Why do planets appear to move with respect to stars?

Imagine gazing up at the night sky and spotting Jupiter amongst a backdrop of twinkling stars. Over successive nights, you observe it seems to wander, changing positions against this stellar tapestry. This perceived wanderlust of planets, like strolling travelers among the relatively still stars, is known as the apparent motion of planets.

This apparent motion arises because while stars are indeed moving, their astronomical distances mean their movement relative to us is practically imperceptible in the short term. Planets, however, are much closer and complete their orbits in periods that are measurable within human lifetimes. As Earth spins on its axis and orbits the Sun, the relative positions of the planets change, giving them their characteristic meandering path in our sky.

For instance, Venus, often called the evening star, can visibly shift positions over just a few nights. But the fascinating part is, this motion isn't just the planets moving on their own. It's also us – aboard our spaceship Earth – moving through space, which collaborates in this cosmic dance, making planets appear to move against the backdrop of more distant stars.

When observing the night sky over several weeks or months, you might notice a planet like Mars taking a peculiar path. Instead of continuing its steady eastward journey across the sky, it pauses, reverses, and treks westward before resuming its original direction. This cosmic two-step is known as retrograde motion, a baffling illusion to early astronomers.

This apparent reversal doesn’t mean planets are changing their orbital direction. It's akin to overtaking a car on the highway; as you pull ahead, the other car appears to fall back, although it continues to move forward. Similarly, Earth sometimes overtakes another planet in their respective laps around the Sun, or vice versa, creating the illusion of retrograde motion when charted against the stationary star background.

During retrograde, planets draw a loop or zigzag in the sky. This loop isn't an actual change in their physical trajectory; it's a perspective trick because we're viewing two orbits in motion from the inside of one. Understanding this helps clarify how our observations from Earth can sometimes be deceiving.

Why do the planets not stray, but follow a predictable path across the sky through seasons and years? The gripping force of our solar system's maestro, the Sun, ensures each planet is held in a delicate balance of motion—this is the essence of planetary orbits.

Planets whirl around the Sun in ellipses, stretched circles, governed by gravity. The Sun's mass tugs on them, directing their paths, while their inertia wishes to send them flying off into space. This tug-of-war creates the elliptical orbits. Each planet’s orbit is unique, with varying distances and speeds, resulting in distinct orbital periods—the time taken to complete one full circuit around the Sun.

For instance, Mercury zips around in just 88 Earth days, while Neptune lumbers through its orbit in 165 Earth years! These variances in orbits and speeds lead to the rich tapestry of movement we observe in the celestial sphere. Recognizing the individual paths and periods of planets helps explain their various appearances and disappearances from our vantage point here on Earth—none is more evident than the retrograde motion during particular alignments in their orbital dance.