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  2. Aphrodite Terra - Wikipedia

    en.wikipedia.org/wiki/Aphrodite_Terra

    Aphrodite Terra / æ f r oʊ ˈ d aɪ t iː ˈ t ɛr ə / is one of the three continental regions on the planet Venus, the others being Ishtar Terra and Lada Terra.It is named for Aphrodite, the Greek equivalent of the goddess Venus, and is found near the equator of the planet.

  3. 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.

  4. List of orbits - Wikipedia

    en.wikipedia.org/wiki/List_of_orbits

    In such a system, L 3 –L 5 are situated slightly outside of the secondary's orbit despite their appearance in this small scale diagram. Horseshoe orbit: An orbit that appears to a ground observer to be orbiting a certain planet but is actually in co-orbit with the planet. See asteroids 3753 Cruithne and 2002 AA 29.

  5. Classical planet - Wikipedia

    en.wikipedia.org/wiki/Classical_planet

    A classical planet is an astronomical object that is visible to the naked eye and moves across the sky and its backdrop of fixed stars (the common stars which seem still in contrast to the planets). Visible to humans on Earth there are seven classical planets (the seven luminaries).

  6. List of terrae on Venus - Wikipedia

    en.wikipedia.org/wiki/List_of_terrae_on_Venus

    Aphrodite Terra is named after the Greek love goddess, the counterpart to Venus in Roman mythology. It is located on the southern hemisphere, just below the Equator. Ishtar Terra is named after a Babylonian love goddess. It is located on the northern hemisphere. Among its prominent features is the highest point on Venus, Maxwell Montes

  7. List of Solar System objects by size - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System...

    For the giant planets, the "radius" is defined as the distance from the center at which the atmosphere reaches 1 bar of atmospheric pressure. [ 11 ] Because Sedna and 2002 MS 4 have no known moons, directly determining their mass is impossible without sending a probe (estimated to be from 1.7x10 21 to 6.1×10 21 kg for Sedna [ 12 ] ).

  8. Geology of Venus - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Venus

    The surface of Venus is comparatively flat. When 93% of the topography was mapped by Pioneer Venus Orbiter, scientists found that the total distance from the lowest point to the highest point on the entire surface was about 13 kilometres (8.1 mi), about the same as the vertical distance between the Earth's ocean floor and the higher summits of the Himalayas.

  9. Ishtar Terra - Wikipedia

    en.wikipedia.org/wiki/Ishtar_Terra

    Topographic radar image view of Venus, with Ishtar Terra near center. Ishtar Terra / ˈ ɪ ʃ t ɑːr ˈ t ɛr ə / [1] is the second largest of the three continental terrae regions on the planet Venus, the others being Aphrodite Terra and Lada Terra. It is a highland region named after the Akkadian goddess Ishtar, [2] and is found in the north ...