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  2. Observations and explorations of Venus - Wikipedia

    en.wikipedia.org/wiki/Observations_and...

    The radar observations also allowed astronomers to determine that the rotation period of Venus was 243.1 days, [31] and that its axis of rotation was almost perpendicular to its orbital plane. It was also established that the radius of the planet was 6,052 kilometres (3,761 mi), some 70 kilometres (43 mi) less than the best previous figure ...

  3. List of missions to Venus - Wikipedia

    en.wikipedia.org/wiki/List_of_missions_to_Venus

    Flew past Venus on 6 December 2010 after failing to enter orbit. Insertion was successfully reattempted on 7 December 2015. Last contact April 2024 H-IIA 202: IKAROS: 20 May 2010: JAXA Japan: Flyby Successful Experimental solar sail released from the Akatsuki spacecraft. Flew past Venus on 8 December 2010 but did not make observations. H-IIA ...

  4. Orbit of Venus - Wikipedia

    en.wikipedia.org/wiki/Orbit_of_Venus

    Observation of the phases of Venus was inconsistent with this view but was consistent with the Polish astronomer Nicolaus Copernicus’s idea that the solar system is centered on the Sun. Galileo’s observation of the phases of Venus provided the first direct observational evidence for Copernican theory. [14]

  5. Venus - Wikipedia

    en.wikipedia.org/wiki/Venus

    Venus is the second planet from the Sun.It is a terrestrial planet and is the closest in mass and size to its orbital neighbour Earth.Venus has by far the densest atmosphere of the terrestrial planets, composed mostly of carbon dioxide with a thick, global sulfuric acid cloud cover.

  6. Phases of Venus - Wikipedia

    en.wikipedia.org/wiki/Phases_of_Venus

    The first observations of the full planetary phases of Venus were by Galileo at the end of 1610 (though not published until 1613 in the Letters on Sunspots).Using a telescope, Galileo was able to observe Venus going through a full set of phases, something prohibited by the Ptolemaic system that assumed Venus to be a perfect celestial body.

  7. 524522 Zoozve - Wikipedia

    en.wikipedia.org/wiki/524522_Zoozve

    524522 Zoozve (/ ˈ z uː z v eɪ / ⓘ; provisional designation 2002 VE 68) is a sub-kilometer sized asteroid and temporary quasi-satellite of Venus. [5] Discovered in 2002, it was the first such object to be discovered around a major planet in the Solar System.

  8. Atmosphere of Venus - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Venus

    The atmosphere of Venus is the very dense layer of gases surrounding the planet Venus. Venus's atmosphere is composed of 96.5% carbon dioxide and 3.5% nitrogen , with other chemical compounds present only in trace amounts. [ 1 ]

  9. CubeSat UV Experiment - Wikipedia

    en.wikipedia.org/wiki/CubeSat_UV_Experiment

    CubeSat UV Experiment (CUVE) is a space mission concept to study the atmospheric processes of the planet Venus with a small satellite. Specifically, the orbiter mission would study an enigmatic ultraviolet light absorber of unknown composition situated within the planet's uppermost cloud layer that absorbs about half the solar radiation downwelling in the planet's atmosphere.