Mars opposition is in mid-January next year. At that time, Mars will appear brightest, and through a telescope it’ll be as large as it gets (at about 14 arcseconds). If you’ve got the right type of telescope (see below), you should be in for a treat. The excellent photo above was taken at the last Mars Opposition (November 2022) by George Schwab using a Celestron Schmidt-Cassegrain. I’m loving those colours.
I was preparing my regular talk for the Astro society the other day and I found myself on a tangent (that never happens). I was describing events for the month and I noticed that the 8th of December 2024 is a busy day for planets. On that day, Jupiter is at opposition, and both Neptune and Mars are stationary, with Neptune’s retrograde ending, and Mars’ retrograde starting.
I wanted to say some things about retrograde motion, but I found that it’s not a well-understood thing any more. Back in the days of the great Greek and Arabic astronomers, it was of huge importance, destroying cosmologies and furrowing many brows.
So what is retrograde motion, and why was it so important in the development in human scientific thinking?
Retrograde motion
From our perspective, planets are different from stars in that they wander the heavens (the word “planet” means just this: a wanderer). Against the background of the stars they move over time.
If you watch the stars night after night, you’ll notice that as the year gets older, everything moves towards the west. In relation to the Sun, stars rise and set about four minutes earlier each night. You can confirm this in a planetary app on your phone. However, if you look at a planet, for most of the year, it still moves westwards, but it travels a bit slower, setting a little more than four minutes earlier.
Comparing the planet to the background stars, it looks like the stars are overtaking the planet as they both move westwards. In terms of celestial coordinates, the Right Ascension (RA) of the planet increases each day (again, check your phone app).
I say for most of the year, because planets don’t always do this. Every so often they stop moving slower than the background stars, and move faster for a while, overtaking the stars in the background. Then, after another while, they stop and resume their normal pace again. In terms of coordinates, the RA decreases each day during this time. What’s even more puzzling, is that some of the planets get significantly brighter while they’re being overtaken by the background stars.
What’s going on here?
Ancient astronomers’ view
Nobody believes that astronomers in the past were unintelligent. Starting from a basic understanding of what they saw, these people started to make hypotheses as to what was going on in the sky. Early Greek theories made the assumption that stars and planets were a fixed distance from a central Earth, and that the planets wandered around amongst the stars.
It wasn’t long before that most powerful phrase in science came up, “that can’t be right, look!” Brightening during retrograde indicated that the planet was getting nearer to the Earth, which destroyed the “fixed distance” hypotheses. Making a very long story very short, one theory led to another falsification, and eventually we made our way to how we currently understand our solar system. Nobody really thinks we’ve got it completely ironed out though.
So what’s going on with Mars?
Our current understanding of retrograde is that orbiting planets catch and pass each other like runners on a track.
The following five maps (courtesy of https://www.heavens-above.com/) shows the relative positions of the Earth and Mars at five dates.