Question: What type of path does Venus and Retrograde and prograde motion have in common?

Context paragraphs:
Capitoline Venus: The Capitoline Venus is a type of statue of Venus, specifically one of several "Venus Pudica" (modest Venus) types (others include the Venus de' Medici type), of which several examples exist.  The type ultimately derives from the Aphrodite of Cnidus.  The Capitoline Venus and her variants are recognisable from the position of the arms—standing after a bath, Venus begins to cover her breasts with her right hand, and her groin with her left hand.

Earth's rotation: Earth's rotation is the rotation of Planet Earth around its own axis.  Earth rotates eastward, in prograde motion.  As viewed from the north pole star Polaris, Earth turns counterclockwise.

Retrograde and prograde motion: Retrograde motion is motion in the direction opposite to the movement of something else and the contrary of direct or prograde motion.  This "motion" can be the orbit of one body about another body or about some other point, or the rotation of a single body about its axis, or other phenomena such as precession or nutation of the axis.  In reference to celestial "systems", retrograde motion "usually" means motion that is contrary to the rotation of the primary, that is, the object that forms the system's hub.

Non-inclined orbit: A non-inclined orbit is an orbit coplanar with a plane of reference.  The orbital inclination is 0° for prograde orbits, and π (180°) for retrograde ones.  If the plane of reference is a massive spheroid body's equatorial plane, these orbits are called equatorial; if the plane of reference is the ecliptic plane, they are called ecliptic.

Venus: Venus is the second planet from the Sun, orbiting it every 224.7 Earth days.  It has the longest rotation period (243 days) of any planet in the Solar System and rotates in the opposite direction to most other planets.  It has no natural satellites.  It is named after the Roman goddess of love and beauty.  It is the second-brightest natural object in the night sky after the Moon, reaching an apparent magnitude of −4.6 – bright enough to cast shadows at night and, rarely, visible to the naked eye in broad daylight.  Orbiting within Earth's orbit, Venus is an inferior planet and never appears to venture far from the Sun; its maximum angular distance from the Sun (elongation) is 47.8°.

Apparent retrograde motion: Apparent retrograde motion is the apparent motion of a planet in a direction opposite to that of other bodies within its system, as observed from a particular vantage point.  Direct motion or prograde motion is motion in the same direction as other bodies.

Retrograde ejaculation: Retrograde ejaculation occurs when semen, which would, in most cases, be ejaculated via the urethra, is redirected to the urinary bladder.  Normally, the sphincter of the bladder contracts before ejaculation forcing the semen to exit via the urethra, the path of least resistance.  When the bladder sphincter does not function properly, retrograde ejaculation may occur.  It can also be induced deliberately by a male as a primitive form of male birth control (known as "coitus saxonicus") or as part of certain alternative medicine practices.

Triple conjunction: A triple conjunction is an astronomical event, where two planets or a planet and a star meet each other three times in a short period either in opposition or at the time of inferior conjunction, if an inferior planet is involved.  The visible movement of the planet or the planets in the sky is therefore normally prograde at the first conjunction, retrograde at the second conjunction and again prograde at the third conjunction.

Tide clock: A tide clock is a specially designed clock that keeps track of the Moon's apparent motion around the Earth.  Along many coastlines, the Moon contributes the major part (67%) of the combined lunar and solar tides.  The exact interval between tides is influenced by the position of the Moon and Sun relative to the Earth, as well as the specific location on Earth where the tide is being measured.  Due to the Moon's orbital prograde motion, it takes a particular point on the Earth (on average) 24 hours and 50.5 minutes to rotate under the Moon, so the time between high lunar tides fluctuates between 12 and 13 hours.  A tide clock is divided into two roughly 6-hour tidal periods that shows the average length of time between high and low tides in a semi-diurnal tide region, such as most areas of the Atlantic Ocean.

High Earth orbit: A high Earth orbit is a geocentric orbit with an altitude entirely above that of a geosynchronous orbit (35,786 km ).  The orbital periods of such orbits are greater than twenty-four hours, therefore satellites in such orbits have an apparent retrograde motion – that is, even if they are in a prograde orbit (90° > inclination >= 0°), their orbital velocity is lower than Earth's rotational speed, causing their ground track to move westward on Earth's surface.

Supporting paragraphs: Venus Retrograde and prograde motion
Answer: orbit