http://lfvn.astronomer.ru/images/AiT.png http://www.astronomer.ru http://www.astronomer.ru/publications.php?act=view id=188 Доклады проекта ISON Tue, 01 Mar 2016 00:00:00 +0300 Доклад на 53-й сессии Научно-технического подкомитета Комитета ООН по использованию космического пространства в мирных целях - Вена, Австрия, 15-26 февраля 2016 г. http://www.astronomer.ru/publications.php?act=view id=187 Новости проекта ...
... Луне суждено было стать тем небесным телом, с которым связаны едва ли не самые эффектные и впечатляющие успехи человечества за пределами Земли. Непосредственное изучение естественного спутника нашей планеты началось со старта советской Лунной программы. 2 января 1959 года автоматическая станция 'Луна-1' впервые в истории осуществила полет к Луне, спустя 9 месяцев 'Луна-2' достигла лунной поверхности, а еще через месяц 'Луна-3' сфотографировала невидимую доселе обратную сторону нашего спутника. ...
... Р?С?С?С?Р?Р?Р?Р?РеС?Р?С?Р?РеР? ... Launched on February 17, 1996, the Near Earth Asteroid Rendezvous (NEAR) mission is to be the first of NASA's Discovery missions, a series of small-scale spacecraft designed to proceed from development to flight in under three years for a cost of less than $150 million. ... The ultimate goal of the mission is to rendezvous with and achieve orbit around the near Earth asteroid 433 Eros in February, 1999, and study the asteroid for approximately one year. ...
Главная Проекты Mars Exploration Rover . ... With far greater mobility than the 1997 Mars Pathfinder rover, these robotic explorers will be able to trek up to 100 meters (about 110 yards) across the surface in a Martian day. ... The rovers will be identical to each other, but will land at different regions of Mars. ... Where Pathfinder had scientific instruments on both the lander and the small Sojourner rover, these larger rovers will carry all their instruments with them. ...
. Authors . Problem . Method . Advises . Contact Analysis of an accuracy of CCD asteroid observations carried out by professional and amateur astronomers . An accuracy estimation of CCD asteroid observations contained in the Minor Planet Center Database and carried out in the years 1999 - 2006 is realized. About 20 millions individual positions of the Numbered and Unnumbered Minor Planets were tested by means of calculations of (O-C) residuals to derive "mean error of a single observation" for more than 400