"0"^^ . "0"^^ . . "C\u00EDlem projektu je zajistit podrobn\u00E9 astrometrick\u00E9 sledov\u00E1n\u00ED a fotometrick\u00E9 studium nov\u00FDch planetek v okol\u00ED Zem\u011B (NEAs), jejich\u017E o\u010Dek\u00E1van\u00E1 frekvence objev\u016F b\u011Bhem p\u0159\u00ED\u0161t\u00EDch t\u0159\u00ED let v d\u016Fsledku startu nov\u00FDch vyhled\u00E1vac\u00EDch program\u016F ve sv\u011Bt\u011B \u0159\u00E1dov\u011B vzroste. K \u0159e\u0161en\u00ED projektu bude pou\u017Eit CCD syst\u00E9m O.65-m dalekohledu na observato\u0159i v Ond\u0159ejov\u011B, kter\u00FD umo\u017E\u0148uje detekci NEAs do 20.-21. hv\u011Bzdn\u00E9 velikosti. To umo\u017En\u00ED b\u011Bhem doby trv\u00E1n\u00ED projektu z\u00EDskat m\u011B\u0159en\u00ED pro celkem 500 a\u017E 1000 nov\u011B objeven\u00FDch NEAs. Astrometrick\u00E1 m\u011B\u0159en\u00ED v r\u00E1mci navrhovan\u00E9ho projektu poskytnou data nezbytn\u00E1 k ur\u010Den\u00ED drah nov\u00FDch NEAs. Hlavn\u00EDm v\u011Bdeck\u00FDm c\u00EDlem fotometrick\u00FDch m\u011B\u0159en\u00ED je ur\u010Den\u00ED rotac\u00ED, tvaru a povrchov\u00FDch vlastnost\u00ED NEAs, co\u017E roz\u0161\u00ED\u0159\u00ED vzorek zn\u00E1m\u00FDch vlastnost\u00ED t\u011Bchto t\u011Bles nezbytn\u00FDch k pochopen\u00ED jejich vzniku, v\u00FDvoje a nebezpe\u010D\u00ED pro Zemi. Vedlej\u0161\u00EDm produktem projektu bude objeven\u00ED \u0159\u00E1dov\u011B 100 nov\u00FDch planetek hlavn\u00EDho p\u00E1su. T\u011Bsn\u00E1 spolupr\u00E1ce stanic ve sv\u011Bt\u011B je nezbytn\u00E1."@cs . . . "Optick\u00E9 sledov\u00E1n\u00ED nov\u00FDch t\u011Bles v okol\u00ED Zem\u011B"@cs . . "The objective of the project is a thorough astrometric follow-up and photometric study of new Near-Earth Asteroids (NEAs), which will be discovered within new search programmes (such as NEAT and LONEOS) with rapidly increasing rate during the next three years. CCD based camera system on the 0.65-m telescope at the Ond\u0159ejov Observatory will be used within this project. NEAs up to V=21 can be delected with the telescope system. It will allow observations of 500 to 1000 newly discovered NEAs during. the project duration.The global of the astrometric observations within the project is to provide data for orbital determinations of new NEAs, The main scientific aim of the photometrics observations is the investigation of rotation, shape, and surface properties of NEAs. The obtained results will enlarge an available sample of physical properties of NEAs, which will allow more reliable conclusions about their origin, evolution and risk for the Earth."@en . . "1"^^ . . "1834"^^ . . . "557"^^ . "Optical follow-up of new Near-Earth asteroids"@en . "15"^^ . . "15"^^ .