NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

... part 1 | ... The Basic Stages in Earth's Pre-geological Development . ... After fragments of the Vortex sleeves separated, whirlwinds of second and third orders ("NC" - new micro-vortex) were generated- future planet cores and their satellites - all of them developing independently, governed by the common laws of development of cosmogenic vortexes. ... Our planet's core today is comprised of considerably deteriorated cosmogenic vortex; consequently, the Earth has a moderated magnetic field. ...

Электронная библиотека астронома-любителя. ... Июль 1998 . ... Дата: 20 июля 1998 (1998-07-20) От: Alexander Bondugin Тема: Sky Telescope News Bulletin - July 17, 1998 Привет всем! ... SKY TELESCOPE'S NEWS BULLETIN JULY 17, 1998 CLOSE-UPS OF GANYMEDE On July 15th, the Jet Propulsion Laboratory released a bevy of new images of Jupiter's largest moon Ganymede taken by the Galileo spacecraft. ... Дата: 20 июля 1998 (1998-07-20) От: Alexander Bondugin Тема: Galileo - Countdown To Europa Привет всем! ...

Preliminary results of astroclimate parameters measurements at the Sternberg 2.5m telescope installation site V.Kornilov, N.Shatsky, S.Potanin, O.Voziakova, B.Safonov Moscow, 2008 Acknowledgements A.Belinskiy M.Kornilov A.Tokovinin M.Kuznetsov P.Kortunov E.Gorbovskoy SAI administration some SAI students Pulkovo solar station (KHSS) staff RFBR support MAVEG Gmbh Why to study optical turbulence and some other relevant ... Mean seeing by DIMM data for this night is 1''5. ...

... Phyllosilicates may form in EKB bodies during aqueous alteration [7]. ... The time m required to heat a large EKB body to the water - ice melting point and to melt the ice in its interiors can be estimated from the equation 0 Q exp(-t )dt = Tm T0 c p dT + L f m w , (1) where T0 = 30 K is the adopted value for the initial temperature of the body , Tm = 273 K is the melting temperature of water ice (a good approximation to at P 25 MPa, characteristic for interiors of a EKB ...

... Membership . ... The name of this organization shall be Amateur Astronomers Association of Princeton, Incorporated (hereinafter abbreviated as AAAP). ... General membership shall be open to any person paying dues with the proviso that any member under the age of 18 must be accompanied by a responsible adult while at any AAAP meeting, other function, or observatory. ... A. Director The Director shall preside at all meetings of the Board of Trustees and at all general membership meetings. ...

... The words are numbered according to the reference mentioned above. ... 59 WORD wSecond ; // 0 .. 59 satellite tracking start time (GMT) float fStep ; // reserved WORD wMass ; // reserved BYTE reserved [12] ; // reserved WORD wExtraBytes ; // reserved } TRAJECTORYHEADER ; NOTE: the satellite tracking start time is a hardware operating start time to follow satellite. typedef struct { // ephemeris at satellite tracking start time double time ; // Epoch time (yyddd.ddddddddd)...

RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Radio telescope 's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases Publication SSRT - Siberian Solar Radio Telescope . ...

... Printed in the U.S.A. LENTICULAR GALAXY IC 719 : CURRENT BUILDING OF THE COUNTERROTATING LARGE-SCALE STELLAR DISK Sternberg Astronomical Institute, M. V. Lomonosov Moscow State University, Moscow 119992, Russia; katkov.ivan@gmail.com, olga@sai ... In this gas-rich S0 galaxy, its large-scale gaseous disk counterrotates the global stellar disk. Moreover, in the IC 719 disk, we have detected a secondary stellar component corotating the ionized gas. ... Figure 7. ...

... 000, 1­13 (2010) Printed 21 September 2011 A (MN L TEX style file v2.2) A universal ultraviolet-optical colour­colour­magnitude relation of galaxies I1gor V. Chilingarian1,2, and Ivan Yu. ... Received 2011 Sep 15; in original form 2011 Feb 6 ABSTRACT The bimodal galaxy distribution in the optical colour­magnitude diagram (CMD) comprises a narrow "red sequence" populated mostly by early-type galaxies and a broad "blue cloud" dominated by star-forming systems. ...

Previous Editions of the M111: . ... New Website Feature - NSN "Request A Program" . ... Sunglasses For A Solar Observatory . ... On Line"! ... Back to top.. ... Our newer members quickly learn to use the big scope and those just learning astronomy learn quickly! ... If you're a member of the public at large and interested in having the Observatory provide you with an educational program, you can now easily request one by visiting the NASA NightSky Network site and simply enter it in. ... Programs . ...

Journal of the Amateur Astrono mers Association of New York October 2011 Volume 59 Number 10 ISSN 0146 -7662 EYEPIECE Earth, Juno will be the first solar power ed spacecraft to operate this far from the Sun. ... With Jupiter receiving 25 times less sunlight than the EYEPIECE October 2011 What's Up In The Sky AAA Observer's Guide for October 2011 By Richard Rosenberg October's Evening Planets. ... In early October it sets only a half hour after the Sun. ... October 12, 13 ­ The Moon passes Jupiter. ...

... Миссия "Cassini - Huygens" (NASA и ESA) . ... Хронология за 2004-2006 года . ... Close (altitude = 2,100 km; 1,300 mi) of moon . ... Distant (altitude = 68,000 km; 42,000 mi) of moon . ... Cassini passage through plane [South to North] (160,000 km; 100,000 mi wrt ) . ... Closest distance (78,000 km; 49,000 mi) to on rev number 0 . ... Distant (altitude = 107,000 km; 67,000 mi) of moon . ... 01/03/2005 . ... Closest distance (211,000 km; 131,000 mi) to on rev number 3 . ... Start rev number 3. ...

... 4 .D.Dolgov (INFN, Ferrara, Italy) STOCHASTIC BACKGROUND GRAVITATIONAL WAVES FORM PRIMORDIAL BLACK HOLES OF G.Tsarevsky (PRAO ASC LPI) PROJECT "RADIOASTRON" AND THE FUTURE OF SPACE RADIOASTRONOMY V.N.Melnikov (VNIIMS, Moscow) SCALAR FIELDS AND MULTIDIMENSIONAL MODELS IN GRAVITY AND COSMOLOGY Wednesday, 24.08.2011 Cosmology, Gravitation and High Energy Physics Conference hall "Sovinyon" 09.00 ? ... 8 Section 2. Astrophysics University Recreation Centre "Chernomorka" (2 ) Tuesday, 23.08.2011 14.30 ? ...

2 June 2006 2007-2009 Work Plan v1 2007-2009 WORK PLAN: TOWARD CONVERGENCE DRAFT 1 for Technical Review COVER NOTE The following is the first version for a three-year plan for GEO, 2007 to 2009. ... Page 1 of 38 2 June 2006 2007-2009 Work Plan v1 ACRONYMS ADM AMDAR AMMA APAN AVHRR CBD CEOS CERN DAPHNE DEM EC EPA EPIDEMIO FAPAR FDSN GEANT GEO GEOSS GIS GMES GOFC-GOLD GOS GPM GSN IGCO IGDDS InSAR INSPIRE IPY ITU MODIS NASA NGO NIEHS SAR SBA SPOT -VGT SST THORPEX UN UNFCCC COP ... Task No. ...