... Space flight . ... Space Hotel . ... The program of deployment of small orbital station (SOS) consisting of a family of spacecrafts and module-spacecrafts represents a consecutive realization of flight scenarios with consecutive building up of functions. ... Scenario 1 - the regular and revised spacecrafts of class "Soyuz" - TMSC and MNMSC (MNMSC-cargo, MNMSC-MR) are used, pls. see fig fig.8 . ... The terms of transition to this scenario are determined by terms of readiness of one or another module....

The Star called the Sun. The Sun as the star . ... The visible star value . ... Spectrum class . ... 149 597 870 km . ... The Solar energy sourse is the core transformation of the Sun, where temperature is 15 000 000 K. The energy from inside is carried by irradiation and then in the external layer with 0,2 Ra of thikness - by convection. ... The Earth, situating far from the Sun (149 mil km), receives about 2.1017 W of the Solar beam energy (see item "The Solar constant" ). ...

Kent, Great Britain . ... school. ... We go to Derwent Lodge School, private . school for girls. ... We go to Derwent Lodge, Sommerhill a private school ( where our parents pay). ... We have to get to school by 8:30 and school ends at 4:30, Yippee at last; . ... Our school is called Derwent Lodge; it is in a group of schools called . ... Our school is called The Schools at . ... Our names are Alex and Oona we go to a school called Derwent Lodge. ... Hello, we go to Derwent Lodge School for girls. ...

Observational Stellar Astronomy . Articles | ... We are made of star stuff" . ... TEMPERATURE OF A STAR: . ... The temperature of a star can be found out easily by simple observations. ... STAR . ... SPECTRAL CLASS: . All the stars in this universe are divided in to spectral classes based on their spectral lines. ... The spectral class of a star and the temperature of a star are related. So the spectral class can be found for a star since we know its temperature. ... www.astronomy.net . ...

... Tabs . ... 90% -contents change but tab appearance is constant . ... HTML for the tabs div, tabs, and contents (see HTML tab) . ... div id="tabs"> <span id="tab1" class="tab tabActive" >Overview</span> <span id="tab2" class="tab" >The CSS</span> <span id="tab3" class="tab" >Event Object</span> </div> . div id="tabs"> <img id="tab1" class="tab tabActive" src="img/discography.gif" hoversrc="img/discographyo.gif" activesrc="img/discographya.gif" width="135" height="28" alt="discography" /> </div> . ...

... NOTE: If event is correlated to an optical flare in data prior to 1997, the event times are for the optical event. ... 28 1X 29 A1 N or S for north or south latitude of correlated optical flare, if known. ... 32 A1 E or W for east or west central meridian distance of correlated optical flare, if known. 33-34 I2 Central meridian distance of correlated optical flare, if known. ... 37-59 33X 60 A1 X-ray class: C,M,X code the maximum power of 10 the 1-8 Angstrom flux attains.* ...

... Therefore, the observatory supports educational events, occured in the SAO, including astronomical and astrophysical schools, lectures and excursions at the SAO's telescopes. ... Thursday 9-00 Breakfast 9-30 Opening of the School and Astronomical Olimpiad 10-15 Photo of particapants (near the SAO entrance) 10-30 Lecture about Specail Astrophysical observatory. Chentsov E.L. 13-30 Lunch 14-00 Excursion to historical places of Nizhnij Arkhyz 18-00 Dinner 19-00 Acquaintance evening. ...

. animdown.class . animleft.class . animright.class . animup.class . Сохранить страницу. Загрузить по ссылкам апплеты в ту же директорию где и страница. Туда же переместить и изображения из папки, в которую ори сохранились при сохранении страницы. Изображения можно менять. Из этого набора можно сделать что ни будь интересное! . eye.class .