... В теме В разделе По форуму . ... Вселенная, жизнь, разум (Модераторы: ivanij , AlexAV , Nucleosome ) ? Ссылки на новости по тематике раздела "Вселенная, Жизнь, Разум" . ... несколько вольная редакция моей недавней статьи Past -- Present -- Future , где у меня ни слова не было о том, что добавлено в НГ в начало -- про Optical SETI.. ... Обновления на сайте SETI League, . ... Cogan Station, PA, United States . ... Dr. Seth Shostak, The SETI Institute, Mountain View, CA, United States . ...

... Capability of space means for the solution of problems of military character . ... Classification and functions of space systems of military purpose(assignment) . ... Ground complex of maintenance of launch and control of space vehicles . ... Capability of space systems of optical reconnaissance . ... Complexes topographical and earthresource shooting on base of "Zenit" space vehicle . ... Space vehicle for optical-electronic reconnaissance . ... System with space vehicle on low-altitude orbits . ...

... Количество полетов - 4 . Продолжительность полетов - 230 суток 13 часов 7 минут 6 секунд. ... С 1979 года служит в ВВС США. ... Космическая подготовка: . ... 16.09.1993 года - продолжительностью 7 часов 5 минут; . Продолжительность полета составила 9 суток 20 часов 11 минут 56 секунд. ... Продолжительность полета составила 10 суток 3 часа 19 минут 45 секунд. 17 ноября 1997 года был назначен членом дублирующего экипажа МКС-2 и основного экипажа МКС-4 вместе с Ю.Онуфриенко и Д.Бершем. ...

... Under certain conditions, like those in the nucleus of a QSO, all atoms can be made to emit light at particular wavelengths. ... If that source is approaching the observer, the wave is squashed up onto itself making the wavelength shorter. ... This is redshift. ... You can see how the section of the QSO spectrum which we observe changes with redshift. ... We then see how far we had to slide the observed spectrum along the scale to make it match and that is the objects redshift. ... The 2QZ team . ...

... 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 . ...

... GRIN lenses for telecommunication optics applications ? GTC (gradient telecom) lenses. ... GTC lenses are used in different fiber-optic devices: collimators, couplers, isolators and WDM etc . ... 2.Diameter . GTC lenses diameters are 1.0 mm, 1.8 mm, 3.0 mm and 4.0mm. ... 1.0 mm -3.0 mm diam GTC lenses are supplied in 0.22P, 0.23P, 0.25P, 0.27P and 0.29P length. 4.0 mm diam GTC lenses are supplied in 0.11P length. ... GTC . ... 3 scratches with 5mkm max width and 200mkm max length are allowed . ...

... ROSAT ? германская космическая рентгеновская обсерватория. ... На борту спутника находился созданный в Германии рентгеновский телескоп с возможностью получения изображений, в фокальной плоскости которого находилось 3 прибора: два германских позиционно-чувствительных пропорциональных счетчика и американский прибор получения высококачественных изображений. ... 1М (космический аппарат) . ... 2МВ (космический аппарат) . 3МВ (космический аппарат) . ... Союз (космический корабль) . Союз 7К-Л1 . ...

... The spectrum of the brightest star, our Sun, shows several dark gaps perpendicular to the flow of it’s colours (figure 1). These so called spectral absorption lines where discovered in 1802 by the English scientist William Wollaston. ... Some stars as Pollux show a spectrum similar to that of our sun with strong Ca II and Fe II lines, others as Sirius or Vega show strong absorption lines of hydrogen, others, as Mira show very complicated spectra due to molecular absorption lines (see figure 5). ...

... 000, 1­12 (2009) Printed 11 February 2010 A (MN L TEX style file v2.2) Analytical approximations of K -corrections in optical and near-infrared bands I1gor V. Chilingarian1 2 ,2,3 , Anne-Laure Melchior 1,4 and Ivan Yu. ... Received 2010 February 01; in original form 2009 August 14 ABSTRACT To compare photometric properties of galaxies at different redshifts, the fluxes need to be corrected for the changes of effective rest-frame wavelengths of filter bandpasses, called K -corrections. ... Table 1. ...

... 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. ...

... Страна-разработчик МКА Китай2. Назначение МКА Исследование магнитосферы Земли3. Количество МКА в системе 24. Год запуска МКА Декабрь 2002 г. и апрель 2003 г.6. Баллистические характеристики МКА МКА DSP-E, будет выведен на близкую к экваториальной орбиту с наклонением 28,5њ и высотой 550 км ? ... МКА DSP-P, будет работать на полярной орбите с наклонением 90њ, высотой 350 км ? ... Средство выведения МКА Китайские РН класса 'Великий поход'9. Масса МКА 270 кг13. ...

... RI , : Stelmacher-Wiehr 1975, SW75 = 30 , cos = 1.0, EWan - der -Waals = 2.0 t = 0.0 / H 1000 3000 500 . ... W = kH + b H = K W + B , 25% VMa (Gs) cro = 2km / s H = 44.60 * (W6127 - W6134 ) + 656 H = 60.75 * (W6143 - W6134 ) + 869 H = 167.8 * (W6127 - W6143 ) + 67 VMa cro = 2km / s - H = 45.17 * (W6127 - W6134 ) + 502 H = 61.20 * (W6143 - W6134 ) + 680 H = 172.41* (W6127 - W6143 ) , H = 49.07 * (W6127 - W6134 ) H = 67.93 * (W6143 - W6134 ) H = 176.68 * (W6127 - W6143 ) 15.05.2009 10 . Vmi = 0.0 /. ...

... 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. ...