Return-path: X-Andrew-Authenticated-as: 0;andrew.cmu.edu;Network-Mail Received: from po2.andrew.cmu.edu via trymail for +dist+/afs/andrew.cmu.edu/usr1/ota/space/space.dl@andrew.cmu.edu (->+dist+/afs/andrew.cmu.edu/usr1/ota/space/space.dl) (->ota+space.digests) ID ; Wed, 31 Aug 88 22:07:39 -0400 (EDT) Received: from andrew.cmu.edu via qmail ID ; Wed, 31 Aug 88 22:06:34 -0400 (EDT) Received: by andrew.cmu.edu (5.54/3.15) id for +dist+/afs/andrew.cmu.edu/usr1/ota/space/space.dl; Wed, 31 Aug 88 22:04:12 EDT Received: by angband.s1.gov id AA06414; Wed, 31 Aug 88 19:05:41 PDT id AA06414; Wed, 31 Aug 88 19:05:41 PDT Date: Wed, 31 Aug 88 19:05:41 PDT From: Ted Anderson Message-Id: <8809010205.AA06414@angband.s1.gov> To: Space+@andrew.cmu.edu Reply-To: Space+@andrew.cmu.edu Subject: SPACE Digest V8 #344 SPACE Digest Volume 8 : Issue 344 Today's Topics: Re: Space Station power supply Life on Jupiter (was: Re: SETI) Re: SETI: Why don't we hear anything? RE: SETI Condensed CANOPUS - July 1988 Re: SETI: Why don't we hear anything? ---------------------------------------------------------------------- Date: 19 Aug 88 16:55:10 GMT From: Portia!Jessica!paulf@labrea.stanford.edu (Paul Flaherty) Subject: Re: Space Station power supply Not too many moons ago, I was hacking pdp-11 code for a biomedical research lab, which was looking into the question of electrical tissue damage. They had some interesting experiments, and conclusions; for example, that 60 Hz was probably the most lethal frequency possible. "As I recall", ventricular fibriliation is the most common cause of death; this probably does not occur at 20 KHz (although burns probably would). 20 KHz also means smaller (less massive) transformers... -=Paul Flaherty, N9FZX | "There is no distinctly American criminal class ->paulf@shasta.Stanford.EDU | except Congress." -- Mark Twain ------------------------------ Date: 19 Aug 88 18:41:57 GMT From: rochester!dietz@bbn.com (Paul Dietz) Subject: Life on Jupiter (was: Re: SETI) willner@cfa250.harvard.edu (Steve Willner) writes: >> Jupiter cannot be left out. At some altitudes, the atmosphere >> is much the same as Earth's. > >In temperature and pressure yes, but the composition is radically >different. Jupiter's atmosphere is "reducing", consisting mostly of >hydrogen, water, methane, and ammonia. Earth's atmosphere is >"oxidizing", as we all know. > >Being reducing doesn't mean Jupiter's atmosphere cannot contain life; >on the contrary, it may be better for life than Earth's because the >poison gas oxygen is not present. At high pressure and temperature, hydrogen reacts exothermically with organic compounds to form methane, ammonia and water. Vertical circulation in Jupiter's atmosphere carries any given parcel downward to great depth every few days or so. It is unlikely that life could have originated or could survive there. Paul F. Dietz dietz@cs.cornell.edu ------------------------------ Date: 19 Aug 88 18:59:54 GMT From: vsi1!unisv!vanpelt@ames.arc.nasa.gov (Mike Van Pelt) Subject: Re: SETI: Why don't we hear anything? In article <1948@looking.UUCP> brad@looking.UUCP (Brad Templeton) writes: >Well there are quite a few options, each with interesting implications: (several options deleted) >b) There's something inherently wrong with the V.N. machine idea: That's what I think: Self-replicating machines are too difficult or perhaps even not possible. (To point at an animal as a counterexample is to beg the question. Maybe the reductionist worldview is wrong...) Many of the AI people take it as Revealed Truth that there's nothing to intelligence that can't be done with a little hardware and some software. I'm not convinced. The more you look at it, the problem of making a machine that can do even what a cockroach does is not as easy as it may appear at first glance. (Which is one of the brick walls I think the nanotechnology folks are going to run into.) -- Mike Van Pelt Here lies a Technophobe, Unisys, Silicon Valley No whimper, no blast. vanpelt@unisv.UUCP His life's goal accomplished, Zero risk at last. ------------------------------ Date: 19 Aug 88 18:10:00 GMT From: apollo!nelson_p@beaver.cs.washington.edu (Peter Nelson) Subject: RE: SETI >> Presumably it wouldn't be all that difficult for an advanced >> civilization to build probes that would be more than a match for >> any civilization that had only a few years before mastered the use >> of radio, on which the probes would home in. > >If it is possible for an advanced civilization to build and deploy >self-reproducing, interstellar probes, probes could be continuously >resident in each solar system. If the civilization constructing the >probes were irrationally hostile to other life forms, the probes >could be programmed to detect life and sterilize any planets long >before radio could be developed. Obviously this has not happened, so >at least one of the assumptions is wrong (or else we are just >incredibly lucky that all the probes in our solar system have >malfunctioned). Wrong. We're it, or them, I mean. WE are the self-reproducing probes programmed to sterilize all life before the true intelligent life can arise on this planet. And it's working! --Peter Nelson ------------------------------ Date: 19 Aug 88 22:29:58 GMT From: cfa!cfa250!willner@husc6.harvard.edu (Steve Willner P-316 x57123) Subject: Condensed CANOPUS - July 1988 Here is the unabridged CANOPUS for July 1987. There are three articles. All are highly condensed, and the first is frequently rephrased. Material in {braces} is from me and is signed {--SW} when it represents an expression of opinion. CANOPUS is published by the American Institute of Aeronautics and Astronautics. Send correspondence about its contents to the executive editor, William W. L. Taylor (taylor%trwatd.span@star.stanford.edu; e-mail to canopus@cfa.uucp will probably be forwarded). Send correspondence about business matters to Mr. John Newbauer, AIAA, 1633 Broadway, NY, NY 10019. Although AIAA has copyrighted CANOPUS and registered its name, you are encouraged to distribute CANOPUS widely, either electronically or as printout copies. If you do, however, please send a brief message to Taylor estimating how many others receive copies. CANOPUS is partially supported by the National Space Science Data Center. SPACE SCIENCE IN THE 21st CENTURY, N.R.C. Report Issued - can880701.txt - 7/6/88 [Report to NASA from National Research Council on scientific goals in space. Requested by NASA in 1984. The report is a comprehensive wish list rather than a setting of priorities. Setting priorities may not be possible until some current missions are completed.] In his cover letter, National Academy of Sciences Chairman Frank Press, calls attention to two severe problems that must be faced. 1) Challenger accident has deprived us of access to space, and 2) available funding and talent are insufficient. Here are the categories and some of the missions suggested. PLANETARY AND LUNAR EXPLORATION For the terrestrial planets: landers, rovers and sample return missions For the outer planets: atmospheric probes For primitive bodies (comets and asteroids): rendezvous and sample-return missions Search for planets around other stars (Even planets as small as Uranus and Neptune should be detectable.) "A Mars-focused program is recommended in parallel with the general program" and not as a substitute. Venus, Earth and Mars present a great potential payoff in comparative planetology. SOLAR SYSTEM PLASMA PHYSICS An ultraviolet and X-ray telescope to give 1-100 km resolution images of the Sun's surface. (The planned High Resolution Solar Observatory will have 70-km resolution, but the UV capability has been cancelled.) Plasma observations as part of outer planet missions Remote sensing of magnetospheric plasmas in the Earth-moon system Active experimentation {I think this means missions like particle releases in the Earth's ionosphere.--SW} Solar Probe (sometimes called Star Probe), a mission to fly within 1.9 million km of the visible surface of the Sun {This is about 1.4 solar diameters.} An Interstellar probe (also called TAU, for Thousand Astronomical Units) would enter the interstellar medium 10 years after launch. ASTRONOMY AND ASTROPHYSICS o Imaging interferometry, comprising large arrays of telescopes for optical and radio VLBI observations, o Large-area and high-throughput telescopes, including a 20- to 30-m large deployable sub-mm reflector, an 8- to 16-m optical telescope, a large 20 to 20,000 keV X-ray telescope, and a large 0.1-10 meV Compton telescope, and o Astro-Mag, a massive cosmic ray analyzer using a superconducting magnet spectrometer. FUNDAMENTAL PHYSICS AND CHEMISTRY (relativistic gravitation and microgravity sciences) o Laser hetereodyne interferometer to attempt detection of gravitational waves below 10 Hz, o Microwave ranging to a Mercury orbiter to measure the time rate of change in gravitational coupling, o A Precision Optical Interferometer in Space to measure the second order effect of the Sun on electromagnetic radiation. o A hydrogen maser clock aboard Solar probe or Star Probe to measure the gravitational red shift to second order. o A free-flying spacecraft to test the weak principle of equivalence to one part in 1,000 more than a planned Shuttle experiment, and o A large-area X-ray detector (possibly from the astrophysics category) for microseceond timing to allow detection of X- ray pulsars. HUMAN PRESENCE IN SPACE The SSB study found no category of space science depends on manned space flight other than space medicine. Rather than falling into the man-vs-machine argument that has divided the space community for decades, the study team wrote that, "At present, we lack enough information to judge where the balance between manned and unmanned missions should lie." PRECONDITIONS AND INFRASTRUCTURE To train the next generation of scientists, the SSB said that Explorers, Spartans, Observers, and suborbital programs "must be allowed to flourish." Projects that take one to three years are needed to match the training of graduate and post-doctoral students. FRED SCARF, NOTED SPACE SCIENTIST, DIES AT 57 - CAN990702.txt - 7/19/88 Frederick L. Scarf, a chief scientist for research and technology at TRW, died Sunday, in Moscow. Dr. Scarf, 57, was part of an international delegation attending the launch of two Russian probes designed to investigate one of the moons of Mars, Phobos. He was a co-investigator of an instrument aboard each of the spacecraft. RESTORING COMMITMENT TO OUR FUTURE IN SPACE - CAN880703.TXT - 7/26/88 A Joint Statement by American Astronomical Society, American Institute of Aeronautics and Astronautics, and Institute of Electrical and Electronics Engineers {highly condensed}: We believe NASA's program is neither sufficiently understood nor adequately supported. It is our responsibility to call to the nation's attention the great value of NASA's historic contributions to education, science, exploration, and leadership. We urgently recommend restoring national commitment to purposeful civilian space programs and policies. From both the manned and unmanned space programs, we and the world community have received manifold benefits that range from the practical to the intellectually sublime. Observing the earth from space has put within our grasp the ability to understand and stabilize this--the only known--environment of life. We can now study the earth's interior, global atmosphere, oceans, and landmasses as whole entities. In our time, heavenly bodies have moved into the realm of human experience. These discoveries stimulate a deeper understanding of the earth itself. New classes of objects and phenomena have been discovered by past telescopes in space. In the future, space astronomy can open for study new wavelength ranges and new volumes of the universe. NASA's scientific achievements are echoed in space applications such as satellite communications... and remote sensing from space, which has revolutionized weather forecasting and the assessment of our planet's resources. Life sciences research ... The future of these beneficial space activities is at risk. The problem is that budgetary growth is required through the remainder of the century to exploit the technology and infrastructure created by NASA. That is the conclusion of the May 1988 report by the Congressional Budget Office entitled "The NASA Program in the 1990s and Beyond." We urge the leadership of the United States to reverse this nation's current retreat from exploration and development in space by providing adequate resources to NASA. We have serious business in space. Other nations recognize the benefits of civilian space activities, and they are creating their own opportunities. If the United States can be a reliable partner, we might travel with them -- but we cannot stay home. The space frontier is no less significant to our future than our terrestrial boundaries: through each will come the new knowledge, fresh challenges, economic strength, and the critical resources that will spur us on and secure our place in the competitive future. We call for a restored commitment to space. -- Steve Willner Phone 617-495-7123 Bitnet: willner@cfa 60 Garden St. FTS: 830-7123 UUCP: willner@cfa Cambridge, MA 02138 USA Internet: willner@cfa.harvard.edu ------------------------------ Date: 18 Aug 88 14:45:41 GMT From: uplherc!esunix!bpendlet@gr.utah.edu (Bob Pendleton) Subject: Re: SETI: Why don't we hear anything? From article <1123@ndsuvax.UUCP>, by nekinsel@ndsuvax.UUCP (Peter Kinsella): > In article <561@unisv.UUCP>, vanpelt@unisv.UUCP (Mike Van Pelt) writes: > >> Presumably it wouldn't be all that >> difficult for an advanced civilization to build probes that would be >> more than a match for any civilization that had only a few years >> before mastered the use of radio, on which the probes would home in. > > Why would would the get along fine with each other but be afraid of a > a little puny underdeveloped planet. If we assume that the galaxy is as > expansive as most people claim. And if we assume that the Race is > suffiently developed to send probes to wipe out other planets, wouldn't ^^^^^^^^ > they also be advanced enough to harvest resources from uninhabited worlds. > Wouldn't the later also be more economically efficent, especially if the > world be taken over detonates atomic weapons in its self defense. ^^^^^^^^^^ wipe out != taken over. In fact, they might want us to use our own nuclear weapons. It might help them wipe us out. Flame ON! Did you ever hear about phobias? Individual humans can develop irrational fears that can drive them to extreme behavior. Did you ever hear of WWI, WWII, Vietnam, Afganistan, or Iraq, and Iran? Human cultures can also exihbit irrational behavior. And then you ask why members of another species, the result of independant evolution in a different environment would not act like we HOPE human beings might act some day? Humanity is an example of a species with high technology and irrational behavior. If the wrong mass insanity sets in, WE could be the ones launching the sterilizer probes! Flame OFF! Look, my neighbor spent about 3 days with a bubble level and bags of sand making sure that his front lawn was absolutely level. Every month or so he goes out and checks to make sure it is still level. His side and back yards are weed covered dirt. He is considered to be sane. But, his behavior makes no sense to me at all. Beyond a few basics, like maybe reproduction, what can we really claim to know about what an alien intelligence might do? Bob P. -- Bob Pendleton @ Evans & Sutherland UUCP Address: {decvax,ucbvax,allegra}!decwrl!esunix!bpendlet Alternate: utah-cs!esunix!bpendlet I am solely responsible for what I say. ------------------------------ End of SPACE Digest V8 #344 *******************