Observing Jupiter's Galilean Moons is a great activity to undertake when the planet is approaching opposition.
Jupiter is next at opposition on 10 January 2026, meaning the planet is improving as we head into autumn and winter 2025.
Opposition is when a planet appears largest and brightest to us viewing from Earth.
For more advice, read our guide on how to observe Jupiter through a telescope
Jupiter Galilean Moon transit events
With Jupiter well placed for observation in autumn and winter 2025, there’s great opportunity to catch some of the planet’s interactions with its moons.
There are several excellent Jupiter moon events to watch out for in September 2025.
Because we’re nearing a Jovian equinox (next year), Callisto is now geometrically positioned to be involved in visible events again: the outer Galilean moon can be seen reappearing from behind Jupiter’s disc on 7 September at 04:46 BST (03:46 UT).
If you have the means to locate Jupiter in daylight, there’s a Ganymede shadow transit visible in the daytime on 14 September at 11:25–14:36 BST (10:25–13:36 UT).
A Callisto shadow transit occurs on 15 September between 02:30 and 05:13 BST (01:30–04:13 UT).
Callisto casts a large, dark shadow on Jupiter, something that can only occur when Jupiter is nearing an equinox.
Ganymede is eclipsed by Jupiter’s shadow on 25 September at 05:08 BST (04:08 UT) and there’s a double shadow transit involving Io’s and Europa’s shadows on 27 September at 05:54–06:41 BST (04:54–05:41 UT).
Finally, on the night of 28/29 September, Io’s shadow begins to cross Jupiter’s disc at 00:26 BST (23:26 UT), with Ganymede transiting at the same time.
Io itself follows onto the disc from 01:38 BST (00:38 UT), while its shadow moves off the disc at 02:39 BST (01:39 UT).
Ganymede completes its crossing at 03:41 BST (02:41 UT) and, just minutes later, Io exits at 03:54 BST (02:54 UT), just as Europa reappears from behind Jupiter. A busy evening!
Using WinJUPOS
A good challenge is to observe or image as many different types of Jupiter moon events as you can. A freeware application such as WinJUPOS can be used to determine when these events will occur.
Jupiter has many moons, but only four are large and bright enough to be seen easily through a telescope.
As they orbit Jupiter, Earth gets to view various interactions between them and the planet’s globe. A common event is a transit, which is when a moon appears to cross Jupiter’s disc.
The point of first contact at the start of the event is called transit ingress, abbreviated as TrI.
The point of last contact is known as transit egress (TrE).
A moon transit will be accompanied by a shadow transit.
This too has an ingress (ShI) and egress (ShE). A moon trails its shadow before opposition and precedes it after.
At opposition both transit in sync, a phenomenon which only lasts for a day or so.
All four Galilean moons can show the transits described, but outermost Callisto’s orbit, combined with the shallow 3.1° axial tilt of Jupiter, means for most of the time Callisto misses Jupiter’s disc, passing north or south of it.
Only near a Jovian equinox do Callisto and its shadow transit Jupiter’s disc.
Jupiter Galilean Moon eclipses and occultations
In addition to transit events, there are eclipses and occultations, events caused by Jupiter itself.
An occultation occurs when a moon passes behind Jupiter’s globe.
The two parts of this event are the occultation disappearance (OcD) and occultation reappearance (OcR).
Eclipses occur when one of the moons passes into Jupiter’s shadow.
When the moon disappears, this is referred to as eclipse disappearance (EcD) and when the moon reappears it’s an eclipse reappearance (EcR).
How occultations and eclipses occur depends on the angle between the Sun, Jupiter and Earth.
Before opposition, Jupiter’s shadow hangs west of the planet and a moon undergoes an eclipse disappearance but may remain within the shadow as it passes behind Jupiter, re-emerging as an occultation reappearance.
After opposition the reverse is true: a moon undergoes occultation disappearance then re-emerges from Jupiter’s shadow as an eclipse reappearance.
This slightly more complex scenario has a twist for the three outer Galileans, Europa, Ganymede and Callisto.
At certain times before opposition, these may enter Jupiter’s shadow (EcD), reappear from it (EcR) and then disappear behind Jupiter (OcD), finally re-emerging from the opposite side (OcR).
After opposition the sequence would be OcD, OcR, EcD and finally EcR.
This isn’t always the case, and the extra reappearance–disappearance stage in the middle doesn’t happen if Jupiter is close to opposition.
Observing Jupiter's Galilean moons: tips and tricks
Not only is Jupiter the largest of the planets – it would take 1,321 Earths to fill the volume of Jupiter – it’s also more than likely that it keeps the largest entourage of moons.
It’s the massive gravitational effect of Jupiter that does the trick, attracting more than 100 moons into orbit around the planet at the latest estimate.
Many of these satellites are fairly small and can’t be observed from Earth, but the biggest four are easy to spot with just a small pair of binoculars.
Binoculars
A minimum size pair of binoculars for spotting the four Galilean moons of Jupiter would be 7x50s, which magnify what your eyes see seven times and have front lenses that are 50mm in diameter.
You can certainly catch glimpses of these Galilean moons (named after Galileo, who first observed them) with hand-held binoculars.
However, your view will be much improved by resting the binoculars on a wall or fence, or even attaching them to a binocular tripod or mount with an inexpensive bracket.
With binoculars though, Jupiter itself will not appear as anything more than a large, slightly oval-shaped disc.
Telescope
The next step in viewing Jupiter Moons is to use a small telescope – one with a front lens 3 to 6 inches in diameter.As this gathers more light, it can magnify the view more, so the Moons will appear brighter and fill more of the field of view.
Don’t necessarily expect to see all four, however: as the moons travel around the planet they may be behind or in front of Jupiter when you’re looking.
It’s by using a larger scope with a front lens over 6 inches in diameter that you really start to see detail on Jupiter itself: not only the darker belts and lighter zones, but features within the gaseous atmosphere as well.
At this level of detail, observers can also see the occasional dark spot caused by the moons casting their shadows onto Jupiter’s atmosphere.
The joy of Jupiter is that whatever your level of equipment, there’s always something to see.
Galilean Moons at opposition
At opposition an interesting thing happens to the Galilean Moons when they transit the planet.
At this time their shadows appear to fall directly in line with the moons.
The alignment would be perfect if the declination of the Sun from Jupiter were 0° and the Sun–Earth–Jupiter alignment a perfect straight line.
In practice the declination won’t be 0°, but a little off at 3.1°.
Catching a moon passing at the exact point of opposition is down to luck and an offset of just a few hours either side is enough to show a misalignment.
However, it is interesting to see how a moon’s shadow precedes the moon that’s casting it before opposition and follows it after opposition.
Owners of smaller scopes will even be able to enjoy some amazing interactions between the planet and its 4 largest moons: Io, Europa, Ganymede and Callisto.
These moons are bright and easily visible through smaller instruments as points of light.
For those with larger-aperture scopes, it may be possible to perceive the moons as tiny discs, the apparent diameters being:
- Io: 1.2 arcseconds
- Europa: 1.0 arcseconds
- Ganymede: 1.7 arcseconds
- Callisto: 1.5 arcseconds
Facts about the Galilean Moons
Io
Diameter: 3,650km
The tremendous gravitational pull of Jupiter on this innermost of the four Galilean moons, together with its closeness to the planet, means Io whizzes round Jupiter in just 1.75 Earth days.
This fast orbital speed is easily seen in a small telescope: it visibly shifts position in just a few hours.
Physically, Io is the most volcanic place in the entire Solar System.
The whole world is covered in sulphurous lava flows and volcanoes erupting in plumes more than 500km high.
Europa
Diameter: 3,140km
The second Galilean moon out from Jupiter, Europa, should theoretically be visible with the naked eye since it shines at magnitude +5.3.
But Jupiter’s overwhelming brightness makes it difficult to separate the moon from the planet.
Europa’s brightness is due to its surface being smooth and icy.
Scientists suspect that underneath is a liquid water ocean, leaving open the possibility that life may lurk in the depths.
Ganymede
Diameter: 5,260km
The third major moon out from the planet is not only Jupiter’s biggest, but it is also the largest moon in the entire Solar System.
This is a world with a cold ice surface, a large warm ice (possibly water) mantle, a rocky interior and a liquid iron core. It measures a tremendous 5,260km across, which is bigger than Mercury.
Indeed, if Ganymede was released into space, it would be classed as a planet.
Callisto
Diameter: 4,820km
The last of the four giant Galilean satellites is Callisto.
It is the third largest of the Solar System, after Titan, the biggest of Saturn’s moons.
Callisto ranks as one of the most cratered worlds known – its entire icy, ancient surface is covered with impact craters that date right back to the time of the early Solar System, when the moon formed.
Like Europa, it is thought that beneath the surface may lie a watery ocean.
Share your observations and images of Jupiter's moons with us by emailing contactus@skyatnightmagazine.com
