Avtory i prava: Adam Tomashevskii
Perevod: Vol'nova A.A.
Poyasnenie:
30 iyunya na zakate Venera i Yupiter okazalis' ryadom nad zapadnym gorizontom, hotya na
samom dele oni vse eshe byli daleko drug ot druga.
Vblizi kul'minacii etogo zamechatel'nogo soedineniya dvuh vechernih planet ih udalos' zapechatlet' na
odnom teleskopicheskom kadre, i poluchilas' vot eta cifrovaya
slozhennaya fotografiya
iz Poznani v zapadnoi chasti central'noi Pol'shi.
Na samom dele, pokrytyi poloskami gazovyh oblakov Yupiter nahoditsya primerno v 910 millionah kilometrov.
Eto bolee chem v 11 raz dal'she serpa Venery, kotoraya v tot zhe moment byla v 78 millionah kilometrov.
No tak kak diametr Yupitera bolee chem v 11 raz prevyshaet razmer Venery, to obe planety vyglyadyat odinakovogo
uglovogo diametra.
V XVI veke pol'skii astronom Nikolai Kopernik tozhe naslazhdalsya podobnym zrelishem chetyreh Gallileevyh
sputnikov Yupitera i serpa Venery.
Nablyudeniya chetyreh sputnikov Yupitera i Venery v faze polumesyaca stali podtverzhdeniem
Kopernikovoi
geliocentricheskoi
modeli Solnechnoi sistemy.
1998 1999 2000 2001 2002 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018 2019 2020 2021 2022 2023 2024 |
Yanvar' Fevral' Mart Aprel' Mai Iyun' Iyul' Avgust Sentyabr' Oktyabr' Noyabr' Dekabr' |
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
|
Publikacii s klyuchevymi slovami:
conjunction - angular size - Copernicus - Galileo - Yupiter - Venera - Soedinenie planet
Publikacii so slovami: conjunction - angular size - Copernicus - Galileo - Yupiter - Venera - Soedinenie planet | |
Sm. takzhe:
Vse publikacii na tu zhe temu >> | |
