Steven Philley
Science Astronomy Atmosphere Site contents

Vol. Science · Astronomy · Passing

Retrograde
a line of sight

Mars does not stop and turn around. Earth does the passing. We ride a smaller orbit, and we move faster, so every so often we catch the outer planet and look past it. For a stretch the line of sight swings backward against the stars. That apparent reversal is retrograde. The orbit arrows on this cartoon never flip. Pair it with the solar map (where the planets actually sit), with seasons (Earth’s axis, not this passing), and with gravity, the pull that keeps both worlds on those tracks.

Educational schematic — circular orbits, flattened onto one plane, disks exaggerated so a phone can see them. Circle radii use the semimajor-axis ratio on NASA’s Mars Fact Sheet, 1.524, as if both paths were circles. They are not. That sheet lists Mars’s eccentricity as 0.0935 and its orbit inclination as 1.848°. Not an ephemeris. Not a date. Not for pointing a telescope from Campbell or anywhere else.

Interactive · Top-down

North up · both orbits counterclockwise · dashed ray is the line of sight

Apparent ecliptic longitude · the backward stretch is the dip

  • Sun
  • Earth · inner, faster
  • Mars · outer planet
  • Westward stretch · schematic
0 d

Literacy · words for the passing

Prograde
The usual apparent drift: west to east through the stars, night to night. StarChild uses that name for the ordinary direction. On this cartoon it is the rising parts of the longitude strip. Both planets are also moving prograde around the Sun the whole time — counterclockwise here — including during the backward stretch.
Retrograde
An apparent east-to-west drift against the stars. It is not a reversal of the orbit. StarChild: it happens roughly when a faster moving planet catches up to and passes a slower one. For Mars, that faster planet is Earth. APOD says the same loop shows up each time Earth laps a planet orbiting farther from the Sun. Jupiter and Saturn do this too. This drawing uses Mars as the outer planet.
Stationary
The pause between those directions, when the line of sight almost stops changing ecliptic longitude. There is one as Earth closes in, and one as Earth pulls away. The orbit arrow does not stop. “Stationary” is about the sky, not about a planet hanging in space.
Opposition
NASA’s Basics of Space Flight: Earth and the outer planet on the same side of the Sun, all three in a line. Night Sky Notes says the same thing from the ground — the planet is directly opposite the Sun as seen from Earth. On this slider that lineup is the middle of the westward stretch. The space-flight chapter calls opposition a good time to observe, and says the planet is then nearest. Mars’s eccentricity on the fact sheet is 0.0935, so a real closest approach can miss that instant. These circles do not time it.
Superior conjunction
The far-side lineup. Basics of Space Flight: Mars is a superior planet because its orbit is farther from the Sun than Earth’s, and superior planets have only superior conjunctions with the Sun — Earth and Mars on opposite sides, nearly in a straight line, Sun between. That is not the backward loop. The Conjunction preset jumps there. The strip stays on the passing, so the playhead leaves the zigzag.
Synodic period
The repeat of the same Sun–Earth–Mars alignment. NASA’s Mars Fact Sheet lists the synodic period as 779.94 days. Sidereal orbit periods on that sheet are 365.256 days for Earth and 686.980 days for Mars. This slider can walk one schematic lap using those mean periods on circles. It is not a calendar of the next opposition.
Apparent motion
What the line of sight does against the stars, not what the orbit does. StarChild’s classroom picture: stand beside a friend, walk faster, and as you pass they appear to drift backward even though they never turned around. The longitude strip is that illusion, unwrapped. A real retrograde also wanders a little in latitude and draws a loop on the sky — APOD’s photograph is that loop. This page keeps the orbits coplanar, so you get the east–west zigzag and not a star chart.

Sources · public NASA education

Cited, not invented

Classroom picture of a faster inner orbit overtaking a slower outer one. Not an ephemeris, not a pointing aid, and not a Campbell observing plan. Days on the slider are a coordinate of these circles, counted from a schematic opposition. Speeds, periods, and the 779.94-day synodic figure are the ones NASA publishes on the pages above. Earthrise preview: NASA / Bill Anders (public domain).

Keep going

Neighborhood

Solar map

Where Earth and Mars sit among the planets — day and local time, still a schematic.

Luna

Moon

A synodic month you can drag. A different clock from Mars’s 779.94-day lap.

Shadows

Eclipses

A lineup plus a node. Opposition here is a planet opposite the Sun, not a lunar eclipse.

Bulges

Tides

The Moon’s gravity, two bulges. Not this passing of worlds.

Tilt

Seasons

Earth’s axis, about 23.4°, kept parallel. Distance is not the reason for July.

Viewpoint

Local sky

What sits over Campbell. This page still will not place Mars in that chart.

The pull

Gravity

Why the inner orbit is the quicker one, and why neither path reverses.