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Archive-name: space/controversy |
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Last-modified: $Date: 93/04/01 14:39:06 $ |
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These issues periodically come up with much argument and few facts being |
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offered. The summaries below attempt to represent the position on which |
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much of the net community has settled. Please DON'T bring them up again |
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unless there's something truly new to be discussed. The net can't set |
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public policy, that's what your representatives are for. |
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Despite a widespread belief to the contrary, the Saturn V blueprints |
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have not been lost. They are kept at Marshall Space Flight Center on |
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microfilm. |
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The problem in re-creating the Saturn V is not finding the drawings, it |
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is finding vendors who can supply mid-1960's vintage hardware (like |
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guidance system components), and the fact that the launch pads and VAB |
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have been converted to Space Shuttle use, so you have no place to launch |
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from. |
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By the time you redesign to accommodate available hardware and re-modify |
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the launch pads, you may as well have started from scratch with a clean |
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sheet design. |
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Investigators associated with NASA missions are allowed exclusive access |
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for one year after the data is obtained in order to give them an |
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opportunity to analyze the data and publish results without being |
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"scooped" by people uninvolved in the mission. However, NASA frequently |
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releases examples (in non-digital form, e.g. photos) to the public early |
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in a mission. |
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There has been extensive discussion on this topic sparked by attempts to |
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block the Galileo and Ulysses launches on grounds of the plutonium |
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thermal sources being dangerous. Numerous studies claim that even in |
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worst-case scenarios (shuttle explosion during launch, or accidental |
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reentry at interplanetary velocities), the risks are extremely small. |
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Two interesting data points are (1) The May 1968 loss of two SNAP 19B2 |
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RTGs, which landed intact in the Pacific Ocean after a Nimbus B weather |
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satellite failed to reach orbit. The fuel was recovered after 5 months |
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with no release of plutonium. (2) In April 1970, the Apollo 13 lunar |
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module reentered the atmosphere and its SNAP 27 RTG heat source, which |
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was jettisoned, fell intact into the 20,000 feet deep Tonga Trench in |
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the Pacific Ocean. The corrosion resistant materials of the RTG are |
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expected to prevent release of the fuel for a period of time equal to 10 |
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half-lives of the Pu-238 fuel or about 870 years [DOE 1980]. |
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To make your own informed judgement, some references you may wish to |
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pursue are: |
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A good review of the technical facts and issues is given by Daniel |
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Salisbury in "Radiation Risk and Planetary Exploration-- The RTG |
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Controversy," *Planetary Report*, May-June 1987, pages 3-7. Another good |
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article, which also reviews the events preceding Galileo's launch, |
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"Showdown at Pad 39-B," by Robert G. Nichols, appeared in the November |
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1989 issue of *Ad Astra*. (Both magazines are published by pro-space |
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organizations, the Planetary Society and the National Space Society |
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respectively.) |
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Gordon L Chipman, Jr., "Advanced Space Nuclear Systems" (AAS 82-261), in |
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*Developing the Space Frontier*, edited by Albert Naumann and Grover |
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Alexander, Univelt, 1983, p. 193-213. |
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"Hazards from Plutonium Toxicity", by Bernard L. Cohen, Health Physics, |
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Vol 32 (may) 1977, page 359-379. |
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NUS Corporation, Safety Status Report for the Ulysses Mission: Risk |
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Analysis (Book 1). Document number is NUS 5235; there is no GPO #; |
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published Jan 31, 1990. |
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NASA Office of Space Science and Applications, *Final Environmental |
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Impact Statement for the Ulysses Mission (Tier 2)*, (no serial number or |
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GPO number, but probably available from NTIS or NASA) June 1990. |
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[DOE 1980] U.S. Department of Energy, *Transuranic Elements in the |
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Environment*, Wayne C. Hanson, editor; DOE Document No. DOE/TIC-22800; |
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Government Printing Office, Washington, D.C., April 1980.) |
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From time to time, claims are made that chemicals released from |
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the Space Shuttle's Solid Rocket Boosters (SRBs) are responsible |
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for a significant amount of damage to the ozone layer. Studies |
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indicate that they in reality have only a minute impact, both in |
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absolute terms and relative to other chemical sources. The |
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remainder of this item is a response from the author of the quoted |
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study, Charles Jackman. |
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The atmospheric modelling study of the space shuttle effects on the |
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stratosphere involved three independent theoretical groups, and was |
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organized by Dr. Michael Prather, NASA/Goddard Institute for Space |
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Studies. The three groups involved Michael Prather and Maria Garcia |
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(NASA/GISS), Charlie Jackman and Anne Douglass (NASA/Goddard Space |
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Flight Center), and Malcolm Ko and Dak Sze (Atmospheric and |
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Environmental Research, Inc.). The effort was to look at the effects |
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of the space shuttle and Titan rockets on the stratosphere. |
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The following are the estimated sources of stratospheric chlorine: |
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Industrial sources: 300,000,000 kilograms/year |
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Natural sources: 75,000,000 kilograms/year |
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Shuttle sources: 725,000 kilograms/year |
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The shuttle source assumes 9 space shuttles and 6 Titan rockets are |
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launched yearly. Thus the launches would add less than 0.25% to the |
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total stratospheric chlorine sources. |
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The effect on ozone is minimal: global yearly average total ozone would |
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be decreased by 0.0065%. This is much less than total ozone variability |
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associated with volcanic activity and solar flares. |
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The influence of human-made chlorine products on ozone is computed |
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by atmospheric model calculations to be a 1% decrease in globally |
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averaged ozone between 1980 and 1990. The influence of the space shuttle and |
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Titan rockets on the stratosphere is negligible. The launch |
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schedule of the Space Shuttle and Titan rockets would need to be |
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increased by over a factor of a hundred in order to have about |
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the same effect on ozone as our increases in industrial halocarbons |
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do at the present time. |
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Theoretical results of this study have been published in _The Space |
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Shuttle's Impact on the Stratosphere_, MJ Prather, MM Garcia, AR |
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Douglass, CH Jackman, M.K.W. Ko and N.D. Sze, Journal of Geophysical |
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Research, 95, 18583-18590, 1990. |
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Charles Jackman, Atmospheric Chemistry and Dynamics Branch, |
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Code 916, NASA/Goddard Space Flight Center, |
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Greenbelt, MD 20771 |
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Also see _Chemical Rockets and the Environment_, A McDonald, R Bennett, |
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J Hinshaw, and M Barnes, Aerospace America, May 1991. |
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If you *don't* try to hold your breath, exposure to space for half a |
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minute or so is unlikely to produce permanent injury. Holding your |
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breath is likely to damage your lungs, something scuba divers have to |
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watch out for when ascending, and you'll have eardrum trouble if your |
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Eustachian tubes are badly plugged up, but theory predicts -- and animal |
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experiments confirm -- that otherwise, exposure to vacuum causes no |
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immediate injury. You do not explode. Your blood does not boil. You do |
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not freeze. You do not instantly lose consciousness. |
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Various minor problems (sunburn, possibly "the bends", certainly some |
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[mild, reversible, painless] swelling of skin and underlying tissue) |
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start after ten seconds or so. At some point you lose consciousness from |
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lack of oxygen. Injuries accumulate. After perhaps one or two minutes, |
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you're dying. The limits are not really known. |
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References: |
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_The Effect on the Chimpanzee of Rapid Decompression to a Near Vacuum_, |
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Alfred G. Koestler ed., NASA CR-329 (Nov 1965). |
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_Experimental Animal Decompression to a Near Vacuum Environment_, R.W. |
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Bancroft, J.E. Dunn, eds, Report SAM-TR-65-48 (June 1965), USAF School |
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of Aerospace Medicine, Brooks AFB, Texas. |
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The Challenger shuttle launch was not destroyed in an explosion. This is |
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a well-documented fact; see the Rogers Commission report, for example. |
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What looked like an explosion was fuel burning after the external tank |
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came apart. The forces on the crew cabin were not sufficient to kill the |
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astronauts, never mind destroy their bodies, according to the Kerwin |
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team's medical/forensic report. |
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The astronauts were killed when the more-or-less intact cabin hit the |
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water at circa 200MPH, and their bodies then spent several weeks |
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underwater. Their remains were recovered, and after the Kerwin team |
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examined them, they were sent off to be buried. |
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You can't use the shuttle orbiter for missions beyond low Earth orbit |
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because it can't get there. It is big and heavy and does not carry |
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enough fuel, even if you fill part of the cargo bay with tanks. |
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Furthermore, it is not particularly sensible to do so, because much of |
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that weight is things like wings, which are totally useless except in |
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the immediate vicinity of the Earth. The shuttle orbiter is highly |
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specialized for travel between Earth's surface and low orbit. Taking it |
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higher is enormously costly and wasteful. A much better approach would |
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be to use shuttle subsystems to build a specialized high-orbit |
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spacecraft. |
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[Yet another concise answer by Henry Spencer.] |
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There really is a big rock on Mars that looks remarkably like a humanoid |
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face. It appears in two different frames of Viking Orbiter imagery: |
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35A72 (much more facelike in appearance, and the one more often |
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published, with the Sun 10 degrees above western horizon) and 70A13 |
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(with the Sun 27 degrees from the west). |
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Science writer Richard Hoagland has championed the idea that the Face is |
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artificial, intended to resemble a human, and erected by an |
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extraterrestrial civilization. Most other analysts concede that the |
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resemblance is most likely accidental. Other Viking images show a |
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smiley-faced crater and a lava flow resembling Kermit the Frog elsewhere |
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on Mars. There exists a Mars Anomalies Research Society (sorry, don't |
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know the address) to study the Face. |
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The Mars Observer mission will carry an extremely high-resolution |
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camera, and better images of the formation will hopefully settle this |
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question in a few years. In the meantime, speculation about the Face is |
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best carried on in the altnet group alt.alien.visitors, not sci.space or |
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sci.astro. |
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V. DiPeitro and G. Molenaar, *Unusual Martian Surface Features*, Mars |
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Research, P.O. Box 284, Glen Dale, Maryland, USA, 1982. $18 by mail. |
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R.R. Pozos, *The Face of Mars*, Chicago Review Press, 1986. [Account of |
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an interdisciplinary speculative conference Hoagland organized to |
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investigate the Face] |
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R.C. Hoagland, *The Monuments of Mars: A City on the Edge of Forever*, |
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North Atlantic Books, Berkeley, California, USA, 1987. [Elaborate |
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discussion of evidence and speculation that formations near the Face |
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form a city] |
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M.J. Carlotto, "Digital Imagery Analysis of Unusual Martian Surface |
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Features," *Applied Optics*, 27, pp. 1926-1933, 1987. [Extracts |
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three-dimensional model for the Face from the 2-D images] |
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M.J. Carlotto & M.C. Stein, "A Method of Searching for Artificial |
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Objects on Planetary Surfaces," *Journal of the British Interplanetary |
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Society*, Vol. 43 no. 5 (May 1990), p.209-216. [Uses a fractal image |
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analysis model to guess whether the Face is artificial] |
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B. O'Leary, "Analysis of Images of the `Face' on Mars and Possible |
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Intelligent Origin," *JBIS*, Vol. 43 no. 5 (May 1990), p. 203-208. |
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[Lights Carlotto's model from the two angles and shows it's consistent; |
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shows that the Face doesn't look facelike if observed from the surface] |
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NEXT: FAQ #13/15 - Space activist/interest/research groups & space publications |
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