectation" and even some personal grandstanding, in return for his discoveries. -- Michael McNeil michaelm@vax.DSD.3Com.COM (3comvax.UUCP) 3Com Corporation ucbvax!hplabs!oliveb!3comvax!michaelm Santa Clara, California work telephone: (408) 492-1790 x 5-208 Extremely little is known of the nature of nebulae; and no classification has yet been suggested.... The agreement [between the velocity of escape from a spiral nebula and that of our galaxy] is such as to lend some color to the hypothesis that the spirals are stellar systems at distances to be measured often in millions of light years. Edwin P. Hubble, 1920, "Photographic investigations of faint nebulae" (Ph.D. thesis), publication delayed 3 years by World War I Critical tests made with the 100-inch reflector, the highest resolving power available, show no difference between the photographic images of the so-called condensations in Messier 33 and the images of ordinary galactic stars.... The period-luminosity relation is conspiculus among the thirty-five Cepheids and indicates a distance about 8.1 times that of the Small Magellanic Cloud. Using Shapley's value for the latter, the distance of the spiral is about 263,000 parsecs. Edwin P. Hubble, 1926a, "A spiral nebula as a stellar system," *Astrophys. J. 63*, 236-274 The present investigation [using Cepheid variables for the first time as an indicator of distances beyond the Magellanic clouds] identifies NGC 6822 as an isolated system of stars and nebulae of the same type as the Magellanic clouds, although somewhat smaller and much more distant. A consistent structure is thus reared on the foundation of the Cepheid criterion, in which the dimensions, luminosities, and densities, both of the system [NGC 6822] as a whole and its separate members, are of orders of magnitude which are thoroughly familiar. The distance is the only quantity of a new order. The principle of the uniformity of nature thus seems to rule undisturbed in this remote region of space. Edwin P. Hubble, "NGC 6822, a remote stellar system," *Astrophys. J. 62*, 409-433 The data ... indicate a linear correlation between distances and velocities [for extragalactic nebulae]. Two solutions have been made, one using the 24 nebulae individually, the other combining them into 9 groups according the proximity in direction and distance. The results are ... 24 objects: K = 465 +- 50 km/sec per 10**6 parsecs; 9 groups: K = 513 +- 60 km/sec per 10**6 parsecs.... The outstanding feature, however, is the possibility that the velocity-distance relation may represent the de Sitter effect, and hence that numerical data may be introduced into discussions of the general curvature of space. Edwin P. Hubble, 1929, "A relation between distance and radial velocity among extragalactic nebulae," *Proc. Nat. Acad. Sci. U.S. 15*, 169-173 Many ways of producing such effects [redshifts in extragalactic nebulae] are known, but of them all, only one will produce large redshifts without introducing other effects which should be conspicuous but actually are not found. This one known permissible explanation interprets redshifts as due to actual motion away from the observer. Edwin P. Hubble, 1934a, *Red-shifts in the spectra of nebulae* (Halley Lecture) We now have a hasty sketch of some of the general features of the observable region as a unit. The next step will be to follow the reconnaissance with a survey -- to repeat carefully the explorations with an eye to accuracy and completeness. The program, with its emphasis on methods, will be a tedious series of successive approximations. Edwin P. Hubble, 1934b, "The distribution of extra-galactic nebulae," *Astrophys. J. 79*, 8-76 ------------------------------ Date: 2 Jul 90 20:41:57 GMT From: mojo!SYSMGR%KING.ENG.UMD.EDU@mimsy.umd.edu (Doug Mohney) Subject: Re: RE Hubble Space Telescope Update - 06/28/90 In article <5188@plains.UUCP>, overby@plains.UUCP (Glen Overby) writes: >In article <00938EED.5338EF60@KING.ENG.UMD.EDU> sysmgr@KING.ENG.UMD.EDU (Doug Mohney) writes: >>If Hubble was run on a shoe-string budget, instead of big bucks...well... >>I can't help but think the thing would have A) Gotten off the ground about >>4 years sooner and B) Given us more than we bargained for. > >HST was trundled across the country for launch two previous times, but was >delayed both times by shuttle problems. Complaint "A" above isn't the HST >project's fault (except that they should have chosen a different booster). If Hubble hadn't been designed as an "oversized payload" (ie: Shuttle bay) they could have popped it onto a Titan just as easily. Instead, it is an exceptionally complex piece of machinery in LEO.... What kind of science do you think we could have gotten out of two "Half-Hubbles" which could have been launched either by Titan or Shuttle? ------------------------------ Date: 29 Jun 90 18:36:02 GMT From: sdd.hp.com!elroy.jpl.nasa.gov!peregrine!ccicpg!felix!dhw68k!ofa123!Mark.Perew@ucsd.edu (Mark Perew) Subject: Unexplained Circles I thought that I had read somewhere that this phenomena of near perfect circles was caused by the freezing of subsurface water. A somewhat complex mechanism of expansion and contraction was (over time) causing the soil to ripple when the water found at a depth of a few centimeters froze. I wish I could provide a reference, but I can't recall where I saw this. --- Opus-CBCS 1.13 * Origin: Universal Electronics, Inc. (1:103/302.0) -- uucp: Mark Perew Internet: Mark.Perew@ofa123.fidonet.org BBS: 714 544-0934 2400/1200/300 ------------------------------ End of SPACE Digest V12 #7 *******************