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... This accuracy allows HARPS to detect planets with masses slightly greater than the Earth. Among the 50 new HARPS planet discoveries announced in September, the one that garnered the most attention orbits the star HD 85512 (aka Gliese 370), 36 light-years awa y in the southern constellation Vela. The planet, given the prosaic designation HD 85512 b, has a mass of about 3.6 times that of Earth and orbits its star, an orange K-type dwarf, in 59 days. ... Happy People Dancing on Planet Earth." ...

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• Astro Imaging Workshop: Deep Sky Astro Imaging with a DSLR ? September 14, 2014

Copyright ї 1994 by Maxim V. Tarasenko. ... The end of confrontation, associated with the Cold War, led to political feasibility and economic desirability of extended international cooperation in space. ... For example, during the first half of 1994 the Russian Space Agency got only 10 per cent of its annual request. ... Another aspect of an inter-FSU cooperation is what was supposed to be a joint use of results from space activity, both in terms of scientific research and space applications. ...

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• RUSSIAN MILITARY SPACE

Tuesday, September 28th, 2010 . 14-17 сентября 2010 года прошла международная конференция WEGENER (http://www NULL .koeri NULL .boun NULL .edu NULL .tr/jeodezi/wegener2010/) (Bogazici University, Istanbul / TURKEY), в которой мы приняли участие и сделали два доклада: . ... You are currently browsing the Лаборатория лазерной интерферометрии blog archives for September, 2010. ... Публикации за 2011 . Публикации за 2012 . ... Лаборатория лазерной интерферометрии is proudly powered by WordPress . ...

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• September 2013 Лаборатория лазерной интерферометрии

... Skalnatґ Pleso 43, 1 ­ 2, (2014) e Mini-MegaTORTORA ­ multichannel system for wide-field optical monitoring with high temp oral resolution V. Sasyuk1 , G. Beskin2 , S. Karp ov2 , S. Bondar3 , A. Perkov3 , E. Ivanov3 , E. Katkova3 and A. Shearer4 2 Kazan Federal University, Russia Special Astrophysical Observatory of Russian Academy of Sciences, Russia 3 Insttitute for Precise Instrumentation, Russia 4 National University of Ireland, Galway, Ireland Received: November 4, 2013; Accepted: ?? ...

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• SAI CAS: About the SAI CAS project
• SAI CAS:
• astro-ph

... Recherche dans le site : . Ciel Espace, le magazine qui vous guide toujours plus loin . ... des actualit†йs . ... des pages consacr†йes †а la publication de vos photos Mais c'est aussi une vraie communaut†й avec laquelle partager votre passion et nourrir votre curiosit†й. Accueil NGC 6872, galaxie tentaculaire . ... Cette interaction a notamment engendr†й une flamb†йe de naissances d'†йtoiles dans les bras de NGC 6872, mais aussi une galaxie dite €л de mar†йe €Ё (entour†йe sur l'image). ...

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• Cinq zones dв?Tatterrissages choisies sur la comГЕte Churyumov-Gerasimenko |
• Un Fran–?ais choisi pour Mars 500 | Ciel et Espace
• Instruments | Ciel et Espace

... GCR and SCR are primary cosmic rays. 10-15 years after the discovery of cosmic radiation (1919) there emerged two main avenues of investigation in the physics of cosmic rays (CR): 1) nuclear - elucidation of the origin of elementary particles and nuclear interactions; and 2) astrophysical (space physics) - solution of the problem related to the origin and variations (changes in intensity) of CR. ... Besides, the CR flux in interplanetary space is, strictly speaking, not isotropic. ...

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... It is reasonable to expect that UV part of the irradiating spectrum is most influenced by the grain evolution (growth and sedimentation ) which marks the very initial stage of planet formation. 2 log J [erg s­1 cm­2] 1 0 -1 -2 -3 1000 BB 40 0 0 (A5 ) BB 20 0 00 (A5) Drai ne (A5 ) BP Ta u (A5) BB 40 0 0 (GS) BB 20 0 00 (GS) Drai ne (GS) BP Ta u (GS) Disk Model Density distribution is based on a 1+1D disk ... Green lines are used for a model with dust growth and sedimentation. ...

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• http://www.inasan.rssi.ru/~okochina/

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

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• VISTA ETC - Exposure Time Calculator

... March 13 2001 09:00 (Moscow time) . The operation with OC "Mir" scheduled for March 12 is complete. During the previous day apart from routine OC "Mir" onboard systems checkout and orbit parametres monitoring, command software was uploaded into MCS Central Onboard computer. The MCS is in free drift. The received telemetry data was used to assess the onboard systems performance, thermal and humidity condition and complex pressure integrity. ... The complex remains in free drift. ...

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• Обеспечение управляемого спуска с орбиты орбитального пилотируемого комплекса
• Информация для прессы

DISCLAIMER: The larger the aperture, the more light a telescope will gather and the fainter the object you can see. Here is a range of magnitudes you might expect to see. Given excellent sky conditions and good optics, a well trained eye can sometimes add up to 0.8 magnitude to these values. Limiting Magnitude depends on much more than the instruments aperture. ... One formula is for aperture in inches the other is for aperture in millimeters. ... Aperture (inches) . ... 15.2 . ...

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• The Richland Astronomical Society
• The M111 - "On Line"
• A brief tour page 10

... Our tours this year include: Yuri Gagarin Cosmonaut Training Center at Star City, Bauman Moscow State Technical University Orevo Laboratory, Russian Mission Control Center (TsUP), Rocket and Space Corporation Energia, Lavochkin Scientific and Industrial Association, Energomash Scientific and Industrial Association, Scientific and Industrial Association "Zvezda", Khrunichev State Research & Production Space Center, Monino Air Force Museum. Bauman Moscow State Technical University . Moscow) . ...

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Due to technical issues, on September 11, 1998 the radiolink was switched to 465 MHz channel. Data acquisition is presently performed only by SRC "PLANETA", Data Receiving Center in Obninsk and Western Siberia Data Receiving Center in Nobosibirsk . For conditions of obtaining data from RESURS-01 N3 please contact SRC "PLANETA". ... Registration of full data stream (61.44 Mbit/s) is performed only by Data Receiving Center, SRC "PLANETA", Obninsk. ...

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... VaST is a software tool for finding variable objects on a series of astronomical images. ... VaST performs object detection and aperture photometry using SExtractor on each image, cross-matches lists of detected stars, performs magnitude calibration with respect to the first (reference) image and constructs a lightcurve for each object. ... VaST FITS image viewer ./pgfv . ... Part I" PZP, vol. ... K. V. Sokolovsky, S. A. Korotkiy; "New Variable Stars Discovered by the NMW Survey" PZP, vol. ...

95. http://www.simfov.ru/catalogs/ucac2/readme.txt

96. Nove in M32, 1998

97. East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary

98. http://www.astro-soc.odessa.ua/Public-2010.pdf

99. Туфли для девочки. 93047-2 - Kapika - Kapika 93047-2 Банкетка DG-Home

100. radioteleske