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  2. Planetary phase - Wikipedia

    en.wikipedia.org/wiki/Planetary_phase

    The superior planets, orbiting outside the Earth's orbit, do not exhibit a full range of phases since their maximum phase angles are smaller than 90°. Mars often appears significantly gibbous, it has a maximum phase angle of 45°. Jupiter has a maximum phase angle of 11.1° and Saturn of 6°, [1] so their phases are almost always full.

  3. Quadrature (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Quadrature_(astronomy)

    Diagram showing the eastern and western quadratures of a superior planet like Mars. In spherical astronomy, quadrature is the configuration of a celestial object in which its elongation is a right angle (90 degrees), i.e., the direction of the object as viewed from Earth is perpendicular to the position of the Sun relative to Earth.

  4. Inferior and superior planets - Wikipedia

    en.wikipedia.org/wiki/Inferior_and_superior_planets

    "Inferior planet" refers to Mercury and Venus, which are closer to the Sun than Earth is. "Superior planet" refers to Mars, Jupiter, Saturn, Uranus, and Neptune (the latter two added later), which are further from the Sun than Earth is. The terms are sometimes used more generally; for example, Earth is an inferior planet relative to Mars.

  5. Phase angle (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Phase_angle_(astronomy)

    For some objects, such as the Moon (see lunar phases), Venus and Mercury the phase angle (as seen from the Earth) covers the full 0–180° range. The superior planets cover shorter ranges. For example, for Mars the maximum phase angle is about 45°. For Jupiter, the maximum is 11.1° and for Saturn 6°. [1]

  6. Phases of Venus - Wikipedia

    en.wikipedia.org/wiki/Phases_of_Venus

    The orbit of Venus is 224.7 Earth days (7.4 avg. Earth months [30.4 days]). The phases of Venus result from the planet's orbit around the Sun inside the Earth's orbit giving the telescopic observer a sequence of progressive lighting similar in appearance to the Moon's phases.

  7. Transit of Venus - Wikipedia

    en.wikipedia.org/wiki/Transit_of_Venus

    The 1882 transit is a member of #2. The 2004 transit is a member of #3, and the 2012 transit is a member of #4. The 2117 transit is a member of #1, and so on. However, the ascending node (December transits) of the orbit of Venus moves backwards after each 243 years so the transit of 2854 is the last member of series #3 instead of series #1.

  8. Phase curve (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Phase_curve_(astronomy)

    The phase curve of the Moon [26] compared to Mercury. [1] The phase curve of the Moon approximately resembles that of Mercury due to the similarities of the surfaces and the lack of an atmosphere on either body. [27] Clementine spacecraft data analyzed by J. Hillier, B. Buratti and K. Hill [28] indicate a lunar opposition surge.

  9. List of conjunctions (astronomy) - Wikipedia

    en.wikipedia.org/wiki/List_of_conjunctions...

    3.1° East September 3, 2019 10:44:25 Mercury 42' north of Mars 1.1° West September 13, 2019 21:35:21 Mercury 20' south of Venus 8.5° East October 30, 2019 08:29:03 Mercury 2°43' south of Venus 20.3° East November 24, 2019 14:00:35 Venus 1°24' south of Jupiter 26.2° East December 11, 2019 04:42:34 Venus 1°49' south of Saturn 30° East

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