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    Архив RU.SPACE.NEWS за 26 ноября 1998


    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Galileo Update - November 23, 1998 Привет всем! Вот, свалилось из Internet... MEDIA RELATIONS OFFICE JET PROPULSION LABORATORY CALIFORNIA INSTITUTE OF TECHNOLOGY NATIONAL AERONAUTICS AND SPACE ADMINISTRATION PASADENA, CALIF. 91109 TELEPHONE (818) 354-5011 http://www.jpl.nasa.gov Galileo Europa Mission Status November 23, 1998 Galileo project engineers expect the spacecraft to return to normal operations today at about 5 p.m. Pacific Standard Time, following a weekend in which the spacecraft entered safing mode twice. The first of these events prevented Galileo from gathering data on Europa as it flew by the icy moon early Sunday, November 22. Galileo engineers believe the safing events, which act as a built-in protection system, were triggered by resets of the portion of the craft's control and data subsystems that control the non-spinning part of the spacecraft. These subsystems handle Galileo's communications and transmission of data to Earth. Galileo's health and safety are not in jeopardy. The anomalies occurred Saturday, November. 21, at 9:34 pm PST, and Sunday, November 22, at 5:30 p.m. The first safing happened about six hours before Galileo was scheduled to fly by Europa, and two hours before its closest approach to Jupiter's intense radiation. Before entering safing mode, Galileo performed ultraviolet spectrometer observations, and its near infrared mapping spectrometer performed an observation of Jupiter's white oval storm system. It also obtained some radio science measurements of Europa even while in safing mode. However, the craft was unable to gather data on Europa or Io. These anomalies are somewhat similar to a reset that occurred during a previous Europa flyby last June. However, in the latest anomalies, the semi-redundant halves of the control and data subsystems reset simultaneously, while in June they reset one after the other. The Galileo team has been sending commands to the spacecraft to restore its operations. In fact, the Sunday night safing occurred just before the craft recovered from the Saturday safing. Once Galileo is functioning normally again, the project team will develop a plan to have the spacecraft transmit to Earth the data it gathered. This weekend's Europa flyby was the 10th performed by the Galileo spacecraft; another Europa encounter is planned for January 31, 1999. The spacecraft has spent the past three years orbiting Jupiter and its moons, including Europa, and has provided scientists with a wealth of information and pictures. Its primary mission ended in December 1997, and the spacecraft is currently in the midst of a two-year extension, known as Galileo Europa Mission. ##### Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Mars Global Surveyor Aerobraking Update - November 22, 1998 Привет всем! Вот, свалилось из Internet... Mars Global Surveyor Aerobraking Status Report Sunday, November 22 (DOY 323/19:00:00 to DOY 326/19:00:00 UTC) Last Orbit Covered by this Report = 752 Total Phase I Aerobraking orbits accomplished = 180 Total Phase II Aerobraking orbits accomplished = 179 Total Science Phasing orbits accomplished = 290 Apoapsis altitude = 8128 km Apoapsis altitude decrease since start of aerobraking = 45898 km Periapsis altitude = 114.7 km Current Orbit Period = 05:29:17 Orbit Period decrease since start of aerobraking = 39:30:16 Starting Phase II orbit period = 11:38:02 RECENT EVENTS: The Mars Global Surveyor spacecraft continues successful phase 2 aerobraking operations with no concerns. The past 13 drag passes have provided about 13.5 minutes of orbit period reduction. About 1 minute reduction per drag pass is desired to maintain the baseline plan. The current period maintains about a 9 minute lead on the baseline. The 6-orbit running mean is 0.155 N/m2 which is below the 0.23 N/m2 corridor control trigger limit. There was 1 corridor control maneuver executed on the apoapsis portion of orbit 747 to raise periapsis and lower the drag force. Currently, sequence P749 is controlling the S/C activities. It will be replaced early this evening with P753 which will control activities starting with orbit 753 through orbit 756. Each sequence continues to be built with 5 primary orbits even though, in order to maintain prime shift builds, only four may be allowed to execute at times. Orbit timing predictions continue to be very good. Subsystems continue to report excellent S/C health and performance. The -Y solar array yoke has shown no change in structural performance. Attitude knowledge has been maintained throughout the period with excellent star processing. The power subsystem reports strong performance with 11.5 % maximum battery discharge depths each orbit. There is now 9.3 minutes of primary charger margin. The minimum MOLA laser temperature observed this period was 12.1°C using a 35 minute warming maneuver each orbit. The largest temperature increase due to aero-heating was 61°C on the -Y solar array, cell side. The telecommunications subsystem continues solid performance. UPCOMING EVENTS: Periapsis for Orbit 753 DOY327/00:09:49 UTC Through Periapsis for Orbit 760 DOY328/14:07:22 UTC (Note: MST = UTC-7 hours DOY327=11/23) SPACECRAFT COMMANDING: There were 7 command files radiated to the S/C during this period. The total files radiated since launch is now 2982. These commands were sent in support of the following activities: Nominal drag pass sequences (P740, P744, P749) Nominal corridor control maneuver sequences (A747) Command loss timer resets Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Deep Space 1 Ion Propulsion System Starts Up Привет всем! Вот, свалилось из Internet... MEDIA RELATIONS OFFICE JET PROPULSION LABORATORY CALIFORNIA INSTITUTE OF TECHNOLOGY NATIONAL AERONAUTICS AND SPACE ADMINISTRATION PASADENA, CALIF. 91109 TELEPHONE (818) 354-5011 http://www.jpl.nasa.gov Contact: Franklin O'Donnell FOR IMMEDIATE RELEASE November 25, 1998 DEEP SPACE 1 ION PROPULSION SYSTEM STARTS UP The ion propulsion system on NASA's Deep Space 1 spacecraft came to life Tuesday, November 24, and has continued running smoothly since. The engine started up at 2:53 p.m. Pacific Standard Time in response to commands sent to the spacecraft. After running overnight in low-thrust mode, engineers commanded the engine to switch to higher-thrust modes today. The mission team plans to leave the engine running over the four-day Thanksgiving weekend. The team originally powered up the engine November 10, but the system shut itself off after running for 4-1/2 minutes. When controllers sent commands to the engine to turn itself on Tuesday, they planned to collect more data on the status of the system but believed it was unlikely the engine would keep running. "We are very pleased that the engine started and continued to thrust," said Dr. Marc Rayman, Deep Space 1's chief mission engineer and deputy mission manager at NASA's Jet Propulsion Laboratory, Pasadena, CA. "In fact, it has been running very smoothly over the first day of its operation." Engineers believe that the engine probably shut itself off when it was started two weeks ago because of metallic grit or other contamination between the two high-voltage grids at the rear of the advanced engine. It is likely that changes in temperature as the spacecraft conducted other technology validation activities affected the flakes, and powering-up the thruster may have vaporized the remains. "It's common for new ion engines on the ground or on Earth- orbiting spacecraft to shut themselves off a few times when they are first exercised," said Rayman. "We would not be surprised if the engine shut itself off again over the first few days or weeks that it runs. "Deep Space 1's charter is to test new, advanced technologies," Rayman added. "If everything worked perfectly on the first try, it would be an indication we had not been sufficiently aggressive in selecting the technologies. Diagnosing the behavior we have seen is a very valuable part of Deep Space 1's objective of enabling future space science missions." The fuel used in Deep Space 1's ion engine is xenon, a colorless, odorless and tasteless gas more than 4-1/2 times heavier than air. When the ion engine is running, electrons are emitted from a hollow bar called a cathode into a chamber ringed by magnets, much like the cathode in a TV picture tube or computer monitor. The electrons strike atoms of xenon, knocking away one of the 54 electrons orbiting each atom's nucleus. This leaves each atom one electron short, giving it a net positive charge -- making the atom what is known as an ion. At the rear of the chamber is a pair of metal grids which are charged positive and negative, respectively, with up to 1,280 volts of electric potential. The force of this electric charge exerts a strong "electrostatic" pull on the xenon ions -- much like the way that bits of lint are pulled to a pocket comb that has been given a static electricity charge by rubbing it on wool on a dry day. The electrostatic force in the ion engine's chamber, however, is much more powerful, causing the xenon ions to shoot past at a speed of more than 100,000 kilometers per hour (60,000 miles per hour), continuing right on out the back of the engine and into space. At full throttle, the ion engine would consume about 2,500 watts of electrical power and put out 90 millinewtons (1/50th of a pound) of thrust. This is comparable to the force exerted by a single sheet of paper resting on the palm of a hand. When the engine was started Tuesday, it ran overnight thrusting at a power level of 500 watts. This morning engineers commanded it to thrust at a level of 885 watts, then at 1,300 watts. Engineers may decide to have the engine thrust at a lower level while it runs over the next few days. The ion propulsion system flight hardware was built for Deep Space 1 by Hughes Electron Dynamics Division, Torrance, CA; Spectrum Astro Inc., Gilbert, AZ; Moog Inc., East Aurora, NY; and Physical Science Inc., Andover, MA. Development of the ion propulsion system was supported by NASA's Office of Space Science and Office of Aeronautics and Space Transportation Technology, Washington, DC. JPL is managed for NASA by the California Institute of Technology. ##### Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: STARDUST Update - November 20, 1998 Привет всем! Вот, свалилось из Internet... STARDUST Status Report November 20, 1998 Ken Atkins STARDUST Project Manager Assembly, Test, and Launch Operations (ATLO) activities: The principal ATLO activities this week have been opening the spacecraft and installing thermal tape, heaters and thermostats and installing the reworked (for glass body diodes) solar array switching unit (SASU). All support equipment was also checked out. The first week activities at Kennedy Space Center (KSC) have been very efficient and smooth with work accomplished well inside the scheduled timeline. KSC support has been outstanding. Daily time-lapse movies are now being created of the launch preparations at KSC: http://stardust.jpl.nasa.gov/webcam/ Members of the STARDUST team attended the grand opening of the Omniplex's STARDUST Cafe exhibit and STARDUST Planetarium show in Oklahoma City. Principal Investigator Dr. Don Brownlee of the University of Washington led a panel with Joe Vellinga (our Lockheed Martin Program Manager), Dr. Peter Tsou of JPL (Deputy Principal Investigator and "Mr. Aerogel"), Dr. Ben Clark (Lockheed Martin Astronautics Chief Scientist) and myself. We gave presentations on STARDUST and interacted with the public for two hours. Aimee Whalen and Julie Malmquist, our Outreach team from JPL accompanied us there, along with Dr. Steve Jones of JPL from the Aerogel Team. Educational Management Group conducted it's final production of the STARDUST series with the "Space Cowboy" last Tuesday. A total of 27 schools throughout the United States participated in live chats with the STARDUST personnel featured in one of the four programs. They threw some great questions at us. It's just wonderful to see the interest and participation of kids in learning about STARDUST. Preliminary numbers estimated that over 1.2 million students viewed the one or all of the programs. For more information on the STARDUST mission - the first ever comet sample return mission - please visit the STARDUST home page: http://stardust.jpl.nasa.gov Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Six Launches, Six Months Привет всем! Вот, свалилось из Internet... Six Launches, Six Months http://www.jpl.nasa.gov/sixlaunches/ NASA's era of "faster, better, cheaper" missions is paying off with an unprecedented schedule of launches in 1998 and 1999. In a six-month period a total of six launches of seven JPL-teamed missions are scheduled: Deep Space 1, a spacecraft that is testing advanced technologies including an ion engine on its way to fly by an asteroid, was launched October 24, 1998 from Cape Canaveral, Florida. See the Deep Space 1 News and Information Page or the Deep Space 1 Project Home Page. http://www.jpl.nasa.gov/ds1news http://nmp.jpl.nasa.gov/ds1 Mars Climate Orbiter, the first of two spacecraft targeted toward the red planet under the Mars Surveyor '98 project, is scheduled for launch December 10, 1998 from Cape Canaveral, Florida. See the Mars News and Information Page or the Mars Surveyor '98 Project Home Page. http://mars.jpl.nasa.gov/msp98 http://www.jpl.nasa.gov/marsnews Mars Polar Lander, the second of two Mars Surveyor '98 missions, will carry a science payload including a robotic arm to a landing near Mars' south pole; launch is scheduled January 3, 1999 from Cape Canaveral, Florida. See the Mars News and Information Page or the Mars Surveyor '98 Project Home Page. http://mars.jpl.nasa.gov/msp98 http://www.jpl.nasa.gov/marsnews Deep Space 2, a project under the New Millennium Program, will send two microprobes along on Mars Polar Lander to smash into the surface of Mars as a test of advanced technologies for future solar system probes; launch is scheduled January 3, 1999 from Cape Canaveral, Florida. See the Mars News and Information Page or the Deep Space 2 Project Home Page. http://nmp.jpl.nasa.gov/ds2 http://www.jpl.nasa.gov/marsnews Quick Scatterometer (QuikScat) is a rapidly developed Earth-orbiting satellite that will carry SeaWinds, a scatterometer instrument studying near-surface ocean winds. Launch is planned for early 1999 from Vandenberg Air Force Base, California. See the SeaWinds on QuickScat Project Home Page. http://winds.jpl.nasa.gov/missions/quikscat/quikindex.htm Stardust will send a spacecraft flying through a comet's coma, or the cloud that surrounds the nucleus of a comet, and for the first time ever bring cometary material back to Earth. Launch is scheduled February 6, 1999 from Cape Canaveral, Florida. See the Stardust Project Home Page. http://stardust.jpl.nasa.gov Wide-field Infrared Explorer (WIRE) is an Earth-orbiting infrared telescope that will make a four-month infrared survey of the universe, focusing on starburst galaxies and luminous protogalaxies. Launch is scheduled February 26, 1999 from Vandenberg Air Force Base, California. See the WIRE Project Home Page. http://www.ipac.caltech.edu/wire/ Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: ESA's plans for a microarcsec space astrometry mission being presented Привет всем! Вот, свалилось из Internet... ESA Science News http://sci.esa.int 23 Nov 1998 ESA's plans for a microarcsec space astrometry mission being presented at the GAIA workshop This week plans for the GAIA space astrometry mission will be presented to more than 70 scientists from all over Europe when they gather in Leiden (Netherlands) for the GAIA workshop. Hosted by The Lorentz Center and Leiden Observatory (University of Leiden), the workshop will provide scientists with the opportunity to learn about the current status and scientific prospects of GAIA. They will also have the opportunity to participate in discussions aimed at consolidating the scientific and technical report to be prepared for the ESA advisory groups. GAIA (Global Astrometric Interferometer for Astrophysics) is an advanced astrometric mission proposed, in 1995, as a Cornerstone Mission within the ESA Horizon 2000+ science plan, which aims: * to measure distances and velocities of more than a billion stars in our Galaxy * to provide: o highly accurate astrometric data: positions, distances and proper motions (10 microarcsecond at 15 mag); o multiplicity and orbital motions; o multi-colour photometry at hundreds of separate epochs; o radial velocities (a few km/sec at 17 mag). GAIA's unique observational strengths are: * its unprecedented accuracy (2-3 orders of magnitudes more accurate than Hipparcos, and five orders of magnitude more accurate than ground observations); * its extremely large sample observational capabilities (with one billion stars, the catalogue will be 10,000 times larger than Hipparcos; and it will observe 1 per cent of the total number of stars in our Galaxy); * its very faint limiting magnitude (at 20 mag, more than 5 orders of magnitude fainter than the completeness limit of Hipparcos); * its on-board source detection and measurement capabilities complete to the detection limit of about 20 mag. This will ensure complete and unbiased samples at the faintest magnitudes, and will mean that variables, burst sources, lensing events, etc will be measured as they occur. As a result GAIA will uniquely address astrophysical issues such as: * the formation and evolution of our Galaxy; * dynamics of the Local Group Galaxies; * the occurrence and statistics of planetary systems (some 200,000 stars within 200 parsec will be rigorously scrutinised for the presence of Jupiter mass planetary companions); * wide angle space metric analyses; * the luminosity and dynamics of rare astrophysical objects. USEFUL LINKS FOR THIS STORY GAIA homepage http://astro.estec.esa.nl/GAIA/ Hipparcos homepage http://astro.estec.esa.nl/hipparcos/ Lorentz Center, Leiden http://lc.leidenuniv.nl/ Andrew Yee ayee@nova.astro.utoronto.ca Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: First direct detection of meteoroid impacts on Saturn rings (Forwarded Привет всем! Вот, свалилось из Internet... Stanford University CONTACT: David F. Salisbury, News Service (650) 725-1944, e-mail: david.salisbury@stanford.edu COMMENT: Mark Showalter, STAR Lab (650) 604-3382, e-mail: showalter@Ringside.Arc.Nasa.Gov 11/6/98 First direct detection of meteoroid impacts on Saturn rings Movies like "Deep Impact" and "Asteroid" have popularized the notion that the solar system contains kilometer-wide chunks of material that represent a potential hazard to life on Earth. But how many of these objects actually lurk in the darkness of space? Mark Showalter's research may help answer that question. A research associate at Stanford's Space, Telecommunications and Radioscience Laboratory (STARLab) who works out of the NASA Ames Research Center, Showalter reports, in the Nov. 6 issue of the journal Science, the first direct and unambiguous detection of basketball-sized meteoroids striking one of Saturn's rings. Using images taken by the two Voyager spacecraft that flew by the ringed planet in 1980 and 1981, Showalter identified objects that he calls "burst events" on the F Ring, a faint and narrow ring that orbits about 3000 kilometers beyond the outer edge of Saturn's main ring system. By tracking these bursts long enough to determine that they have a lifetime of about two weeks, he determined that they are clumps of dust kicked out of the ring when it is hit by small meteoroids ranging from two to 40 centimeters in size. The F Ring has the best conditions for allowing observation of these dust clouds, Showalter says. It is dim enough so that the clumps show up and thin enough so that they do not rapidly collapse back into the ring. That allowed him to follow the evolution of three of these clumps in some detail. Their spreading rates were consistent with that expected if the ring was hit by an object traveling at high velocity, he reports. Showalter estimates that the F Ring experiences about 20 such impacts per year. This, in turn, allowed him to produce the first crude indication of the abundance of centimeter-sized objects in the outer solar system. When the Cassini spacecraft reaches Saturn in 2004, it will be equipped to do a more thorough job of observing these impacts and so should provide a much more precise estimate, he says. There are only two other sources of data about meteoroids in the solar system's outer reaches. The Pioneer 10 and 11 spacecraft, which flew by Saturn in the late 1970s, were equipped with a simple detector that provided an estimate of the population of micrometer-sized particles in the vicinity of Jupiter and Saturn. Observations with Earth-based telescopes also have discovered eight asteriods in the 10- to 100-kilometer size range that cross Saturn's orbit. They have been named the Centaurs. Such research should give scientists a better handle on the number of meteoroids of various sizes that exist in the inner solar system. Objects of this size strike the Earth fairly frequently. They are large enough so that they don't completely burn up in the atmosphere, and the burnt remnant lands on Earth as a meteorite. But they are too small to be picked up in satellite imagery, so the frequency of these fiery collisions is not well known, Showalter says. "People who model these things estimate that the frequency of meteoroids should be about the same throughout the solar system," he says. And, within the rather large uncertainties involved, his observations are consistent with that assumption. More importantly, improved knowledge of the abundance of centimeter-sized meteoroids in the solar system will provide better estimates of the numbers of kilometer-sized objects, which are the real concern. "It is all part of a continuous process," Showalter says. "We know there are so many ping-pong-ball-sized objects for every basketball-sized object and so many basketball-sized objects for every house-sized one. So improved estimates of meteoroids of any given size improve our estimates of the number of meteoroids of all sizes." Andrew Yee ayee@nova.astro.utoronto.ca Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Aussie help Hubble hunt ancient galaxies (Forwarded) Привет всем! Вот, свалилось из Internet... Commonwealth Scientific and Industrial Research Organisation Australia Ms Rosie Schmedding (02) 6276-6520 Mobile (0418) 622-653 Fax (02) 6276-6821 Media Release: 24 November 1998 Ref 98/271 AUSSIES HELP HUBBLE HUNT ANCIENT GALAXIES Australian telescopes have helped the Hubble Space Telescope (HST) find thousands of new galaxies. The Anglo-Australian Observatory and CSIRO helped choose the patch of sky in which the HST found the previously unknown galaxies. They are now helping Hubble astronomers to learn more about these new discoveries. Preliminary HST results were released today by NASA's Space Telescope Science Institute, as were the results from the Australian institutions. The piece of sky is tiny, the size of an echidna's eye on a five-cent piece held at arm's length. Called the Hubble Deep Field South, it complements the original Hubble Deep Field, another small patch in the northern sky. The HST wowed the scientific world when in late 1995 it stared at the apparently blank piece of sky and found in it remarkable distant fossil galaxies, some formed when the Universe was only a tenth of its present age. This time around astronomers wanted a piece of sky with a distant quasar (a galaxy with an extremely bright centre) in it. The quasar lights up and makes visible any material in space between it and the Earth, like a car headlight shining through fog at night. Astronomers of the Anglo-Australian Observatory in Sydney, aided by their colleagues in Cambridge, UK, painstakingly sifted through their photographic records of the whole southern sky until they found a likely quasar, 10 billion light-years distant. CSIRO's Parkes radio telescope and the Anglo- Australian Telescope were used to confirm that the quasar was suitable. CSIRO's Australia Telescope was used to check that there were not too many confusing radio sources in the field. The Hubble Space Telescope spent ten days in October scrutinising the new patch of sky. Every major telescope that can see the Deep Field South has also made observations of the field and is releasing them to the astronomical community at the same time as the HST results come out. "This is a new way of working," said Dr Ray Norris, head of Astrophysics at CSIRO's Australia Telescope National Facility. "Everyone is putting their data on the Web, warts and all. The galaxies in this field are being studied incredibly intensively, with optical, radio, infrared and UV observations all being made at more or less at the same time." "We currently each have one piece of the jigsaw puzzle which will be put together to reveal a new picture of the distant Universe," said Dr Brian Boyle, Director of the Anglo-Australian Observatory. The Anglo-Australian Telescope has measured the distances of about 75 faint far-flung galaxies in the field. "These distances can be combined with other information to produce a 3D map of this part of the Universe," explained Dr Boyle. "Those galaxies for which we have the distances are all young --'newborns', so to speak," he said. "The gas clouds that are lit up by the quasar are probably forming galaxies -- embryos. We want to compare the two kinds, to build up a picture of the life cycle of galaxies from creation through to old age." The radio telescope observations are proving more mysterious. "We have already found one extremely puzzling object," said Dr Norris. "We don't know what it is." "It could be a very distant version of a kind of galaxy we know about, called a starburst galaxy, obscured by dust. But to be at that distance and still look so big, it would have to be enormous. On the other hand, we really don't know what to expect from galaxies at that distance." Astronomers overhauled their theories of how galaxies evolve and how fast stars form after studying the 'core-sample' of galaxies dredged up by the original Hubble Deep Field. Now the Hubble Deep Field South will show if the original Hubble Deep Field North was truly a representative patch of the Universe. "It will take astronomers months to digest all this new data," predicted Dr Boyle. More information: Dr Ray Norris CSIRO (02) 9372 4416 (bh), (02) 9369 9591 (ah), 0417 288 307 (mobile) rnorris@atnf.csiro.au Dr Brian Boyle Anglo-Australian Observatory (02) 9372 4811 (bh), (02) 9498 1584 (ah) director@aaoepp.aao.gov.au Results on the Web: Hubble Space Telescope http://oposite.stsci.edu/pubinfo/1998/41 and http://oposite.stsci.edu/pubinfo/pictures.html CSIRO Australia Telescope National Facility http://www.atnf.csiro.au/~rnorris/hdf-s Anglo-Australian Observatory http://www.aao.gov.au/AAO/hdfs/ Andrew Yee ayee@nova.astro.utoronto.ca Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Cassini Update - November 25, 1998 Привет всем! Вот, свалилось из Internet... Cassini Significant Events for 11/20/98-11/26/98 Spacecraft Status: The most recent Spacecraft status is from the DSN tracking pass on Tuesday, 11/24, over the Canberra tracking station. The Cassini spacecraft is in an excellent state of health and is executing the Cruise 11 sequence normally. Spacecraft Activity Summary: On Friday, 11/20, routine maintenance was performed on the Solid State Recorder (SSR-B) flight software partitions. On Saturday, 11/21, the Solid State Recorder (SSR-B) record and playback pointers were reset as planned (nominally once per week). On Sunday, 11/22, three activities occurred. Science & Engineering Record (S&ER) 3 telemetry mode was installed into the CDS in preparation for the Instrument Checkout in January. An accelerometer calibration was performed. The accelerometer was powered up for this activity and will remain powered ON in preparation for the upcoming Deep Space Maneuver (DSM). The AACS High Watermarks were cleared as the last activity for this day. Upcoming events: Activities scheduled for the week of 11/27-12/03 include: SSR Pointer Reset (11/28), Propulsion Module Subsystem (PMS) Pressurization & Playback (12/01), DSM Mini Sequence Uplink and Execution (12/02), Power on VIMS Decontamination Heaters, Active IVP Vector Update, and AACS High Watermark Clear (12/03), and SSR Memory Load Repair (12/03). Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: WDC-A R&S Launch Announcement 12978: Bonum 1 Привет всем! Вот, свалилось из Internet... COSPAR/ISES WORLD WARNING AGENCY FOR SATELLITES WORLD DATA CENTER-A FOR R & S, NASA/GSFC CODE 633, GREENBELT, MARYLAND, 20771. USA SPACEWARN 12978 COSPAR/WWAS USSPACECOM NUMBER SPACECRAFT INTERNATIONAL ID (CATALOG NUMBER) LAUNCH DATE,UT BONUM 1 1998-068A 25546 22 NOVEMBER 1998 DR. JOSEPH H. KING, DIRECTOR, WDC-A-R&S. [PH: (301) 286 7355. E-MAIL: KING@NSSDCA.GSFC.NASA.GOV 24 NOVEMBER 1998 13:30 UT] Further details will be in a forthcoming SPACEWARN Bulletin Dr. Edwin V. Bell, II _/ _/ _/_/_/ _/_/_/ _/_/_/ _/_/ Mail Code 633 _/_/ _/ _/ _/ _/ _/ _/ _/ NASA Goddard Space _/ _/ _/ _/_/ _/_/ _/ _/ _/ Flight Center _/ _/_/ _/ _/ _/ _/ _/ _/ Greenbelt, MD 20771 _/ _/ _/_/_/ _/_/_/ _/_/_/ _/_/ +1-301-286-1187 ed.bell@gsfc.nasa.gov SPACEWARN home page: http://nssdc.gsfc.nasa.gov/spacewarn/ Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Galileo Update - November 24, 1998 Привет всем! Вот, свалилось из Internet... MEDIA RELATIONS OFFICE JET PROPULSION LABORATORY CALIFORNIA INSTITUTE OF TECHNOLOGY NATIONAL AERONAUTICS AND SPACE ADMINISTRATION PASADENA, CALIF. 91109 TELEPHONE (818) 354-5011 http://www.jpl.nasa.gov Galileo Europa Mission Status November 24, 1998 The Galileo spacecraft is out of safe mode and has resumed normal operations. At 5 p.m. Pacific Standard Time on Monday, November 23, the spacecraft responded to commands sent from the ground and returned to normal sequenced activities. Galileo had been in safe mode after the portion of the spacecraft's command and data subsystems that control Galileo's non-spinning part reset themselves twice over the weekend of November 21-22. These subsystems control the transmission of Galileo's data to Earth. The first safing event occurred Saturday evening, November 21, and the other Sunday afternoon, November 22. Because the first safing took place about six hours before Galileo was scheduled to fly by Europa, the spacecraft was unable to gather data on the icy moon, other than distant observations. Galileo engineers believe the resets were probably induced by the intense radiation environment immediately surrounding Jupiter. Now that the spacecraft is functioning normally again, Galileo will be able to transmit to Earth the information that was gathered by Galileo before the safing events, as well as some radio science measurements of Europa taken while in safe mode. This latest flyby was Galileo's 10th encounter with Europa; another is planned for January 31, 1999. The spacecraft has spent the past three years orbiting Jupiter and its moons, including Europa, gathering a wealth of information and pictures. Its primary mission ended in December 1997, and the spacecraft is currently in the midst of a two-year extension, known as the Galileo Europa Mission. ##### Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Rainfall, not humans, control the size of the Sahara (Forwarded) Привет всем! Вот, свалилось из Internet... Lynn Chandler Goddard Space Flight Center Greenbelt, MD 20771 Lynn.Chandler.1@gsfc.nasa.gov Nov. 24, 1998 (Phone: 301-614-5562) RELEASE NO: 98-189 RAINFALL, NOT HUMANS, CONTROLS THE SIZE OF THE SAHARA The decades-old concern that land misuse by humans is causing the African Sahara desert to extend south into fertile land is not occurring, according to Earth scientists from the NASA Goddard Space Flight Center in Greenbelt, Md. and Florida State University. Looking at nearly two decades of satellite observations of vegetation growing near the Sahara, Dr. Compton "Jim" Tucker, a Goddard biologist, and Dr. Sharon Nicholson, a Florida State meteorologist, found that although the southern border of the Sahara ebbs and flows from year to year, there has been no overall growth in the desert?s size. In the 1970s and early 1980s, scientists had the impression that the desert was steadily moving south into the temperate zones. But according to Tucker, satellite data show that Saharan/Sahelian boundary rebounds to the north with rainfall in wet years such as 1994. "We?re not saying that there is no land degradation," said Nicholson, who has studied the problem for over 20 years. "But this paradigm about the marching sands and the vegetation going away is not happening." An area of semi-arid grassland called the "Sahel," lines the Sahara along its southern border. The Sahelian/Sahara border has received a lot of attention from scientists and policy makers because in very dry years, the border moves south. "The interesting question is how the desert changes through time, and is it changing through time," he said. Tucker studied data collected from 1980 to 1997 by satellite sensors aboard National Oceanic and Atmospheric Administration (NOAA) Advanced Very High-Resolution Radiometer (AVHRR) meteorological satellites. Tucker and Nicholson found that there was significant year-to-year variation in rainfall, with an especially dry year in 1984, making it seem that during drought years the desert was expanding southward. After 1984, the Sahara border rebounded and was especially far north in 1994. The AVHRR sensor aboard the NOAA satellites measures the infrared and near-infrared radiation reflected by plants. From the two wavelengths of radiation, a "greenness index" can be determined. The "greenness index" shows scientists what areas of ground are covered by vegetation, and Tucker has shown that vegetation cover corresponds to the amount of rainfall in a particular region. Over the last 20 years, the Saharan boundary has followed rainfall trends, and Nicholson?s analysis of historical data, recently published in the American Meteorological Society?s Bulletin, confirms this research. "It?s virtually impossible to separate desertification from drought," she said. Desertification is defined as the man-made or natural formation of desert from what once was usable land. This study on desertification is sponsored by NASA and the U.S. Agency for International Development. NASA funded this research as part of its Earth Science Enterprise, a long-term research program designed to study the Earth?s land, oceans, air, ice and life as a total system. Andrew Yee ayee@nova.astro.utoronto.ca Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Submillimeter Wave Astronomy Satellite To Study Star Formation Привет всем! Вот, свалилось из Internet... Doug Isbell/Don Savage Headquarters, Washington, DC November 25, 1998 (Phone: 202/358-1547) Donna Drelick/Jim Sahli Goddard Space Flight Center, Greenbelt, MD (Phone: 301-286-7995) RELEASE: 98-213 SUBMILLIMETER WAVE ASTRONOMY SATELLITE TO STUDY STAR FORMATION NASA's Submillimeter Wave Astronomy Satellite (SWAS) mission, scheduled for launch at 8:40 p.m. EST (5:40 p.m. PST) on Dec. 2, 1998, will gather star-formation data, which have remained invisible from beneath the obscuring effects of the Earth's atmosphere. The overall goal of the two-year mission is to gain a greater understanding of star formation by determining the composition of interstellar clouds, and establishing the means by which these clouds cool as they collapse to form stars and planets. "During its mission, SWAS will observe hundreds of regions of ongoing star formation within our galaxy. The answers SWAS will provide are important not only to the understanding of the formation of future stellar systems, but also to the understanding of the processes that led to the formation of the Sun, the Earth, and the other planets and moons in our own solar system," said Dr. Gary Melnick, Harvard-Smithsonian Center for Astrophysics, principal investigator for the SWAS mission. SWAS will be launched from Vandenberg Air Force Base, CA, via a Pegasus-XL launch vehicle, built by Orbital Sciences Corporation. The launch vehicle is a three-stage, solid- propellant booster system carried aloft by an L-1011 jet aircraft. The system will be released when the aircraft reaches an altitude of about 40,000 feet (12,200 meters) and has airspeed of Mach 0.8. The SWAS mission is designed for a two-year duration. SWAS is one of NASA's Small Explorers (SMEX) satellites, which are both small and economical. The SWAS spacecraft weighs only 625 pounds. The satellite was designed and built by NASA's Goddard Space Flight Center, Greenbelt, MD. The SWAS observatory will be inserted into an orbit with an altitude of 370 miles above the Earth, and will orbit the Earth every 97 minutes. SWAS will typically observe three to five astronomical objects per orbit. The observed data will be stored in the spacecraft memory and sent to a ground station. Within 24 hours of receipt at the ground station, these data are received at the Smithsonian Astrophysical Observatory's Science Operation Center in Cambridge, MA. There, the science content of the data is analyzed and new astronomical targets are selected for observation. Further information about SWAS can be found on the Internet at: http://sunland.gsfc.nasa.gov/smex/swas/ http://sunland.gsfc.nasa.gov/smex/ http://pluto.harvard.edu/cfa/oir/Research/swas.html -end- Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: First US Station Element To Be Launched December 3 Привет всем! Вот, свалилось из Internet... Jennifer McCarter Headquarters, Washington, DC November 25, 1998 (Phone: 202/358-1639) Joel Wells Kennedy Space Center, FL (Phone: 407/867-2468) Eileen Hawley Johnson Space Center, Houston, TX (Phone: 281/483-5111) RELEASE: 98-214 FIRST U.S. STATION ELEMENT TO BE LAUNCHED DEC. 3 NASA program managers set Dec. 3 as the official launch date for the STS-88 mission aboard Space Shuttle Endeavour. This is the first Shuttle mission dedicated to the assembly of the International Space Station (ISS), the largest and most complex international cooperative science and engineering venture in history. The six-member flight crew will work to mate Endeavour's primary payload, the U.S.-made Unity connecting module, to the Russian-built Zarya control module during the 12-day mission. Zarya was launched on a Proton rocket from Baikonur Cosmodrome in Kazakstan on Nov. 20. While the STS-88 Flight Readiness Review was in progress, Russian flight controllers performed tests on Zarya's onboard systems and adjusted its orbital position. The Flight Readiness Review, held at NASA's Kennedy Space Center, FL, began Monday afternoon allowing all Shuttle and ISS project offices to evaluate the flight readiness of the astronaut crew, vehicle and cargo, along with the launch and mission control teams. "Following Zarya's successful launch last week, it is now NASA's responsibility to begin the International Space Station assembly process," said NASA's Johnson Space Center Director George Abbey. "This flight will clearly demonstrate the unique capabilities of the Space Shuttle and of astronauts and cosmonauts to assemble large structures in space. STS-88 will showcase the Shuttle as the safe and reliable workhorse of the space station era and other future activities in Earth orbit." Endeavour is scheduled for launch on Dec. 3 at 3:59 a.m. EST from launch pad 39A. The exact launch time will be determined during the final hour of the launch countdown as mission controllers pinpoint Zarya's exact orbital position. The mission is slated to last 11 days, 19 hours and 49 minutes. An on-time launch will lead to a Kennedy Space Center landing on Monday, Dec. 14, at 11:48 p.m. EST. The STS-88 Mission Commander is Robert Cabana. The pilot is Fredrick Sturckow. Nancy Currie, Russian cosmonaut Sergei Krikalev, Jerry Ross and James Newman will serve as mission specialists on this flight. STS-88 will be the 13th flight of Shuttle Endeavour and the 93rd mission in Shuttle program history. -end- Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: NASA разрабатывает таблетку-передатчик Привет всем! Вот, свалилось из Internet... NASA разрабатывает таблетку-передатчик [NASA] В будущем году NASA планирует начать внедрение своей "таблетки-передатчика", которая может отслеживать температуру, кровяное давление и другие параметры больного и передавать полученную информацию врачам. Разработку этой таблетки ведет Исследовательский центр им. Эймса. Ее размеры составляют 0,8х3,4 см. Позднее планируется создать таблетку меньших размеров, которую перед полетом будут глотать астронавты. Такая таблетка будет передавать на Землю объективные данные о самочувствии астронавтов во время космического путешествия. Источник: InfoArt News Agency Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Запуск научного спутника Landsat-7 намечен на 15 апреля Привет всем! Вот, свалилось из Internet... Запуск научного спутника Landsat-7 намечен на 15 апреля [NASA] Определена новая дата запуска научного спутника Земли Landsat-7 - 15 апреля 1999 г. (ранее предполагалось осуществить запуск в декабре 1998 г.). Спутник будет выведен на орбиту ракетой-носителем Delta II, старт состоится с базы ВВС США "Ванденберг". Hа Landsat-7 установлено оборудование для получения снимков земной поверхности высокого разрешения. С его помощью будет продолжено составление картографической базы данных, начатое в 1982 г. спутником Landsat-4. Снимки, полученные с помощью Landsat-7, предполагается использовать в сельском хозяйстве, для исследования лесов, качества воды и пр. Задержка со стартом Landsat-7 вызвана необходимостью внесения изменений в конструкцию блока электропитания спутника. В ходе испытаний, начавшихся в декабре 1997 г., этот блок отказывал дважды. Следующий спутник из серии Landsat планируется запустить в конце 1999 г. Он будет вращаться по той же орбите, что и Landsat 7, но с задержкой на 1 мин. Это позволит одновременно производить съемку одного и того же участка поверхности Земли для проверки новых технологий обработки изображений. Источник: InfoArt News Agency Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Ракета Delta 2 с российским телевизионным спутником наконец-то взлетел Привет всем! Вот, свалилось из Internet... Ракета Delta 2 с российским телевизионным спутником наконец-то взлетела [SpaceViews] Ракета Delta 2 с российским телевизионным спутником на борту после трех неудачных попыток наконец-то стартовала. Запуск состоялся ночью с 22 на 23 ноября с космодрома на мысе Канаверал. Delta 2 оторвалась от земли 23 ноября в 2 часа 54 мин по московскому времени после более чем получасовой задержки, связанной с сильным ветром в верхних слоях атмосферы. Ракета вывела на орбиту спутник Bonum-1. Далее полет прошел без проблем. Первоначально полет был запланирован на четверг 19 ноября, но был отложен из-за неполадок в креплении сопла основного двигателя ракеты. В пятницу старт был отложен из-за проблем со связью между наземным пунктом управления и спутником, а в субботу был обнаружен дефект в датчике топлива. Спутник Bonum-1 будет обеспечивать передачу 50 телевизионных каналов на западные области России. Спутник был создан компанией Hughes по заказу "Медиа-Мост". Это первый частный российский спутник. Источник: InfoArt News Agency Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Ракета Delta 2 с российским... (картинка) [1/2] Привет всем! Вот, свалилось из Internet... section 1 of 2 of file bonum-1.jpg < uuencode 5.32 by R.E.M. > begin 644 bonum-1.jpg M_]C_X``02D9)1@`!`0```0`!``#_VP!#`!`+#`X,"A`.#0X2$1`3&"D;&!86 M&#(D)AXI.S0^/3HT.3A!25Y004591C@Y4F]366%D:6II/T]S>W)F>EYG:67_ MVP!#`1$2$A@5&#`;&S!E0SE#965E965E965E965E965E965E965E965E965E M965E965E965E965E965E965E965E967_P``1"`#Z`,@#`2(``A$!`Q$!_\0` M'P```04!`0$!`0$```````````$"`P0%!@<("0H+_\0`M1```@$#`P($`P4% M!`0```%]`0(#``01!1(A,4$&$U%A!R)Q%#*!D:$((T*QP152T?`D,V)R@@D* M%A<8&1HE)B<H*2HT-38W.#DZ0T1%1D=(24I35%565UA96F-D969G:&EJ<W1U M=G=X>7J#A(6&AXB)BI*3E)66EYB9FJ*CI*6FIZBIJK*SM+6VM[BYNL+#Q,7& MQ\C)RM+3U-76U]C9VN'BX^3EYN?HZ>KQ\O/T]?;W^/GZ_\0`'P$``P$!`0$! 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    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Ракета Delta 2 с российским... (картинка) [2/2] Привет всем! Вот, свалилось из Internet... section 2 of 2 of file bonum-1.jpg < uuencode 5.32 by R.E.M. > M`+2FACC$0,8)`[D'_P"O^E=>>5KS?0I'37HB@)RV#@=B*](4Y45C;ET.F+NA M#*9(\YPPZBO/=54G7[P$YZ=?H*[V0.$<Q@%AT![UREQIPN+V6Y?S`[\$`C`Q M_P#JH>P,R;=1'(,9ZC/%:('[[\*?Y$"G;A_E_O=*L1B,7:L$!3;A@?7UI),F MQ5T__7J/]H5VD'"CZ5SUA9P&5648;=V)KHXQ@"BUBUL86KMBXE/\OI64UH\J M&ZEX2,XC3/&?7Z_RJ_J$WF7DP`Z.1^55;ZXP%@0':O'X]S183)+$,MK,8TW2 M^6VSW;''ZU/X>T@:<Q0G=(`-[#^]Z#Z5<TNU^SVYEE&&(SCT%6M.4E"YZL23 M30(H^+[O[+H;Q@_-,=@^G4_R_6N)O95DL[?:W*@@X_"NL\5V$FIR11HY41*2 M.,AB>WZ?K7&W&D7MOS]GD('<<_RI73T$T%M/,DD829]NX9`;BM'5[N:#4OW3 M_P`((!`-:6DZ8+6S3[19)+,X\PR.!B/V.>>GIWJQ=VEA/<.DL!\Y1R5#`8QU MSC'7BAA8P$U&?;]E*`KMY.3GUJQK)DCT\M&[+MF7H<<%/\14=S"D4F^,'>RX M)S[<5/K`:33UV`DR!#@#N"W^-:$+<Y];JX;Y?.DSV^8T4):7.=RQ-Q[45-AF MY<DM"JGZFI+5<+2ZL-L\('`*\XIUO]W\OY5M%W=S*2L2NF^%A[5DL,&MI>AK M'E_UC?6J9!++,LUM@G#@C\:H)\MPR]B-U35%_P`O7_`/ZU+92.M\.Q0BTW*J M"1B2Y'4^E=)#G;S7"VK,EM$RL5(8\@_6NNTUV:U4LQ)]2:Y[W.E;%QB$;GOZ M53GCWR95#SUJU3L#TJDQF-+IY=R6P%QP!UJB+$I-\I/'7#5TK@;3P.E4``&X M`ZU6XFAEC"(I0#NSGUK87TJL`-R\5:7K4L9@7%M(U[(QVA&8G)ZYS3UM%\U) M&(+)V*\>U:;J,G@=::%7</E'Y4PL0S+<20E%V`'@GGI5F!?*B`QT%2Q`8Z5! M.27QDXJ6[#2*\BEI7).>>*:T61QUJ;%./05D48;'5;<$M#Y@_P!D@_I4+7C/ M;W!DB\J1AEB1@MP??VKHCT-5;_\`Y!]S_P!<F_D:I,EHXFZANKR5UA7Y0.O; M_/6K7FO:Z?'*(A.`-K'/W<?45JV(!L9<@?>>LC4#LTBUV_+\XZ?2M$]69V(' 8UHI]^R"D>N/\**R6)9<MR?>BCF8K(__9 ` end sum -r/size 19201/1280 section (from first encoded line to "end") sum -r/size 55018/9924 entire input file Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Самолет NASA установил новый рекорд высоты Привет всем! Вот, свалилось из Internet... Самолет NASA установил новый рекорд высоты [NASA] Самолет NASA ER-2 установил новый мировой рекорд высоты, который теперь составляет 20,94 км, что почти вдвое выше, чем высота, на которой летает большинство авиалайнеров. Рекорд был установлен для самолетов среднего класса (стартовый вес - от 12 до 16 тонн). Рекорд был установлен на самолете ER-2 бортовой номер 806, приписанном к принадлежащей NASA базе "Эдвардс". В ходе этого полета проводились измерения различных компонентов атмосферы (воды, озона и пр.). Старый рекорд (19,05 км) был установлен в 1988 г. на канадском самолете P-42. Этот рекорд не был чем-то выдающимся для ER-2. По характеристикам этот самолет близок к известному самолету-разведчику U-2, стоящему на вооружении армии США. Он предназначен для полетов на высотах 19,8-21,3 км, просто впервые этот показатель был официально задокументирован. NASA принадлежит два самолета ER-2, которые используются в специальной научной программе. Они построены компанией Lockheed Martin и предназначаются для сбора информации об окружающей среде (динамика и химический состав атмосферы, океанические процессы, наблюдение различных атмосферных явлений). Самолет также используется для калибровки и проверки данных, передаваемых со спутников. Источник: InfoArt News Agency Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Образцы метеорных частиц из потока Леониды доставлены в лабораторию Привет всем! Вот, свалилось из Internet... Образцы метеорных частиц из потока Леониды доставлены в лабораторию [NASA] Атмосферный зонд, запущенный для наблюдения за метеорным потоком Леониды, приземлился в заросли вереска на севере штата Джорджия. О его местонахождении сообщил сигнал установленной на нем системы глобального позиционирования. Зонд был найден и установленное на нем оборудование (снимок слева) доставлено в лабораторию. Hикакие приборы при приземлении не пострадали. Hа снимке справа - "кометная ловушка". Это матрица из заполненных аэрогелем ячеек. Такие матрицы были установлены на зонде в надежде поймать микрометеоритные частицы потока Леониды. Зонд поднялся на землей на высоту более 30 км (98% высоты атмосферы Земли). Подъем продолжался 1 час 54 минуты. Hа зонде кроме метеоритных ловушек была установлена цифровая камера для съемки метеорного потока (изображения передавались в реальном времени на специальный Web-сайт). В точке максимума, как и планировалось, наполненный гелием шар был проколот и вместе с прикрепленным к нему оборудованием совершил мягкую посадку на парашюте. Ловушки из аэрогеля доставлены в Лабораторию по космическим исследованиям им. Маршалла (NASA Marshall Space Sciences Lab), где они будут исследованы с помощью сканирующего электронного микроскопа на предмет обнаружения метеоритных частиц. Источник: InfoArt News Agency Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Образцы метеорных частиц ... (картинки) [1/3] Привет всем! Вот, свалилось из Internet... section 1 of 2 of file payload.jpg < uuencode 5.32 by R.E.M. > begin 644 payload.jpg M_]C_X``02D9)1@`!`0$`2`!(``#_VP!#``4#!`0$`P4$!`0%!04&!PP(!P<' M!P\+"PD,$0\2$A$/$1$3%AP7$Q0:%1$1&"$8&AT='Q\?$Q<B)"(>)!P>'Q[_ MVP!#`04%!0<&!PX("`X>%!$4'AX>'AX>'AX>'AX>'AX>'AX>'AX>'AX>'AX> M'AX>'AX>'AX>'AX>'AX>'AX>'AX>'A[_P``1"`#"`.H#`2(``A$!`Q$!_\0` M'````00#`0``````````````!@,$!0<``@@!_\0`01```@$"!0$&!`('!P,% M`0```0(#!!$`!082(3$'$R)!46$4<8&1,J$5(T)2L='P"!8D,V)RP8+A\24F M-9*BPO_$`!L!``,``P$!```````````````!`@,$!@4'_\0`-!$``@(!`P," M`P8$!P````````$"$0,$(3$%$D%182)QD08C,F*A\!,S-<$4%21R@;'Q_]H` M#`,!``(1`Q$`/P#GF5]XVW/'N.1_5\:1ON4,I%CZC&^PN?"`!?U_+'K$KMLH M)!!ZXLDT)`1B+7-[<<?ECU=P(4N3ZGJ/KC96O&3XA?KR><:->S#AA\^#@!&? 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    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Образцы метеорных частиц ... (картинки) [2/3] Привет всем! Вот, свалилось из Internet... section 2 of 2 of file payload.jpg < uuencode 5.32 by R.E.M. > MHXX,FI!0S]V$C4+W?X.!8<8J>NU#F>7.E-24D=545/"PR*&C86/B:_ISTQ'Y M?KG.]-YQ/1EUJ:5''ZEC^&X!(4^0!/VP5L+<OG(>V7+M,Y]49%J*"6((5M4Q M^)>1?D=1BSX]3Y+J2@5Z#,8IJ4IO+J_7T&.(]7YY%GV?2YG3J\8EC4%&M<,! 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    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Образцы метеорных частиц ... (картинки) [3/3] Привет всем! Вот, свалилось из Internet... section 1 of 1 of file aerogel.jpg < uuencode 5.32 by R.E.M. > begin 644 aerogel.jpg M_]C_X``02D9)1@`!`0$`2`!(``#_VP!#``4#!`0$`P4$!`0%!04&!PP(!P<' M!P\+"PD,$0\2$A$/$1$3%AP7$Q0:%1$1&"$8&AT='Q\?$Q<B)"(>)!P>'Q[_ MVP!#`04%!0<&!PX("`X>%!$4'AX>'AX>'AX>'AX>'AX>'AX>'AX>'AX>'AX> M'AX>'AX>'AX>'AX>'AX>'AX>'AX>'A[_P``1"`!L`)`#`2(``A$!`Q$!_\0` M'0```04!`0$!````````````!0(#!`8'"``!"?_$`#H0``$#`@4!!@0$!0,% M``````$"`P0%$0`&$B$Q00<3(E%A<10C,H$50I&A"#-28O"QT>$6)$.BP?_$ M`!H!``,!`0$!``````````````(#!`$%``;_Q``I$0`"`@$$`@$#!`,````` M```!`@`1`P02(3$B01,44;%A<<'P!22!_]H`#`,!``(1`Q$`/P#CS'U(N<?. 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    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Проблемы с Deep Space 1 продолжаются Привет всем! Вот, свалилось из Internet... Проблемы с Deep Space 1 продолжаются [SpaceViews] Экспериментальный космический корабль Deep Space 1 (DS1) с момента своего запуска 24 октября 1998 г. столкнулся уже со множеством проблем. 10 ноября через 4,5 минуты после включения прекратил работу ионный двигатель. Через неделю 17 ноября проводились испытания астрономической навигационной системы AutoNav, во время который корабль повернулся таким образом, что Солнце ушло из зоны видимости системы слежения за ним. Хотя инженеры полагают, что такая ситуация является штатной, тем не менее специальное ПО для защиты от сбоев прекратило испытания навигационной системы и корабль был переведен в безопасный режим в ожидании команд с Земли. Hа следующий день группе управления полетом DS1 удалось вернуть корабль в нормальное положение. Hесмотря на проблемы с ориентировкой было объявлено, что навигационная система AutoNav работает отлично. Теперь в центре управления полетом планируют на этой неделе внось попытаться запустить ионный двигатель. Инженеры провели тщательный анализ полученных в результате первого запуска данных и смоделировали возможные причины отказа. Уже проведено тестирование новой программы управления двигателем. Источник: InfoArt News Agency Hа сегодня все, пока! =SANA=
    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: Проблемы с Deep Space 1 продолжаются (картинка) Привет всем! Вот, свалилось из Internet... section 1 of 1 of file ds1.jpg < uuencode 5.32 by R.E.M. > begin 644 ds1.jpg M_]C_X``02D9)1@`!`0```0`!``#_VP!#``<%!@8&!0<&!@8("`<)"Q(,"PH* M"Q<0$0T2&Q<<'!H7&AD=(2HD'1\H(!D:)3(E*"PM+S`O'2,T.#0N-RHN+R[_ MVP!#`0@("`L*"Q8,#!8N'AH>+BXN+BXN+BXN+BXN+BXN+BXN+BXN+BXN+BXN M+BXN+BXN+BXN+BXN+BXN+BXN+BXN+B[_P``1"`"=`,@#`2(``A$!`Q$!_\0` M'P```04!`0$!`0$```````````$"`P0%!@<("0H+_\0`M1```@$#`P($`P4% M!`0```%]`0(#``01!1(A,4$&$U%A!R)Q%#*!D:$((T*QP152T?`D,V)R@@D* M%A<8&1HE)B<H*2HT-38W.#DZ0T1%1D=(24I35%565UA96F-D969G:&EJ<W1U M=G=X>7J#A(6&AXB)BI*3E)66EYB9FJ*CI*6FIZBIJK*SM+6VM[BYNL+#Q,7& MQ\C)RM+3U-76U]C9VN'BX^3EYN?HZ>KQ\O/T]?;W^/GZ_\0`'P$``P$!`0$! 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    Дата: 26 ноября 1998 (1998-11-26) От: Alexander Bondugin Тема: NASA Awards Precollege And Teacher And Curriculum Enhancements Grants Привет всем! Вот, свалилось из Internet... Sonja Alexander November 23, 1998 Headquarters, Washington, DC (Phone: 202/358-1761) RELEASE: 98-211 NASA AWARDS PRECOLLEGE AND TEACHER AND CURRICULUM ENHANCEMENT GRANTS The NASA Office of Equal Opportunity Programs has selected 11 minority universities to receive a Precollege Awards for Excellence in Mathematics, Science, Engineering, and Technology (PACE/MSET) grant, and nine minority universities to receive a Minority University Mathematics, Science and Technology Awards for Teacher and Curriculum Enhancement Program (MASTAP) grant. The PACE grants provide opportunities for minority colleges and universities, in collaboration with NASA and local school districts, to provide for informal educational opportunities that will enhance the numbers and percentage of students enrolled in mathematics and science college preparatory courses. These partnerships will prepare more students to enroll in college mathematics, science, engineering and technology (MSET) disciplines and to pursue MSET careers in the future. Each PACE/MSET university will receive up to $100,000 per year for the three years of the grant based on performance and availability of funds under the program. The 11 universities selected to receive PACE grants: California State University- Dominguez Hills California State University- Northridge College of Santa Fe, NM Delaware State University Jarvis Christian College, TX Lehman College, NY New Mexico State University Pasadena City College, CA Trenholm State Technical College, AL Tuskegee University, AL University of Texas at Brownsville The MASTAP grants provide opportunities for minority colleges and universities to develop diverse and exemplary research-based mathematics, science, technology and geography teacher education curricula, integrated with content from NASA's mission. It is the Agency's desire that the results from these awards serve as models for other colleges and universities. Additionally, these awards will contribute to the following states' efforts to increase the numbers and percentage of state-certified mathematics, science, technology or geography teachers employed in hard-to-staff elementary, middle and secondary schools. Each MASTAP grant award recipient will receive up to $200,000 per year for the three years of the grant based on performance and availability of funds under the program. The nine universities selected to receive MASTAP grants: Bowie State University, MD California State University-Dominguez Hills City University of New York-Medgar Evers College Florida International University Heritage College, WA Jackson State University, MS Mississippi Valley State University South Carolina State University Xavier University of Louisiana -end- Hа сегодня все, пока! =SANA=

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