Return-path: X-Andrew-Authenticated-as: 0;andrew.cmu.edu;Network-Mail Received: from po3.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 ; Mon, 8 Aug 88 04:07:23 -0400 (EDT) Received: from andrew.cmu.edu via qmail ID ; Mon, 8 Aug 88 04:05:58 -0400 (EDT) Received: by andrew.cmu.edu (5.54/3.15) id for +dist+/afs/andrew.cmu.edu/usr1/ota/space/space.dl; Mon, 8 Aug 88 04:04:43 EDT Received: by angband.s1.gov id AA01923; Mon, 8 Aug 88 01:04:01 PDT id AA01923; Mon, 8 Aug 88 01:04:01 PDT Date: Mon, 8 Aug 88 01:04:01 PDT From: Ted Anderson Message-Id: <8808080804.AA01923@angband.s1.gov> To: Space@angband.s1.gov Reply-To: Space@angband.s1.gov Subject: SPACE Digest V8 #318 SPACE Digest Volume 8 : Issue 318 Today's Topics: Re: Are these postings useful? Contractor selected for solid-fueled rocket motor bondline study (Forwarded) Re: Time skew -- does it hurt SETI? Re: Are these postings useful? Re: query about 'escape velocity' Re: query about 'escape velocity' Re: Solar Sails Re: Libertarian space policy Re: E stamp Re: Are these postings useful? orbital mechanics ---------------------------------------------------------------------- Date: 30 Jul 88 17:41:29 GMT From: pyrnj!dasys1!tneff@rutgers.edu (Tom Neff) Subject: Re: Are these postings useful? In article <19880728032142.7.MAEDA@PELE.ACA.MCC.COM> maeda@MCC.COM (Christopher Maeda) writes: >You are sucking up a lot of bandwidth. Perhaps you could make them >available by FTP and just send a message about how to get it. Disagree! It's not a lot of bandwidth -- check the arbitron and uunet charts. And the s/n ratio is BEAUTIFUL -- all hard info. I love it. The only thing I could sincerely do without is "catching up" on 2+ month old AvWeek issues. -- Tom Neff UUCP: ...!cmcl2!phri!dasys1!tneff "None of your toys CIS: 76556,2536 MCI: TNEFF will function..." GEnie: TOMNEFF BIX: t.neff (no kidding) ------------------------------ Date: 31 Jul 88 02:21:58 GMT From: yee@ames.arc.nasa.gov (Peter E. Yee) Subject: Contractor selected for solid-fueled rocket motor bondline study (Forwarded) James Cast Headquarters, Washington, D.C. July 29, 1988 Bob Lessels Marshall Space Flight Center, Huntsville, Ala. RELEASE: 88-107 CONTRACTOR SELECTED FOR SOLID-FUELED ROCKET MOTOR BONDLINE STUDY NASA's Marshall Space Flight Center, Huntsville, Ala., has selected Science Applications International Corp., San Diego, Calif., for final negotiations leading to the award of a contract to perform a study aimed at developing an engineering technology base to improve the bondlines of solid-fueled rocket motors. The value of the contract, including options, is expected to be approximately $21 million and will run for 2 years, with three 1-year options to extend. Bondline integrity is critical to the successful operation of solid-fueled rocket motors. Bondlines are the regions where the solid fuel is bonded to the motor's liner or insulation, which, in turn, is bonded to the motor case walls. These bonds prevent the hot combustion gases inside the motor from reaching the motor case wall, where the gases could burn through the wall and cause failure of the motor. The work is part of the agency's Solid Propulsion Integrity Program. The objective of the program is to increase the success rate of solid-fueled rocket motors by improving basic engineering capability in such areas as material characteristics, design analysis, fabrication and assembly processes and production evaluation and verification. The program originated from joint NASA-Department of Defense-industry studies which identified critical shortfalls in the U.S. engineering technology for solid-fueled rocket motors. In June, Hercules Aerospace Co., Magna, Utah, was selected as the contractor for the Solid Propulsion Integrity Program nozzle work packages. The two work packages represent NASA's contribution to the tripartite effort. NASA engineers managing the program expect to improve confidence in solid rocket motor launch systems by establishing urgently needed engineering tools, techniques and data bases specifically applicable to the current civil and military family of solid-fueled rocket motors. ------------------------------ Date: 31 Jul 88 03:00:30 GMT From: mike@arizona.edu (Mike Coffin) Subject: Re: Time skew -- does it hurt SETI? A point that hasn't been made: even if electromagnetic radiation is the last word in communication, why spray most of the power into empty space? I would think that advanced civilizations would probably use modulated lasers or some other point-to-point method of communicating. Not only would this save power, but it doesn't pollute the electromagnetic spectrum. That would make detection on earth a pretty low probability event --- we would have to me almost exactly in the right place at the right time to detect anything at all, and if we *did* it would probably be a brief, unrepeated message. -- Mike Coffin mike@arizona.edu Univ. of Ariz. Dept. of Comp. Sci. {allegra,cmcl2,ihnp4}!arizona!mike Tucson, AZ 85721 (602)621-4252 ------------------------------ Date: 31 Jul 88 06:40:31 GMT From: jplpub1!jbrown@elroy.jpl.nasa.gov (Jordan Brown) Subject: Re: Are these postings useful? In article <5813@dasys1.UUCP> tneff@dasys1.UUCP (Tom Neff) writes: >The only thing I could sincerely do without is "catching up" on 2+ >month old AvWeek issues. Take heart, Henry - I think your AvWeek digests are one of the greatest things since the airplane... they're one of the few ways I keep in touch with what's happening in aviation & space technology & politics. ------------------------------ Date: 31 Jul 88 15:29:41 GMT From: cfa!cfa250!mcdowell@husc6.harvard.edu (Jonathan McDowell) Subject: Re: query about 'escape velocity' From article <3451@polya.Stanford.EDU>, by crew@polya.Stanford.EDU (Roger Crew): In article <1020@cfa237.cfa250.harvard.edu} mcdowell@cfa250.harvard.edu .. > velocity (in a direction away from the Earth!) Actually, it doesn't matter what direction you're pointed in, so long as there's nothing directly in your path that is going to slow you down (like an atmosphere or a swarm of rocks). . yes, I meant in any direction that does not intersect the Earth's surface. In arguments between the Earth and a spacecraft, the Earth tends to win, it has more momentum you know :-). Sorry, I should ave been more precise in my choice of phrase. Jonathan ------------------------------ Date: 31 Jul 88 15:18:01 GMT From: cfa!cfa250!mcdowell@husc6.harvard.edu (Jonathan McDowell) Subject: Re: query about 'escape velocity' From article <1068@cfa.cfa.harvard.EDU>, by wyatt@cfa.harvard.EDU (Bill Wyatt): > The above is correct except I think you have to emphasize that the > escape velocity varies with the square root of the distance from the > Earth's (or other gravity well's) center. Thus, if you have sufficient > thrust to move away from the Earth at 55 mph, I calculate that > somewhere in the vicinity of Jupiter's orbit you'll be at the escape > velocity of Earth. After that point, even stopping the thrust will not > let you fall back to Earth (assuming no perturbations, etc.), although > you'd presumeably orbit or fall into the Sun! Thanks for the clarification, Bill. You're quite right, at 9 AU ( about the orbit of Saturn) 55 mph is indeed escape velocity from Earth. But what happens if the thrust stops at that point? You're not travelling at 55 mph relative to the Sun.. Either: the problem implies one travels in a straight line with constant velocity relative to an inertial frame instantaneously fixed in the center of the Earth at the moment of takeoff (remember that at 55 mph the Earth has made 1700 revolutions of the Sun by the time you get to the point in question!) In this case one is no longer travelling at 55 mph relative to the Earth, but relative to where the Earth was. Or: You keep a constant 55 mph velocity relative to the center of the Earth at all times. This is very tricky as the Earth is accelerating around the Sun. In either case, you do not have the local orbital velocity relative to the Sun, you have the Earth's Keplerian orbital velocity. Since the escape velocity at a given point is root 2 times the orbital velocity, and both decrease with the root of the distance from the central mass, you just have to double your distance from the central mass while keeping the same velocity to achieve escape; so you have escape velocity relative to the Sun by the time you get to 2 AU. You're headed out into the Great Unknown. Of course, the point you make is that we shouldn't be trying to keep our velocity low anyway, since that's not what costs..it's only relative. The trick is to keep your energy requirements low, since that's what you pay for. Jonathan McDowell. ------------------------------ Date: Sun, 31 Jul 88 14:09:31 CDT From: sedspace@doc.cc.utexas.edu (Steve Abrams) Posted-Date: Sun, 31 Jul 88 14:09:31 CDT Subject: Re: Solar Sails In V8 #306, Eric "TheBoo" Bazan (eric@shorty.cs.wisc.edu) writes: >My question is this: just how does the sun 'push' against the sail? Is it the >solar wind of charged particles (protons and electrons), or the actual >photonic flux, or both? Since the wave and particle paradigms for electromagnetic radiation are equivalent, you can certainly think of "material" photons bouncing off a sail film and, thereby, transferring momentum to the sail. However, I assume you want to view it from the wave perspective. With the propagation of electromagnetic radiation (light energy) there is a flow of energy. However, you've probably also heard that mass and energy are equivalent (E=mc^2). Therefore, you have a mass-equivalent entity traveling with a velocity...the product of mass and velocity is linear momentum. More mathematically, the "momentum density", g, is equal to a constant (the product of the permeability and permittivity of free space) times the "Poynting vector" (since we're in a vacuum). The Poynting vector is simply a vector defining the energy flow of the light (EM radiation). The value for this Poynting vector is just the solar constant you mention, 1.353 kW/m^2. The physical process is (loosely) that the photon is "absorbed" by an atom in the sail film. The energy is used to raise an electron's energy level. That electron then spontaneously decays thereby emitting another photon *with the same energy* as the original photon but in the opposite direction. In each process of absorption and re-emission, momentum is transferred in the same direction to the sail film. The energy of the photon doesn't change (a scalar quantity) and the magnitude of the velocity of the photon doesn't change *BUT* the direction changes. By Newton's Third Law (Action/Reaction), momentum is transferred to the sail from the photon. I realize that this won't satisfy purists, but it should be sufficient for someone with a poor physics background. Incidentally, the book Eric is probably referring to is _Starsailing_ by Louis Friedman. It is an excellent introductory, survey-type book on the subject. Does anyone know if a more technical, mathematically-oriented sequel is in the works? Ad Astra, Steve Abrams \ / --"You have twenty seconds to put down your slide rule...19...18...17..."-- / \ -- RoboDweeb 2721 Hemphill Park, Apt. C ARPANET: sedspace@doc.cc.utexas.edu Austin, TX 78705 CompuServe: [70376,1025] (512)480-0895 OR c/o Students for the Exploration and Development of Space P.O. Box 7338, 358 Texas Union, University of Texas at Austin Austin, TX 78713-7883 (512)471-7097 ------------------------------ Date: 31 Jul 88 06:01:40 GMT From: tektronix!percival!bucket!leonard@ucbvax.berkeley.edu (Leonard Erickson) Subject: Re: Libertarian space policy In article <355@gronk.UUCP> johnl@gronk.UUCP (John Limpert) writes: WALL@BRANDEIS.BITNET (Matt) writes: <> If you would like to see an analagous situation, look at Antarctica. <> The goal of international control for the benefit of humankind was <> corrupted by attaching property "rights" to any sort of presence, in <> fact, specifically to 'scientific' presence. < In article <5813@dasys1.UUCP>, tneff@dasys1.UUCP (Tom Neff) defends the orbital elements summaries: > Disagree! It's not a lot of bandwidth -- check the arbitron and uunet charts. > And the s/n ratio is BEAUTIFUL -- all hard info. I love it. The only thing > I could sincerely do without is "catching up" on 2+ month old AvWeek issues. Disagree! Not only are Henry's summaries from Aviation Week and Space Technology useful to us non-subscribers, they stir up some informative debate. (And some real time wasters, but *no* posting is so pure that it can't be followed up by trash [PLEASE don't prove my point!!!]) > Tom Neff, UUCP: ...!cmcl2!phri!dasys1!tneff, CIS: 76556,2536, MCI: TNEFF > GEnie: TOMNEFF, BIX: t.neff (no kidding) -Paul S. R. Chisholm, {ihnp4,cbosgd,allegra,rutgers}!mtune!lznv!psc AT&T Mail !psrchisholm, Internet psc@lznv.att.com I'm not speaking for my employer, I'm just speaking my mind. ------------------------------ Date: Mon 1 Aug 1988 10:32:11 EST From: Harold Mueller Subject: orbital mechanics To: munck@mitre-bedford.arpa Cc: space@angband.s1.gov I can recommend a couple of good books. Bate, R. R., D. D. Mueller, and J. E. White, "Fundamentals of Astrodynamics", Dover, 1971 is a good general overview. They go into computing position/velocity vector at a future time from a known position/velocity vector at some past time. It's available in paperback. Escobal, "Methods of Orbit Determination", 1965, 1985 Krieger Publishing Company, Inc., Krieger Drive, Malabar Florida 32950, ISBN 0-88275-319-3, $39.50 in April, has a couple of great appendices. Appendix I has transformation matrices between all the commonly used (and not commonly used) coordinate systems. This means you can, say, solve your motion problem in the plane of the orbit (pretty easy) and then transform it into the azimuth/elevation/range of an earth-based observer's POV, or into 3-d rectangular for off-world display. Appendix II is titled "A complete algorithm for two-body motion in space". I haven't tried the stuff in it, but the rest of the book is good so I assume this is as well. It's a skeletal flow chart with equations (not even refined to pseudocode yet), and handles the cases for circular/elliptic, parabolic, and hyperbolic orbits (all require different equations). You are attacking a non-trivial problem. Harold Mueller Bendix Field Engineering Corporation c/o Code 5360 Naval Research Laboratory 4555 Overlook Avenue, SW Washington, DC 20375 (202) 767-3240/3356 AUTOVON 297-3240/3356 ------------------------------ End of SPACE Digest V8 #318 *******************