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of 593
pro vyhledávání: '"Automated telescopes"'
The space probe 'New Horizon' was launched on 19th of January 2006 in order to study Pluto and its moons. Spacecraft will fly by Pluto as close as 12500 km in the middle of July 2015 and will get the most detailed images of Pluto and its moon until t
Externí odkaz:
http://arxiv.org/abs/1504.06199
Publikováno v:
In Planetary and Space Science March 2016 122:66-69
Publikováno v:
ASP Conference Series; 2020, Vol. 527, p439-442, 4p
Autor:
Sokov, E.1, Vereshchagina, I.1, Gnedin, Yu.1 gnedin@gao.spb.ru, Devyatkin, A.1, Gorshanov, D.1, Slesarenko, V.1, Ivanov, A.1, Naumov, K.1, Zinov'ev, S.1, Bekhteva, A.1, Romas, E.1, Karashevich, S.1, Kupriyanov, V.1
Publikováno v:
Astronomy Letters. Mar2012, Vol. 38 Issue 3, p180-190. 11p. 4 Charts, 8 Graphs.
Autor:
Bakos, G.1, Afonso, C.2, Henning, T.2, Jordán, A.2, Holman, M.1, Noyes, R. W.1, Sackett, P. D.3, Sasselov, D.1, Kovács, Gábor1, Csubry, Z.1, Pál, A.1
Publikováno v:
Proceedings of the International Astronomical Union. 05/02/2008, Vol. 4 Issue S253, p354-357. 4p.
Akademický článek
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Publikováno v:
Planetary and Space Science. 122:66-69
The space probe “New Horizons” was launched on 19th of January 2006 in order to study Pluto and its moons. Spacecraft performed close fly-by to Pluto on 14th of July 2015 and obtained the most detailed images of Pluto and its moon until this mome
Akademický článek
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Autor:
Yu. N. Gnedin, I. A. Vereshchagina, K. N. Naumov, E. S. Romas, A. V. Devyatkin, A. S. Bekhteva, V. V. Kupriyanov, S. V. Zinov’ev, S. V. Karashevich, A. V. Ivanov, V. Yu. Slesarenko, D. L. Gorshanov, E. N. Sokov
Publikováno v:
Astronomy Letters. 38:180-190
Exoplanet observations have been performed on the automated Pulkovo Observatory telescopes. We have obtained 33 transit light curves for 16 known exoplanets and six transit observations for three exoplanet candidates discovered by the Kepler telescop
Autor:
Francesco Pepe, M. Mayor
Publikováno v:
Astronomische Nachrichten. 325:501-506
During the past years, precise radial-velocity measurements have been the fundamental tool for the discovery and characterization of almost all the presently known extra-solar planets. The increasing precision and efficiency of this technique has als