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6741. Epimetheus
E pimetheus ( "ep eh MEE thee us" ) is the fifth of Saturn 's known satellites: orbit : 151,422 km from Saturn diameter : 115 km (144 x 108 x 98) mass : 5.6e17 kg E pimetheus was the son of Iapetus and brother of Prometheus and Atlas; husband of Pandora. Epimetheus" is Greek for "hindsight". ... But the situation was confused since Janus is in a very similar orbit. ... E pimetheus and Janus are " co-orbital ". ... Little is known about Epimetheus. ... Saturn .. Pandora .. ... Janus .. ...
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Ссылки http://www.iki.rssi.ru/nineplanets/epimetheus.html -- 3.6 Кб -- 18.03.1998
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6742. Deimos
... It is the smallest known moon in the solar system. orbit : 23,459 km from Mars diameter : 12.6 km (15 x 12.2 x 11) mass : 1.8e15 kg I n Greek mythology, Deimos is one of the sons of Ares (Mars) and Aphrodite (Venus); "deimos" is Greek for "panic". ... D eimos and Phobos are composed of carbon-rich rock like C-type asteroids and ice. ... D eimos and Phobos are probably asteroids perturbed by Jupiter into orbits that allowed them to be captured by Mars. more images . ... Mars .. Phobos .. ...
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Ссылки http://www.iki.rssi.ru/nineplanets/deimos.html -- 3.7 Кб -- 18.03.1998
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6743. Ariel
... A riel and Titania appear quite similar though Titania is 35% larger. All of Uranus' large moons are a mixture of about 40-50% water ice with the rest rock, a somewhat larger fraction of rock than Saturn 's large moons such as Rhea . A riel's surface is a mixture of cratered terrain and systems of interconnected valleys hundreds of kilometers long (left, above) and more than 10 km deep. This is similar to, but much larger and more extensive than the situation on Titania. ... Uranus .. ...
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Ссылки http://www.iki.rssi.ru/nineplanets/ariel.html -- 4.2 Кб -- 18.03.1998
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6744. The Origin of the Solar System
... Here is a brief outline of the current theory of the events in the early history of the solar system: . A cloud of interstellar gas and/or dust (the "solar nebula") is disturbed and collapses under its own gravity. ... The gas cools off enough for the metal, rock and (far enough from the forming star) ice to condense out into tiny particles. (i.e. some of the gas turns back into dust). ... Once the larger of these particles get big enough to have a nontrivial gravity, their growth accelerates. ...
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Ссылки http://www.iki.rssi.ru/nineplanets/origin.html -- 6.2 Кб -- 18.03.1998
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6745. Titania
T itania ("ti TAY nee uh") is the fourteenth and largest of Uranus 's known satellites: orbit : 436,270 km from Uranus diameter : 1578 km mass : 3.49e21 kg T itania is the Queen of the Fairies and wife of Oberon in Shakespeare's Midsummer-Night's Dream . ... T itania and Ariel appear quite similar though Ariel is 25% smaller. All of Uranus' large moons are a mixture of about 40-50% water ice with the rest rock, a somewhat larger fraction of rock than Saturn 's large moons such as Rhea . ...
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Ссылки http://www.iki.rssi.ru/nineplanets/titania.html -- 4.1 Кб -- 16.03.1998
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6746. SL9
... Shortly after its discovery it was determined to be in a highly elliptical path near Jupiter and on a collision course. ... T he size and mass of the original body and the individual fragments is as of this writing still highly uncertain. ... B etween 16 July 1994 and 22 July 1994 the fragments impacted the upper atmosphere of Jupiter. ... T he pictures were posted to the Net within hours of the impacts and caused severe overloading on some ftp and WWW sites. ... JPL's SL9 page . ... Small Bodies .....
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Ссылки http://www.iki.rssi.ru/nineplanets/sl9.html -- 5.8 Кб -- 16.03.1998
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6747. Oberon
O beron ("OH buh ron") is the outermost of Uranus 's known satellites and second largest: orbit : 583,420 km from Uranus diameter : 1523 km mass : 3.03e21 kg O beron is the King of the Fairies and husband of Titania in Shakespeare's Midsummer-Night's Dream . ... O beron and Umbriel appear quite similar though Oberon is 35% larger. ... O beron's heavily cratered surface has probably been stable since its formation. It has far more and larger craters than do Ariel and Titania . ... from APOD . ...
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Ссылки http://www.iki.rssi.ru/nineplanets/oberon.html -- 4.2 Кб -- 16.03.1998
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6748. Saturn's Possible New Moons
... S/ 1981 S 15 174000 S/ 1981 S 16 220000 S/ 1981 S 17 231000 S/ 1981 S 18 185000 S/ 1981 S 19 186000 S/ 1995 S 1 137450 S/ 1995 S 2 139700 S/ 1995 S 3 141050 S/ 1995 S 4 146450 S/ 1995 S 5 140060 S/ 1995 S 6 139910 S/ 1995 S 7 139440 The first two groups are derived from analysis of Voyager 2 data reported in IAUC 6162 ; the third group is from HST observations during the May 1995 ring ... S/1995 S 3 orbits just outside the F ring and is apparently a shepherd moon . ... New Moons ....
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Ссылки http://www.iki.rssi.ru/nineplanets/newsats.html -- 7.2 Кб -- 16.03.1998
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6749. Nereid
N ereid ( "NEER ee ed" ) is the outermost of Neptune 's known satellites and the third largest: orbit : 5,513,400 km distance from Neptune diameter : 340 km mass : ? ... D iscovered in 1949 by Kuiper . N ereid's orbit is the most highly eccentric of any planet or satellite in the solar system; its distance from Neptune varies from 1,353,600 to 9,623,700 kilometers. N ereid's odd orbit indicates that it may be a captured asteroid or Kuiper Belt object. from LANL . ... Neptune .. ...
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Ссылки http://www.iki.rssi.ru/nineplanets/nereid.html -- 3.1 Кб -- 16.03.1998
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6750. Neptune's Small Moons
... N aiad ( "NAY ed" ) is the innermost of Neptune's known satellites: orbit : 48,200 km from Neptune diameter : 58 km mass : ? ... T halassa ("tuh LASS eh") is the second of Neptune's known satellites: orbit : 50,000 km from Neptune diameter : 80 km mass : ? ... D espina is the third of Neptune's known satellites: orbit : 52,600 km from Neptune diameter : 148 km mass : ? ... G alatea ("gal eh TEE eh") is the fourth of Neptune's known satellites: orbit : 62,000 km from Neptune diameter : 158 km mass : ...
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Ссылки http://www.iki.rssi.ru/nineplanets/nepmoons.html -- 5.7 Кб -- 16.03.1998
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6751. Larissa
L arissa ("LA ree suh") is the fifth of Neptune's known satellites: orbit : 73,600 km from Neptune diameter : 193 km (208 x 178) mass : ? L arissa was a daughter of Pelasgus. H arold Reitsma is now usually credited with the discovery of Larissa by ground-based stellar occultation observations. ... L ike Proteus, Larissa is irregular (non-spherical) in shape and appears to be heavily cratered. from LANL . We know next to nothing about Larissa.. ... Bill Arnett ; last updated: 1997 Oct 29 . ...
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Ссылки http://www.iki.rssi.ru/nineplanets/larissa.html -- 2.7 Кб -- 16.03.1998
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6752. Enceladus
E nceladus ("en SEL a dus") is the eighth of Saturn 's known satellites: orbit : 238,020 km from Saturn diameter : 498 km mass : 7.30e19 kg I n Greek mythology Enceladus was a Titan who was defeated in battle and buried under Mount Etna by Athena. ... Its surface is dominated by fresh, clean ice. ... T his means that Enceladus must have been active until very recently (and perhaps is still active today). ... This may provide a heating mechanism but it is probably insufficient to melt water ice. ...
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Ссылки http://www.iki.rssi.ru/nineplanets/enceladus.html -- 4.9 Кб -- 16.03.1998
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6753. Список научных трудов Назирова Равиля Равильевича
... Название научного труда . Печатный или рукописный . ... Препринт ИКИ АН СССР . ... рукописн. ... Закл. отчет ИКИ АН СССР, . ... ИКИ АН СССР, 1978. ... Препринт ИКИ АН СССР, Д-301, 1980. ... ИКИ АН СССР, 1981. ... экспериментальная программа оптических наблюдений спутника 'ИК-Б-1300, М.: АС АН СССР, 1982. ... Возможности повышения точности навигационной привязки научной космической информации и прогноза движения ИСЗ. рукописн. ... Труды VI научных чтений по космонавтике, . ... Отчет ИКИ АН СССР ? ...
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Ссылки http://www.iki.rssi.ru/people/rn_pub.html -- 30.5 Кб -- 12.03.1998
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6754. Albert Galeev Home Page
Albert A.Galeev is the director of the Russian Academy of Sciences Space Research Institute (IKI RAN in Russian), Moscow, Russia. ... Prior to his promotion to the present position, for fifteen years (1973-1988), A.Galeev headed the Space Plasma Physics Department and together with his scientific team contributed to a number of successful international space projects. ... Postal Address Space Research Institute (IKI) . ... e-mail agaleev@iki.rssi.ru ...
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Ссылки http://www.iki.rssi.ru/people/agaleev.html -- 6.7 Кб -- 12.03.1998
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6755. R E F E R E N C E S
... Afonin V.V., O.S.Akentieva, J.Smilauer and I.Simunek, First results of thermal plasma measurements in the Auroral probe mission (experiment KM-7), Cosmic Res ., ... V.24, N8, p.955, 1997. ... Structure of the flank magetopause for horizontal IMF: INTERBALL observations, submitted to J.Geophys. ... G.Zastenker, M.Nozdrachev, A.Skalsky and L.Zelenyi, Plasma populations in the magnetosphere during passage of magnetic cloud of 10-11 January, 1997: INTERBALL/Tail Probe observations, submitted to Geophys....
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Ссылки http://www.iki.rssi.ru/tail/results/publ.html -- 21.0 Кб -- 02.03.1998
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6756. Interball Workshop Posters
... Budnik, E., E.Dubinin, A.Fedorov, N.Pissarenko, S.Romanov, S.Savin, A.Skalsky, L.Zelenyi, I.Sandahl, U.Eklund, The structure and dynamics of the plasma flows observed at the magnetopause in the vicinity of the cusp (INTERBALL-Tail observations). Buechner, J., J.-P. Kuska, B. Nikutowski, S. Klimov, S. Romanov, S. Savin, U. Auster, K.H. Fornacon, J. Rustenbach, Reconnection signatures observed by Interball-1 in relation to auroral substorms . ... BACK to Interball workshop main page. ...
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Ссылки http://www.iki.rssi.ru/interball/posters.html -- 6.2 Кб -- 19.02.1998
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6757. Interball Workshop Programme
... The shape of energetic particles spectra in the geotail plasma sheet: Theory and INTERBALL observations 1520 Yermolaev et al: Magnetosphere response to interplanetary magnetic clouds: INTERBALL multisatellite observations 1540 Petrukovich et al: Substorm -related magnetotail pressure variations observed by INTERBALL and GEOTAIL 1600 Savin et al: The cusp/magnetosheath connection: magnetopause indentation and turbulent boundary effects 1620 Smirnov ...
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Ссылки http://www.iki.rssi.ru/interball/programme.html -- 3.1 Кб -- 19.02.1998
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6758. Latest scientific results
. VDP - instrument: Recent and the most interesting results . Event January 10-11, 1997 . List of publications 1996-1997 . Last update January 15, 1998 . HTML by Pavel Eiges
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Ссылки http://www.iki.rssi.ru/tail/results/index.html -- 1.8 Кб -- 15.01.1998
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6759. Dynamics of Pluto
From a bird's eye view of the ecliptic, it is clear that Pluto's orbit is more eccentric than any other planet's. Pluto's orbit appears to intersect Neptune's, and for a period of about 20 years Pluto is slightly closer to the sun than Neptune. ... The libration of Pluto's orbit is due to an exchange of angular momentum with Neptune. When Pluto is "catching up" to Neptune, it gains angular momentum at Neptune's expense. ...
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Ссылки http://www.iki.rssi.ru/nineplanets/plutodyn.html -- 3.2 Кб -- 11.01.1998
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6760. Paper ID No.SO96.3.3
Paper ID No.S096.3.3 . ... This campaign combined 4 missions: Geotail, Interball Tail, IMP-8 (NASA), Wind (NASA). ... The global situation picture for the TP orbit is shown in the Fig. 1 as a satellite passage time through regions of interest of the magnetosphere. ... Correlation of the situation pictures for two orbits is helpful in choosing proper time for fulfillment of coordinated measurements in conjugate regions: plasma sheet (PS) of magnetosphere tail - auroral region (AUR). ...
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Ссылки http://www.iki.rssi.ru/vprokhor/papers/ops96/3_03.htm -- 11.1 Кб -- 10.01.1998
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