A guide to what's up in the sky for Southern Australia

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Starwatch for October 2026 (3rd Oct 2026)

Astronauts, looking out of the space station windows at night, see great clusters of lights; the glow of hundreds of thousands of individual lights that mark cities on earth.

From the ground, we can see great clusters of lights in the heavens, too; cities of stars we call globular clusters. They're somewhat lost in the background of stars, but binoculars or telescopes reveal their true nature: spherical clumps of thousands or even millions of stars. Our Milky Way galaxy contains a couple of hundred globular clusters.

The 2 greatest of these are to be found in the southern sky, but only one is visible these October nights. NGC 104 (also known as 47 Tuc) is shown on the star chart high in the south, just next to the Small Magellanic Cloud. Imagine a spherical region of space with our Sun at the centre and the outer edge four light-years away - the same distance as Alpha Centauri, our closest star system. Now imagine that this sphere contained a hundred thousand stars. The night sky would look alive with stars - bright stars in every direction, an overpowering cosmic light show. That's how the sky would appear if the solar system were transported to the centre of 47 Tuc!. One of my very favourite sights in a telescope!!

As we gaze to other parts of the spring night sky, we find that it is splashed with references to water. To the northeast we find Pisces, the fishes. The stars that make up this constellation are quite faint, so stay well hidden from direct lights. The mythological legend associated with this constellation tells how Venus and Cupid escaped from a giant by throwing themselves into the Euphrates River and changing into fishes.

Further to the east, Cetus, the Whale greets us. For the naked eye observer, the most interesting object within this constellation is the star named Mira. It is the most famous of all the variable stars, changing its brightness over the period of approximately 330 days from well below naked eye visibility that a small telescope is required to spot it to a brightness even seen from bright light polluted city skies. Because of that change, 17th-century astronomers called the star Mira – from the Latin word for “wonderful.”
The star changes because it pulses in and out like a beating heart. Mira’s in the final stages of its red-giant phase of life. Its core is no longer producing nuclear reactions. Instead, it is fusing hydrogen and helium in thin shells around the core.

Mira’s outer layers are puffed up by radiation from the shells. At the maximum, that inflates the star to about 400 times the diameter of the Sun. That’s also when its surface is coolest and faintest. As the outer layers cool, they fall inward, making the surface hotter and brighter again. At minimum, the star is about 330 times the Sun’s diameter. Each time it puffs up, Mira loses a little of the gas at its surface. Within the next million years or so, it’s likely to expel all the gas in its outer layers, leaving only its hot but dead core – a phase of stellar evolution known as a white dwarf.
Mira reached it’s maximum brightness for this period earlier this year. It’s currently heading to the minimum brightness, so you will need a telescope to see it. Astronomers have discovered thousands of stars like Mira. Our Sun will undergo the same phase in about six billion years.

In the southeastern sky, you can make a splash by jumping into Eridanus, the river. It is one of the largest constellations in the whole sky. It can be traced right across the sky from the far southern sky right to the equator. The southern end is marked by the star Achernar. We’ll need to wait till the summer stars shine in our evening sky before we can see the entire length of Eridanus.

The eastern evening sky is pretty bare at this time of year – lots of dark, empty spaces, but few bright stars. The one notable exception is Fomalhaut. It’s the brightest star of Piscis Austrinus, the southern fish. It’s high in the eastern sky as darkness falls.
The star we see as Fomalhaut is 25 light-years away. It’s about twice as big and heavy as the Sun, and more than 15 times brighter. It’s young – about 10 percent the age of the Sun. And it’s encircled by wide belts of dust. No planets have been discovered orbiting the star.

Fomalhaut has two companion stars, bound to it by their mutual gravitational pull. Both stars are smaller, cooler, and fainter than the Sun. One of them is barely visible to the eye alone, but you need a telescope to see the other.
Both stars are a long way from Fomalhaut itself. One is almost a light-year away, while the other is two and a half light-years. Astronomers know they’re bound to Fomalhaut because they’re moving in the same direction and at the same speed. Their composition is similar to Fomalhaut’s as well, and so is their age.

Fomalhaut itself will shine for another few hundred million years. But the companions will last much longer, billions of years for the larger one, and hundreds of billions of years for the other. So, they’ll still be shining across the galaxy long after the demise of their showy companion.
Let’s come closer to home now. The Orionid meteor shower should be at its most active from the late evening of October 21 to dawn the following morning. Unfortunately this year, the First Quarter Moon will affect observations until it sets around 2:30 am.

The shower is named for Orion because its meteors appear to “rain” into the sky from Orion the hunter. The constellation climbs into good view after midnight, so that’s when the shower is at its best – between midnight and dawn. You don’t have to look at Orion to see the meteors, though – they can blaze across any part of the sky.
The meteors are bits of debris left behind by Comet Halley. The comet sheds grains of dust as it orbits the Sun. When Earth crosses the comet’s path, some of those grains plunge into the atmosphere. They instantly vaporize, creating the streaks of light known as meteors. Chinese observers recorded this shower in 288 CE. Most of the dust grains are no bigger than pebbles. But a few are larger. They form brilliant streaks that are visible even in a somewhat light-polluted sky. And some of them can leave glowing trails that remain visible for a couple of minutes.
The shower has been declining in recent years. Halley’s Comet is near its greatest distance from Earth, so there aren’t as many bits of comet dust in this part of its orbital path left. Even so, the shower could produce 20 or more meteors per hour at its peak.
To watch the Orionids, find a dark but safe site away from city lights. Sit back and watch the sparks from Halley’s Comet. By the way, Comet Halley returns to our part of the solar system in 2061.
The glamour body of the solar system, Saturn, has returned to the evening sky. Easily located in the north-eastern sky as soon as it gets dark. Its rings are starting to open up again. Their tilt has opened up to about 4o, since we crossed the ring plane in March last year. The tilt will gradually increase to their widest of 27o in 2032.

Look low in the western sky soon after sunset, and you’ll be greeted by the planet Venus . In addition to its aesthetic appeal as it hovers in a golden sky, Venus is quite a stunning sight in a telescope. Because it is closer to the Sun than the Earth, it exhibits phases like the Moon. At the moment is resembles a 2-3 day old crescent Moon. Look for it on the evening of October 12. Both objects will be visible in the field of view of 7x50 binoculars, and both will show a thin crescent. Give yourself a celestial treat and look out for this event.
The Moon is at Last Quarter on October 3, at New on the 11th, at First Quarter on the 19th, and Full on October 26.