... Alien Life . ... Earth Satellites . ... Often travelling on holidays you can change your watch to the time at your destination by winding your watch forward or backwards. ... When astronauts travel they use Earth time, i.e. one day/ 24 hours, to help them whilst living in the Space Station. ... A day on Mars is only 39mins longer than here on Earth maybe it could useful when travelling on Mars to adopt Martian time and maybe have an extra 39mins to have a lie-in, or bond with the locals? ...

... The UNIVERSAT-2009 Symposium (28 September - 1 October 2009) will cover a wide variety of topics centered around the theme "University satellites in space sciences education", and is meant to inform the entire university and space-interested community on the new initiatives and university satellites projects in space sciences and technology education. ... I. Space Sciences Education: . ... Hands-On Space Exercises, . ... Cooperation Ideas in Space Sciences Education and Public Outreach. ...

tranback -- Transform an X,Y position from output to input pixel position using the same conventions as drizzle tranback xout yout . xout = 400 [real] . ... The X dimension of the input image (this is used to determine the centre which is the origin of the transformations). (nyin = 800) [real] . ... If "output" the input image center is mapped to the center of the output grid, rotated about that center and then shifted along the grid of the output image. ...

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Brief History of Rocket and Space Technology . ... Experiments and Researches from 2013 . Experiments and Researches (2000-2013) . Rocket Space Complexes . ... Images . ... Automatic Space Systems . Universal Space Platform . ... Crew 43/44 . ... Experiments Program . ISS-43 Images . ... Sixteenth Russian Visiting Crew . ... Support of the Station functionality; . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

As a result of preceding actions the File opening dialog box appears and user is suggested to open the file with observations (the file may be created for the first time). ... To see the list of files with desirable extension in chosen folder define the type of extension with the help of File type drop-down list at the bottom of the dialog box. ... The name of the file will appear in File name dialog box. ... In case you want to open the file with new name, type it in the File name dialog box. ...

Hourly values of parameter foF2 (F2 layer critical frequency) The description of letters in the tables of parameter foF2 A blanketing. ... C non-ionospheric (equipment). D above upper frequency range of equipment. E below lower frequency range of equipment. F frequency spread. ... K particle E layer. L no sufficiently defined cusp between F layers. ... N superimposed layers. O measurement refers to o component. ... Q range spread. R attenuation near critical frequency. ...

... Астрономия для всех (Модераторы: Deimos , AAV ) ? Нулевой меридиан . ... Сообщений: 164 . ... Скажите пожалуйста, как определяется нулевой меридиан для Луны, планет (в особенности, Марса) и их спутников? ... Записан . ... Они выбрали маленький круг (кратер) как точка справки когда они произвесли первую систематическую карту черт Марса в 1830-32 г. Нулевой меридиан Луны находится прямо в середине стороне Луны видна с Земли. ... Вот, нашел немножко на http://en.wikipedia.org/wiki/Prime_meridian . ...

... The VSOP Survey Continuum Source List . The radio sample for the VSOP continuum survey was defined to include all extragalactic radio sources with: . a total flux density at 5 GHz, S>=1.0 Jy . ... The sample also included all sources in the sky with a 5 GHz flux density S>5 Jy, regardless of spectral index and galactic latitude. ... The source would then be included in the VSOP sample (three of the sources were found with a flux density above 1 Jy and added to the sample). ...

Report “Laboratory zero-baseline interferometer tests” (ZBT) was prepared and issued in ASC (35 pages including 17 figures and diagrams in Russian language). ... The Ground-Space radio interferometer (OVLBI) Radioastron includes several space and ground-based segments which are designed and manufactured by different countries and organizations. ... ZBI tests (for OVLBI) were implemented in Russia firstly. The tests were implemented by joint team of ASC, JPL and NRAO in 1999. ...

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05/10/2007 1:01 PM . ... Original: 1936x1296 (418k) . ... Thumbnail: 200x134 (68k) . Flash: Flash fired, auto mode, return light detected . Exposure time: 10/2000s . Focal length: 18.0mm . Aperture: f/8 . ... Original: 1936x1296 (314k) . ... Thumbnail: 200x134 (69k) . Flash: Flash did not fire . Exposure time: 10/1600s . ... Original: 1936x1296 (388k) . ... Flash: Flash did not fire, auto mode . ... Focal length: 7.9mm . ... Focal length: 13.7mm . ... Focal length: 6.3mm . ...

... The changes are important to us, since they affect our time reckoning, our climate, and our understanding of the Earth's past. ... The Invariable Plane . ... The current location of the celestial north pole, the ecliptic north pole, and the north pole of the invariable plane in the northern sky. ... The north pole of the invariable plane lies in Draco, its south pole in Mensa. ... The precession of the celestial north pole, viewed from above the north pole and against the background of northern...

... Meade Instruments Corporation . ... How to Calculate Power . How to Calculate Power: The magnification, or power, at which a telescope is operating is a function of the focal length of the telescope's main (objective) lens (or primary mirror) and the focal length of the eyepiece employed. ... Example: The Meade DS-2070AT telescope has an objective lens focal length of 700mm; when this telescope is used with a 25mm eyepiece, a power of 700/25 = 28 power (written as "28x") results. ... about meade | ...

... GA89 GK89 weight 1 H 1.008 0.911 2 He 4.003 0.089 3 Li 6.939 -10.88 -10.98 4 Be 9.013 -10.89 -10.89 5 B 10.81 - 9.44 6 C 12.01 -3.48 -8.39 7 N 14.01 -3.99 -4.09 8 O 16.00 -3.11 -3.14 9 F 19.00 -7.48 10 Ne 20.18 -3.95 11 Na 22.99 -5.71 -5.72 12 Mg ... -7.44 31 Ga 69.72 -9.16 32 Ge 72.60 -8.63 33 As 74.92 -9.67 34 Se 78.96 -8.69 35 Br 79.91 -9.41 36 Kr 83.80 -8.81 37 Rb 85.48 - 9.44 - 9.44 38 Sr 87.63 -9.14 -9.14 39 Y 88.91 - 9.80 - 9.80 40 Zr 91.22 - ...

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